Author: "T. Young" / Topic: physics - Searchworks@Jio Institute Digital Library Search Results

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1. Performance of a Modular Ton-Scale Pixel-Readout Liquid Argon Time Projection Chamber

Author: A. Abed Abud, B. Abi, R. Acciarri, M. A. Acero, M. R. Adames, G. Adamov, M. Adamowski, D. Adams, M. Adinolfi, C. Adriano, A. Aduszkiewicz, J. Aguilar, B. Aimard, F. Akbar, K. Allison, S. Alonso Monsalve, M. Alrashed, A. Alton, R. Alvarez, T. Alves, H. Amar, P. Amedo, J. Anderson, D. A. Andrade, C. Andreopoulos, M. Andreotti, M. P. Andrews, F. Andrianala, S. Andringa, N. Anfimov, A. Ankowski, M. Antoniassi, M. Antonova, A. Antoshkin, A. Aranda-Fernandez, L. Arellano, E. Arrieta Diaz, M. A. Arroyave, J. Asaadi, A. Ashkenazi, D. Asner, L. Asquith, E. Atkin, D. Auguste, A. Aurisano, V. Aushev, D. Autiero, F. Azfar, A. Back, H. Back, J. J. Back, I. Bagaturia, L. Bagby, N. Balashov, S. Balasubramanian, P. Baldi, W. Baldini, J. Baldonedo, B. Baller, B. Bambah, R. Banerjee, F. Barao, G. Barenboim, P. B̃arham Alzás, G. J. Barker, W. Barkhouse, G. Barr, J. Barranco Monarca, A. Barros, N. Barros, D. Barrow, J. L. Barrow, A. Basharina-Freshville, A. Bashyal, V. Basque, C. Batchelor, L. Bathe-Peters, J. B. R. Battat, F. Battisti, F. Bay, M. C. Q. Bazetto, J. L. L. Bazo Alba, J. F. Beacom, E. Bechetoille, B. Behera, E. Belchior, G. Bell, L. Bellantoni, G. Bellettini, V. Bellini, O. Beltramello, N. Benekos, C. Benitez Montiel, D. Benjamin, F. Bento Neves, J. Berger, S. Berkman, J. Bernal, P. Bernardini, A. Bersani, S. Bertolucci, M. Betancourt, A. Betancur Rodríguez, A. Bevan, Y. Bezawada, A. T. Bezerra, T. J. Bezerra, A. Bhat, V. Bhatnagar, J. Bhatt, M. Bhattacharjee, M. Bhattacharya, S. Bhuller, B. Bhuyan, S. Biagi, J. Bian, K. Biery, B. Bilki, M. Bishai, A. Bitadze, A. Blake, F. D. Blaszczyk, G. C. Blazey, E. Blucher, J. Bogenschuetz, J. Boissevain, S. Bolognesi, T. Bolton, L. Bomben, M. Bonesini, C. Bonilla-Diaz, F. Bonini, A. Booth, F. Boran, S. Bordoni, R. Borges Merlo, A. Borkum, N. Bostan, J. Bracinik, D. Braga, B. Brahma, D. Brailsford, F. Bramati, A. Branca, A. Brandt, J. Bremer, C. Brew, S. J. Brice, V. Brio, C. Brizzolari, C. Bromberg, J. Brooke, A. Bross, G. Brunetti, M. Brunetti, N. Buchanan, H. Budd, J. Buergi, D. Burgardt, S. Butchart, G. Caceres V., I. Cagnoli, T. Cai, R. Calabrese, J. Calcutt, M. Calin, L. Calivers, E. Calvo, A. Caminata, A. F. Camino, W. Campanelli, A. Campani, A. Campos Benitez, N. Canci, J. Capó, I. Caracas, D. Caratelli, D. Carber, J. M. Carceller, G. Carini, B. Carlus, M. F. Carneiro, P. Carniti, I. Caro Terrazas, H. Carranza, N. Carrara, L. Carroll, T. Carroll, A. Carter, E. Casarejos, D. Casazza, J. F. Castaño Forero, F. A. Castaño, A. Castillo, C. Castromonte, E. Catano-Mur, C. Cattadori, F. Cavalier, F. Cavanna, S. Centro, G. Cerati, C. Cerna, A. Cervelli, A. Cervera Villanueva, K. Chakraborty, S. Chakraborty, M. Chalifour, A. Chappell, N. Charitonidis, A. Chatterjee, H. Chen, M. Chen, W. C. Chen, Y. Chen, Z. Chen-Wishart, D. Cherdack, C. Chi, R. Chirco, N. Chitirasreemadam, K. Cho, S. Choate, D. Chokheli, P. S. Chong, B. Chowdhury, D. Christian, A. Chukanov, M. Chung, E. Church, M. F. Cicala, M. Cicerchia, V. Cicero, R. Ciolini, P. Clarke, G. Cline, T. E. Coan, A. G. Cocco, J. A. B. Coelho, A. Cohen, J. Collazo, J. Collot, E. Conley, J. M. Conrad, M. Convery, S. Copello, P. Cova, C. Cox, L. Cremaldi, L. Cremonesi, J. I. Crespo-Anadón, M. Crisler, E. Cristaldo, J. Crnkovic, G. Crone, R. Cross, A. Cudd, C. Cuesta, Y. Cui, F. Curciarello, D. Cussans, J. Dai, O. Dalager, R. Dallavalle, W. Dallaway, H. da Motta, Z. A. Dar, R. Darby, L. Da Silva Peres, Q. David, G. S. Davies, S. Davini, J. Dawson, R. De Aguiar, P. De Almeida, P. Debbins, I. De Bonis, M. P. Decowski, A. de Gouvêa, P. C. De Holanda, I. L. De Icaza Astiz, P. De Jong, P. Del Amo Sanchez, A. De la Torre, G. De Lauretis, A. Delbart, D. Delepine, M. Delgado, A. Dell’Acqua, G. Delle Monache, N. Delmonte, P. De Lurgio, R. Demario, G. De Matteis, J. R. T. de Mello Neto, D. M. DeMuth, S. Dennis, C. Densham, P. Denton, G. W. Deptuch, A. De Roeck, V. De Romeri, J. P. Detje, J. Devine, R. Dharmapalan, M. Dias, A. Diaz, J. S. Díaz, F. Díaz, F. Di Capua, A. Di Domenico, S. Di Domizio, S. Di Falco, L. Di Giulio, P. Ding, L. Di Noto, E. Diociaiuti, C. Distefano, R. Diurba, M. Diwan, Z. Djurcic, D. Doering, S. Dolan, F. Dolek, M. J. Dolinski, D. Domenici, L. Domine, S. Donati, Y. Donon, S. Doran, D. Douglas, T. A. Doyle, A. Dragone, F. Drielsma, L. Duarte, D. Duchesneau, K. Duffy, K. Dugas, P. Dunne, B. Dutta, H. Duyang, D. A. Dwyer, A. S. Dyshkant, S. Dytman, M. Eads, A. Earle, S. Edayath, D. Edmunds, J. Eisch, P. Englezos, A. Ereditato, T. Erjavec, C. O. Escobar, J. J. Evans, E. Ewart, A. C. Ezeribe, K. Fahey, L. Fajt, A. Falcone, M. Fani’, C. Farnese, S. Farrell, Y. Farzan, D. Fedoseev, J. Felix, Y. Feng, E. Fernandez-Martinez, G. Ferry, L. Fields, P. Filip, A. Filkins, F. Filthaut, R. Fine, G. Fiorillo, M. Fiorini, S. Fogarty, W. Foreman, J. Fowler, J. Franc, K. Francis, D. Franco, J. Franklin, J. Freeman, J. Fried, A. Friedland, S. Fuess, I. K. Furic, K. Furman, A. P. Furmanski, R. Gaba, A. Gabrielli, A. M. Gago, F. Galizzi, H. Gallagher, A. Gallas, N. Gallice, V. Galymov, E. Gamberini, T. Gamble, F. Ganacim, R. Gandhi, S. Ganguly, F. Gao, S. Gao, D. Garcia-Gamez, M. Á. García-Peris, F. Gardim, S. Gardiner, D. Gastler, A. Gauch, J. Gauvreau, P. Gauzzi, S. Gazzana, G. Ge, N. Geffroy, B. Gelli, S. Gent, L. Gerlach, Z. Ghorbani-Moghaddam, T. Giammaria, D. Gibin, I. Gil-Botella, S. Gilligan, A. Gioiosa, S. Giovannella, C. Girerd, A. K. Giri, C. Giugliano, V. Giusti, D. Gnani, O. Gogota, S. Gollapinni, K. Gollwitzer, R. A. Gomes, L. V. Gomez Bermeo, L. S. Gomez Fajardo, F. Gonnella, D. Gonzalez-Diaz, M. Gonzalez-Lopez, M. C. Goodman, S. Goswami, C. Gotti, J. Goudeau, E. Goudzovski, C. Grace, E. Gramellini, R. Gran, E. Granados, P. Granger, C. Grant, D. R. Gratieri, G. Grauso, P. Green, S. Greenberg, J. Greer, W. C. Griffith, F. T. Groetschla, K. Grzelak, L. Gu, W. Gu, V. Guarino, M. Guarise, R. Guenette, E. Guerard, M. Guerzoni, D. Guffanti, A. Guglielmi, B. Guo, Y. Guo, A. Gupta, V. Gupta, G. Gurung, D. Gutierrez, P. Guzowski, M. M. Guzzo, S. Gwon, A. Habig, H. Hadavand, L. Haegel, R. Haenni, L. Hagaman, A. Hahn, J. Haiston, J. Hakenmueller, T. Hamernik, P. Hamilton, J. Hancock, F. Happacher, D. A. Harris, J. Hartnell, T. Hartnett, J. Harton, T. Hasegawa, C. Hasnip, R. Hatcher, K. Hayrapetyan, J. Hays, E. Hazen, M. He, A. Heavey, K. M. Heeger, J. Heise, S. Henry, M. A. Hernandez Morquecho, K. Herner, V. Hewes, A. Higuera, C. Hilgenberg, S. J. Hillier, A. Himmel, E. Hinkle, L. R. Hirsch, J. Ho, J. Hoff, A. Holin, T. Holvey, E. Hoppe, S. Horiuchi, G. A. Horton-Smith, M. Hostert, T. Houdy, B. Howard, R. Howell, I. Hristova, M. S. Hronek, J. Huang, R. G. Huang, Z. Hulcher, M. Ibrahim, G. Iles, N. Ilic, A. M. Iliescu, R. Illingworth, G. Ingratta, A. Ioannisian, B. Irwin, L. Isenhower, M. Ismerio Oliveira, R. Itay, C. M. Jackson, V. Jain, E. James, W. Jang, B. Jargowsky, D. Jena, I. Jentz, X. Ji, C. Jiang, J. Jiang, L. Jiang, A. Jipa, F. R. Joaquim, W. Johnson, C. Jollet, B. Jones, R. Jones, D. José Fernández, N. Jovancevic, M. Judah, C. K. Jung, T. Junk, Y. Jwa, M. Kabirnezhad, A. C. Kaboth, I. Kadenko, I. Kakorin, A. Kalitkina, D. Kalra, M. Kandemir, D. M. Kaplan, G. Karagiorgi, G. Karaman, A. Karcher, Y. Karyotakis, S. Kasai, S. P. Kasetti, L. Kashur, I. Katsioulas, A. Kauther, N. Kazaryan, L. Ke, E. Kearns, P. T. Keener, K. J. Kelly, E. Kemp, O. Kemularia, Y. Kermaidic, W. Ketchum, S. H. Kettell, M. Khabibullin, N. Khan, A. Khvedelidze, D. Kim, J. Kim, M. Kim, B. King, B. Kirby, M. Kirby, A. Kish, J. Klein, J. Kleykamp, A. Klustova, T. Kobilarcik, L. Koch, K. Koehler, L. W. Koerner, D. H. Koh, L. Kolupaeva, D. Korablev, M. Kordosky, T. Kosc, U. Kose, V. A. Kostelecký, K. Kothekar, I. Kotler, M. Kovalcuk, V. Kozhukalov, W. Krah, R. Kralik, M. Kramer, L. Kreczko, F. Krennrich, I. Kreslo, T. Kroupova, S. Kubota, M. Kubu, Y. Kudenko, V. A. Kudryavtsev, G. Kufatty, S. Kuhlmann, J. Kumar, P. Kumar, S. Kumaran, P. Kunze, J. Kunzmann, R. Kuravi, N. Kurita, C. Kuruppu, V. Kus, T. Kutter, J. Kvasnicka, T. Labree, T. Lackey, A. Lambert, B. J. Land, C. E. Lane, N. Lane, K. Lang, T. Langford, M. Langstaff, F. Lanni, O. Lantwin, J. Larkin, P. Lasorak, D. Last, A. Laudrain, A. Laundrie, G. Laurenti, E. Lavaut, A. Lawrence, P. Laycock, I. Lazanu, M. Lazzaroni, T. Le, S. Leardini, J. Learned, T. LeCompte, C. Lee, V. Legin, G. Lehmann Miotto, R. Lehnert, M. A. Leigui de Oliveira, M. Leitner, D. Leon Silverio, L. M. Lepin, J.-Y. Li, S. W. Li, Y. Li, H. Liao, C. S. Lin, D. Lindebaum, S. Linden, R. A. Lineros, J. Ling, A. Lister, B. R. Littlejohn, H. Liu, J. Liu, Y. Liu, S. Lockwitz, M. Lokajicek, I. Lomidze, K. Long, T. V. Lopes, J. Lopez, I. López de Rego, N. López-March, T. Lord, J. M. LoSecco, W. C. Louis, A. Lozano Sanchez, X.-G. Lu, K. B. Luk, B. Lunday, X. Luo, E. Luppi, J. Maalmi, D. MacFarlane, A. A. Machado, P. Machado, C. T. Macias, J. R. Macier, M. MacMahon, A. Maddalena, A. Madera, P. Madigan, S. Magill, C. Magueur, K. Mahn, A. Maio, A. Major, K. Majumdar, M. Man, R. C. Mandujano, J. Maneira, S. Manly, A. Mann, K. Manolopoulos, M. Manrique Plata, S. Manthey Corchado, V. N. Manyam, M. Marchan, A. Marchionni, W. Marciano, D. Marfatia, C. Mariani, J. Maricic, F. Marinho, A. D. Marino, T. Markiewicz, F. Das Chagas Marques, C. Marquet, D. Marsden, M. Marshak, C. M. Marshall, J. Marshall, L. Martina, J. Martín-Albo, N. Martinez, D. A. Martinez Caicedo, F. Martínez López, P. Martínez Miravé, S. Martynenko, V. Mascagna, C. Massari, A. Mastbaum, F. Matichard, S. Matsuno, G. Matteucci, J. Matthews, C. Mauger, N. Mauri, K. Mavrokoridis, I. Mawby, R. Mazza, A. Mazzacane, T. McAskill, N. McConkey, K. S. McFarland, C. McGrew, A. McNab, L. Meazza, V. C. N. Meddage, B. Mehta, P. Mehta, P. Melas, O. Mena, H. Mendez, P. Mendez, D. P. Méndez, A. Menegolli, G. Meng, A. C. E. A. Mercuri, A. Meregaglia, M. D. Messier, S. Metallo, J. Metcalf, W. Metcalf, M. Mewes, H. Meyer, T. Miao, A. Miccoli, G. Michna, V. Mikola, R. Milincic, F. Miller, G. Miller, W. Miller, O. Mineev, A. Minotti, L. Miralles, O. G. Miranda, C. Mironov, S. Miryala, S. Miscetti, C. S. Mishra, S. R. Mishra, A. Mislivec, M. Mitchell, D. Mladenov, I. Mocioiu, A. Mogan, N. Moggi, R. Mohanta, T. A. Mohayai, N. Mokhov, J. Molina, L. Molina Bueno, E. Montagna, A. Montanari, C. Montanari, D. Montanari, D. Montanino, L. M. Montaño Zetina, M. Mooney, A. F. Moor, Z. Moore, D. Moreno, O. Moreno-Palacios, L. Morescalchi, D. Moretti, R. Moretti, C. Morris, C. Mossey, M. Mote, C. A. Moura, G. Mouster, W. Mu, L. Mualem, J. Mueller, M. Muether, F. Muheim, A. Muir, M. Mulhearn, D. Munford, L. J. Munteanu, H. Muramatsu, J. Muraz, M. Murphy, T. Murphy, J. Muse, A. Mytilinaki, J. Nachtman, Y. Nagai, S. Nagu, R. Nandakumar, D. Naples, S. Narita, A. Nath, A. Navrer-Agasson, N. Nayak, M. Nebot-Guinot, A. Nehm, J. K. Nelson, O. Neogi, J. Nesbit, M. Nessi, D. Newbold, M. Newcomer, R. Nichol, F. Nicolas-Arnaldos, A. Nikolica, J. Nikolov, E. Niner, K. Nishimura, A. Norman, A. Norrick, P. Novella, J. A. Nowak, M. Oberling, J. P. Ochoa-Ricoux, S. Oh, S. B. Oh, A. Olivier, A. Olshevskiy, T. Olson, Y. Onel, Y. Onishchuk, A. Oranday, M. Osbiston, J. A. Osorio Vélez, L. Otiniano Ormachea, J. Ott, L. Pagani, G. Palacio, O. Palamara, S. Palestini, J. M. Paley, M. Pallavicini, C. Palomares, S. Pan, P. Panda, W. Panduro Vazquez, E. Pantic, V. Paolone, V. Papadimitriou, R. Papaleo, A. Papanestis, D. Papoulias, S. Paramesvaran, A. Paris, S. Parke, E. Parozzi, S. Parsa, Z. Parsa, S. Parveen, M. Parvu, D. Pasciuto, S. Pascoli, L. Pasqualini, J. Pasternak, C. Patrick, L. Patrizii, R. B. Patterson, T. Patzak, A. Paudel, L. Paulucci, Z. Pavlovic, G. Pawloski, D. Payne, V. Pec, E. Pedreschi, S. J. M. Peeters, W. Pellico, A. Pena Perez, E. Pennacchio, A. Penzo, O. L. G. Peres, Y. F. Perez Gonzalez, L. Pérez-Molina, C. Pernas, J. Perry, D. Pershey, G. Pessina, G. Petrillo, C. Petta, R. Petti, M. Pfaff, V. Pia, L. Pickering, F. Pietropaolo, V. L. Pimentel, G. Pinaroli, J. Pinchault, K. Pitts, K. Plows, R. Plunkett, C. Pollack, T. Pollman, D. Polo-Toledo, F. Pompa, X. Pons, N. Poonthottathil, V. Popov, F. Poppi, J. Porter, M. Potekhin, R. Potenza, J. Pozimski, M. Pozzato, T. Prakash, C. Pratt, M. Prest, F. Psihas, D. Pugnere, X. Qian, J. L. Raaf, V. Radeka, J. Rademacker, B. Radics, A. Rafique, E. Raguzin, M. Rai, S. Rajagopalan, M. Rajaoalisoa, I. Rakhno, L. Rakotondravohitra, L. Ralte, M. A. Ramirez Delgado, B. Ramson, A. Rappoldi, G. Raselli, P. Ratoff, R. Ray, H. Razafinime, E. M. Rea, J. S. Real, B. Rebel, R. Rechenmacher, M. Reggiani-Guzzo, J. Reichenbacher, S. D. Reitzner, H. Rejeb Sfar, E. Renner, A. Renshaw, S. Rescia, F. Resnati, D. Restrepo, C. Reynolds, M. Ribas, S. Riboldi, C. Riccio, G. Riccobene, J. S. Ricol, M. Rigan, E. V. Rincón, A. Ritchie-Yates, S. Ritter, D. Rivera, R. Rivera, A. Robert, J. L. Rocabado Rocha, L. Rochester, M. Roda, P. Rodrigues, M. J. Rodriguez Alonso, J. Rodriguez Rondon, S. Rosauro-Alcaraz, P. Rosier, D. Ross, M. Rossella, M. Rossi, M. Ross-Lonergan, N. Roy, P. Roy, C. Rubbia, A. Ruggeri, G. Ruiz Ferreira, B. Russell, D. Ruterbories, A. Rybnikov, A. Saa-Hernandez, R. Saakyan, S. Sacerdoti, S. K. Sahoo, N. Sahu, P. Sala, N. Samios, O. Samoylov, M. C. Sanchez, A. Sánchez Bravo, P. Sanchez-Lucas, V. Sandberg, D. A. Sanders, S. Sanfilippo, D. Sankey, D. Santoro, N. Saoulidou, P. Sapienza, C. Sarasty, I. Sarcevic, I. Sarra, G. Savage, V. Savinov, G. Scanavini, A. Scaramelli, A. Scarff, T. Schefke, H. Schellman, S. Schifano, P. Schlabach, D. Schmitz, A. W. Schneider, K. Scholberg, A. Schukraft, B. Schuld, A. Segade, E. Segreto, A. Selyunin, C. R. Senise, J. Sensenig, M. H. Shaevitz, P. Shanahan, P. Sharma, R. Kumar, K. Shaw, T. Shaw, K. Shchablo, J. Shen, C. Shepherd-Themistocleous, A. Sheshukov, W. Shi, S. Shin, S. Shivakoti, I. Shoemaker, D. Shooltz, R. Shrock, B. Siddi, M. Siden, J. Silber, L. Simard, J. Sinclair, G. Sinev, Jaydip Singh, J. Singh, L. Singh, P. Singh, V. Singh, S. Singh Chauhan, R. Sipos, C. Sironneau, G. Sirri, K. Siyeon, K. Skarpaas, J. Smedley, E. Smith, J. Smith, P. Smith, J. Smolik, M. Smy, M. Snape, E. L. Snider, P. Snopok, D. Snowden-Ifft, M. Soares Nunes, H. Sobel, M. Soderberg, S. Sokolov, C. J. Solano Salinas, S. Söldner-Rembold, S. R. Soleti, N. Solomey, V. Solovov, W. E. Sondheim, M. Sorel, A. Sotnikov, J. Soto-Oton, A. Sousa, K. Soustruznik, F. Spinella, J. Spitz, N. J. C. Spooner, K. Spurgeon, D. Stalder, M. Stancari, L. Stanco, J. Steenis, R. Stein, H. M. Steiner, A. F. Steklain Lisbôa, A. Stepanova, J. Stewart, B. Stillwell, J. Stock, F. Stocker, T. Stokes, M. Strait, T. Strauss, L. Strigari, A. Stuart, J. G. Suarez, J. Subash, A. Surdo, L. Suter, C. M. Sutera, K. Sutton, Y. Suvorov, R. Svoboda, S. K. Swain, B. Szczerbinska, A. M. Szelc, A. Sztuc, A. Taffara, N. Talukdar, J. Tamara, H. A. Tanaka, S. Tang, N. Taniuchi, A. M. Tapia Casanova, B. Tapia Oregui, A. Tapper, S. Tariq, E. Tarpara, E. Tatar, R. Tayloe, D. Tedeschi, A. M. Teklu, J. Tena Vidal, P. Tennessen, M. Tenti, K. Terao, F. Terranova, G. Testera, T. Thakore, A. Thea, A. Thiebault, S. Thomas, A. Thompson, C. Thorn, S. C. Timm, E. Tiras, V. Tishchenko, N. Todorović, L. Tomassetti, A. Tonazzo, D. Torbunov, M. Torti, M. Tortola, F. Tortorici, N. Tosi, D. Totani, M. Toups, C. Touramanis, D. Tran, R. Travaglini, J. Trevor, E. Triller, S. Trilov, J. Truchon, D. Truncali, W. H. Trzaska, Y. Tsai, Y.-T. Tsai, Z. Tsamalaidze, K. V. Tsang, N. Tsverava, S. Z. Tu, S. Tufanli, C. Tunnell, J. Turner, M. Tuzi, J. Tyler, E. Tyley, M. Tzanov, M. A. Uchida, J. Ureña González, J. Urheim, T. Usher, H. Utaegbulam, S. Uzunyan, M. R. Vagins, P. Vahle, S. Valder, G. A. Valdiviesso, E. Valencia, R. Valentim, Z. Vallari, E. Vallazza, J. W. F. Valle, R. Van Berg, R. G. Van de Water, D. V. Forero, A. Vannozzi, M. Van Nuland-Troost, F. Varanini, D. Vargas Oliva, S. Vasina, N. Vaughan, K. Vaziri, A. Vázquez-Ramos, J. Vega, S. Ventura, A. Verdugo, S. Vergani, M. Verzocchi, K. Vetter, M. Vicenzi, H. Vieira de Souza, C. Vignoli, C. Vilela, E. Villa, S. Viola, B. Viren, A. Vizcaya-Hernandez, T. Vrba, Q. Vuong, A. V. Waldron, M. Wallbank, J. Walsh, T. Walton, H. Wang, J. Wang, L. Wang, M. H. L. S. Wang, X. Wang, Y. Wang, K. Warburton, D. Warner, L. Warsame, M. O. Wascko, D. Waters, A. Watson, K. Wawrowska, A. Weber, C. M. Weber, M. Weber, H. Wei, A. Weinstein, H. Wenzel, S. Westerdale, M. Wetstein, K. Whalen, J. Whilhelmi, A. White, L. H. Whitehead, D. Whittington, M. J. Wilking, A. Wilkinson, C. Wilkinson, F. Wilson, R. J. Wilson, P. Winter, W. Wisniewski, J. Wolcott, J. Wolfs, T. Wongjirad, A. Wood, K. Wood, E. Worcester, M. Worcester, M. Wospakrik, K. Wresilo, C. Wret, S. Wu, W. Wu, M. Wurm, J. Wyenberg, Y. Xiao, I. Xiotidis, B. Yaeggy, N. Yahlali, E. Yandel, K. Yang, T. Yang, A. Yankelevich, N. Yershov, K. Yonehara, T. Young, B. Yu, H. Yu, J. Yu, Y. Yu, W. Yuan, R. Zaki, J. Zalesak, L. Zambelli, B. Zamorano, A. Zani, O. Zapata, L. Zazueta, G. P. Zeller, J. Zennamo, K. Zeug, C. Zhang, S. Zhang, M. Zhao, E. Zhivun, E. D. Zimmerman, S. Zucchelli, J. Zuklin, V. Zutshi, R. Zwaska, and on behalf of the DUNE Collaboration
Subjects: neutrino, near detector, Deep Underground Neutrino Experiment, DUNE, Physics, QC1-999, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: The Module-0 Demonstrator is a single-phase 600 kg liquid argon time projection chamber operated as a prototype for the DUNE liquid argon near detector. Based on the ArgonCube design concept, Module-0 features a novel 80k-channel pixelated charge readout and advanced high-coverage photon detection system. In this paper, we present an analysis of an eight-day data set consisting of 25 million cosmic ray events collected in the spring of 2021. We use this sample to demonstrate the imaging performance of the charge and light readout systems as well as the signal correlations between the two. We also report argon purity and detector uniformity measurements and provide comparisons to detector simulations.
Published: 2024
Full Text: View/download PDF

2. Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report

Author: A. Abed Abud, B. Abi, R. Acciarri, M. A. Acero, G. Adamov, D. Adams, M. Adinolfi, A. Aduszkiewicz, Z. Ahmad, J. Ahmed, T. Alion, S. Alonso Monsalve, M. Alrashed, C. Alt, A. Alton, P. Amedo, J. Anderson, C. Andreopoulos, M. P. Andrews, F. Andrianala, S. Andringa, N. Anfimov, A. Ankowski, M. Antonova, S. Antusch, A. Aranda-Fernandez, A. Ariga, L. O. Arnold, M. A. Arroyave, J. Asaadi, A. Aurisano, V. Aushev, D. Autiero, M. Ayala-Torres, F. Azfar, A. Back, H. Back, J. J. Back, C. Backhouse, P. Baesso, I. Bagaturia, L. Bagby, S. Balasubramanian, P. Baldi, B. Baller, B. Bambah, F. Barao, G. Barenboim, G. J. Barker, W. Barkhouse, C. Barnes, G. Barr, J. Barranco Monarca, N. Barros, J. L. Barrow, A. Basharina-Freshville, A. Bashyal, V. Basque, E. Belchior, J. B. R. Battat, F. Battisti, F. Bay, J. L. Bazo Alba, J. F. Beacom, E. Bechetoille, B. Behera, L. Bellantoni, G. Bellettini, V. Bellini, O. Beltramello, D. Belver, N. Benekos, F. Bento Neves, S. Berkman, P. Bernardini, R. M. Berner, H. Berns, S. Bertolucci, M. Betancourt, A. Betancur Rodríguez, M. Bhattacharjee, S. Bhuller, B. Bhuyan, S. Biagi, J. Bian, M. Biassoni, K. Biery, B. Bilki, M. Bishai, A. Bitadze, A. Blake, F. D. M. Blaszczyk, G. C. Blazey, E. Blucher, J. Boissevain, S. Bolognesi, T. Bolton, L. Bomben, M. Bonesini, M. Bongrand, F. Bonini, A. Booth, C. Booth, S. Bordoni, A. Borkum, T. Boschi, N. Bostan, P. Bour, C. Bourgeois, S. B. Boyd, D. Boyden, J. Bracinik, D. Braga, D. Brailsford, A. Brandt, J. Bremer, C. Brew, E. Brianne, S. J. Brice, C. Brizzolari, C. Bromberg, G. Brooijmans, J. Brooke, A. Bross, G. Brunetti, M. Brunetti, N. Buchanan, H. Budd, I. Cagnoli, D. Caiulo, P. Calafiura, J. Calcutt, M. Calin, S. Calvez, E. Calvo, A. Caminata, M. Campanelli, K. Cankocak, D. Caratelli, G. Carini, B. Carlus, P. Carniti, I. Caro Terrazas, H. Carranza, T. Carroll, J. F. Castaño Forero, A. Castillo, C. Castromonte, E. Catano-Mur, C. Cattadori, F. Cavalier, F. Cavanna, S. Centro, G. Cerati, A. Cervelli, A. Cervera Villanueva, M. Chalifour, A. Chappell, E. Chardonnet, N. Charitonidis, A. Chatterjee, S. Chattopadhyay, H. Chen, M. Chen, Y. Chen, Z. Chen, D. Cherdack, C. Chi, S. Childress, A. Chiriacescu, G. Chisnall, K. Cho, S. Choate, D. Chokheli, S. Choubey, A. Christensen, D. Christian, G. Christodoulou, A. Chukanov, E. Church, V. Cicero, P. Clarke, T. E. Coan, A. G. Cocco, J. A. B. Coelho, E. Conley, R. Conley, J. M. Conrad, M. Convery, S. Copello, L. Corwin, L. Cremaldi, L. Cremonesi, J. I. Crespo-Anadón, E. Cristaldo, R. Cross, A. Cudd, C. Cuesta, Y. Cui, D. Cussans, M. Dabrowski, O. Dalager, H. da Motta, L. Da Silva Peres, C. David, Q. David, G. S. Davies, S. Davini, J. Dawson, K. De, R. M. De Almeida, P. Debbins, I. De Bonis, M. P. Decowski, A. de Gouvêa, P. C. De Holanda, I. L. De Icaza Astiz, A. Deisting, P. De Jong, A. Delbart, D. Delepine, M. Delgado, A. Dell’Acqua, P. De Lurgio, J. R. T. de Mello Neto, D. M. DeMuth, S. Dennis, C. Densham, G. W. Deptuch, A. De Roeck, V. De Romeri, G. De Souza, R. Dharmapalan, F. Diaz, J. S. Díaz, S. Di Domizio, L. Di Giulio, P. Ding, L. Di Noto, C. Distefano, R. Diurba, M. Diwan, Z. Djurcic, N. Dokania, S. Dolan, M. J. Dolinski, L. Domine, D. Douglas, D. Douillet, G. Drake, F. Drielsma, D. Duchesneau, K. Duffy, P. Dunne, T. Durkin, H. Duyang, O. Dvornikov, D. A. Dwyer, A. S. Dyshkant, M. Eads, A. Earle, D. Edmunds, J. Eisch, L. Emberger, S. Emery, A. Ereditato, C. O. Escobar, G. Eurin, J. J. Evans, E. Ewart, A. C. Ezeribe, K. Fahey, A. Falcone, C. Farnese, Y. Farzan, J. Felix, M. Fernandes Carneiro da Silva, E. Fernandez-Martinez, P. Fernandez Menendez, F. Ferraro, L. Fields, F. Filthaut, A. Fiorentini, R. S. Fitzpatrick, W. Flanagan, B. Fleming, R. Flight, D. V. Forero, J. Fowler, W. Fox, J. Franc, K. Francis, D. Franco, J. Freeman, J. Freestone, J. Fried, A. Friedland, S. Fuess, I. Furic, A. P. Furmanski, A. Gabrielli, A. Gago, H. Gallagher, A. Gallas, A. Gallego-Ros, N. Gallice, V. Galymov, E. Gamberini, T. Gamble, R. Gandhi, R. Gandrajula, F. Gao, S. Gao, D. Garcia-Gamez, M. Á. García-Peris, S. Gardiner, D. Gastler, G. Ge, B. Gelli, A. Gendotti, S. Gent, Z. Ghorbani-Moghaddam, D. Gibin, I. Gil-Botella, S. Gilligan, C. Girerd, A. K. Giri, D. Gnani, O. Gogota, M. Gold, S. Gollapinni, K. Gollwitzer, R. A. Gomes, L. V. Gomez Bermeo, L. S. Gomez Fajardo, F. Gonnella, J. A. Gonzalez-Cuevas, D. Gonzalez-Diaz, M. Gonzalez-Lopez, M. C. Goodman, O. Goodwin, S. Goswami, C. Gotti, E. Goudzovski, C. Grace, M. Graham, R. Gran, E. Granados, P. Granger, A. Grant, C. Grant, D. Gratieri, P. Green, L. Greenler, J. Greer, W. C. Griffith, M. Groh, J. Grudzinski, K. Grzelak, W. Gu, V. Guarino, R. Guenette, E. Guerard, M. Guerzoni, A. Guglielmi, B. Guo, K. K. Guthikonda, R. Gutierrez, P. Guzowski, M. M. Guzzo, S. Gwon, A. Habig, H. Hadavand, R. Haenni, A. Hahn, J. Haiston, P. Hamacher-Baumann, T. Hamernik, P. Hamilton, J. Han, D. A. Harris, J. Hartnell, J. Harton, T. Hasegawa, C. Hasnip, R. Hatcher, K. W. Hatfield, A. Hatzikoutelis, C. Hayes, E. Hazen, A. Heavey, K. M. Heeger, J. Heise, K. Hennessy, S. Henry, M. A. Hernandez Morquecho, K. Herner, L. Hertel, J. Hewes, A. Higuera, T. Hill, S. J. Hillier, A. Himmel, J. Hoff, C. Hohl, A. Holin, E. Hoppe, G. A. Horton-Smith, M. Hostert, A. Hourlier, B. Howard, R. Howell, J. Huang, J. Hugon, G. Iles, N. Ilic, A. M. Iliescu, R. Illingworth, G. Ingratta, A. Ioannisian, L. Isenhower, R. Itay, A. Izmaylov, S. Jackson, V. Jain, E. James, B. Jargowsky, F. Jediny, D. Jena, Y. S. Jeong, C. Jesús-Valls, X. Ji, L. Jiang, S. Jiménez, A. Jipa, R. Johnson, N. Johnston, B. Jones, S. B. Jones, M. Judah, C. K. Jung, T. Junk, Y. Jwa, M. Kabirnezhad, A. Kaboth, I. Kadenko, I. Kakorin, F. Kamiya, N. Kaneshige, G. Karagiorgi, G. Karaman, A. Karcher, M. Karolak, Y. Karyotakis, S. Kasai, S. P. Kasetti, L. Kashur, N. Kazaryan, E. Kearns, P. Keener, K. J. Kelly, E. Kemp, O. Kemularia, W. Ketchum, S. H. Kettell, M. Khabibullin, A. Khotjantsev, A. Khvedelidze, D. Kim, B. King, B. Kirby, M. Kirby, J. Klein, K. Koehler, L. W. Koerner, S. Kohn, P. P. Koller, L. Kolupaeva, M. Kordosky, T. Kosc, U. Kose, V. A. Kostelecký, K. Kothekar, F. Krennrich, I. Kreslo, Y. Kudenko, V. A. Kudryavtsev, S. Kulagin, J. Kumar, P. Kumar, R. Kumar, P. Kunze, N. Kurita, C. Kuruppu, V. Kus, T. Kutter, A. Lambert, B. Land, K. Lande, C. E. Lane, K. Lang, T. Langford, J. Larkin, P. Lasorak, D. Last, C. Lastoria, A. Laundrie, G. Laurenti, A. Lawrence, I. Lazanu, R. LaZur, T. Le, S. Leardini, J. Learned, P. LeBrun, T. LeCompte, G. Lehmann Miotto, R. Lehnert, M. A. Leigui de Oliveira, M. Leitner, L. Li, S. W. Li, T. Li, Y. Li, H. Liao, C. S. Lin, Q. Lin, S. Lin, A. Lister, B. R. Littlejohn, J. Liu, S. Lockwitz, T. Loew, M. Lokajicek, I. Lomidze, K. Long, K. Loo, D. Lorca, T. Lord, J. M. LoSecco, W. C. Louis, X. G. Lu, K. B. Luk, X. Luo, N. Lurkin, T. Lux, V. P. Luzio, D. MacFarlane, A. A. Machado, P. Machado, C. T. Macias, J. R. Macier, A. Maddalena, A. Madera, P. Madigan, S. Magill, K. Mahn, A. Maio, A. Major, J. A. Maloney, G. Mandrioli, R. C. Mandujano, J. Maneira, L. Manenti, S. Manly, A. Mann, K. Manolopoulos, M. Manrique Plata, V. N. Manyam, L. Manzanillas, M. Marchan, A. Marchionni, W. Marciano, D. Marfatia, C. Mariani, J. Maricic, R. Marie, F. Marinho, A. D. Marino, D. Marsden, M. Marshak, C. M. Marshall, J. Marshall, J. Marteau, J. Martin-Albo, N. Martinez, D. A. Martinez Caicedo, S. Martynenko, K. Mason, A. Mastbaum, M. Masud, S. Matsuno, J. Matthews, C. Mauger, N. Mauri, K. Mavrokoridis, I. Mawby, R. Mazza, A. Mazzacane, E. Mazzucato, T. McAskill, E. McCluskey, N. McConkey, K. S. McFarland, C. McGrew, A. McNab, A. Mefodiev, P. Mehta, P. Melas, O. Mena, S. Menary, H. Mendez, D. P. Méndez, A. Menegolli, G. Meng, M. D. Messier, W. Metcalf, T. Mettler, M. Mewes, H. Meyer, T. Miao, G. Michna, T. Miedema, J. Migenda, V. Mikola, R. Milincic, W. Miller, J. Mills, C. Milne, O. Mineev, O. G. Miranda, S. Miryala, C. S. Mishra, S. R. Mishra, A. Mislivec, D. Mladenov, I. Mocioiu, K. Moffat, N. Moggi, R. Mohanta, T. A. Mohayai, N. Mokhov, J. Molina, L. Molina Bueno, A. Montanari, C. Montanari, D. Montanari, E. Montagna, L. M. Montano Zetina, J. Moon, M. Mooney, A. F. Moor, D. Moreno, C. Morris, C. Mossey, E. Motuk, C. A. Moura, J. Mousseau, W. Mu, L. Mualem, J. Mueller, M. Muether, S. Mufson, F. Muheim, A. Muir, M. Mulhearn, D. Munford, H. Muramatsu, S. Murphy, J. Musser, J. Nachtman, S. Nagu, M. Nalbandyan, R. Nandakumar, D. Naples, S. Narita, D. Navas-Nicolás, A. Navrer-Agasson, N. Nayak, M. Nebot-Guinot, K. Negishi, J. K. Nelson, J. Nesbit, M. Nessi, D. Newbold, M. Newcomer, D. Newhart, H. Newton, M. Niccolo, R. Nichol, F. Nicolas-Arnaldos, M. Nicoletta, E. Niner, K. Nishimura, A. Norman, A. Norrick, R. Northrop, P. Novella, J. A. Nowak, M. Oberling, J. P. Ochoa-Ricoux, A. Olivares Del Campo, A. Olivier, A. Olshevskiy, Y. Onel, Y. Onishchuk, J. Ott, L. Pagani, S. Pakvasa, G. Palacio, O. Palamara, S. Palestini, J. M. Paley, M. Pallavicini, C. Palomares, J. L. Palomino-Gallo, E. Pantic, V. Paolone, V. Papadimitriou, R. Papaleo, A. Papanestis, S. Paramesvaran, S. Parke, Z. Parsa, M. Parvu, S. Pascoli, L. Pasqualini, J. Pasternak, J. Pater, C. Patrick, L. Patrizii, R. B. Patterson, S. J. Patton, T. Patzak, A. Paudel, B. Paulos, L. Paulucci, Z. Pavlovic, G. Pawloski, D. Payne, V. Pec, S. J. M. Peeters, E. Pennacchio, A. Penzo, O. L. G. Peres, J. Perry, D. Pershey, G. Pessina, G. Petrillo, C. Petta, R. Petti, F. Piastra, L. Pickering, F. Pietropaolo, R. Plunkett, R. Poling, X. Pons, N. Poonthottathil, F. Poppi, S. Pordes, J. Porter, M. Potekhin, R. Potenza, B. V. K. S. Potukuchi, J. Pozimski, M. Pozzato, S. Prakash, T. Prakash, S. Prince, D. Pugnere, X. Qian, M. C. Queiroga Bazetto, J. L. Raaf, V. Radeka, J. Rademacker, B. Radics, A. Rafique, E. Raguzin, M. Rai, M. Rajaoalisoa, I. Rakhno, A. Rakotonandrasana, L. Rakotondravohitra, Y. A. Ramachers, R. Rameika, M. A. Ramirez Delgado, B. Ramson, A. Rappoldi, G. Raselli, P. Ratoff, S. Raut, R. F. Razakamiandra, J. S. Real, B. Rebel, M. Reggiani-Guzzo, T. Rehak, J. Reichenbacher, S. D. Reitzner, H. Rejeb Sfar, A. Renshaw, S. Rescia, F. Resnati, A. Reynolds, C. Riccio, G. Riccobene, L. C. J. Rice, J. Ricol, A. Rigamonti, Y. Rigaut, D. Rivera, L. Rochester, M. Roda, P. Rodrigues, M. J. Rodriguez Alonso, E. Rodriguez Bonilla, J. Rodriguez Rondon, S. Rosauro-Alcaraz, M. Rosenberg, P. Rosier, B. Roskovec, M. Rossella, J. Rout, P. Roy, S. Roy, A. Rubbia, C. Rubbia, F. C. Rubio, B. Russell, D. Ruterbories, R. Saakyan, S. Sacerdoti, T. Safford, R. Sahay, N. Sahu, P. Sala, N. Samios, O. Samoylov, M. C. Sanchez, D. A. Sanders, D. Sankey, S. Santana, M. Santos-Maldonado, N. Saoulidou, P. Sapienza, C. Sarasty, I. Sarcevic, G. Savage, V. Savinov, A. Scaramelli, A. Scarff, A. Scarpelli, T. Schaffer, H. Schellman, P. Schlabach, D. Schmitz, K. Scholberg, A. Schukraft, E. Segreto, J. Sensenig, I. Seong, A. Sergi, D. Sgalaberna, M. H. Shaevitz, S. Shafaq, M. Shamma, R. Sharankova, H. R. Sharma, R. Sharma, T. Shaw, C. Shepherd-Themistocleous, S. Shin, D. Shooltz, R. Shrock, L. Simard, F. Simon, N. Simos, J. Sinclair, G. Sinev, J. Singh, V. Singh, R. Sipos, F. W. Sippach, G. Sirri, A. Sitraka, K. Siyeon, K. Skarpaas VIII, A. Smith, E. Smith, P. Smith, J. Smolik, M. Smy, E. L. Snider, P. Snopok, M. Soares Nunes, H. Sobel, M. Soderberg, C. J. Solano Salinas, S. Söldner-Rembold, S. Soleti, N. Solomey, V. Solovov, W. E. Sondheim, M. Sorel, J. Soto-Oton, A. Sousa, K. Soustruznik, F. Spagliardi, M. Spanu, J. Spitz, N. J. C. Spooner, K. Spurgeon, R. Staley, M. Stancari, L. Stanco, R. Stanley, R. Stein, H. M. Steiner, J. Stewart, B. Stillwell, J. Stock, F. Stocker, T. Stokes, M. Strait, T. Strauss, S. Striganov, A. Stuart, J. G. Suarez, H. Sullivan, D. Summers, A. Surdo, V. Susic, L. Suter, C. M. Sutera, R. Svoboda, B. Szczerbinska, A. M. Szelc, R. Talaga, H. A. Tanaka, B. Tapia Oregui, A. Tapper, S. Tariq, E. Tatar, R. Tayloe, A. M. Teklu, M. Tenti, K. Terao, C. A. Ternes, F. Terranova, G. Testera, A. Thea, J. L. Thompson, C. Thorn, S. C. Timm, J. Todd, A. Tonazzo, D. Torbunov, M. Torti, M. Tortola, F. Tortorici, D. Totani, M. Toups, C. Touramanis, N. Tosi, R. Travaglini, J. Trevor, S. Trilov, W. H. Trzaska, Y. T. Tsai, Z. Tsamalaidze, K. V. Tsang, N. Tsverava, S. Tufanli, C. Tull, E. Tyley, M. Tzanov, M. A. Uchida, J. Urheim, T. Usher, S. Uzunyan, M. R. Vagins, P. Vahle, G. A. Valdiviesso, E. Valencia, P. Valerio, Z. Vallari, J. W. F. Valle, S. Vallecorsa, R. Van Berg, R. G. Van de Water, F. Varanini, D. Vargas, G. Varner, J. Vasel, S. Vasina, G. Vasseur, N. Vaughan, K. Vaziri, S. Ventura, A. Verdugo, S. Vergani, M. A. Vermeulen, M. Verzocchi, M. Vicenzi, H. Vieira de Souza, C. Vignoli, C. Vilela, B. Viren, T. Vrba, T. Wachala, A. V. Waldron, M. Wallbank, H. Wang, J. Wang, L. Wang, M. H. L. S. Wang, Y. Wang, K. Warburton, D. Warner, M. Wascko, D. Waters, A. Watson, P. Weatherly, A. Weber, M. Weber, H. Wei, A. Weinstein, D. Wenman, M. Wetstein, A. White, L. H. Whitehead, D. Whittington, M. J. Wilking, C. Wilkinson, Z. Williams, F. Wilson, R. J. Wilson, J. Wolcott, T. Wongjirad, A. Wood, K. Wood, E. Worcester, M. Worcester, C. Wret, W. Wu, Y. Xiao, E. Yandel, G. Yang, K. Yang, S. Yang, T. Yang, A. Yankelevich, N. Yershov, K. Yonehara, T. Young, B. Yu, H. Yu, J. Yu, W. Yuan, R. Zaki, J. Zalesak, L. Zambelli, B. Zamorano, A. Zani, L. Zazueta, G. Zeit, G. P. Zeller, J. Zennamo, K. Zeug, C. Zhang, M. Zhao, E. Zhivun, G. Zhu, P. Zilberman, E. D. Zimmerman, M. Zito, S. Zucchelli, J. Zuklin, V. Zutshi, R. Zwaska, and On behalf of the DUNE Collaboration
Subjects: neutrino, near detector, neutrino oscillations, Deep Underground Neutrino Experiment, DUNE, Physics, QC1-999, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: The Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment consists of a near detector, sited close to the source of the beam, and a far detector, sited along the beam at a large distance. This document, the DUNE Near Detector Conceptual Design Report (CDR), describes the design of the DUNE near detector and the science program that drives the design and technology choices. The goals and requirements underlying the design, along with projected performance are given. It serves as a starting point for a more detailed design that will be described in future documents.
Published: 2021
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3. Structural, magnetic, and ferroelectric properties of T-like cobalt-doped BiFeO3 thin films

Author: T. Young, P. Sharma, D. H. Kim, Thai Duy Ha, Jenh-Yih Juang, Y.-H. Chu, J. Seidel, V. Nagarajan, S. Yasui, M. Itoh, and D. Sando
Subjects: Biotechnology, TP248.13-248.65, Physics, QC1-999
Abstract: We present a comprehensive study of the physical properties of epitaxial cobalt-doped BiFeO3 films ∼50 nm thick grown on (001) LaAlO3 substrates. X-ray diffraction and magnetic characterization demonstrate high quality purely tetragonal-like (T′) phase films with no parasitic impurities. Remarkably, the step-and-terrace film surface morphology can be fully recovered following a local electric-field-induced rhombohedral-like to T′ phase transformation. Local switching spectroscopy experiments confirm the ferroelectric switching to follow previously reported transition pathways. Critically, we show unequivocal evidence for conduction at domain walls between polarization variants in T′-like BFO, making this material system an attractive candidate for domain wall-based nanoelectronics.
Published: 2018
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4. Accurate and efficient modeling of the transverse mode instability in high-energy laser amplifiers using the phase-matched model

Author: David M. Brown, Jonathan Hu, Joshua T. Young, Michael L. Dennis, Andy Goers, and Curtis R. Menyuk
Subjects: Physics, Nonlinear system, Speedup, Amplifier, Fiber laser, Mode (statistics), Phase (waves), Instability, Transverse mode, Computational physics
Abstract: We review recent work in which we developed a phase-matched model to study the transverse mode instability (TMI) in high-energy laser amplifiers. The standard models for TMI have contributions that vary rapidly compared to the beat period between the fundamental mode and the higher-order modes in the problem. In the phase-matched model, we neglect these rapidly varying contributions. We consider a realistic example with a Yb-doped fiber amplifier that is similar to the amplifier that was considered by Naderi et al. [Opt. Exp., 21(13), 16111 (2013)], but with a more realistic 10-m length. In this example, only one higher-order mode is present. We show that the computational speedup of the phase-matched model is on the order of 100 with no loss of accuracy even in the highly-saturated nonlinear regime.
Published: 2021

5. Surprising Twists in Nucleosomal DNA with Implication for Higher-order Folding

Author: Stefjord Todolli, Abigail S. Watkins, John Yager, Wilma K. Olson, Antonio Bu Sha, and Robert T. Young
Subjects: Physics, Models, Molecular, biology, Nucleosome disassembly, DNA Folding, computer.file_format, DNA, Protein Data Bank, Chromatin Assembly and Disassembly, Article, Nucleosomes, Folding (chemistry), Histones, chemistry.chemical_compound, Histone, chemistry, Structural Biology, biology.protein, Nucleosome, Nucleic Acid Conformation, Statistical physics, Twist, Molecular Biology, computer
Abstract: While nucleosomes are dynamic entities that must undergo structural deformations to perform their functions, the general view from available high-resolution structures is a largely static one. Even though numerous examples of twist defects have been documented, the DNA wrapped around the histone core is generally thought to be overtwisted. Analysis of available high-resolution structures from the Protein Data Bank reveals a heterogeneous distribution of twist along the nucleosomal DNA, with clear patterns that are consistent with the literature, and a significant fraction of structures that are undertwisted. The subtle differences in nucleosomal DNA folding, which extend beyond twist, have implications for nucleosome disassembly and modeled higher-order structures. Simulations of oligonucleosome arrays built with undertwisted models behave very differently from those constructed from overtwisted models, in terms of compaction and inter-nucleosome contacts, introducing configurational changes equivalent to those associated with 2-3 base-pair changes in nucleosome spacing. Differences in the nucleosomal DNA pathway, which underlie the way that DNA enters and exits the nucleosome, give rise to different nucleosome-decorated minicircles and affect the topological mix of configurational states.
Published: 2021

6. Physics Graduate Record Exam does not help applicants 'stand out'

Author: Marcos D. Caballero and Nicholas T. Young
Subjects: Medical education, LC8-6691, Physics, QC1-999, ComputingMilieux_COMPUTERSANDEDUCATION, General Physics and Astronomy, Special aspects of education, Education
Abstract: One argument for keeping the physics Graduate Record Exam (GRE) is that it can help applicants who might otherwise be missed in the admissions process stand out. In this work, we evaluate whether this claim is supported by physics graduate school admissions decisions. We used admissions data from five Ph.D.-granting physics departments over a 2-year period (N=2537) to see how the fraction of applicants admitted varied based on their physics GRE scores. We compared applicants with low GPAs to applicants with higher GPAs, applicants from large undergraduate universities to applicants from smaller undergraduate universities, and applicants from selective undergraduate institutions to applicants from less selective undergraduate institutions. We also performed a mediation and moderation analysis to provide statistical rigor and to better understand the previous relationships. We find that for applicants who might otherwise have been missed (e.g., have a low GPA or attended a small or less selective school), having a high physics GRE score did not seem to increase the applicant’s chances of being admitted to the schools. However, having a low physics GRE score seemed to penalize otherwise competitive applicants (i.e., applicants with mid to high GPAs). Thus, our work suggests that the physics GRE does not, in fact, help applicants who might otherwise be missed stand out.
Published: 2021

7. Accurate and efficient modeling of the transverse mode instability in high energy laser amplifiers

Author: Jonathan Hu, Curtis R. Menyuk, Andy Goers, Joshua T. Young, Michael L. Dennis, and David M. Brown
Subjects: Physics, business.industry, Amplifier, FOS: Physical sciences, Beat (acoustics), 02 engineering and technology, Grating, 021001 nanoscience & nanotechnology, 01 natural sciences, Instability, Atomic and Molecular Physics, and Optics, Transverse mode, 010309 optics, symbols.namesake, Optics, Amplitude, 0103 physical sciences, symbols, Rayleigh scattering, 0210 nano-technology, business, Refractive index, Optics (physics.optics), Physics - Optics
Abstract: We study the transverse mode instability (TMI) in the limit where a single higher-order mode (HOM) is present. We demonstrate that when the beat length between the fundamental mode and the HOM is small compared to the length scales on which the pump amplitude and the optical mode amplitudes vary, TMI is a three-wave mixing process in which the two optical modes beat with the phase-matched component of the index of refraction that is induced by the thermal grating. This limit is the usual limit in applications, and in this limit TMI is identified as a stimulated thermal Rayleigh scattering (STRS) process. We demonstrate that a phase-matched model that is based on the three-wave mixing equations can have a large computational advantage over current coupled mode methods that must use longitudinal step sizes that are small compared to the beat length.
Published: 2021

8. Feedback-stabilized dynamical steady states in the Bose-Hubbard model

Author: Ian B. Spielman, Alexey V. Gorshkov, and Jeremy T. Young
Subjects: Physics, Phase transition, Quantum Physics, Atomic Physics (physics.atom-ph), FOS: Physical sciences, Exact differential equation, State (functional analysis), Bose–Hubbard model, Physics - Atomic Physics, Quantum Gases (cond-mat.quant-gas), Weak measurement, Limit (mathematics), Statistical physics, Quantum Physics (quant-ph), Condensed Matter - Quantum Gases, Quantum, Quantum fluctuation
Abstract: The implementation of a combination of continuous weak measurement and classical feedback provides a powerful tool for controlling the evolution of quantum systems. In this work, we investigate the potential of this approach from three perspectives. First, we consider a double-well system in the classical large-atom-number limit, deriving the exact equations of motion in the presence of feedback. Second, we consider the same system in the limit of small atom number, revealing the effect that quantum fluctuations have on the feedback scheme. Finally, we explore the behavior of modest sized Hubbard chains using exact numerics, demonstrating the near-deterministic preparation of number states, a tradeoff between local and non-local feedback for state preparation, and evidence of a feedback-driven symmetry-breaking phase transition., 10 pages, 8 figures
Published: 2021

9. Critical theory for the breakdown of photon blockade

Author: Alexey V. Gorshkov, Michael Foss-Feig, H. J. Carmichael, Mohammad F. Maghrebi, Jeremy T. Young, Jonathan B. Curtis, and Igor Boettcher
Subjects: Physics, Quantum Physics, Phase transition, Photon, Statistical Mechanics (cond-mat.stat-mech), Atomic Physics (physics.atom-ph), FOS: Physical sciences, General Physics and Astronomy, Physics::Data Analysis, Statistics and Probability, 01 natural sciences, Physics - Atomic Physics, 010305 fluids & plasmas, Blockade, Quantum Gases (cond-mat.quant-gas), Quantum electrodynamics, 0103 physical sciences, Dissipative system, Physics::Atomic Physics, Condensed Matter - Quantum Gases, Quantum Physics (quant-ph), 010306 general physics, Condensed Matter - Statistical Mechanics
Abstract: Photon blockade is the result of the interplay between the quantized nature of light and strong optical nonlinearities, whereby strong photon-photon repulsion prevents a quantum optical system from absorbing multiple photons. We theoretically study a single atom coupled to the light field, described by the resonantly driven Jaynes--Cummings model, in which case the photon blockade breaks down in a second order phase transition at a critical drive strength. We show that this transition is associated to the spontaneous breaking of an anti-unitary PT-symmetry. Within a semiclassical approximation we calculate the expectation values of observables in the steady state. We then move beyond the semiclassical approximation and approach the critical point from the disordered (blockaded) phase by reducing the Lindblad quantum master equation to a classical rate equation that we solve. The width of the steady-state distribution in Fock space is found to diverge as we approach the critical point with a simple power-law, allowing us to calculate the critical scaling of steady state observables without invoking mean-field theory. We propose a simple physical toy model for biased diffusion in the space of occupation numbers, which captures the universal properties of the steady state. We list several experimental platforms where this phenomenon may be observed., Comment: 20 pages, 6 figures
Published: 2021

10. Investigating institutional influence on graduate program admissions by modeling physics Graduate Record Examination cutoff scores

Author: Nicholas T. Young, Nils J. Mikkelsen, and Marcos D. Caballero
Subjects: Medical education, LC8-6691, Physics, QC1-999, education, General Physics and Astronomy, Cutoff, Racial differences, Special aspects of education, Education
Abstract: Despite limiting access to applicants from underrepresented racial and ethnic groups, the practice of using hard or soft Graduate Record Examination (GRE) cutoff scores in physics graduate program admissions is still a popular method for reducing the pool of applicants. The present study considers whether the undergraduate institutions of applicants have any influence on the admissions process by modeling a physics GRE cutoff score with application data from admissions offices of five universities. Two distinct approaches based on inferential and predictive modeling are conducted. While there is some disagreement regarding the relative importance between features, the two approaches largely agree that including institutional information significantly aids the analysis. Both models identify cases where the institutional effects are comparable to factors of known importance such as gender and undergraduate GPA. As the results are stable across many cutoff scores, we advocate against the practice of employing physics GRE cutoff scores in admissions.
Published: 2021

11. The Photo-z Infrared Telescope (PIRT) -- a space instrument for rapid follow up of high-redshift gamma-ray bursts and electromagnetic counterparts to gravitational wave events

Author: J. Rodriguez, V. Torossian, A. Woodmansee, M. Hart, A. Balady, Sylvain Guiriec, T. C. Chang, A. J. van der Horst, R. O. Morris, P. Willems, R. Sambruna, David M. Russell, E. T. Young, N. E. White, M. Rud, R. Dyer, R. Terrile, Peter W. A. Roming, H. Fausey, and M. Seiffert
Subjects: Physics, Gravitational wave, Astrophysics::High Energy Astrophysical Phenomena, James Webb Space Telescope, Infrared telescope, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, FOS: Physical sciences, Field of view, Astrophysics::Cosmology and Extragalactic Astrophysics, Redshift, law.invention, Telescope, law, Target of opportunity, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Gamma-ray burst, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: The Photo-z InfraRed Telescope (PIRT) is an instrument on the Gamow Explorer, currently proposed for a NASA Astrophysics Medium Explorer. PIRT works in tandem with a companion wide-field instrument, the Lobster Eye X-ray Telescope (LEXT), that will identify x-ray transients likely to be associated with high redshift gamma-ray bursts (GRBs) or electromagnetic counterparts to gravitational wave (GW) events. After receiving an alert trigger from LEXT, the spacecraft will slew to center the PIRT field of view on the transient source. PIRT will then begin accumulating data simultaneously in five bands spanning 0.5 - 2.5 microns over a 10 arc-minute field of view. Each PIRT field will contain many hundreds of sources, only one of which is associated with the LEXT transient. PIRT will gather the necessary data in order to identify GRB sources with redshift $z > 6$, with an expected source localization better than 1 arcsec. A near real-time link to the ground will allow timely follow-up as a target of opportunity for large ground-based telescopes or the James Webb Space Telescope (JWST). PIRT will also allow localization and characterization of GW event counterparts. We discuss the instrument design, the on-board data processing approach, and the expected performance of the system., 10 pages, 5 figures
Published: 2021
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12. Supernova neutrino burst detection with the deep underground neutrino experiment: DUNE Collaboration

Author: M. A. Hernandez Morquecho, Jonas Rademacker, P. De Lurgio, C. A. Ternes, E. T. Worcester, H. Schellman, G. P. Zeller, C. J. Solano Salinas, Mingshui Chen, Andrew White, S. Berkman, André Rubbia, C. Barnes, Joshua Barrow, B. Bhuyan, O. V. Mineev, M. Bishai, Sandip Pakvasa, M. Chalifour, N. Poonthottathil, H. Berns, A. S. Hesam, S. H. Kettell, John Marshall, G. Sirri, Evgueni Goudzovski, M. A. Arroyave, J. Hugon, M. Kirby, D. Brailsford, Laura Paulucci, A. Hourlier, E. Hazen, L. Pasqualini, Christian Farnese, Armin Karcher, D. Smargianaki, Christopher L. Marshall, M. Karolak, H. Mendez, Y.-J. Jwa, Y. Karyotakis, Artur M. Ankowski, B. Morgan, L. Patrizii, Stefan Antusch, Paola Sala, N. Moggi, Claire Shepherd-Themistocleous, G. Mandrioli, M. R. While, A. M. Gago, R. Diurba, J. Berger, Alessandro Menegolli, B. Carlus, D. Boyden, T. Le, G. Christodoulou, L. Hertel, J. S. Díaz, B. Ramson, R. Gandrajula, Akitaka Ariga, Marvin L Marshak, R. Zaki, Ina Sarcevic, Eric W. Hoppe, Manuel Alejandro Segura Delgado, Kam-Biu Luk, M. Tzanov, K. Qi, J. A. B. Coelho, C. Vignoli, C. E. Lane, Giuseppe Benedetto Cerati, N. Bostan, David Delepine, Dave M Newbold, F. Krennrich, C. Mauger, J. Yu, D. Edmunds, P. Novella, K. Zeug, Z. Parsa, L. O. Arnold, Janice L. Thompson, F. Kamiya, K. Kothekar, S. Calvez, A. Chiriacescu, T. Rehak, M. V. Diwan, V. Savinov, P. Melas, T. Safford, E. Tatar, Hui Wang, V. Bellini, C. Alt, B. Abi, W. Flanagan, V. Papadimitriou, G. Zhu, S. Centro, J. J. Russell, W. C. Griffith, H. R. Gallagher, M. A. Uchida, N. Martinez, L. Greenler, Bo Yu, A. V. Waldron, D. J. Payne, C. Gotti, T. Miedema, S. Magill, Deywis Moreno, Utku Kose, Julián Félix, D. MacFarland, K. Gollwitzer, F. Varanini, S. Henry, K. Grzelak, B. Guo, Frank Filthaut, J. Reichenbacher, F. Muheim, Ralf Lehnert, T. A. Bolton, J. Greer, Y. T. Tsai, L. Camilleri, S. Nagu, J. A. Maloney, Z. Vallari, F. Bay, H.E. Rogers, Andrea Dell'Acqua, Y. Cui, P. A. Rodrigues, C. Wret, J. Zuklin, Paul Keener, D. A. Harris, Andrea Zani, Mario Campanelli, M. Newcomer, H. W. Sobel, C. Distefano, Ornella Palamara, M. A. Ramirez Delgado, J. D. Eisch, Riccardo Papaleo, D. Cherdack, Paolo Carniti, Leigh H. Whitehead, Karol Hennessy, S. Söldner-Rembold, P. Fernandez Menendez, J. Han, C. Y. Chi, M. Groh, Jeremy Wolcott, R. LaZur, Yu. Onishchuk, T. Hamernik, L. Pickering, John Evans, A. Weinstein, A. Sitraka, L. Bagby, S. J. Brice, Nicolas Lurkin, E. Raguzin, L. C. J. Rice, H. Carranza, Milos Lokajicek, K. Nishimura, H. S. Budd, C. S. Lin, A. A. Machado, Kevin J. Kelly, D. Sgalaberna, J. M. LoSecco, R. Petti, Y. Xiao, Ionel Lazanu, E. Zhivun, C. McGrew, Marzio Nessi, Chia-Chan Chang, M. Nebot-Guinot, C. Grant, Jaroslaw Pasternak, Z. Djurcic, W. Gu, D. Duchesneau, N. Kazaryan, Kendall Mahn, Jorge Molina, M. Oberling, H. O. Back, S. Sacerdoti, J. Sensenig, C. Montanari, E. Conley, B. Howard, D. M. DeMuth, A. Chatterjee, S. Kohn, F. Drielsma, J. L. Bazo Alba, Jane Nachtman, Y. A. Ramachers, D. A. Martinez Caicedo, R. M. de Almeida, Yasar Onel, V. Zutshi, Sandeep Miryala, Enrique Calvo, V. Radeka, C. Touramanis, S. Manly, P. Hamilton, R. G. Van de Water, J. Hoff, K. V. Tsang, J. Maneira, C. Rubbia, J. Calcutt, K. Warburton, M. Nalbandyan, T. Loew, P. Ding, F. Diaz, R. Hatcher, M. Zhao, A. Olivares Del Campo, F. Cavalier, Joshua R. Klein, Vasundhara Singh, Christopher Brew, Pavel Snopok, Y. Rigaut, Dave Sankey, J. Asaadi, E. Valencia, E. James, Roberto Gutiérrez, J. Pinzino, Rakesh Kumar, Ranjan Dharmapalan, Lynn Wood, S. Narita, R.A. Rameika, R. Illingworth, D. Vargas, Patrick Dunne, A. Bitadze, Yichen Li, A. G. Cocco, C. Andreopoulos, T. Kosc, R. J. Wilson, S. Fuess, E. Cristaldo, H. Razafinime, Alessandro Montanari, B. Zamorano, Warner A. Miller, M. C. Sanchez, Marc Weber, Wladyslaw Henryk Trzaska, A. Izmaylov, C. Morris, Dong Jo Kim, H. Muramatsu, K. Spurgeon, Z. Pavlovic, R. Gran, Claudia Brizzolari, D. Vanegas Forero, S. Biagi, M. Tenti, Alberto Cervelli, M. Roda, F. Terranova, C. Cuesta, J. Marteau, Irakli Lomidze, W. Metcalf, X. Luo, A. Booth, G. Petrillo, N.V. Mokhov, J. Barranco Monarca, Jianbei Liu, Zviad Tsamalaidze, H. da Motta, L. M. Cremaldi, Carl Grace, M. Bonesini, M. Muether, O. G. Miranda, A. N. Khotjantsev, N. Tsverava, R. B. Patterson, T. Young, A. Stuart, M. J. Wilking, D. Redondo, S. R. Mishra, F. Bento Neves, A. Gendotti, A. Himmel, M. Rajaoalisoa, P. Bour, C. Wilkinson, M. Greenwood, F. F. Wilson, Nektarios Benekos, Marco Adinolfi, D. Pugnere, T. Wongjirad, M. A. Vermeulen, Andrew Brandt, E. Bechetoille, S. Roy, A. Delbart, N. J. C. Spooner, J. M. Paley, C. Patrick, Antonio Ereditato, José W. F. Valle, N. Yershov, Renato Potenza, D. Lorca, M. Toups, R. Guenette, E. Pantic, L. Di Giulio, J. Martin-Albo, L. Molina Bueno, M. P. Decowski, Gustaaf Brooijmans, K. Moffat, V. Galymov, Dario Gnani, L. Mualem, S. Tufanli, J. Mills, Irina Mocioiu, D. Mladenov, A. L. Renshaw, C. N. Booth, L. Zambelli, Orlando L. G. Peres, S. Menary, P. C. de Holanda, D. A. Dwyer, S. Prince, J. Haiston, Marco Pallavicini, T. J. Langford, E. Niner, Nikolaos Simos, L. V. Gomez Bermeo, E. Gamberini, Haleh Khani Hadavand, E. Chardonnet, A. Mastbaum, G. Prior, Filippo Resnati, J. Stock, M. Kordosky, F. Andrianala, B. Tapia Oregui, N. Nayak, James Stewart, W. Ketchum, C. A. Moura, J. Spitz, L. Stanco, E. McCluskey, Ihn Sik Seong, L. W. Koerner, J. Franc, B. R. Littlejohn, R. M. Berner, K. Vaziri, A. Marchionni, K. Mason, A. Rafique, Randall P. Johnson, E. Motuk, J. A. Nowak, T. Patzak, M. D. Messier, G. Savage, A. M. Iliescu, Yasaman Farzan, David Cussans, J. Soto-Oton, Alex Reynolds, K. Biery, Yanchu Wang, Konstantinos Manolopoulos, S. Bordoni, James Mueller, William J. Marciano, V. Aushev, W. Fox, G. Pessina, C. M. Sutera, E. Smith, A. D. Marino, J. J. De Vries, S. Shafaq, Olga Mena, S. Ravat, W. Mu, D. Marfatia, C. Hohl, R. Haenni, R. K. Plunkett, P. Cotte, C. Jesús-Valls, J.V. Dawson, F. Azfar, T. Wachala, A. P. Furmanski, Barry King, P.T. Smith, Juraj Bracinik, Andrew Blake, L. Jiang, Kristian Harder, J. Hewes, D. Newhart, A. J. Roeth, R. Acciarri, A. Borkum, N. McConkey, R. Mazza, Keith Rielage, J. G. Boissevain, J. Smolik, A. McNab, Stephen P. Gent, C. Castromonte, G. Vasseur, G. Lehmann Miotto, N. Dokania, Paolo Calafiura, Q. David, C. S. Mishra, Vlastimil Kus, Seodong Shin, M. Santos-Maldonado, S. Li, Sukalyan Chattopadhyay, Laura Dominé, Silvia Pascoli, Kim Siyeon, J. Zalesak, Gabriella Carini, Thorsten Lux, M. Dabrowski, Pedro A. N. Machado, T. Alion, A. Scarff, L. Corwin, L. Simard, S. L. Mufson, L. Pagani, J. Rodriguez Rondon, Alec Habig, Sandro Palestini, P. N. Ratoff, Timothy M. Shaw, D. Braga, S. Di Domizio, G. Meng, C. Petta, T. Kutter, Matheus Hostert, S. Murphy, R. Bajou, R. Northrop, V. J. Guarino, A. Joglekar, Marco Verzocchi, L. S. Gomez Fajardo, K. S. McFarland, C. T. Macias, Jürgen Pozimski, R. Raboanary, F. Sergiampietri, P. Schlabach, Z. Ahmad, Rex Tayloe, F. Marinho, F. Barao, Jianming Bian, D. Autiero, Poonam Mehta, C. Backhouse, Stephen J. Parke, J. Perry, T. Schaffer, B. Russell, K. Herner, R. Van Berg, J. Chaves, Francesco Gonnella, B. Paulos, N. Solomey, Laura Manenti, R. Sipos, S. Matsuno, Z. Ghorbani-Moghaddam, J. K. Nelson, Hem Raj Sharma, Karol Lang, S. Bertolucci, Piera Sapienza, M. Shamma, A. Lambert, N. P. Samios, Andrew Smith, M. Manrique Plata, J. Bremer, C. K. Jung, G. Yang, I. Kreslo, Kyung-Suk Cho, A. Sousa, J. Urheim, D. Montanari, Giorgio Riccobene, A. Heavey, Grzegorz Deptuch, Stephen Hillier, M. Gold, Sergei Striganov, G. Brunetti, M. Vagins, T. Yang, A. Rappoldi, S. Ventura, S. Dennis, J. Ahmed, Narendra Sahu, Yi Chen, S. P. Kasetti, M. Betancourt, E. Pennacchio, Y. Penichot, K. Francis, F. Cavanna, Chao Zhang, A. Muir, A. Mazzacane, P. P. Koller, D. Whittington, N. Gallice, Wei Wu, G. Karagiorgi, F. W. Sippach, T. Li, F. Bonini, S. J. Patton, E. Church, M. Parvu, James A. Anderson, V. A. Kostelecký, S. Gao, D. Garcia-Gamez, V. Paolone, V. Pec, J. Pillow, S. Vergani, P. Vahle, G. A. Horton-Smith, C. Lastoria, E. Ewart, Claire David, D. Naples, I. Rakhno, Kazuhiro Terao, A. Paudel, V. Basque, G. S. Varner, M. H. Shaevitz, N. Barros, I. Caro Terrazas, R. Itay, Simon Lin, K. Wood, H. Duyang, H. Meyer, Katsuya Yonehara, S. Bolognesi, J. L. Raaf, J. Singh, V. A. Kudryavtsev, J. Wang, E. Kearns, A. C. Ezeribe, D. Belver, S. Zucchelli, S. Gollapinni, C. Sarasty, A. de Gouvea, Rukmani Mohanta, S. Martynenko, D. Shooltz, A. Schukraft, Andrew Norman, T. E. Coan, A. Lister, G. S. Davies, I. De Bonis, R. S. Fitzpatrick, B. Radics, Alan Watson, M. Spanu, Xiaolu Ji, L. Di Noto, A. M. Szelc, Alessandro Thea, K. Lande, E. D. Zimmerman, M. A. Leigui de Oliveira, Mafalda Dias, M. Wetstein, Ph. Lebrun, A. Christensen, S. Gwon, Matthew L Strait, L. Da Silva Peres, O. Goodwin, Jitendra Kumar, A. Gallego-Ros, M. Zito, G. Barenboim, N. Buchanan, S. Pordes, P. Weatherly, K. K. Guthikonda, James John Brooke, N. Mauri, A. Lawrence, Michael Mulhearn, I. K. Furic, M. M. Khabibullin, G. Testera, A. M. Teklu, John Matthews, A. Olivier, E. Blucher, L. Rakotondravohitra, B. Stillwell, M. Wallbank, S. B. Boyd, Matthew Mewes, Kai Loo, J. Trevor, W. E. Sondheim, Nikolina Ilic, T. Hill, M. O. Wascko, C. E. Tull, I. Kadenko, D. Waters, S. Prakash, D. Ruterbories, Antonino Sergi, S. Childress, T. Miao, A. Verdugo, D. Wenman, S. C. Timm, Y. Bezawada, R. Sharma, M. Biassoni, D. Pershey, V. P. Luzio, R. Saakyan, R. Nandakumar, E. Kemp, Aldo Penzo, R. J. Nichol, P. Guzowski, M. Eads, S. Rosauro-Alcaraz, M. Sorel, D. Totani, Sandhya Choubey, Burak Bilki, Christopher J. Milne, J. C. Freeman, Kaushik De, Jordan Ott, Niki Saoulidou, A. Aranda-Fernandez, A. Mefodiev, V. N. Solovov, A. Holin, Gareth J. Barker, C. Cattadori, Patrick Green, R. Howell, M. Soderberg, A. C. Weber, X. Pons, J. G. Learned, T. Stokes, M. J. Dolinski, L. Montaño Zetina, M. J. Rodriguez Alonso, M. A. Acero, Yu. Kudenko, L. Li, J. Fowler, J. A. Musser, M. Leyton, M. E. Convery, D. Gratieri, J. R. T. de Mello Neto, S. Balasubramanian, G. A. Valdiviesso, E. Brianne, C. Mossey, Kenneth Long, F. Pietropaolo, Raj Gandhi, T. Hasegawa, Giovanni Bellettini, M. Bhattacharjee, E. Granados, T. Lord, L. Zazueta, Alexander Deisting, B. Rebel, S. Green, Mathieu Bongrand, B. Behera, S. Emery, E. Mazzucato, H. Y. Liao, M. Masud, Amelia Maio, W. C. Louis, J. Freestone, D. Rivera, A. Surdo, S. Kasai, M. Worcester, H. S. Chen, George Adamov, A. Guglielmi, D. Franco, Joleen Pater, S. J. M. Peeters, K. Koehler, S. Alonso Monsalve, M. C. Goodman, G. Ge, Alexander Tapper, Thomas Strauss, D. C. Christian, Gregory Iles, A. Friedland, K. M. Heeger, K. Mavrokoridis, P. Lasorak, Srubabati Goswami, Z. Williams, S. Rescia, Andrés Castillo, David H. Adams, S. Santana, C. Mariani, D. A. Sanders, Carlos Escobar, R. A. Gomes, E. Gramellini, G. C. Blazey, J. Vasel, T. Durkin, H. Y. Wei, Alexandru Jipa, Olga Beltramello, M. Soares Nunes, J. A. Gonzalez-Cuevas, J. T. Haigh, L.S. Rochester, L. Escudero Sanchez, Ara Ioannisian, T. L. Usher, H. T. Rakotondramanana, H. A. Tanaka, Marcelo M. Guzzo, P. Baesso, C. Kuruppu, T. R. Junk, A. Maddalena, M. Antonova, F. Spagliardi, John F. Beacom, Janet Conrad, T. Boschi, B. Kirby, A. Bross, A. Caminata, D. Warner, J. Rout, C. E. Thorn, Steven Gardiner, P. Madigan, B. Gelli, Gregory J. Michna, D. Douglas, I. L. De Icaza Astiz, D. Gibin, A. Mann, P. de Jong, B. T. Fleming, F. D. M. Blaszczyk, R. Poling, K. Negishi, M. Pozzato, M. Stancari, Francesco Tortorici, J. Nesbit, Kate Scholberg, O. Gogota, A. Tonazzo, M. P. Andrews, Simon Jones, John Heise, A. F. Moor, Daniel Gastler, J. Moon, P. E. L. Clarke, C. Palomares, M. Potekhin, J. Hartnell, B. Viren, D. J. Summers, L. Cremonesi, L. Fields, J. R. Macier, R. Milincic, P. Bernardini, Robert Shrock, J. Zennamo, Lina Necib, J. Migenda, L. Suter, A. Laundrie, B. Szczerbinska, Enrique Fernandez-Martinez, R. Flight, J. Mousseau, H. Vieira de Souza, P. Debbins, J. Sinclair, Matthaeus Leitner, K. Fahey, F. Ferraro, Bindu A. Bambah, J. I. Crespo-Anadón, J. S. Real, A. De Roeck, M. Calin, L. Kashur, A. Scaramelli, M. Mellinato, F. Jediny, C. J. Densham, D. W. Schmitz, F. Piastra, H. Steiner, S. Lockwitz, Sudarshan Paramesvaran, C. Bromberg, G. Sinev, Massimo Rossella, Jack Fried, C. Girerd, B. V. K. S. Potukuchi, Alastair Grant, A. K. Giri, S. Davini, R. L. Talaga, Shu Li, F. Stocker, T. Gamble, R.J. Staley, R. Cross, J. J. Grudzinski, M. Torti, M. Tortola, B. Jargowsky, S. Tariq, I. Gil-Botella, Gregory J Pawloski, T. Prakash, Arsen Khvedelidze, A.S. Dyshkant, M. Reggiani-Guzzo, M. Á. García-Peris, Wayne A. Barkhouse, A. Mislivec, A. Filkins, Cari L. Johnson, M. Kabirnezhad, Pierre Baldi, M. Mooney, E. Tyley, A. Hahn, G.L. Raselli, G.D. Barr, Junwei Huang, V. De Romeri, A. Cervera Villanueva, Robert Svoboda, A. Falcone, M. Rai, A. Scarpelli, A. C. Kaboth, T. Vrba, D. Caratelli, L. Bellantoni, A. Hackenburg, D. Caiulo, S. Andringa, A. Papanestis, A. Aurisano, A. Norrick, B. J. P. Jones, C. Vilela, J. J. Back, Sergey A. Kulagin, A. Bashyal, Beatriz B. Siffert, Sofia Vallecorsa, K. E. Duffy, M. T. Graham, E. Segreto, Xin Qian, T. A. Mohayai, O.V. Dvornikov, V. Susic, S. D. Reitzner, M. B. Smy, K. Soustruznik, A. Higuera, Diana Navas-Nicolas, S. Jiménez, R. Zwaska, J. Maricic, Abi B., Acciarri R., Acero M.A., Adamov G., Adams D., Adinolfi M., Ahmad Z., Ahmed J., Alion T., Alonso Monsalve S., Alt C., Anderson J., Andreopoulos C., Andrews M.P., Andrianala F., Andringa S., Ankowski A., Antonova M., Antusch S., Aranda-Fernandez A., Ariga A., Arnold L.O., Arroyave M.A., Asaadi J., Aurisano A., Aushev V., Autiero D., Azfar F., Back H., Back J.J., Backhouse C., Baesso P., Bagby L., Bajou R., Balasubramanian S., Baldi P., Bambah B., Barao F., Barenboim G., Barker G.J., Barkhouse W., Barnes C., Barr G., Barranco Monarca J., Barros N., Barrow J.L., Bashyal A., Basque V., Bay F., Alba J.L.B., Beacom J.F., Bechetoille E., Behera B., Bellantoni L., Bellettini G., Bellini V., Beltramello O., Belver D., Benekos N., Bento Neves F., Berger J., Berkman S., Bernardini P., Berner R.M., Berns H., Bertolucci S., Betancourt M., Bezawada Y., Bhattacharjee M., Bhuyan B., Biagi S., Bian J., Biassoni M., Biery K., Bilki B., Bishai M., Bitadze A., Blake A., Blanco Siffert B., Blaszczyk F.D.M., Blazey G.C., Blucher E., Boissevain J., Bolognesi S., Bolton T., Bonesini M., Bongrand M., Bonini F., Booth A., Booth C., Bordoni S., Borkum A., Boschi T., Bostan N., Bour P., Boyd S.B., Boyden D., Bracinik J., Braga D., Brailsford D., Brandt A., Bremer J., Brew C., Brianne E., Brice S.J., Brizzolari C., Bromberg C., Brooijmans G., Brooke J., Bross A., Brunetti G., Buchanan N., Budd H., Caiulo D., Calafiura P., Calcutt J., Calin M., Calvez S., Calvo E., Camilleri L., Caminata A., Campanelli M., Caratelli D., Carini G., Carlus B., Carniti P., Caro Terrazas I., Carranza H., Castillo A., Castromonte C., Cattadori C., Cavalier F., Cavanna F., Centro S., Cerati G., Cervelli A., Cervera Villanueva A., Chalifour M., Chang C., Chardonnet E., Chatterjee A., Chattopadhyay S., Chaves J., Chen H., Chen M., Chen Y., Cherdack D., Chi C., Childress S., Chiriacescu A., Cho K., Choubey S., Christensen A., Christian D., Christodoulou G., Church E., Clarke P., Coan T.E., Cocco A.G., Coelho J.A.B., Conley E., Conrad J.M., Convery M., Corwin L., Cotte P., Cremaldi L., Cremonesi L., Crespo-Anadon J.I., Cristaldo E., Cross R., Cuesta C., Cui Y., Cussans D., Dabrowski M., da Motta H., Da Silva Peres L., David C., David Q., Davies G.S., Davini S., Dawson J., De K., De Almeida R.M., Debbins P., De Bonis I., Decowski M.P., de Gouvea A., De Holanda P.C., De Icaza Astiz I.L., Deisting A., De Jong P., Delbart A., Delepine D., Delgado M., Dell-Acqua A., De Lurgio P., de Mello Neto J.R.T., DeMuth D.M., Dennis S., Densham C., Deptuch G., De Roeck A., De Romeri V., De Vries J.J., Dharmapalan R., Dias M., Diaz F., Diaz J.S., Di Domizio S., Di Giulio L., Ding P., Di Noto L., Distefano C., Diurba R., Diwan M., Djurcic Z., Dokania N., Dolinski M.J., Domine L., Douglas D., Drielsma F., Duchesneau D., Duffy K., Dunne P., Durkin T., Duyang H., Dvornikov O., Dwyer D.A., Dyshkant A.S., Eads M., Edmunds D., Eisch J., Emery S., Ereditato A., Escobar C.O., Escudero Sanchez L., Evans J.J., Ewart E., Ezeribe A.C., Fahey K., Falcone A., Farnese C., Farzan Y., Felix J., Fernandez-Martinez E., Fernandez Menendez P., Ferraro F., Fields L., Filkins A., Filthaut F., Fitzpatrick R.S., Flanagan W., Fleming B., Flight R., Fowler J., Fox W., Franc J., Francis K., Franco D., Freeman J., Freestone J., Fried J., Friedland A., Fuess S., Furic I., Furmanski A.P., Gago A., Gallagher H., Gallego-Ros A., Gallice N., Galymov V., Gamberini E., Gamble T., Gandhi R., Gandrajula R., Gao S., Garcia-Gamez D., Garcia-Peris M.A., Gardiner S., Gastler D., Ge G., Gelli B., Gendotti A., Gent S., Ghorbani-Moghaddam Z., Gibin D., Gil-Botella I., Girerd C., Giri A.K., Gnani D., Gogota O., Gold M., Gollapinni S., Gollwitzer K., Gomes R.A., Gomez Bermeo L.V., Gomez Fajardo L.S., Gonnella F., Gonzalez-Cuevas J.A., Goodman M.C., Goodwin O., Goswami S., Gotti C., Goudzovski E., Grace C., Graham M., Gramellini E., Gran R., Granados E., Grant A., Grant C., Gratieri D., Green P., Green S., Greenler L., Greenwood M., Greer J., Griffith W.C., Groh M., Grudzinski J., Grzelak K., Gu W., Guarino V., Guenette R., Guglielmi A., Guo B., Guthikonda K.K., Gutierrez R., Guzowski P., Guzzo M.M., Gwon S., Habig A., Hackenburg A., Hadavand H., Haenni R., Hahn A., Haigh J., Haiston J., Hamernik T., Hamilton P., Han J., Harder K., Harris D.A., Hartnell J., Hasegawa T., Hatcher R., Hazen E., Heavey A., Heeger K.M., Heise J., Hennessy K., Henry S., Hernandez Morquecho M.A., Herner K., Hertel L., Hesam A.S., Hewes J., Higuera A., Hill T., Hillier S.J., Himmel A., Hoff J., Hohl C., Holin A., Hoppe E., Horton-Smith G.A., Hostert M., Hourlier A., Howard B., Howell R., Huang J., Hugon J., Iles G., Ilic N., Iliescu A.M., Illingworth R., Ioannisian A., Itay R., Izmaylov A., James E., Jargowsky B., Jediny F., Jesus-Valls C., Ji X., Jiang L., Jimenez S., Jipa A., Joglekar A., Johnson C., Johnson R., Jones B., Jones S., Jung C.K., Junk T., Jwa Y., Kabirnezhad M., Kaboth A., Kadenko I., Kamiya F., Karagiorgi G., Karcher A., Karolak M., Karyotakis Y., Kasai S., Kasetti S.P., Kashur L., Kazaryan N., Kearns E., Keener P., Kelly K.J., Kemp E., Ketchum W., Kettell S.H., Khabibullin M., Khotjantsev A., Khvedelidze A., Kim D., King B., Kirby B., Kirby M., Klein J., Koehler K., Koerner L.W., Kohn S., Koller P.P., Kordosky M., Kosc T., Kose U., Kostelecky V.A., Kothekar K., Krennrich F., Kreslo I., Kudenko Y., Kudryavtsev V.A., Kulagin S., Kumar J., Kumar R., Kuruppu C., Kus V., Kutter T., Lambert A., Lande K., Lane C.E., Lang K., Langford T., Lasorak P., Last D., Lastoria C., Laundrie A., Lawrence A., Lazanu I., LaZur R., Le T., Learned J., LeBrun P., Lehmann Miotto G., Lehnert R., Leigui de Oliveira M.A., Leitner M., Leyton M., Li L., Li S., Li S.W., Li T., Li Y., Liao H., Lin C.S., Lin S., Lister A., Littlejohn B.R., Liu J., Lockwitz S., Loew T., Lokajicek M., Lomidze I., Long K., Loo K., Lorca D., Lord T., LoSecco J.M., Louis W.C., Luk K.B., Luo X., Lurkin N., Lux T., Luzio V.P., MacFarland D., Machado A.A., Machado P., Macias C.T., Macier J.R., Maddalena A., Madigan P., Magill S., Mahn K., Maio A., Major A., Maloney J.A., Mandrioli G., Maneira J., Manenti L., Manly S., Mann A., Manolopoulos K., Manrique Plata M., Marchionni A., Marciano W., Marfatia D., Mariani C., Maricic J., Marinho F., Marino A.D., Marshak M., Marshall C., Marshall J., Marteau J., Martin-Albo J., Martinez N., Martinez Caicedo D.A., Martynenko S., Mason K., Mastbaum A., Masud M., Matsuno S., Matthews J., Mauger C., Mauri N., Mavrokoridis K., Mazza R., Mazzacane A., Mazzucato E., McCluskey E., McConkey N., McFarland K.S., McGrew C., McNab A., Mefodiev A., Mehta P., Melas P., Mellinato M., Mena O., Menary S., Mendez H., Menegolli A., Meng G., Messier M.D., Metcalf W., Mewes M., Meyer H., Miao T., Michna G., Miedema T., Migenda J., Milincic R., Miller W., Mills J., Milne C., Mineev O., Miranda O.G., Miryala S., Mishra C.S., Mishra S.R., Mislivec A., Mladenov D., Mocioiu I., Moffat K., Moggi N., Mohanta R., Mohayai T.A., Mokhov N., Molina J., Molina Bueno L., Montanari A., Montanari C., Montanari D., Montano Zetina L.M., Moon J., Mooney M., Moor A., Moreno D., Morgan B., Morris C., Mossey C., Motuk E., Moura C.A., Mousseau J., Mu W., Mualem L., Mueller J., Muether M., Mufson S., Muheim F., Muir A., Mulhearn M., Muramatsu H., Murphy S., Musser J., Nachtman J., Nagu S., Nalbandyan M., Nandakumar R., Naples D., Narita S., Navas-Nicolas D., Nayak N., Nebot-Guinot M., Necib L., Negishi K., Nelson J.K., Nesbit J., Nessi M., Newbold D., Newcomer M., Newhart D., Nichol R., Niner E., Nishimura K., Norman A., Norrick A., Northrop R., Novella P., Nowak J.A., Oberling M., Olivares Del Campo A., Olivier A., Onel Y., Onishchuk Y., Ott J., Pagani L., Pakvasa S., Palamara O., Palestini S., Paley J.M., Pallavicini M., Palomares C., Pantic E., Paolone V., Papadimitriou V., Papaleo R., Papanestis A., Paramesvaran S., Parke S., Parsa Z., Parvu M., Pascoli S., Pasqualini L., Pasternak J., Pater J., Patrick C., Patrizii L., Patterson R.B., Patton S.J., Patzak T., Paudel A., Paulos B., Paulucci L., Pavlovic Z., Pawloski G., Payne D., Pec V., Peeters S.J.M., Penichot Y., Pennacchio E., Penzo A., Peres O.L.G., Perry J., Pershey D., Pessina G., Petrillo G., Petta C., Petti R., Piastra F., Pickering L., Pietropaolo F., Pillow J., Pinzino J., Plunkett R., Poling R., Pons X., Poonthottathil N., Pordes S., Potekhin M., Potenza R., Potukuchi B.V.K.S., Pozimski J., Pozzato M., Prakash S., Prakash T., Prince S., Prior G., Pugnere D., Qi K., Qian X., Raaf J.L., Raboanary R., Radeka V., Rademacker J., Radics B., Rafique A., Raguzin E., Rai M., Rajaoalisoa M., Rakhno I., Rakotondramanana H.T., Rakotondravohitra L., Ramachers Y.A., Rameika R., Ramirez Delgado M.A., Ramson B., Rappoldi A., Raselli G., Ratoff P., Ravat S., Razafinime H., Real J.S., Rebel B., Redondo D., Reggiani-Guzzo M., Rehak T., Reichenbacher J., Reitzner S.D., Renshaw A., Rescia S., Resnati F., Reynolds A., Riccobene G., Rice L.C.J., Rielage K., Rigaut Y., Rivera D., Rochester L., Roda M., Rodrigues P., Rodriguez Alonso M.J., Rodriguez Rondon J., Roeth A.J., Rogers H., Rosauro-Alcaraz S., Rossella M., Rout J., Roy S., Rubbia A., Rubbia C., Russell B., Russell J., Ruterbories D., Saakyan R., Sacerdoti S., Safford T., Sahu N., Sala P., Samios N., Sanchez M.C., Sanders D.A., Sankey D., Santana S., Santos-Maldonado M., Saoulidou N., Sapienza P., Sarasty C., Sarcevic I., Savage G., Savinov V., Scaramelli A., Scarff A., Scarpelli A., Schaffer T., Schellman H., Schlabach P., Schmitz D., Scholberg K., Schukraft A., Segreto E., Sensenig J., Seong I., Sergi A., Sergiampietri F., Sgalaberna D., Shaevitz M.H., Shafaq S., Shamma M., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Smargianaki D., Smith A., Smith E., Smith P., Smolik J., Smy M., Snopok P., Soares Nunes M., Sobel H., Soderberg M., Solano Salinas C.J., Soldner-Rembold S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Tapia Oregui B., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Tonazzo A., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Trevor J., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Vallari Z., Valle J.W.F., Vallecorsa S., Van Berg R., Van de Water R.G., Vanegas Forero D., Varanini F., Vargas D., Varner G., Vasel J., Vasseur G., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., Vieira de Souza H., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., Yang T., Yershov N., Yonehara K., Young T., Yu B., Yu J., Zaki R., Zalesak J., Zambelli L., Zamorano B., Zani A., Zazueta L., Zeller G.P., Zennamo J., Zeug K., Zhang C., Zhao M., Zhivun E., Zhu G., Zimmerman E.D., Zito M., Zucchelli S., Zuklin J., Zutshi V., Zwaska R., Abi, B., Acciarri, R., Acero, M. 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I., Cristaldo, E., Cross, R., Cuesta, C., Cui, Y., Cussans, D., Dabrowski, M., da Motta, H., Da Silva Peres, L., David, C., David, Q., Davies, G. S., Davini, S., Dawson, J., De, K., De Almeida, R. M., Debbins, P., De Bonis, I., Decowski, M. P., de Gouvea, A., De Holanda, P. C., De Icaza Astiz, I. L., Deisting, A., De Jong, P., Delbart, A., Delepine, D., Delgado, M., Dell-Acqua, A., De Lurgio, P., de Mello Neto, J. R. T., Demuth, D. M., Dennis, S., Densham, C., Deptuch, G., De Roeck, A., De Romeri, V., De Vries, J. J., Dharmapalan, R., Dias, M., Diaz, F., Diaz, J. S., Di Domizio, S., Di Giulio, L., Ding, P., Di Noto, L., Distefano, C., Diurba, R., Diwan, M., Djurcic, Z., Dokania, N., Dolinski, M. J., Domine, L., Douglas, D., Drielsma, F., Duchesneau, D., Duffy, K., Dunne, P., Durkin, T., Duyang, H., Dvornikov, O., Dwyer, D. A., Dyshkant, A. S., Eads, M., Edmunds, D., Eisch, J., Emery, S., Ereditato, A., Escobar, C. O., Escudero Sanchez, L., Evans, J. J., Ewart, E., Ezeribe, A. 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Subjects: Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, Computer Science::Digital Libraries, 01 natural sciences, Physics::Geophysics, Neutrino experiment, 0103 physical sciences, Deep Underground Neutrino Experiment, 010303 astronomy & astrophysics, Engineering (miscellaneous), Supernova, Neutrino, Physics, Time projection chamber, Neutrino, LAr TPC, Accretion (meteorology), 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Galaxy, Supernova, Neutrino detector, Computer Science::Mathematical Software, Liquid argon, High Energy Physics::Experiment, Neutrino
Abstract: This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada;CERN;MŠMT,Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa” and MICINN, Spain; SERI and SNSF, Switzerland; TÜB˙ITAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231., Data Availability Statement This manuscript has no associated data or the data will not be deposited. [Authors’ comment: This manuscript describes sensitivity studies for the DUNE experiment using simulation only, and as such there are no experimental data to report.], The deep underground neutrino experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE’s ability to constrain the νe spectral parameters of the neutrino burst will be considered., Commissariat à l'Énergie Atomique et aux Énergies Alternatives CEA, Fundação de Amparo à Pesquisa do Estado de São Paulo FAPESP, U.S. Department of Energy DE-AC02-05CH11231 USDOE, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro FAPERJ, Ministerstvo Školství, Mládeže a Tělovýchovy MŠMT, Fundação para a Ciência e a Tecnologia FCT, Royal Society, Ministerio de Ciencia e Innovación MICINN, Natural Sciences and Engineering Research Council of Canada NSERC, UK Research and Innovation UKRI, Instituto Nazionale di Fisica Nucleare INFN, Centre National de la Recherche Scientifique CNRS, Conselho Nacional de Desenvolvimento Científico e Tecnológico CNPq, National Research Foundation of Korea NRF, Institut National de Physique Nucléaire et de Physique des Particules IN2P3, H2020-EU, European Commission EC, European Regional Development Fund ERDF, TÜBİTAK, CERN, U.S. Department of Energy USDOE, Fundação de Amparo à Pesquisa do Estado de Goiás FAPEG, Multiple Sclerosis Center of Atlanta MSCA, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung SNF, Singapore Eye Research Institute SERI, Fermi Research Alliance, LLC DE-AC02-07CH11359, National Science Foundation NSF, Science and Technology Facilities Council STFC
Published: 2021
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13. Neutrino interaction classification with a convolutional neural network in the DUNE far detector

Author: R.A. Rameika, J. Perry, M. Kirby, E. Zhivun, K. Zeug, R. LaZur, Marzio Nessi, D. Lorca, R. M. Berner, Sandip Pakvasa, J. J. De Vries, S. Shafaq, Jonas Rademacker, G. P. Zeller, R. Guenette, A. Hourlier, A. McNab, G. Vasseur, C. Petta, C. Grant, A. Olivares Del Campo, Joshua R. Klein, Vasundhara Singh, D. M. DeMuth, A. Chatterjee, P. Debbins, Paola Sala, G. Mandrioli, John G. Learned, S. Kohn, F. Drielsma, Joshua Barrow, John Marshall, Janice L. Thompson, F. Kamiya, E. Motuk, E. Gamberini, B. J. P. Jones, L. Di Giulio, J. Martin-Albo, E. Bechetoille, Gustaaf Brooijmans, K. Moffat, L.S. Rochester, T. L. Usher, R. Staley, Bo Yu, A. V. Waldron, Gabriella Carini, M. Dabrowski, Francesco Gonnella, C. Vilela, B. Zamorano, Warner A. Miller, Wladyslaw Henryk Trzaska, A. M. Gago, R. Diurba, N. Bostan, J. Spitz, M. Pozzato, Y. Cui, P. A. Rodrigues, J. D. Eisch, F. Cavanna, Sofia Vallecorsa, K. E. Duffy, Danny Marfatia, E. Segreto, Xin Qian, T. A. Mohayai, C. J. 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Rout, P. de Jong, B. T. Fleming, R. Poling, J. Hartnell, Robert Shrock, J. Zennamo, A. De Roeck, M. Calin, M. Mellinato, Shu Li, Kristian Harder, J. Hewes, Sandro Palestini, M. Parvu, James A. Anderson, G. S. Davies, I. De Bonis, L. Di Noto, W. E. Sondheim, Nikolina Ilic, C. E. Tull, K. Soustruznik, M. Leyton, J. Hugon, K. V. Tsang, J. Maneira, Abi, B., Acciarri, R., Acero, M. A., Adamov, G., Adams, D., Adinolfi, M., Ahmad, Z., Ahmed, J., Alion, T., Alonso Monsalve, S., Alt, C., Anderson, J., Andreopoulos, C., Andrews, M. P., Andrianala, F., Andringa, S., Ankowski, A., Antonova, M., Antusch, S., Aranda-Fernandez, A., Ariga, A., Arnold, L. O., Arroyave, M. A., Asaadi, J., Aurisano, A., Aushev, V., Autiero, D., Azfar, F., Back, H., Back, J. J., Backhouse, C., Baesso, P., Bagby, L., Bajou, R., Balasubramanian, S., Baldi, P., Bambah, B., Barao, F., Barenboim, G., Barker, G. J., Barkhouse, W., Barnes, C., Barr, G., Barranco Monarca, J., Barros, N., Barrow, J. L., Bashyal, A., Basque, V., Bay, F., Bazo Alba, J. L., Beacom, J. F., Bechetoille, E., Behera, B., Bellantoni, L., Bellettini, G., Bellini, V., Beltramello, O., Belver, D., Benekos, N., Bento Neves, F., Berger, J., Berkman, S., Bernardini, P., Berner, R. M., Berns, H., Bertolucci, S., Betancourt, M., Bezawada, Y., Bhattacharjee, M., Bhuyan, B., Biagi, S., Bian, J., Biassoni, M., Biery, K., Bilki, B., Bishai, M., Bitadze, A., Blake, A., Blanco Siffert, B., Blaszczyk, F. D. M., Blazey, G. C., Blucher, E., Boissevain, J., Bolognesi, S., Bolton, T., Bonesini, M., Bongrand, M., Bonini, F., Booth, A., Booth, C., Bordoni, S., Borkum, A., Boschi, T., Bostan, N., Bour, P., Boyd, S. B., Boyden, D., Bracinik, J., Braga, D., Brailsford, D., Brandt, A., Bremer, J., Brew, C., Brianne, E., Brice, S. 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C., Fahey, K., Falcone, A., Farnese, C., Farzan, Y., Felix, J., Fernandez-Martinez, E., Fernandez Menendez, P., Ferraro, F., Fields, L., Filkins, A., Filthaut, F., Fitzpatrick, R. S., Flanagan, W., Fleming, B., Flight, R., Fowler, J., Fox, W., Franc, J., Francis, K., Franco, D., Freeman, J., Freestone, J., Fried, J., Friedland, A., Fuess, S., Furic, I., Furmanski, A. P., Gago, A., Gallagher, H., Gallego-Ros, A., Gallice, N., Galymov, V., Gamberini, E., Gamble, T., Gandhi, R., Gandrajula, R., Gao, S., Garcia-Carballeira, F., Garcia-Gamez, D., Garcia-Peris, M. A., Gardiner, S., Gastler, D., Ge, G., Gelli, B., Gendotti, A., Gent, S., Ghorbani-Moghaddam, Z., Gibin, D., Gil-Botella, I., Girerd, C., Giri, A. K., Gnani, D., Gogota, O., Gold, M., Gollapinni, S., Gollwitzer, K., Gomes, R. A., Gomez Bermeo, L. V., Gomez Fajardo, L. S., Gonnella, F., Gonzalez-Cuevas, J. A., Goodman, M. C., Goodwin, O., Goswami, S., Gotti, C., Goudzovski, E., Grace, C., Graham, M., Gramellini, E., Gran, R., Granados, E., Grant, A., Grant, C., Gratieri, D., Green, P., Green, S., Greenler, L., Greenwood, M., Greer, J., Griffith, W. C., Groh, M., Grudzinski, J., Grzelak, K., Gu, W., Guarino, V., Guenette, R., Guglielmi, A., Guo, B., Guthikonda, K. K., Gutierrez, R., Guzowski, P., Guzzo, M. M., Gwon, S., Habig, A., Hackenburg, A., Hadavand, H., Haenni, R., Hahn, A., Haigh, J., Haiston, J., Hamernik, T., Hamilton, P., Han, J., Harder, K., Harris, D. A., Hartnell, J., Hasegawa, T., Hatcher, R., Hazen, E., Heavey, A., Heeger, K. M., Heise, J., Hennessy, K., Henry, S., Hernandez Morquecho, M. A., Herner, K., Hertel, L., Hesam, A. S., Hewes, J., Higuera, A., Hill, T., Hillier, S. J., Himmel, A., Hoff, J., Hohl, C., Holin, A., Hoppe, E., Horton-Smith, G. A., Hostert, M., Hourlier, A., Howard, B., Howell, R., Huang, J., Hugon, J., Iles, G., Ilic, N., Iliescu, A. M., Illingworth, R., Ioannisian, A., Itay, R., Izmaylov, A., James, E., Jargowsky, B., Jediny, F., Jesus-Valls, C., Ji, X., Jiang, L., Jimenez, S., Jipa, A., Joglekar, A., Johnson, C., Johnson, R., Jones, B., Jones, S., Jung, C. K., Junk, T., Jwa, Y., Kabirnezhad, M., Kaboth, A., Kadenko, I., Kamiya, F., Karagiorgi, G., Karcher, A., Karolak, M., Karyotakis, Y., Kasai, S., Kasetti, S. P., Kashur, L., Kazaryan, N., Kearns, E., Keener, P., Kelly, K. J., Kemp, E., Ketchum, W., Kettell, S. H., Khabibullin, M., Khotjantsev, A., Khvedelidze, A., Kim, D., King, B., Kirby, B., Kirby, M., Klein, J., Koehler, K., Koerner, L. W., Kohn, S., Koller, P. P., Kordosky, M., Kosc, T., Kose, U., Kostelecky, V. A., Kothekar, K., Krennrich, F., Kreslo, I., Kudenko, Y., Kudryavtsev, V. A., Kulagin, S., Kumar, J., Kumar, R., Kuruppu, C., Kus, V., Kutter, T., Lambert, A., Lande, K., Lane, C. 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A., Martynenko, S., Mason, K., Mastbaum, A., Masud, M., Matsuno, S., Matthews, J., Mauger, C., Mauri, N., Mavrokoridis, K., Mazza, R., Mazzacane, A., Mazzucato, E., Mccluskey, E., Mcconkey, N., Mcfarland, K. S., Mcgrew, C., Mcnab, A., Mefodiev, A., Mehta, P., Melas, P., Mellinato, M., Mena, O., Menary, S., Mendez, H., Menegolli, A., Meng, G., Messier, M. D., Metcalf, W., Mewes, M., Meyer, H., Miao, T., Michna, G., Miedema, T., Migenda, J., Milincic, R., Miller, W., Mills, J., Milne, C., Mineev, O., Miranda, O. G., Miryala, S., Mishra, C. S., Mishra, S. R., Mislivec, A., Mladenov, D., Mocioiu, I., Moffat, K., Moggi, N., Mohanta, R., Mohayai, T. A., Mokhov, N., Molina, J., Molina Bueno, L., Montanari, A., Montanari, C., Montanari, D., Montano Zetina, L. M., Moon, J., Mooney, M., Moor, A., Moreno, D., Morgan, B., Morris, C., Mossey, C., Motuk, E., Moura, C. A., Mousseau, J., Mu, W., Mualem, L., Mueller, J., Muether, M., Mufson, S., Muheim, F., Muir, A., Mulhearn, M., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nagu, S., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navas-Nicolas, D., Nayak, N., Nebot-Guinot, M., Necib, L., Negishi, K., Nelson, J. K., Nesbit, J., Nessi, M., Newbold, D., Newcomer, M., Newhart, D., Nichol, R., Niner, E., Nishimura, K., Norman, A., Norrick, A., Northrop, R., Novella, P., Nowak, J. A., Oberling, M., Olivares Del Campo, A., Olivier, A., Onel, Y., Onishchuk, Y., Ott, J., Pagani, L., Pakvasa, S., Palamara, O., Palestini, S., Paley, J. M., Pallavicini, M., Palomares, C., Pantic, E., Paolone, V., Papadimitriou, V., Papaleo, R., Papanestis, A., Paramesvaran, S., Parke, S., Parsa, Z., Parvu, M., Pascoli, S., Pasqualini, L., Pasternak, J., Pater, J., Patrick, C., Patrizii, L., Patterson, R. B., Patton, S. J., Patzak, T., Paudel, A., Paulos, B., Paulucci, L., Pavlovic, Z., Pawloski, G., Payne, D., Pec, V., Peeters, S. J. M., Penichot, Y., Pennacchio, E., Penzo, A., Peres, O. L. G., Perry, J., Pershey, D., Pessina, G., Petrillo, G., Petta, C., Petti, R., Piastra, F., Pickering, L., Pietropaolo, F., Pillow, J., Pinzino, J., Plunkett, R., Poling, R., Pons, X., Poonthottathil, N., Pordes, S., Potekhin, M., Potenza, R., Potukuchi, B. V. K. S., Pozimski, J., Pozzato, M., Prakash, S., Prakash, T., Prince, S., Prior, G., Pugnere, D., Qi, K., Qian, X., Raaf, J. L., Raboanary, R., Radeka, V., Rademacker, J., Radics, B., Radovic, A., Rafique, A., Raguzin, E., Rai, M., Rajaoalisoa, M., Rakhno, I., Rakotondramanana, H. T., Rakotondravohitra, L., Ramachers, Y. A., Rameika, R., Ramirez Delgado, M. A., Ramson, B., Rappoldi, A., Raselli, G., Ratoff, P., Ravat, S., Razafinime, H., Real, J. S., Rebel, B., Redondo, D., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, S. D., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Rigaut, Y., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Rodriguez Alonso, M. J., Rodriguez Rondon, J., Roeth, A. J., Rogers, H., Rosauro-Alcaraz, S., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Russell, B., Russell, J., Ruterbories, D., Saakyan, R., Sacerdoti, S., Safford, T., Sahu, N., Sala, P., Samios, N., Sanchez, M. C., Sanders, D. A., Sankey, D., Santana, S., Santos-Maldonado, M., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Savinov, V., Scaramelli, A., Scarff, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schmitz, D., Scholberg, K., Schukraft, A., Segreto, E., Sensenig, J., Seong, I., Sergi, A., Sergiampietri, F., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shamma, M., Sharma, H. R., Sharma, R., Shaw, T., Shepherd-Themistocleous, C., Shin, S., Shooltz, D., Shrock, R., Simard, L., Simos, N., Sinclair, J., Sinev, G., Singh, J., Singh, V., Sipos, R., Sippach, F. W., Sirri, G., Sitraka, A., Siyeon, K., Smargianaki, D., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snopok, P., Soares Nunes, M., Sobel, H., Soderberg, M., Solano Salinas, C. J., Soldner-Rembold, S., Solomey, N., Solovov, V., Sondheim, W. E., Sorel, M., Soto-Oton, J., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Spurgeon, K., Staley, R., Stancari, M., Stanco, L., Steiner, H. M., Stewart, J., Stillwell, B., Stock, J., Stocker, F., Stokes, T., Strait, M., Strauss, T., Striganov, S., Stuart, A., Summers, D., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Talaga, R., Tanaka, H. A., Tapia Oregui, B., Tapper, A., Tariq, S., Tatar, E., Tayloe, R., Teklu, A. M., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, J. L., Thorn, C., Timm, S. C., Tonazzo, A., Torti, M., Tortola, M., Tortorici, F., Totani, D., Toups, M., Touramanis, C., Trevor, J., Trzaska, W. H., Tsai, Y. T., Tsamalaidze, Z., Tsang, K. V., Tsverava, N., Tufanli, S., Tull, C., Tyley, E., Tzanov, M., Uchida, M. A., Urheim, J., Usher, T., Vagins, M. R., Vahle, P., Valdiviesso, G. A., Valencia, E., Vallari, Z., Valle, J. W. F., Vallecorsa, S., Van Berg, R., Van De Water, R. G., Vanegas Forero, D., Varanini, F., Vargas, D., Varner, G., Vasel, J., Vasseur, G., Vaziri, K., Ventura, S., Verdugo, A., Vergani, S., Vermeulen, M. A., Verzocchi, M., Vieira De Souza, H., Vignoli, C., Vilela, C., Viren, B., Vrba, T., Wachala, T., Waldron, A. V., Wallbank, M., Wang, H., Wang, J., Wang, Y., Warburton, K., Warner, D., Wascko, M., Waters, D., Watson, A., Weatherly, P., Weber, A., Weber, M., Wei, H., Weinstein, A., Wenman, D., Wetstein, M., While, M. R., White, A., Whitehead, L. H., Whittington, D., Wilking, M. J., Wilkinson, C., Williams, Z., Wilson, F., Wilson, R. J., Wolcott, J., Wongjirad, T., Wood, K., Wood, L., Worcester, E., Worcester, M., Wret, C., Wu, W., Xiao, Y., Yang, G., Yang, T., Yershov, N., Yonehara, K., Young, T., Yu, B., Yu, J., Zaki, R., Zalesak, J., Zambelli, L., Zamorano, B., Zani, A., Zazueta, L., Zeller, G. P., Zennamo, J., Zeug, K., Zhang, C., Zhao, M., Zhivun, E., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., Zwaska, R., Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), DUNE, XENON (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), Abi, B, Acciarri, R, Acero, M, Adamov, G, Adams, D, Adinolfi, M, Ahmad, Z, Ahmed, J, Alion, T, Alonso Monsalve, S, Alt, C, Anderson, J, Andreopoulos, C, Andrews, M, Andrianala, F, Andringa, S, Ankowski, A, Antonova, M, Antusch, S, Aranda-Fernandez, A, Ariga, A, Arnold, L, Arroyave, M, Asaadi, J, Aurisano, A, Aushev, V, Autiero, D, Azfar, F, Back, H, Back, J, Backhouse, C, Baesso, P, Bagby, L, Bajou, R, Balasubramanian, S, Baldi, P, Bambah, B, Barao, F, Barenboim, G, Barker, G, Barkhouse, W, Barnes, C, Barr, G, Barranco Monarca, J, Barros, N, Barrow, J, Bashyal, A, Basque, V, Bay, F, Bazo Alba, J, Beacom, J, Bechetoille, E, Behera, B, Bellantoni, L, Bellettini, G, Bellini, V, Beltramello, O, Belver, D, Benekos, N, Bento Neves, F, Berger, J, Berkman, S, Bernardini, P, Berner, R, Berns, H, Bertolucci, S, Betancourt, M, Bezawada, Y, Bhattacharjee, M, Bhuyan, B, Biagi, S, Bian, J, Biassoni, M, Biery, K, Bilki, B, Bishai, M, Bitadze, A, Blake, A, Blanco Siffert, B, Blaszczyk, F, Blazey, G, Blucher, E, Boissevain, J, Bolognesi, S, Bolton, T, Bonesini, M, Bongrand, M, Bonini, F, Booth, A, Booth, C, Bordoni, S, Borkum, A, Boschi, T, Bostan, N, Bour, P, Boyd, S, Boyden, D, Bracinik, J, Braga, D, Brailsford, D, Brandt, A, Bremer, J, Brew, C, Brianne, E, Brice, S, Brizzolari, C, Bromberg, C, Brooijmans, G, Brooke, J, Bross, A, Brunetti, G, Buchanan, N, Budd, H, Caiulo, D, Calafiura, P, Calcutt, J, Calin, M, Calvez, S, Calvo, E, Camilleri, L, Caminata, A, Campanelli, M, Caratelli, D, Carini, G, Carlus, B, Carniti, P, Caro Terrazas, I, Carranza, H, Castillo, A, Castromonte, C, Cattadori, C, Cavalier, F, Cavanna, F, Centro, S, Cerati, G, Cervelli, A, Cervera Villanueva, A, Chalifour, M, Chang, C, Chardonnet, E, Chatterjee, A, Chattopadhyay, S, Chaves, J, Chen, H, Chen, M, Chen, Y, Cherdack, D, Chi, C, Childress, S, Chiriacescu, A, Cho, K, Choubey, S, Christensen, A, Christian, D, Christodoulou, G, Church, E, Clarke, P, Coan, T, Cocco, A, Coelho, J, Conley, E, Conrad, J, Convery, M, Corwin, L, Cotte, P, Cremaldi, L, Cremonesi, L, Crespo-Anadon, J, Cristaldo, E, Cross, R, Cuesta, C, Cui, Y, Cussans, D, Dabrowski, M, Da Motta, H, Da Silva Peres, L, David, C, David, Q, Davies, G, Davini, S, Dawson, J, De, K, De Almeida, R, Debbins, P, De Bonis, I, Decowski, M, De Gouvea, A, De Holanda, P, De Icaza Astiz, I, Deisting, A, De Jong, P, Delbart, A, Delepine, D, Delgado, M, Dell'Acqua, A, De Lurgio, P, De Mello Neto, J, Demuth, D, Dennis, S, Densham, C, Deptuch, G, De Roeck, A, De Romeri, V, De Vries, J, Dharmapalan, R, Dias, M, Diaz, F, Diaz, J, Di Domizio, S, Di Giulio, L, Ding, P, Di Noto, L, Distefano, C, Diurba, R, Diwan, M, Djurcic, Z, Dokania, N, Dolinski, M, Domine, L, Douglas, D, Drielsma, F, Duchesneau, D, Duffy, K, Dunne, P, Durkin, T, Duyang, H, Dvornikov, O, Dwyer, D, Dyshkant, A, Eads, M, Edmunds, D, Eisch, J, Emery, S, Ereditato, A, Escobar, C, Escudero Sanchez, L, Evans, J, Ewart, E, Ezeribe, A, Fahey, K, Falcone, A, Farnese, C, Farzan, Y, Felix, J, Fernandez-Martinez, E, Fernandez Menendez, P, Ferraro, F, Fields, L, Filkins, A, Filthaut, F, Fitzpatrick, R, Flanagan, W, Fleming, B, Flight, R, Fowler, J, Fox, W, Franc, J, Francis, K, Franco, D, Freeman, J, Freestone, J, Fried, J, Friedland, A, Fuess, S, Furic, I, Furmanski, A, Gago, A, Gallagher, H, Gallego-Ros, A, Gallice, N, Galymov, V, Gamberini, E, Gamble, T, Gandhi, R, Gandrajula, R, Gao, S, Garcia-Carballeira, F, Garcia-Gamez, D, Garcia-Peris, M, Gardiner, S, Gastler, D, Ge, G, Gelli, B, Gendotti, A, Gent, S, Ghorbani-Moghaddam, Z, Gibin, D, Gil-Botella, I, Girerd, C, Giri, A, Gnani, D, Gogota, O, Gold, M, Gollapinni, S, Gollwitzer, K, Gomes, R, Gomez Bermeo, L, Gomez Fajardo, L, Gonnella, F, Gonzalez-Cuevas, J, Goodman, M, Goodwin, O, Goswami, S, Gotti, C, Goudzovski, E, Grace, C, Graham, M, Gramellini, E, Gran, R, Granados, E, Grant, A, Grant, C, Gratieri, D, Green, P, Green, S, Greenler, L, Greenwood, M, Greer, J, Griffith, W, Groh, M, Grudzinski, J, Grzelak, K, Gu, W, Guarino, V, Guenette, R, Guglielmi, A, Guo, B, Guthikonda, K, Gutierrez, R, Guzowski, P, Guzzo, M, Gwon, S, Habig, A, Hackenburg, A, Hadavand, H, Haenni, R, Hahn, A, Haigh, J, Haiston, J, Hamernik, T, Hamilton, P, Han, J, Harder, K, Harris, D, Hartnell, J, Hasegawa, T, Hatcher, R, Hazen, E, Heavey, A, Heeger, K, Heise, J, Hennessy, K, Henry, S, Hernandez Morquecho, M, Herner, K, Hertel, L, Hesam, A, Hewes, J, Higuera, A, Hill, T, Hillier, S, Himmel, A, Hoff, J, Hohl, C, Holin, A, Hoppe, E, Horton-Smith, G, Hostert, M, Hourlier, A, Howard, B, Howell, R, Huang, J, Hugon, J, Iles, G, Ilic, N, Iliescu, A, Illingworth, R, Ioannisian, A, Itay, R, Izmaylov, A, James, E, Jargowsky, B, Jediny, F, Jesus-Valls, C, Ji, X, Jiang, L, Jimenez, S, Jipa, A, Joglekar, A, Johnson, C, Johnson, R, Jones, B, Jones, S, Jung, C, Junk, T, Jwa, Y, Kabirnezhad, M, Kaboth, A, Kadenko, I, Kamiya, F, Karagiorgi, G, Karcher, A, Karolak, M, Karyotakis, Y, Kasai, S, Kasetti, S, Kashur, L, Kazaryan, N, Kearns, E, Keener, P, Kelly, K, Kemp, E, Ketchum, W, Kettell, S, Khabibullin, M, Khotjantsev, A, Khvedelidze, A, Kim, D, King, B, Kirby, B, Kirby, M, Klein, J, Koehler, K, Koerner, L, Kohn, S, Koller, P, Kordosky, M, Kosc, T, Kose, U, Kostelecky, V, Kothekar, K, Krennrich, F, Kreslo, I, Kudenko, Y, Kudryavtsev, V, Kulagin, S, Kumar, J, Kumar, R, Kuruppu, C, Kus, V, Kutter, T, Lambert, A, Lande, K, Lane, C, Lang, K, Langford, T, Lasorak, P, Last, D, Lastoria, C, Laundrie, A, Lawrence, A, Lazanu, I, Lazur, R, Le, T, Learned, J, Lebrun, P, Lehmann Miotto, G, Lehnert, R, Leigui De Oliveira, M, Leitner, M, Leyton, M, Li, L, Li, S, Li, T, Li, Y, Liao, H, Lin, C, Lin, S, Lister, A, Littlejohn, B, Liu, J, Lockwitz, S, Loew, T, Lokajicek, M, Lomidze, I, Long, K, Loo, K, Lorca, D, Lord, T, Losecco, J, Louis, W, Luk, K, Luo, X, Lurkin, N, Lux, T, Luzio, V, Macfarland, D, Machado, A, Machado, P, Macias, C, Macier, J, Maddalena, A, Madigan, P, Magill, S, Mahn, K, Maio, A, Maloney, J, Mandrioli, G, Maneira, J, Manenti, L, Manly, S, Mann, A, Manolopoulos, K, Manrique Plata, M, Marchionni, A, Marciano, W, Marfatia, D, Mariani, C, Maricic, J, Marinho, F, Marino, A, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, N, Martinez Caicedo, D, Martynenko, S, Mason, K, Mastbaum, A, Masud, M, Matsuno, S, Matthews, J, Mauger, C, Mauri, N, Mavrokoridis, K, Mazza, R, Mazzacane, A, Mazzucato, E, Mccluskey, E, Mcconkey, N, Mcfarland, K, Mcgrew, C, Mcnab, A, Mefodiev, A, Mehta, P, Melas, P, Mellinato, M, Mena, O, Menary, S, Mendez, H, Menegolli, A, Meng, G, Messier, M, Metcalf, W, Mewes, M, Meyer, H, Miao, T, Michna, G, Miedema, T, Migenda, J, Milincic, R, Miller, W, Mills, J, Milne, C, Mineev, O, Miranda, O, Miryala, S, Mishra, C, Mishra, S, Mislivec, A, Mladenov, D, Mocioiu, I, Moffat, K, Moggi, N, Mohanta, R, Mohayai, T, Mokhov, N, Molina, J, Molina Bueno, L, Montanari, A, Montanari, C, Montanari, D, Montano Zetina, L, Moon, J, Mooney, M, Moor, A, Moreno, D, Morgan, B, Morris, C, Mossey, C, Motuk, E, Moura, C, Mousseau, J, Mu, W, Mualem, L, Mueller, J, Muether, M, Mufson, S, Muheim, F, Muir, A, Mulhearn, M, Muramatsu, H, Murphy, S, Musser, J, Nachtman, J, Nagu, S, Nalbandyan, M, Nandakumar, R, Naples, D, Narita, S, Navas-Nicolas, D, Nayak, N, Nebot-Guinot, M, Necib, L, Negishi, K, Nelson, J, Nesbit, J, Nessi, M, Newbold, D, Newcomer, M, Newhart, D, Nichol, R, Niner, E, Nishimura, K, Norman, A, Norrick, A, Northrop, R, Novella, P, Nowak, J, Oberling, M, Olivares Del Campo, A, Olivier, A, Onel, Y, Onishchuk, Y, Ott, J, Pagani, L, Pakvasa, S, Palamara, O, Palestini, S, Paley, J, Pallavicini, M, Palomares, C, Pantic, E, Paolone, V, Papadimitriou, V, Papaleo, R, Papanestis, A, Paramesvaran, S, Parke, S, Parsa, Z, Parvu, M, Pascoli, S, Pasqualini, L, Pasternak, J, Pater, J, Patrick, C, Patrizii, L, Patterson, R, Patton, S, Patzak, T, Paudel, A, Paulos, B, Paulucci, L, Pavlovic, Z, Pawloski, G, Payne, D, Pec, V, Peeters, S, Penichot, Y, Pennacchio, E, Penzo, A, Peres, O, Perry, J, Pershey, D, Pessina, G, Petrillo, G, Petta, C, Petti, R, Piastra, F, Pickering, L, Pietropaolo, F, Pillow, J, Pinzino, J, Plunkett, R, Poling, R, Pons, X, Poonthottathil, N, Pordes, S, 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Sarasty, C, Sarcevic, I, Savage, G, Savinov, V, Scaramelli, A, Scarff, A, Scarpelli, A, Schaffer, T, Schellman, H, Schlabach, P, Schmitz, D, Scholberg, K, Schukraft, A, Segreto, E, Sensenig, J, Seong, I, Sergi, A, Sergiampietri, F, Sgalaberna, D, Shaevitz, M, Shafaq, S, Shamma, M, Sharma, H, Sharma, R, Shaw, T, Shepherd-Themistocleous, C, Shin, S, Shooltz, D, Shrock, R, Simard, L, Simos, N, Sinclair, J, Sinev, G, Singh, J, Singh, V, Sipos, R, Sippach, F, Sirri, G, Sitraka, A, Siyeon, K, Smargianaki, D, Smith, A, Smith, E, Smith, P, Smolik, J, Smy, M, Snopok, P, Soares Nunes, M, Sobel, H, Soderberg, M, Solano Salinas, C, Soldner-Rembold, S, Solomey, N, Solovov, V, Sondheim, W, Sorel, M, Soto-Oton, J, Sousa, A, Soustruznik, K, Spagliardi, F, Spanu, M, Spitz, J, Spooner, N, Spurgeon, K, Staley, R, Stancari, M, Stanco, L, Steiner, H, Stewart, J, Stillwell, B, Stock, J, Stocker, F, Stokes, T, Strait, M, Strauss, T, Striganov, S, Stuart, A, Summers, D, Surdo, A, Susic, V, Suter, L, Sutera, C, Svoboda, R, Szczerbinska, B, Szelc, A, Talaga, R, Tanaka, H, Tapia Oregui, B, Tapper, A, Tariq, S, Tatar, E, Tayloe, R, Teklu, A, Tenti, M, Terao, K, Ternes, C, Terranova, F, Testera, G, Thea, A, Thompson, J, Thorn, C, Timm, S, Tonazzo, A, Torti, M, Tortola, M, Tortorici, F, Totani, D, Toups, M, Touramanis, C, Trevor, J, Trzaska, W, Tsai, Y, Tsamalaidze, Z, Tsang, K, Tsverava, N, Tufanli, S, Tull, C, Tyley, E, Tzanov, M, Uchida, M, Urheim, J, Usher, T, Vagins, M, Vahle, P, Valdiviesso, G, Valencia, E, Vallari, Z, Valle, J, Vallecorsa, S, Van Berg, R, Van De Water, R, Vanegas Forero, D, Varanini, F, Vargas, D, Varner, G, Vasel, J, Vasseur, G, Vaziri, K, Ventura, S, Verdugo, A, Vergani, S, Vermeulen, M, Verzocchi, M, Vieira De Souza, H, Vignoli, C, Vilela, C, Viren, B, Vrba, T, Wachala, T, Waldron, A, Wallbank, M, Wang, H, Wang, J, Wang, Y, Warburton, K, Warner, D, Wascko, M, Waters, D, Watson, A, Weatherly, P, Weber, A, Weber, M, Wei, H, Weinstein, A, Wenman, D, Wetstein, M, While, M, White, A, Whitehead, L, Whittington, D, Wilking, M, Wilkinson, C, Williams, Z, Wilson, F, Wilson, R, Wolcott, J, Wongjirad, T, Wood, K, Wood, L, Worcester, E, Worcester, M, Wret, C, Wu, W, Xiao, Y, Yang, G, Yang, T, Yershov, N, Yonehara, K, Young, T, Yu, B, Yu, J, Zaki, R, Zalesak, J, Zambelli, L, Zamorano, B, Zani, A, Zazueta, L, Zeller, G, Zennamo, J, Zeug, K, Zhang, C, Zhao, M, Zhivun, E, Zhu, G, Zimmerman, E, Zito, M, Zucchelli, S, Zuklin, J, Zutshi, V, Zwaska, R, Abi B., Acciarri R., Acero M.A., Adamov G., Adams D., Adinolfi M., Ahmad Z., Ahmed J., Alion T., Alonso Monsalve S., Alt C., Anderson J., Andreopoulos C., Andrews M.P., Andrianala F., Andringa S., Ankowski A., Antonova M., Antusch S., Aranda-Fernandez A., Ariga A., Arnold L.O., Arroyave M.A., Asaadi J., Aurisano A., Aushev V., Autiero D., Azfar F., Back H., Back J.J., Backhouse C., Baesso P., Bagby L., Bajou R., Balasubramanian S., Baldi P., Bambah B., Barao F., Barenboim G., Barker G.J., Barkhouse W., Barnes C., Barr G., Barranco Monarca J., Barros N., Barrow J.L., Bashyal A., Basque V., Bay F., Bazo Alba J.L., Beacom J.F., Bechetoille E., Behera B., Bellantoni L., Bellettini G., Bellini V., Beltramello O., Belver D., Benekos N., Bento Neves F., Berger J., Berkman S., Bernardini P., Berner R.M., Berns H., Bertolucci S., Betancourt M., Bezawada Y., Bhattacharjee M., Bhuyan B., Biagi S., Bian J., Biassoni M., Biery K., Bilki B., Bishai M., Bitadze A., Blake A., Blanco Siffert B., Blaszczyk F.D.M., Blazey G.C., Blucher E., Boissevain J., Bolognesi S., Bolton T., Bonesini M., Bongrand M., Bonini F., Booth A., Booth C., Bordoni S., Borkum A., Boschi T., Bostan N., Bour P., Boyd S.B., Boyden D., Bracinik J., Braga D., Brailsford D., Brandt A., Bremer J., Brew C., Brianne E., Brice S.J., Brizzolari C., Bromberg C., Brooijmans G., Brooke J., Bross A., Brunetti G., Buchanan N., Budd H., Caiulo D., Calafiura P., Calcutt J., Calin M., Calvez S., Calvo E., Camilleri L., Caminata A., Campanelli M., Caratelli D., Carini G., Carlus B., Carniti P., Caro Terrazas I., Carranza H., Castillo A., Castromonte C., Cattadori C., Cavalier F., Cavanna F., Centro S., Cerati G., Cervelli A., Cervera Villanueva A., Chalifour M., Chang C., Chardonnet E., Chatterjee A., Chattopadhyay S., Chaves J., Chen H., Chen M., Chen Y., Cherdack D., Chi C., Childress S., Chiriacescu A., Cho K., Choubey S., Christensen A., Christian D., Christodoulou G., Church E., Clarke P., Coan T.E., Cocco A.G., Coelho J.A.B., Conley E., Conrad J.M., Convery M., Corwin L., Cotte P., Cremaldi L., Cremonesi L., Crespo-Anadon J.I., Cristaldo E., Cross R., Cuesta C., Cui Y., Cussans D., Dabrowski M., Da Motta H., Da Silva Peres L., David C., David Q., Davies G.S., Davini S., Dawson J., De K., De Almeida R.M., Debbins P., De Bonis I., Decowski M.P., De Gouvea A., De Holanda P.C., De Icaza Astiz I.L., Deisting A., De Jong P., Delbart A., Delepine D., Delgado M., Dell'acqua A., De Lurgio P., De Mello Neto J.R.T., Demuth D.M., Dennis S., Densham C., Deptuch G., De Roeck A., De Romeri V., De Vries J.J., Dharmapalan R., Dias M., Diaz F., Diaz J.S., Di Domizio S., Di Giulio L., Ding P., Di Noto L., Distefano C., Diurba R., Diwan M., Djurcic Z., Dokania N., Dolinski M.J., Domine L., Douglas D., Drielsma F., Duchesneau D., Duffy K., Dunne P., Durkin T., Duyang H., Dvornikov O., Dwyer D.A., Dyshkant A.S., Eads M., Edmunds D., Eisch J., Emery S., Ereditato A., Escobar C.O., Escudero Sanchez L., Evans J.J., Ewart E., Ezeribe A.C., Fahey K., Falcone A., Farnese C., Farzan Y., Felix J., Fernandez-Martinez E., Fernandez Menendez P., Ferraro F., Fields L., Filkins A., Filthaut F., Fitzpatrick R.S., Flanagan W., Fleming B., Flight R., Fowler J., Fox W., Franc J., Francis K., Franco D., Freeman J., Freestone J., Fried J., Friedland A., Fuess S., Furic I., Furmanski A.P., Gago A., Gallagher H., Gallego-Ros A., Gallice N., Galymov V., Gamberini E., Gamble T., Gandhi R., Gandrajula R., Gao S., Garcia-Carballeira F., Garcia-Gamez D., Garcia-Peris M.A., Gardiner S., Gastler D., Ge G., Gelli B., Gendotti A., Gent S., Ghorbani-Moghaddam Z., Gibin D., Gil-Botella I., Girerd C., Giri A.K., Gnani D., Gogota O., Gold M., Gollapinni S., Gollwitzer K., Gomes R.A., Gomez Bermeo L.V., Gomez Fajardo L.S., Gonnella F., Gonzalez-Cuevas J.A., Goodman M.C., Goodwin O., Goswami S., Gotti C., Goudzovski E., Grace C., Graham M., Gramellini E., Gran R., Granados E., Grant A., Grant C., Gratieri D., Green P., Green S., Greenler L., Greenwood M., Greer J., Griffith W.C., Groh M., Grudzinski J., Grzelak K., Gu W., Guarino V., Guenette R., Guglielmi A., Guo B., Guthikonda K.K., Gutierrez R., Guzowski P., Guzzo M.M., Gwon S., Habig A., Hackenburg A., Hadavand H., Haenni R., Hahn A., Haigh J., Haiston J., Hamernik T., Hamilton P., Han J., Harder K., Harris D.A., Hartnell J., Hasegawa T., Hatcher R., Hazen E., Heavey A., Heeger K.M., Heise J., Hennessy K., Henry S., Hernandez Morquecho M.A., Herner K., Hertel L., Hesam A.S., Hewes J., Higuera A., Hill T., Hillier S.J., Himmel A., Hoff J., Hohl C., Holin A., Hoppe E., Horton-Smith G.A., Hostert M., Hourlier A., Howard B., Howell R., Huang J., Hugon J., Iles G., Ilic N., Iliescu A.M., Illingworth R., Ioannisian A., Itay R., Izmaylov A., James E., Jargowsky B., Jediny F., Jesus-Valls C., Ji X., Jiang L., Jimenez S., Jipa A., Joglekar A., Johnson C., Johnson R., Jones B., Jones S., Jung C.K., Junk T., Jwa Y., Kabirnezhad M., Kaboth A., Kadenko I., Kamiya F., Karagiorgi G., Karcher A., Karolak M., Karyotakis Y., Kasai S., Kasetti S.P., Kashur L., Kazaryan N., Kearns E., Keener P., Kelly K.J., Kemp E., Ketchum W., Kettell S.H., Khabibullin M., Khotjantsev A., Khvedelidze A., Kim D., King B., Kirby B., Kirby M., Klein J., Koehler K., Koerner L.W., Kohn S., Koller P.P., Kordosky M., Kosc T., Kose U., Kostelecky V.A., Kothekar K., Krennrich F., Kreslo I., Kudenko Y., Kudryavtsev V.A., Kulagin S., Kumar J., Kumar R., Kuruppu C., Kus V., Kutter T., Lambert A., Lande K., Lane C.E., Lang K., Langford T., Lasorak P., Last D., Lastoria C., Laundrie A., Lawrence A., Lazanu I., Lazur R., Le T., Learned J., Lebrun P., Lehmann Miotto G., Lehnert R., Leigui De Oliveira M.A., Leitner M., Leyton M., Li L., Li S., Li S.W., Li T., Li Y., Liao H., Lin C.S., Lin S., Lister A., Littlejohn B.R., Liu J., Lockwitz S., Loew T., Lokajicek M., Lomidze I., Long K., Loo K., Lorca D., Lord T., Losecco J.M., Louis W.C., Luk K.B., Luo X., Lurkin N., Lux T., Luzio V.P., MacFarland D., MacHado A.A., MacHado P., MacIas C.T., MacIer J.R., Maddalena A., Madigan P., Magill S., Mahn K., Maio A., Maloney J.A., Mandrioli G., Maneira J., Manenti L., Manly S., Mann A., Manolopoulos K., Manrique Plata M., Marchionni A., Marciano W., Marfatia D., Mariani C., Maricic J., Marinho F., Marino A.D., Marshak M., Marshall C., Marshall J., Marteau J., Martin-Albo J., Martinez N., Martinez Caicedo D.A., Martynenko S., Mason K., Mastbaum A., Masud M., Matsuno S., Matthews J., Mauger C., Mauri N., Mavrokoridis K., Mazza R., Mazzacane A., Mazzucato E., McCluskey E., McConkey N., McFarland K.S., McGrew C., McNab A., Mefodiev A., Mehta P., Melas P., Mellinato M., Mena O., Menary S., Mendez H., Menegolli A., Meng G., Messier M.D., Metcalf W., Mewes M., Meyer H., Miao T., Michna G., Miedema T., Migenda J., Milincic R., Miller W., Mills J., Milne C., Mineev O., Miranda O.G., Miryala S., Mishra C.S., Mishra S.R., Mislivec A., Mladenov D., Mocioiu I., Moffat K., Moggi N., Mohanta R., Mohayai T.A., Mokhov N., Molina J., Molina Bueno L., Montanari A., Montanari C., Montanari D., Montano Zetina L.M., Moon J., Mooney M., Moor A., Moreno D., Morgan B., Morris C., Mossey C., Motuk E., Moura C.A., Mousseau J., Mu W., Mualem L., Mueller J., Muether M., Mufson S., Muheim F., Muir A., Mulhearn M., Muramatsu H., Murphy S., Musser J., Nachtman J., Nagu S., Nalbandyan M., Nandakumar R., Naples D., Narita S., Navas-Nicolas D., Nayak N., Nebot-Guinot M., Necib L., Negishi K., Nelson J.K., Nesbit J., Nessi M., Newbold D., Newcomer M., Newhart D., Nichol R., Niner E., Nishimura K., Norman A., Norrick A., Northrop R., Novella P., Nowak J.A., Oberling M., Olivares Del Campo A., Olivier A., Onel Y., Onishchuk Y., Ott J., Pagani L., Pakvasa S., Palamara O., Palestini S., Paley J.M., Pallavicini M., Palomares C., Pantic E., Paolone V., Papadimitriou V., Papaleo R., Papanestis A., Paramesvaran S., Parke S., Parsa Z., Parvu M., Pascoli S., Pasqualini L., Pasternak J., Pater J., Patrick C., Patrizii L., Patterson R.B., Patton S.J., Patzak T., Paudel A., Paulos B., Paulucci L., Pavlovic Z., Pawloski G., Payne D., Pec V., Peeters S.J.M., Penichot Y., Pennacchio E., Penzo A., Peres O.L.G., Perry J., Pershey D., Pessina G., Petrillo G., Petta C., Petti R., Piastra F., Pickering L., Pietropaolo F., Pillow J., Pinzino J., Plunkett R., Poling R., Pons X., Poonthottathil N., Pordes S., Potekhin M., Potenza R., Potukuchi B.V.K.S., Pozimski J., Pozzato M., Prakash S., Prakash T., Prince S., Prior G., Pugnere D., Qi K., Qian X., Raaf J.L., Raboanary R., Radeka V., Rademacker J., Radics B., Radovic A., Rafique A., Raguzin E., Rai M., Rajaoalisoa M., Rakhno I., Rakotondramanana H.T., Rakotondravohitra L., Ramachers Y.A., Rameika R., Ramirez Delgado M.A., Ramson B., Rappoldi A., Raselli G., Ratoff P., Ravat S., Razafinime H., Real J.S., Rebel B., Redondo D., Reggiani-Guzzo M., Rehak T., Reichenbacher J., Reitzner S.D., Renshaw A., Rescia S., Resnati F., Reynolds A., Riccobene G., Rice L.C.J., Rielage K., Rigaut Y., Rivera D., Rochester L., Roda M., Rodrigues P., Rodriguez Alonso M.J., Rodriguez Rondon J., Roeth A.J., Rogers H., Rosauro-Alcaraz S., Rossella M., Rout J., Roy S., Rubbia A., Rubbia C., Russell B., Russell J., Ruterbories D., Saakyan R., Sacerdoti S., Safford T., Sahu N., Sala P., Samios N., Sanchez M.C., Sanders D.A., Sankey D., Santana S., Santos-Maldonado M., Saoulidou N., Sapienza P., Sarasty C., Sarcevic I., Savage G., Savinov V., Scaramelli A., Scarff A., Scarpelli A., Schaffer T., Schellman H., Schlabach P., Schmitz D., Scholberg K., Schukraft A., Segreto E., Sensenig J., Seong I., Sergi A., Sergiampietri F., Sgalaberna D., Shaevitz M.H., Shafaq S., Shamma M., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Smargianaki D., Smith A., Smith E., Smith P., Smolik J., Smy M., Snopok P., Soares Nunes M., Sobel H., Soderberg M., Solano Salinas C.J., Soldner-Rembold S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Tapia Oregui B., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Tonazzo A., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Trevor J., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Vallari Z., Valle J.W.F., Vallecorsa S., Van Berg R., Van De Water R.G., Vanegas Forero D., Varanini F., Vargas D., Varner G., Vasel J., Vasseur G., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., Vieira De Souza H., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., Yang T., Yershov N., Yonehara K., Young T., Yu B., Yu J., Zaki R., Zalesak J., Zambelli L., Zamorano B., Zani A., Zazueta L., Zeller G.P., Zennamo J., Zeug K., Zhang C., Zhao M., Zhivun E., Zhu G., Zimmerman E.D., Zito M., Zucchelli S., Zuklin J., Zutshi V., Zwaska R., UAM. Departamento de Física Teórica, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Ministerio de Ciencia, Innovación y Universidades (España)
Subjects: Neutrino Oscillations. Neutrino detectors, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, far detector, 01 natural sciences, Physics, Particles & Fields, High Energy Physics - Experiment, charged current, High Energy Physics - Experiment (hep-ex), [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Particle Physics Experiments, Muon neutrino, neutrino/e: particle identification, Neutrino detectors, Detectors and Experimental Techniques, physics.ins-det, Charged current, neutrino: interaction, Informática, Physics, Telecomunicaciones, Neutrino oscillations, Neutrino interactions, neural network, DUNE, Deep Underground Neutrino Experiment, Instrumentation and Detectors (physics.ins-det), Experiment (hep-ex), Neutrino detector, Physical Sciences, CP violation, Neutrino, Particle Physics - Experiment, Particle physics, data analysis method, 530 Physics, neural network, Astrophysics::High Energy Astrophysical Phenomena, CONSERVATION, FOS: Physical sciences, Astronomy & Astrophysics, Deep Learning, neutrino: deep underground detector, neutrino physics, 0103 physical sciences, Object Detection, CP: violation, Deep Underground Neutrino Experiment, High Energy Physics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinos, 010306 general physics, Neutrino oscillation, neutrino/mu: particle identification, IOU, Science & Technology, DUNE, Neutrino interactions, 010308 nuclear & particles physics, hep-ex, High Energy Physics::Phenomenology, Física, Neutrino Interaction, Detector, 530 Physik, sensitivity, efficiency, High Energy Physics::Experiment, Electron neutrino
Abstract: The Deep Underground Neutrino Experiment is a next-generation neutrino oscillation experiment that aims to measure CP-violation in the neutrino sector as part of a wider physics program. A deep learning approach based on a convolutional neural network has been developed to provide highly efficient and pure selections of electron neutrino and muon neutrino charged-current interactions. The electron neutrino (antineutrino) selection efficiency peaks at 90% (94%) and exceeds 85% (90%) for reconstructed neutrino energies between 2–5 GeV. The muon neutrino (antineutrino) event selection is found to have a maximum efficiency of 96% (97%) and exceeds 90% (95%) efficiency for reconstructed neutrino energies above 2 GeV. When considering all electron neutrino and antineutrino interactions as signal, a selection purity of 90% is achieved. These event selections are critical to maximize the sensitivity of the experiment to CP-violating effects., Fermi Research Alliance, LLC (FRA) DE-AC02-07CH11359, National Council for Scientific and Technological Development (CNPq), Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ), FAPEG, Brazil, Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Canada Foundation for Innovation, Institute of Particle Physics, Canada, Natural Sciences and Engineering Research Council of Canada (NSERC), CERN, Ministry of Education, Youth & Sports - Czech Republic Czech Republic Government, ERDF, European Union, H2020-EU, European Union, MSCA, European Union, Centre National de la Recherche Scientifique (CNRS), French Atomic Energy Commission, Istituto Nazionale di Fisica Nucleare (INFN), Portuguese Foundation for Science and Technology European Commission, NRF, South Korea, Comunidad de Madrid, La Caixa Foundation, Spanish Government, State Secretariat for Education, Research and Innovation, Switzerland, Swiss National Science Foundation (SNSF), Turkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK), Royal Society of London, UKRI/STFC, United Kingdom, United States Department of Energy (DOE), National Science Foundation (NSF)
Published: 2020

14. Target Detection in Underwater Lidar using Machine Learning to Classify Peak Signals

Author: Connor F. Hunt, Jacob T. Young, Jacob A. Brothers, Jonathan O. Hutchins, Luke K. Rumbaugh, and David W. Illig
Subjects: Physics, business.industry, Attenuation, Shot noise, Binary number, Ranging, Machine learning, computer.software_genre, Object detection, Lidar, Frequency domain, Artificial intelligence, Underwater, business, computer, Physics::Atmospheric and Oceanic Physics
Abstract: A machine learning model was used to detect target signals for an underwater lidar system operating in turbid water. For this system, scatter returns from the underwater environment and shot noise can create false alarms with signatures resembling true target peaks. A binary peak classifier model was implemented that classifies each peak in the lidar signal as a target or a non-target. For a gray target positioned at 7 m downrange, ≥97% target detection accuracy was achieved at turbidities of $\mathrm{c}\leq 0.8\ \mathrm{m}^{-1}$ , ranging from clear waters up to simulated open ocean conditions, and ≥85% target accuracy was achieved at simulated harbor-like turbidities of $1.0\ \mathrm{m}^{-1}\leq \mathrm{c}\leq 1.2\ \mathrm{m}^{-1}$ , where c is the attenuation coefficient of the turbid water. This approach can enhance the detection capabilities of a system already using frequency-domain discrimination techniques.
Published: 2020

15. Piecewise Parabolic Phase Modulation Scheme for Suppression of Stimulated Brillouin Scattering

Author: Curtis R. Menyuk, Chengli Wei, Joshua T. Young, Jeffrey O. White, and Jonathan Hu
Subjects: Physics, Optical fiber, 020205 medical informatics, business.industry, Nonlinear optics, 02 engineering and technology, Sawtooth wave, law.invention, Optics, Modulation, law, Brillouin scattering, Scheme (mathematics), 0202 electrical engineering, electronic engineering, information engineering, Piecewise, business, Phase modulation
Abstract: We study piecewise parabolic sawtooth and triangle phase modulation for the suppression of stimulated Brillouin scattering. We compare different modulation schemes and show threshold enhancement using piecewise parabolic phase modulation.
Published: 2020

16. Symmetry Breaking and Error Correction in Open Quantum Systems

Author: Alexey V. Gorshkov, Victor V. Albert, Rex Lundgren, Ron Belyansky, Jeremy T. Young, and Simon Lieu
Subjects: Quantum optics, Physics, Quantum Physics, Phase transition, Photon, Condensed Matter - Mesoscale and Nanoscale Physics, FOS: Physical sciences, General Physics and Astronomy, 01 natural sciences, Symmetry (physics), Quantum Gases (cond-mat.quant-gas), Qubit, Quantum mechanics, Mesoscale and Nanoscale Physics (cond-mat.mes-hall), 0103 physical sciences, Symmetry breaking, Connection (algebraic framework), Quantum Physics (quant-ph), Condensed Matter - Quantum Gases, 010306 general physics, Quantum, Optics (physics.optics), Physics - Optics
Abstract: Symmetry-breaking transitions are a well-understood phenomenon of closed quantum systems in quantum optics, condensed matter, and high energy physics. However, symmetry breaking in open systems is less thoroughly understood, in part due to the richer steady-state and symmetry structure that such systems possess. For the prototypical open system---a Lindbladian---a unitary symmetry can be imposed in a "weak" or a "strong" way. We characterize the possible $\mathbb{Z}_n$ symmetry breaking transitions for both cases. In the case of $\mathbb{Z}_2$, a weak-symmetry-broken phase guarantees at most a classical bit steady-state structure, while a strong-symmetry-broken phase admits a partially-protected steady-state qubit. Viewing photonic cat qubits through the lens of strong-symmetry breaking, we show how to dynamically recover the logical information after any gap-preserving strong-symmetric error; such recovery becomes perfect exponentially quickly in the number of photons. Our study forges a connection between driven-dissipative phase transitions and error correction., 5 + 6 pages
Published: 2020

17. Asymmetric blockade and multi-qubit gates via dipole-dipole interactions

Author: Adam Kaufman, Alexey V. Gorshkov, Przemyslaw Bienias, Jeremy T. Young, and Ron Belyansky
Subjects: Physics, Quantum Physics, Atomic Physics (physics.atom-ph), General Physics and Astronomy, FOS: Physical sciences, 01 natural sciences, 010305 fluids & plasmas, Physics - Atomic Physics, symbols.namesake, Dipole, Computer Science::Emerging Technologies, Quantum mechanics, Qubit, 0103 physical sciences, Rydberg atom, Rydberg formula, symbols, Quantum algorithm, Physics::Atomic Physics, 010306 general physics, Quantum Physics (quant-ph)
Abstract: Due to their strong and tunable interactions, Rydberg atoms can be used to realize fast two-qubit entangling gates. We propose a generalization of a generic two-qubit Rydberg-blockade gate to multi-qubit Rydberg-blockade gates which involve both many control qubits and many target qubits simultaneously. This is achieved by using strong microwave fields to dress nearby Rydberg states, leading to asymmetric blockade in which control-target interactions are much stronger than control-control and target-target interactions. The implementation of these multi-qubit gates can drastically simplify both quantum algorithms and state preparation. To illustrate this, we show that a 25-atom GHZ state can be created using only three gates with an error of 7.8%., 5+4 pages, 3+2 figures
Published: 2020

18. Volume IV The DUNE far detector single-phase technology

Author: L. Di Giulio, J. Martin-Albo, S. Ravat, W. Mu, D. Marfatia, T. Kosc, D. Autiero, Poonam Mehta, A. Borkum, N. McConkey, G. Karagiorgi, Robert Wilson, L. M. Cremaldi, Stephen P. Gent, T. Young, Julián Félix, D. MacFarland, Andrew Smith, M. Manrique Plata, J. Freestone, D. Rivera, B. Stillwell, Marco Verzocchi, A. Lambert, Orlando L. G. Peres, K. Gollwitzer, E. Kemp, G. Yang, I. Kreslo, F. Varanini, M. Chalifour, A. Holin, S. J. Patton, R. J. Nichol, Giovanni Bellettini, V. A. Kudryavtsev, M. Sorel, E. Church, S. Kasai, H. O. Back, A. Lister, S. Santana, C. Mariani, Carlos Escobar, J. C. Freeman, Kaushik De, M. J. Rodriguez Alonso, M. A. Acero, A. Christensen, G. S. Varner, S. Sacerdoti, D. Shooltz, Seodong Shin, M. Santos-Maldonado, T. Schaffer, Jeremy Wolcott, J. Vasel, J. A. Gonzalez-Cuevas, J. Franc, C. Mossey, Jonas Rademacker, G. P. Zeller, Joshua Barrow, John Marshall, Alessandro Thea, H. A. Tanaka, W. C. Louis, E. Hazen, Armin Karcher, D. Smargianaki, Christopher L. Marshall, M. Soderberg, A. C. Weber, Christopher J. Milne, E. Brianne, A. Aranda-Fernandez, J. Calcutt, K. Warburton, M. Nalbandyan, Dave Sankey, J. Asaadi, F. Diaz, E. Valencia, B. Kirby, A. Bross, K. Koehler, M. A. Uchida, Y. Bezawada, D. Warner, C. E. Thorn, Srubabati Goswami, Z. Williams, Gregory Iles, A. Friedland, K. M. Heeger, V. P. Luzio, G. C. Blazey, J. Barranco Monarca, Carl Grace, A. M. Gago, E. James, M. Newcomer, H. W. Sobel, Roberto Gutiérrez, C. Vignoli, R. Hatcher, M. Zhao, F. Cavalier, M. A. Hernandez Morquecho, N. Poonthottathil, Ara Ioannisian, W. Metcalf, T. Wongjirad, H. T. Rakotondramanana, D. Cherdack, M. A. Ramirez Delgado, R. Diurba, G. Christodoulou, S. Calvez, T. Durkin, H. Y. Wei, M. Muether, S. Roy, A. Caminata, A. Scarpelli, Christopher Brew, Pavel Snopok, Y. Rigaut, L. Escudero Sanchez, K. Kothekar, W. Flanagan, V. Papadimitriou, S. J. Brice, Nicolas Lurkin, M. V. Diwan, Andrew White, S. Berkman, H. Muramatsu, Z. Pavlovic, A. A. Machado, Christian Farnese, A. Mastbaum, Alfredo G. Cocco, G. Zhu, S. Centro, S. Henry, J. Rout, P. de Jong, H. Carranza, Milos Lokajicek, K. Nishimura, A. Delbart, N. J. C. Spooner, C. McGrew, E. Pantic, Mario Campanelli, David Cussans, B. T. Fleming, K. Negishi, F. Spagliardi, J. Nesbit, André Rubbia, Akitaka Ariga, Marvin L Marshak, F. Pietropaolo, F. D. M. Blaszczyk, T. Hasegawa, Kate Scholberg, O. Gogota, R. Poling, Simon Jones, A. Tonazzo, M. P. Andrews, R. Petti, S. Bertolucci, M. Bonesini, A. F. Moor, C. Barnes, A. S. Hesam, S. H. Kettell, M. Bongrand, M. R. While, D. J. Payne, C. Gotti, A. Chiriacescu, Paul Keener, Leigh H. Whitehead, James Stewart, A. Mazzacane, L. W. Koerner, T. Rehak, C. Andreopoulos, F. Terranova, Jaroslaw Pasternak, E. Raguzin, L. C. J. Rice, J. L. Bazo Alba, S. Li, J. Hartnell, M. Potekhin, N. Moggi, D. J. Summers, J. Berger, L. Cremonesi, Katsuya Yonehara, T. E. Coan, Claire Shepherd-Themistocleous, B. Radics, Karol Hennessy, S. Söldner-Rembold, C. S. Lin, L. Greenler, B. Guo, Frank Filthaut, R. B. Patterson, E. Pennacchio, E. Zhivun, C. Cuesta, T. Loew, G. Prior, D. Duchesneau, Lina Necib, S. Rescia, W. Gu, Andrés Castillo, N. Kazaryan, O. G. Miranda, C. Patrick, Robert Shrock, José W. F. Valle, J. Reichenbacher, D. A. Sanders, John F. Beacom, S. Tufanli, S. Ventura, Riccardo Papaleo, J. Zennamo, A. De Roeck, M. Calin, P. Ding, Alessandro Menegolli, B. V. K. S. Potukuchi, T. Le, T. Wachala, L. O. Arnold, J. R. Macier, A. M. Teklu, E. Blucher, L. Hertel, F. W. Sippach, S. Childress, T. Miao, P. Fernandez Menendez, J. Han, R. Gandrajula, C. Y. Chi, Marzio Nessi, Aldo Penzo, Ina Sarcevic, Kendall Mahn, Jorge Molina, F. Bonini, Eric W. Hoppe, M. Groh, Barry King, R. Mazza, Keith Rielage, Patrick Dunne, M. Mellinato, D. Lorca, R. Guenette, F. Bento Neves, L. Pickering, Manuel Alejandro Segura Delgado, J. J. Russell, H. R. Gallagher, J. Zuklin, Steven Gardiner, P. Madigan, D. Douglas, Daniel Gastler, S. Manly, P. Hamilton, L. Montaño Zetina, R. G. Van de Water, S. Dennis, M. Tenti, N. Dokania, Kim Siyeon, E. Fernandez-Martinez, P. P. Koller, D. Whittington, T. Li, M. C. Sanchez, S. Biagi, C. Sarasty, Juraj Bracinik, A. N. Khotjantsev, N. Tsverava, Yasaman Farzan, M. Tzanov, J. G. Boissevain, J. Smolik, Andrew Brandt, J. Hoff, D. A. Harris, C. Distefano, Ornella Palamara, H. S. Budd, Alastair Grant, A. K. Giri, Thorsten Lux, C. E. Lane, J. Marteau, Irakli Lomidze, E. Kearns, Zviad Tsamalaidze, L. S. Gomez Fajardo, H. da Motta, J. S. Real, Sukalyan Chattopadhyay, B. Viren, J. Mousseau, Ihn Sik Seong, C. M. Sutera, A. C. Ezeribe, F. Ferraro, Marco Adinolfi, Nikolaos Simos, A. Stuart, D. Brailsford, N. Solomey, Laura Manenti, L. V. Gomez Bermeo, Andrea Zani, Kristian Harder, Timothy M. Shaw, J. Hewes, Sandro Palestini, D. Braga, D. Garcia-Gamez, J. Stock, S. Bolognesi, D. Belver, Laura Paulucci, J. Ahmed, Narendra Sahu, Sandip Pakvasa, L. Pasqualini, D. Mladenov, M. Kordosky, S. Zucchelli, L. Stanco, M. 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Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., Yang T., Yershov N., Yonehara K., Young T., Yu B., Yu J., Zalesak J., Zambelli L., Zamorano B., Zani A., Zazueta L., Zeller G., Zennamo J., Zeug K., Zhang C., Zhao M., Zhivun E., Zhu G., Zimmerman E.D., Zito M., Zucchelli S., Zuklin J., Zutshi V., and Zwaska R.
Subjects: Technology, 530 Physics, media_common.quotation_subject, Neutrino oscillations, liquid Argon TPC, DUNE technical design report, single phase LArTPC, Electrons, FREE-ELECTRONS, 01 natural sciences, 7. Clean energy, 09 Engineering, 030218 nuclear medicine & medical imaging, Standard Model, 03 medical and health sciences, neutrino, 0302 clinical medicine, LIQUID ARGON, 0103 physical sciences, Grand Unified Theory, High Energy Physics, Aerospace engineering, Instrumentation, Instruments & Instrumentation, Mathematical Physics, media_common, Physics, Science & Technology, 02 Physical Sciences, 010308 nuclear & particles physics, business.industry, Detector, Lıquıd Argonfree, Nuclear & Particles Physics, Symmetry (physics), Universe, Long baseline neutrino experiment, CP violation, Antimatter, Neutrino, business, Event (particle physics)
Abstract: This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. The DUNE collaboration also acknowledges the international, national, and regional funding agencies supporting the institutions who have contributed to completing this Technical Design Report., The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay—these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. DUNE is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. Central to achieving DUNE's physics program is a far detector that combines the many tens-of-kiloton fiducial mass necessary for rare event searches with sub-centimeter spatial resolution in its ability to image those events, allowing identification of the physics signatures among the numerous backgrounds. In the single-phase liquid argon time-projection chamber (LArTPC) technology, ionization charges drift horizontally in the liquid argon under the influence of an electric field towards a vertical anode, where they are read out with fine granularity. A photon detection system supplements the TPC, directly enhancing physics capabilities for all three DUNE physics drivers and opening up prospects for further physics explorations. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. Volume IV presents an overview of the basic operating principles of a single-phase LArTPC, followed by a description of the DUNE implementation. Each of the subsystems is described in detail, connecting the high-level design requirements and decisions to the overriding physics goals of DUNE., Fermi Research Alliance, LLC (FRA) DE-AC02-07CH11359
Published: 2020

19. Quench Dynamics of a Fermi Gas with Strong Non-Local Interactions

Author: Elmer Guardado-Sanchez, Waseem Bakr, Ron Belyansky, Alexey V. Gorshkov, Benjamin M. Spar, Przemyslaw Bienias, Jeremy T. Young, Thomas Iadecola, and Peter Schauss
Subjects: Physics, Optical lattice, Condensed matter physics, Atomic Physics (physics.atom-ph), QC1-999, General Physics and Astronomy, Charge density, FOS: Physical sciences, 01 natural sciences, Square lattice, 3. Good health, 010305 fluids & plasmas, Physics - Atomic Physics, symbols.namesake, Ramsey interferometry, Quantum Gases (cond-mat.quant-gas), 0103 physical sciences, Rydberg formula, symbols, Relaxation (physics), 010306 general physics, Fermi gas, Condensed Matter - Quantum Gases, Quantum tunnelling
Abstract: We induce strong non-local interactions in a 2D Fermi gas in an optical lattice using Rydberg dressing. The system is approximately described by a $t-V$ model on a square lattice where the fermions experience isotropic nearest-neighbor interactions and are free to hop only along one direction. We measure the interactions using many-body Ramsey interferometry and study the lifetime of the gas in the presence of tunneling, finding that tunneling does not reduce the lifetime. To probe the interplay of non-local interactions with tunneling, we investigate the short-time relaxation dynamics of charge density waves in the gas. We find that strong nearest-neighbor interactions slow down the relaxation. Our work opens the door for quantum simulations of systems with strong non-local interactions such as extended Fermi-Hubbard models., Comment: 12 pages, 6 figures in main text, 3 figures in appendix
Published: 2020
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20. First results on ProtoDUNE-SP liquid argon time projection chamber performance from a beam test at the CERN Neutrino Platform

Author: Francesco Tortorici, Andrea Zani, J. Moon, P. E. L. Clarke, C. Palomares, M. B. Smy, M. Oberling, J. Migenda, F. Pietropaolo, T. Hasegawa, A. de Gouvea, N.V. Mokhov, S. Rescia, Andrés Castillo, F. Marinho, Mario Campanelli, Jürgen Pozimski, R. Raboanary, F. Sergiampietri, D. A. Sanders, John F. Beacom, Steven Gardiner, P. Madigan, R. Sulej, M. V. Diwan, D. J. Payne, L. Pickering, S. Manly, P. Hamilton, R. G. Van de Water, Chao Zhang, J. Wang, J. Hoff, Burak Bilki, Rex Tayloe, M. A. Uchida, A. Stuart, O. Dvornikov, P. De Lurgio, C. A. Ternes, J. A. Nowak, R. Bajou, P. Schlabach, E. Seltskaya, C. Lastoria, D. Naples, Kazuhiro Terao, A. Paudel, E. T. Worcester, C. Gotti, Michael Mulhearn, S. B. Boyd, T. Hill, D. Douglas, Daniel Gastler, G. A. Valdiviesso, S. Emery, M. C. Goodman, D. C. Christian, M. Newcomer, H. W. Sobel, N. Poonthottathil, Mingshui Chen, J. Urheim, B. Viren, D. Montanari, Giorgio Riccobene, I. Rakhno, M. A. Ramirez Delgado, J. Mousseau, Ara Ioannisian, H. T. Rakotondramanana, L. Molina Bueno, A. Rappoldi, Matthaeus Leitner, K. Fahey, S. J. Brice, M. E. Convery, Nicolas Lurkin, Bindu A. Bambah, S. Ravat, W. Mu, M. A. Arroyave, A. A. Machado, R. Petti, Rukmani Mohanta, Andrew Norman, V. N. Solovov, X. Pons, J. Marteau, Irakli Lomidze, Zviad Tsamalaidze, H. da Motta, M. Mellinato, M. Karolak, D. Autiero, Poonam Mehta, G. Karagiorgi, Sudarshan Paramesvaran, S. Davini, R. L. Talaga, V. Paolone, V. Pec, J. Pillow, S. Vergani, Simon Lin, K. Wood, Jaroslaw Pasternak, G. C. Blazey, Katsuya Yonehara, T. E. Coan, B. Radics, W. Gu, A. M. Teklu, E. Blucher, S. Childress, S. Matsuno, Christian Farnese, Akitaka Ariga, Marvin L Marshak, A. Chiriacescu, F. Terranova, E. Raguzin, L. C. J. Rice, L. Domine, M. Pozzato, T. Miao, L. Da Silva Peres, D. Mladenov, T. Durkin, H. Y. Wei, L. Escudero Sanchez, T. Usher, A. Rafique, A. Verdugo, B. Stillwell, A. Lambert, K. Negishi, A. Falcone, A. Holin, J. L. Bazo Alba, J. Rout, E. D. Zimmerman, M. A. Leigui de Oliveira, A. Olivier, J. Nesbit, Aldo Penzo, Kate Scholberg, Giovanni Bellettini, S. Kasai, O. Gogota, B. Ramson, P. de Jong, R. Zaki, A. Tonazzo, H. Schellman, E. Kemp, T. Rehak, I. De Bonis, Pedro A. N. Machado, B. T. Fleming, M. P. Andrews, M. Bishai, T. Alion, N. Martinez, L. Greenler, Deywis Moreno, T. Loew, H. Berns, P. Ding, M. J. Dolinski, R. J. Nichol, B. Guo, Frank Filthaut, Stefan Antusch, Nikolaos Charitonidis, Patrick Green, R. Howell, Z. Parsa, M. Sorel, J. C. Freeman, J. A. Musser, D. Gratieri, J. Reichenbacher, S. Ventura, Kaushik De, M. J. Rodriguez Alonso, Patrick Dunne, A. Scaramelli, M. Tenti, J. R. T. de Mello Neto, Raj Gandhi, Riccardo Papaleo, M. C. Sanchez, V. Zutshi, Sandeep Miryala, Enrique Calvo, N. Tsverava, V. Radeka, C. Touramanis, J. M. Paley, Antonio Ereditato, J. S. Díaz, Marco Pallavicini, D. MacFarland, G. Savage, J. Soto-Oton, P. Fernandez Menendez, J. Han, C. Y. Chi, M. Groh, N. Yershov, M. Chalifour, E. Hazen, M. A. Acero, C. Mossey, L. M. Montano Zetina, W. C. Louis, S. Di Domizio, F. Bento Neves, A. Gendotti, A. Himmel, M. Masud, M. Rajaoalisoa, P. Bour, G. Pessina, P. Novella, Armin Karcher, D. Smargianaki, Christopher L. Marshall, M. Gold, C. Vignoli, L. Mualem, A. Sousa, K. Kothekar, A. Surdo, J. Martín-Albo, Z. Ghorbani-Moghaddam, K. Spurgeon, E. Niner, M. Spanu, Xiaolu Ji, E. Fernandez-Martinez, W. Flanagan, Jonas Rademacker, G. P. Zeller, Joshua Barrow, John Marshall, A. M. Szelc, J. J. Russell, M. J. Wilking, V. Papadimitriou, Gareth J. Barker, A. M. Gago, R. Diurba, G. Christodoulou, S. Calvez, Jeremy Wolcott, R. S. Fitzpatrick, D. Redondo, S. R. Mishra, Gregory Iles, Andrew Brandt, S. Bordoni, James Mueller, G. Zhu, S. Centro, S. Henry, L. Rakotondravohitra, K. Grzelak, Paul Keener, Leigh H. Whitehead, Matthew Mewes, Kai Loo, Karol Hennessy, S. Söldner-Rembold, C. S. Lin, J. Trevor, N. Kazaryan, Kendall Mahn, Jorge Molina, J. Fowler, Dave Sankey, Luca Stanco, W. Fox, K. M. Heeger, R. Poling, S. J. M. 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A., Martynenko, S., Mason, K., Mastbaum, A., Masud, M., Matsuno, S., Matthews, J., Mauger, C., Mauri, N., Mavrokoridis, K., Mazza, R., Mazzacane, A., Mazzucato, E., Mccluskey, E., Mcconkey, N., Mcfarland, K. S., Mcgrew, C., Mcnab, A., Mefodiev, A., Mehta, P., Melas, P., Mellinato, M., Mena, O., Menary, S., Mendez, H., Menegolli, A., Meng, G., Messier, M. D., Metcalf, W., Mewes, M., Meyer, H., Miao, T., Michna, G., Miedema, T., Migenda, J., Milincic, R., Miller, W., Mills, J., Milne, C., Mineev, O., Miranda, O. G., Miryala, S., Mishra, C. S., Mishra, S. R., Mislivec, A., Mladenov, D., Mocioiu, I., Moffat, K., Moggi, N., Mohanta, R., Mohayai, T. A., Mokhov, N., Molina, J., Bueno, L. M., Montanari, A., Montanari, C., Montanari, D., Zetina, L. M. M., Moon, J., Mooney, M., Moor, A., Moreno, D., Morgan, B., Morris, C., Mossey, C., Motuk, E., Moura, C. A., Mousseau, J., Mu, W., Mualem, L., Mueller, J., Muether, M., Mufson, S., Muheim, F., Muir, A., Mulhearn, M., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nagu, S., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navas-Nicolas, D., Nayak, N., Nebot-Guinot, M., Necib, L., Negishi, K., Nelson, J. K., Nesbit, J., Nessi, M., Newbold, D., Newcomer, M., Newhart, D., Nichol, R., Niner, E., Nishimura, K., Norman, A., Norrick, A., Northrop, R., Novella, P., Nowak, J. A., Oberling, M., Campo, A. O. D., Olivier, A., Onel, Y., Onishchuk, Y., Ott, J., Pagani, L., Pakvasa, S., Palamara, O., Palestini, S., Paley, J. M., Pallavicini, M., Palomares, C., Pantic, E., Paolone, V., Papadimitriou, V., Papaleo, R., Papanestis, A., Paramesvaran, S., Parke, S., Parsa, Z., Parvu, M., Pascoli, S., Pasqualini, L., Pasternak, J., Pater, J., Patrick, C., Patrizii, L., Patterson, R. B., Patton, S. J., Patzak, T., Paudel, A., Paulos, B., Paulucci, L., Pavlovic, Z., Pawloski, G., Payne, D., Pec, V., Peeters, S. J. M., Penichot, Y., Pennacchio, E., Penzo, A., Peres, O. L. G., Perry, J., Pershey, D., Pessina, G., Petrillo, G., Petta, C., Petti, R., Piastra, F., Pickering, L., Pietropaolo, F., Pillow, J., Pinzino, J., Plunkett, R., Poling, R., Pons, X., Poonthottathil, N., Pordes, S., Potekhin, M., Potenza, R., Potukuchi, B. V. K. S., Pozimski, J., Pozzato, M., Prakash, S., Prakash, T., Prince, S., Prior, G., Pugnere, D., Qi, K., Qian, X., Raaf, J. L., Raboanary, R., Radeka, V., Rademacker, J., Radics, B., Rafique, A., Raguzin, E., Rai, M., Rajaoalisoa, M., Rakhno, I., Rakotondramanana, H. T., Rakotondravohitra, L., Ramachers, Y. A., Rameika, R., Delgado, M. A. R., Ramson, B., Rappoldi, A., Raselli, G., Ratoff, P., Ravat, S., Razafinime, H., Real, J. S., Rebel, B., Redondo, D., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, S. D., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Rigamonti, A., Rigaut, Y., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. R., Rondon, J. R., Roeth, A. J., Rogers, H., Rosauro-Alcaraz, S., Rosenthal, M., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Russell, B., Russell, J., Ruterbories, D., Saakyan, R., Sacerdoti, S., Safford, T., Sahu, N., Sala, P., Salukvadze, G., Samios, N., Sanchez, M. C., Sanders, D. A., Sankey, D., Santana, S., Santos-Maldonado, M., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Savinov, V., Scaramelli, A., Scarff, A., Scarpelli, A., Schellman, H., Schlabach, P., Schmitz, D., Scholberg, K., Schukraft, A., Segreto, E., Seltskaya, E., Sensenig, J., Seong, I., Sergi, A., Sergiampietri, F., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shamma, M., Sharma, H. R., Sharma, R., Shaw, T., Shepherd-Themistocleous, C., Shin, S., Shooltz, D., Shrock, R., Simard, L., Simos, N., Sinclair, J., Sinev, G., Singh, J., Singh, V., Sipos, R., Sippach, F. W., Sirri, G., Sitraka, A., Siyeon, K., Smargianaki, D., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snopok, P., Nunes, M. S., Sobel, H., Soderberg, M., Salinas, C. J. S., Soldner-Rembold, S., Solomey, N., Solovov, V., Sondheim, W. E., Sorel, M., Soto-Oton, J., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Spurgeon, K., Staley, R., Stancari, M., Stanco, L., Stefan, D., Steiner, H. M., Stewart, J., Stillwell, B., Stock, J., Stocker, F., Stokes, T., Strait, M., Strauss, T., Striganov, S., Stuart, A., Sulej, R., Summers, D., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Talaga, R., Tanaka, H. A., Oregui, B. T., Tapper, A., Tariq, S., Tatar, E., Tayloe, R., Teklu, A. M., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, J. L., Thorn, C., Timm, S. C., Tonazzo, A., Torti, M., Tortola, M., Tortorici, F., Totani, D., Toups, M., Touramanis, C., Trevor, J., Trzaska, W. H., Tsai, Y. T., Tsamalaidze, Z., Tsang, K. V., Tsverava, N., Tufanli, S., Tull, C., Tyley, E., Tzanov, M., Uchida, M. A., Urheim, J., Usher, T., Vagins, M. R., Vahle, P., Valdiviesso, G. A., Valencia, E., Vallari, Z., Valle, J. W. F., Vallecorsa, S., Berg, R. V., De Water, R. G. V., Forero, D. V., Varanini, F., Vargas, D., Varner, G., Vasel, J., Vasseur, G., Vaziri, K., Ventura, S., Verdugo, A., Vergani, S., Vermeulen, M. A., Verzocchi, M., De Souza, H. V., Vignoli, C., Vilela, C., Viren, B., Vrba, T., Wachala, T., Waldron, A. V., Wallbank, M., Wang, H., Wang, J., Wang, Y., Warburton, K., Warner, D., Wascko, M., Waters, D., Watson, A., Weatherly, P., Weber, A., Weber, M., Wei, H., Weinstein, A., Wenman, D., Wetstein, M., While, M. R., White, A., Whitehead, L. 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D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., Zwaska, R., Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), DUNE, Abi, B, Abud, A, Acciarri, R, Acero, M, Adamov, G, Adamowski, M, Adams, D, Adrien, P, Adinolfi, M, Ahmad, Z, Ahmed, J, Alion, T, Monsalve, S, Alt, C, Anderson, J, Andreopoulos, C, Andrews, M, Andrianala, F, Andringa, S, Ankowski, A, Antonova, M, 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Almeida, R, Debbins, P, Bonis, I, Decowski, M, De Gouv a, A, Holanda, P, Astiz, I, Deisting, A, Jong, P, Delbart, A, Delepine, D, Delgado, M, Dell'Acqua, A, Lurgio, P, Neto, J, Demuth, D, Dennis, S, Densham, C, Deptuch, G, Roeck, A, Romeri, V, Vries, J, Dharmapalan, R, Dias, M, Diaz, F, Diaz, J, Domizio, S, Giulio, L, Ding, P, Noto, L, Distefano, C, Diurba, R, Diwan, M, Djurcic, Z, Dokania, N, Dolinski, M, Domine, L, Douglas, D, Drielsma, F, Duchesneau, D, Duffy, K, Dunne, P, Durkin, T, Duyang, H, Dvornikov, O, Dwyer, D, Dyshkant, A, Eads, M, Edmunds, D, Eisch, J, Emery, S, Ereditato, A, Escobar, C, Sanchez, L, Evans, J, Ewart, E, Ezeribe, A, Fabre, C, Fahey, K, Falcone, A, Farnese, C, Farzan, Y, Felix, J, Fernandez-Martinez, E, Menendez, P, Ferraro, F, Fields, L, Filkins, A, Filthaut, F, Fitzpatrick, R, Flanagan, W, Fleming, B, Flight, R, Fowler, J, Fox, W, Franc, J, Francis, K, Franco, D, Freeman, J, Freestone, J, Fried, J, Friedland, A, Fuess, S, Furic, I, Furmanski, A, Gago, A, Gallagher, H, Gallego-Ros, A, Gallice, N, Galymov, V, Gamberini, E, Gamble, T, Gandhi, R, Gandrajula, R, Gao, S, Garcia-Gamez, D, Garcia-Peris, M, Gardiner, S, Gastler, D, Ge, G, Gelli, B, Gendotti, A, Gent, S, Ghorbani-Moghaddam, Z, Gibin, D, Gil-Botella, I, Girerd, C, Giri, A, Gnani, D, Gogota, O, Gold, M, Gollapinni, S, Gollwitzer, K, Gomes, R, Bermeo, L, Fajardo, L, Gonnella, F, Gonzalez-Cuevas, J, Goodman, M, Goodwin, O, Goswami, S, Gotti, C, Goudzovski, E, Grace, C, Graham, M, Gramellini, E, Gran, R, Granados, E, Grant, A, Grant, C, Gratieri, D, Green, P, Green, S, Greenler, L, Greenwood, M, Greer, J, Griffith, W, Groh, M, Grudzinski, J, Grzelak, K, Gu, W, Guarino, V, Guenette, R, Guglielmi, A, Guo, B, Guthikonda, K, Gutierrez, R, Guzowski, P, Guzzo, M, Gwon, S, Haaf, K, Habig, A, Hackenburg, A, Hadavand, H, Haenni, R, Hahn, A, Haigh, J, Haiston, J, Hamernik, T, Hamilton, P, Han, J, Harder, K, Harris, D, Hartnell, J, Hasegawa, T, Hatcher, R, Hazen, E, Heavey, A, Heeger, K, Heise, 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Kulagin, S, Kumar, J, Kumar, R, Kuruppu, C, Kus, V, Kutter, T, Lacarelle, B, Lambert, A, Lande, K, Lane, C, Lang, K, Langford, T, Lasorak, P, Last, D, Lastoria, C, Laundrie, A, Lawrence, A, Lazanu, I, Lazur, R, Le, T, Learned, J, Lebrun, P, Miotto, G, Lehnert, R, De Oliveira, M, Leitner, M, Leyton, M, Li, L, Li, S, Li, T, Li, Y, Liao, H, Lin, C, Lin, S, Lister, A, Littlejohn, B, Liu, J, Liu, T, Lockwitz, S, Loew, T, Lokajicek, M, Lomidze, I, Long, K, Loo, K, Lorca, D, Lord, T, Losecco, J, Louis, W, Luk, K, Luo, X, Lurkin, N, Lux, T, Luzio, V, Macfarland, D, Machado, A, Machado, P, Macias, C, Macier, J, Maddalena, A, Madigan, P, Magill, S, Mahn, K, Maio, A, Maloney, J, Mandrioli, G, Maneira, J, Manenti, L, Manly, S, Mann, A, Manolopoulos, K, Plata, M, Marchionni, A, Marciano, W, Marfatia, D, Mariani, C, Maricic, J, Marinho, F, Marino, A, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, N, Martinez Caicedo, D, Martynenko, S, Mason, K, Mastbaum, A, Masud, M, Matsuno, S, Matthews, J, Mauger, C, Mauri, N, Mavrokoridis, K, Mazza, R, Mazzacane, A, Mazzucato, E, Mccluskey, E, Mcconkey, N, Mcfarland, K, Mcgrew, C, Mcnab, A, Mefodiev, A, Mehta, P, Melas, P, Mellinato, M, Mena, O, Menary, S, Mendez, H, Menegolli, A, Meng, G, Messier, M, Metcalf, W, Mewes, M, Meyer, H, Miao, T, Michna, G, Miedema, T, Migenda, J, Milincic, R, Miller, W, Mills, J, Milne, C, Mineev, O, Miranda, O, Miryala, S, Mishra, C, Mishra, S, Mislivec, A, Mladenov, D, Mocioiu, I, Moffat, K, Moggi, N, Mohanta, R, Mohayai, T, Mokhov, N, Molina, J, Bueno, L, Montanari, A, Montanari, C, Montanari, D, Zetina, L, Moon, J, Mooney, M, Moor, A, Moreno, D, Morgan, B, Morris, C, Mossey, C, Motuk, E, Moura, C, Mousseau, J, Mu, W, Mualem, L, Mueller, J, Muether, M, Mufson, S, Muheim, F, Muir, A, Mulhearn, M, Muramatsu, H, Murphy, S, Musser, J, Nachtman, J, Nagu, S, Nalbandyan, M, Nandakumar, R, Naples, D, Narita, S, Navas-Nicolas, D, Nayak, N, Nebot-Guinot, M, Necib, L, Negishi, K, Nelson, J, Nesbit, J, Nessi, M, Newbold, D, Newcomer, M, Newhart, D, Nichol, R, Niner, E, Nishimura, K, Norman, A, Norrick, A, Northrop, R, Novella, P, Nowak, J, Oberling, M, Campo, A, Olivier, A, Onel, Y, Onishchuk, Y, Ott, J, Pagani, L, Pakvasa, S, Palamara, O, Palestini, S, Paley, J, Pallavicini, M, Palomares, C, Pantic, E, Paolone, V, Papadimitriou, V, Papaleo, R, Papanestis, A, Paramesvaran, S, Parke, S, Parsa, Z, Parvu, M, Pascoli, S, Pasqualini, L, Pasternak, J, Pater, J, Patrick, C, Patrizii, L, Patterson, R, Patton, S, Patzak, T, Paudel, A, Paulos, B, Paulucci, L, Pavlovic, Z, Pawloski, G, Payne, D, Pec, V, Peeters, S, Penichot, Y, Pennacchio, E, Penzo, A, Peres, O, Perry, J, Pershey, D, Pessina, G, Petrillo, G, Petta, C, Petti, R, Piastra, F, Pickering, L, Pietropaolo, F, Pillow, J, Pinzino, J, Plunkett, R, Poling, R, Pons, X, Poonthottathil, N, Pordes, S, Potekhin, M, Potenza, R, Potukuchi, B, Pozimski, J, Pozzato, M, Prakash, S, Prakash, T, Prince, S, Prior, G, Pugnere, D, Qi, K, Qian, X, Raaf, J, Raboanary, R, Radeka, V, Rademacker, J, Radics, B, Rafique, A, Raguzin, E, Rai, M, Rajaoalisoa, M, Rakhno, I, Rakotondramanana, H, Rakotondravohitra, L, Ramachers, Y, Rameika, R, Ramson, B, Rappoldi, A, Raselli, G, Ratoff, P, Ravat, S, Razafinime, H, Real, J, Rebel, B, Redondo, D, Reggiani-Guzzo, M, Rehak, T, Reichenbacher, J, Reitzner, S, Renshaw, A, Rescia, S, Resnati, F, Reynolds, A, Riccobene, G, Rice, L, Rielage, K, Rigamonti, A, Rigaut, Y, Rivera, D, Rochester, L, Roda, M, Rodrigues, P, Alonso, M, Rondon, J, Roeth, A, Rogers, H, Rosauro-Alcaraz, S, Rosenthal, M, Rossella, M, Rout, J, Roy, S, Rubbia, A, Rubbia, C, Russell, B, Russell, J, Ruterbories, D, Saakyan, R, Sacerdoti, S, Safford, T, Sahu, N, Sala, P, Salukvadze, G, Samios, N, Sanchez, M, Sanders, D, Sankey, D, Santana, S, Santos-Maldonado, M, Saoulidou, N, Sapienza, P, Sarasty, C, Sarcevic, I, Savage, G, Savinov, V, Scaramelli, A, Scarff, A, Scarpelli, A, Schellman, H, Schlabach, P, Schmitz, D, Scholberg, K, Schukraft, A, Segreto, E, Seltskaya, E, Sensenig, J, Seong, I, Sergi, A, Sergiampietri, F, Sgalaberna, D, Shaevitz, M, Shafaq, S, Shamma, M, Sharma, H, Sharma, R, Shaw, T, Shepherd-Themistocleous, C, Shin, S, Shooltz, D, Shrock, R, Simard, L, Simos, N, Sinclair, J, Sinev, G, Singh, J, Singh, V, Sipos, R, Sippach, F, Sirri, G, Sitraka, A, Siyeon, K, Smargianaki, D, Smith, A, Smith, E, Smith, P, Smolik, J, Smy, M, Snopok, P, Nunes, M, Sobel, H, Soderberg, M, Salinas, C, Soldner-Rembold, S, Solomey, N, Solovov, V, Sondheim, W, Sorel, M, Soto-Oton, J, Sousa, A, Soustruznik, K, Spagliardi, F, Spanu, M, Spitz, J, Spooner, N, Spurgeon, K, Staley, R, Stancari, M, Stanco, L, Stefan, D, Steiner, H, Stewart, J, Stillwell, B, Stock, J, Stocker, F, Stokes, T, Strait, M, Strauss, T, Striganov, S, Stuart, A, Sulej, R, Summers, D, Surdo, A, Susic, V, Suter, L, Sutera, C, Svoboda, R, Szczerbinska, B, Szelc, A, Talaga, R, Tanaka, H, Oregui, B, Tapper, A, Tariq, S, Tatar, E, Tayloe, R, Teklu, A, Tenti, M, Terao, K, Ternes, C, Terranova, F, Testera, G, Thea, A, Thompson, J, Thorn, C, Timm, S, Tonazzo, A, Torti, M, Tortola, M, Tortorici, F, Totani, D, Toups, M, Touramanis, C, Trevor, J, Trzaska, W, Tsai, Y, Tsamalaidze, Z, Tsang, K, Tsverava, N, Tufanli, S, Tull, C, Tyley, E, Tzanov, M, Uchida, M, Urheim, J, Usher, T, Vagins, M, Vahle, P, Valdiviesso, G, Valencia, E, Vallari, Z, Valle, J, Vallecorsa, S, Berg, R, De Water, R, Forero, D, Varanini, F, Vargas, D, Varner, G, Vasel, J, Vasseur, G, Vaziri, K, Ventura, S, Verdugo, A, Vergani, S, Vermeulen, M, Verzocchi, M, De Souza, H, Vignoli, C, Vilela, C, Viren, B, Vrba, T, Wachala, T, Waldron, A, Wallbank, M, Wang, H, Wang, J, Wang, Y, Warburton, K, Warner, D, Wascko, M, Waters, D, Watson, A, Weatherly, P, Weber, A, Weber, M, Wei, H, Weinstein, A, Wenman, D, Wetstein, M, While, M, White, A, Whitehead, L, Whittington, D, Wilking, M, Wilkinson, C, Williams, Z, Wilson, F, Wilson, R, Wolcott, J, Wongjirad, T, Wood, K, Wood, L, Worcester, E, Worcester, M, Wret, C, Wu, W, Xiao, Y, Yang, G, Yang, T, Yershov, N, Yonehara, K, Young, T, Yu, B, Yu, H, Yu, J, Yu, Z, Zaki, R, Zalesak, J, Zambelli, L, Zamorano, B, Zani, A, Zazueta, L, Zeller, G, Zennamo, J, Zeug, K, Zhang, C, Zhao, M, Zhivun, E, Zhu, G, Zimmerman, E, Zito, M, Zucchelli, S, Zuklin, J, Zutshi, V, Zwaska, R, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), XENON (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), Abi B., Abud A.A., Acciarri R., Acero M.A., Adamov G., Adamowski M., Adams D., Adrien P., Adinolfi M., Ahmad Z., Ahmed J., Alion T., Monsalve S.A., Alt C., Anderson J., Andreopoulos C., Andrews M.P., Andrianala F., Andringa S., Ankowski A., Antonova M., Antusch S., Aranda-Fernandez A., Ariga A., Arnold L.O., Arroyave M.A., Asaadi J., Aurisano A., Aushev V., Autiero D., Azfar F., Back H., Back J.J., Backhouse C., Baesso P., Bagby L., Bajou R., Balasubramanian S., Baldi P., Bambah B., Barao F., Barenboim G., Barker G.J., Barkhouse W., Barnes C., Barr G., Monarca J.B., Barros N., Barrow J.L., Bashyal A., Basque V., Bay F., Alba J.L.B., Beacom J.F., Bechetoille E., Behera B., Bellantoni L., Bellettini G., Bellini V., Beltramello O., Belver D., Benekos N., Neves F.B., Berger J., Berkman S., Bernardini P., Berner R.M., Berns H., Bertolucci S., Betancourt M., Bezawada Y., Bhattacharjee M., Bhuyan B., Biagi S., Bian J., Biassoni M., Biery K., Bilki B., Bishai M., Bitadze A., Blake A., Siffert B.B., Blaszczyk F.D.M., Blazey G.C., Blucher E., Boissevain J., Bolognesi S., Bolton T., Bonesini M., Bongrand M., Bonini F., Booth A., Booth C., Bordoni S., Borkum A., Boschi T., Bostan N., Bour P., Boyd S.B., Boyden D., Bracinik J., Braga D., Brailsford D., Brandt A., Bremer J., Brew C., Brianne E., Brice S.J., Brizzolari C., Bromberg C., Brooijmans G., Brooke J., Bross A., Brunetti G., Buchanan N., Budd H., Caiulo D., Calafiura P., Calcutt J., Calin M., Calvez S., Calvo E., Camilleri L., Caminata A., Campanelli M., Caratelli D., Carini G., Carlus B., Carniti P., Terrazas I.C., Carranza H., Castillo A., Castromonte C., Cattadori C., Cavalier F., Cavanna F., Centro S., Cerati G., Cervelli A., Villanueva A.C., Chalifour M., Chang C., Chardonnet E., Charitonidis N., Chatterjee A., Chattopadhyay S., Chatzidaki P., Chaves J., Chen H., Chen M., Chen Y., Cherdack D., Chi C., Childress S., Chiriacescu A., Cho K., Choubey S., Christensen A., Christian D., Christodoulou G., Church E., Clarke P., Coan T.E., Cocco A.G., Coelho 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Grudzinski J., Grzelak K., Gu W., Guarino V., Guenette R., Guglielmi A., Guo B., Guthikonda K.K., Gutierrez R., Guzowski P., Guzzo M.M., Gwon S., Haaf K., Habig A., Hackenburg A., Hadavand H., Haenni R., Hahn A., Haigh J., Haiston J., Hamernik T., Hamilton P., Han J., Harder K., Harris D.A., Hartnell J., Hasegawa T., Hatcher R., Hazen E., Heavey A., Heeger K.M., Heise J., Hennessy K., Henry S., Morquecho M.A.H., Herner K., Hertel L., Hesam A.S., Hewes J., Higuera A., Hill T., Hillier S.J., Himmel A., Hoff J., Hohl C., Holin A., Hoppe E., Horton-Smith G.A., Hostert M., Hourlier A., Howard B., Howell R., Hrivnak J., Huang J., Hugon J., Iles G., Ilic N., Iliescu A.M., Illingworth R., Ioannisian A., Itay R., Izmaylov A., James E., Jargowsky B., Jediny F., Jes s-Valls C., Ji X., Jiang L., Jimenez S., Jipa A., Joglekar A., Johnson C., Johnson R., Jones B., Jones S., Jung C.K., Junk T., Jwa Y., Kabirnezhad M., Kaboth A., Kadenko I., Kamiya F., Karagiorgi G., Karcher A., Karolak M., Karyotakis 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T., Paudel A., Paulos B., Paulucci L., Pavlovic Z., Pawloski G., Payne D., Pec V., Peeters S.J.M., Penichot Y., Pennacchio E., Penzo A., Peres O.L.G., Perry J., Pershey D., Pessina G., Petrillo G., Petta C., Petti R., Piastra F., Pickering L., Pietropaolo F., Pillow J., Pinzino J., Plunkett R., Poling R., Pons X., Poonthottathil N., Pordes S., Potekhin M., Potenza R., Potukuchi B.V.K.S., Pozimski J., Pozzato M., Prakash S., Prakash T., Prince S., Prior G., Pugnere D., Qi K., Qian X., Raaf J.L., Raboanary R., Radeka V., Rademacker J., Radics B., Rafique A., Raguzin E., Rai M., Rajaoalisoa M., Rakhno I., Rakotondramanana H.T., Rakotondravohitra L., Ramachers Y.A., Rameika R., Delgado M.A.R., Ramson B., Rappoldi A., Raselli G., Ratoff P., Ravat S., Razafinime H., Real J.S., Rebel B., Redondo D., Reggiani-Guzzo M., Rehak T., Reichenbacher J., Reitzner S.D., Renshaw A., Rescia S., Resnati F., Reynolds A., Riccobene G., Rice L.C.J., Rielage K., Rigamonti A., Rigaut Y., Rivera D., Rochester L., Roda M., Rodrigues P., Alonso M.J.R., Rondon J.R., Roeth A.J., Rogers H., Rosauro-Alcaraz S., Rosenthal M., Rossella M., Rout J., Roy S., Rubbia A., Rubbia C., Russell B., Russell J., Ruterbories D., Saakyan R., Sacerdoti S., Safford T., Sahu N., Sala P., Salukvadze G., Samios N., Sanchez M.C., Sanders D.A., Sankey D., Santana S., Santos-Maldonado M., Saoulidou N., Sapienza P., Sarasty C., Sarcevic I., Savage G., Savinov V., Scaramelli A., Scarff A., Scarpelli A., Schellman H., Schlabach P., Schmitz D., Scholberg K., Schukraft A., Segreto E., Seltskaya E., Sensenig J., Seong I., Sergi A., Sergiampietri F., Sgalaberna D., Shaevitz M.H., Shafaq S., Shamma M., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Smargianaki D., Smith A., Smith E., Smith P., Smolik J., Smy M., Snopok P., Nunes M.S., Sobel H., Soderberg M., Salinas C.J.S., Soldner-Rembold S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Stefan D., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Sulej R., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Oregui B.T., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Tonazzo A., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Trevor J., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Vallari Z., Valle J.W.F., Vallecorsa S., Berg R.V., De Water R.G.V., Forero D.V., Varanini F., Vargas D., Varner G., Vasel J., Vasseur G., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., De Souza H.V., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., Yang T., Yershov N., Yonehara K., Young T., Yu B., Yu H.W., Yu H.Z., Yu J., Yu Z.Y., Zaki R., Zalesak J., Zambelli L., Zamorano B., Zani A., Zazueta L., Zeller G.P., Zennamo J., Zeug K., Zhang C., Zhao M., Zhivun E., Zhu G., Zimmerman E.D., Zito M., Zucchelli S., Zuklin J., Zutshi V., Zwaska R., and Science and Technology Facilities Council (STFC)
Subjects: Technology, HIGH-ENERGY, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, far detector, beam transport, Noble liquid detectors (scintillation, ionization, double-phase), Cms Experıment, 01 natural sciences, 7. Clean energy, 09 Engineering, Particle identification, High Energy Physics - Experiment, 030218 nuclear medicine & medical imaging, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, Noble liquid detectors (scintillation, Detectors and Experimental Techniques, Instrumentation, Instruments & Instrumentation, physics.ins-det, time resolution, Mathematical Physics, Physics, 02 Physical Sciences, Time projection chamber, Large Hadron Collider, Detector, Instrumentation and Detectors (physics.ins-det), double-phase), Nuclear & Particles Physics, LIGHT, Neutrino, Particle Physics - Experiment, performance, Noble liquid detectors,(scintillation, ionization, double-phase), noise, CERN Lab, Large detector systems for particle and astroparticle physics, Noble liquid detectors (scintillation, ionization, double-phase), Time projection Chambers (TPC), 530 Physics, energy loss, Time projection chambers, FOS: Physical sciences, Particle detector, Nuclear physics, 03 medical and health sciences, neutrino: deep underground detector, 0103 physical sciences, ionization, Deep Underground Neutrino Experiment, High Energy Physics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], signal processing, activity report, Science & Technology, 010308 nuclear & particles physics, hep-ex, Large detector systems for particle and astroparticle physics, Time projection Chambers (TPC), 530 Physik, sensitivity, calibration, time projection chamber: liquid argon, Experimental High Energy Physics, Large detector systems for particle and astroparticle physic, single-phase), High Energy Physics::Experiment, photon: detector, particle identification, charged particle: irradiation, Beam (structure)
Abstract: The ProtoDUNE-SP detector was constructed and operated on the CERN Neutrino Platform. We thank the CERN management for providing the infrastructure for this experiment and gratefully acknowledge the support of the CERN EP, BE, TE, EN, IT and IPT Departments for NP04/ProtoDUNE-SP. This documentwas prepared by theDUNEcollaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MSMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundacion "La Caixa" and MICINN, Spain; SERI and SNSF, Switzerland; TUBITAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231., The ProtoDUNE-SP detector is a single-phase liquid argon time projection chamber with an active volume of 7.2× 6.1× 7.0 m3. It is installed at the CERN Neutrino Platform in a specially-constructed beam that delivers charged pions, kaons, protons, muons and electrons with momenta in the range 0.3 GeV/c to 7 GeV/c. Beam line instrumentation provides accurate momentum measurements and particle identification. The ProtoDUNE-SP detector is a prototype for the first far detector module of the Deep Underground Neutrino Experiment, and it incorporates full-size components as designed for that module. This paper describes the beam line, the time projection chamber, the photon detectors, the cosmic-ray tagger, the signal processing and particle reconstruction. It presents the first results on ProtoDUNE-SP's performance, including noise and gain measurements, dE/dx calibration for muons, protons, pions and electrons, drift electron lifetime measurements, and photon detector noise, signal sensitivity and time resolution measurements. The measured values meet or exceed the specifications for the DUNE far detector, in several cases by large margins. ProtoDUNE-SP's successful operation starting in 2018 and its production of large samples of high-quality data demonstrate the effectiveness of the single-phase far detector design., National Council for Scientific and Technological Development (CNPq), Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ), FAPEG, Brazil, Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Canada Foundation for Innovation, Natural Sciences and Engineering Research Council of Canada (NSERC), Ministry of Education, Youth & Sports - Czech Republic Czech Republic Government, European Union (EU), H2020-EU, French Atomic Energy Commission, Istituto Nazionale di Fisica Nucleare (INFN), NRF, South Korea, La Caixa Foundation, Spanish Government, Swiss National Science Foundation (SNSF), Turkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK), Royal Society of London, United States Department of Energy (DOE), National Science Foundation (NSF) DE-AC02-05CH11231, IPP, Canada, CERN, MSCA, Centre National de la Recherche Scientifique (CNRS), Portuguese Foundation for Science and Technology, CAM, Spain, SERI, Switzerland, UKRI/STFC, United Kingdom, DE-AC02-07CH11359
Published: 2020

21. Long-baseline neutrino oscillation physics potential of the DUNE experiment: DUNE Collaboration

Author: M. Spanu, Xiaolu Ji, A. M. Szelc, Gareth J. Barker, C. Cattadori, J. Fried, J. Fowler, S. J. M. Peeters, S. Alonso Monsalve, G. Ge, Alexander Tapper, Thomas Strauss, B. Bhuyan, D. Vanegas Forero, A. L. Renshaw, A. P. Furmanski, P.T. Smith, D. Newhart, E. Raguzin, A. J. Roeth, R. Acciarri, Karol Lang, V. Savinov, P. Melas, A. Heavey, Grzegorz Deptuch, Kevin J. Kelly, D. Sgalaberna, R. LaZur, E. Pennacchio, F. W. Sippach, Kristian Harder, M. A. Uchida, J. Hewes, Sandro Palestini, K. Spurgeon, Sandip Pakvasa, F. Stocker, H. W. Sobel, A. Gallego-Ros, N. Buchanan, C. Grant, T. Li, T. Gamble, J. J. Grudzinski, N. Mauri, L. Molina Bueno, Jeremy Wolcott, Andrea Zani, M. J. Wilking, A. Olivares Del Campo, Joshua R. Klein, A. Hourlier, Jonas Rademacker, G. P. Zeller, A. Lawrence, D. Brailsford, M. Chalifour, I. Gil-Botella, R. Flight, H. Vieira de Souza, D. Redondo, S. R. Mishra, Paola Sala, Joshua Barrow, John Marshall, K. Francis, S. Ravat, W. Mu, D. Marfatia, Vasundhara Singh, Ranjan Dharmapalan, S. Striganov, Laura Paulucci, Mario Campanelli, D. Cherdack, M. A. Ramirez Delgado, S. J. Brice, Nicolas Lurkin, Wayne A. Barkhouse, A. Filkins, D. Autiero, Poonam Mehta, Dave Sankey, J. Asaadi, E. Valencia, E. James, N.V. Mokhov, A. Booth, E. Hazen, Armin Karcher, D. Smargianaki, S. Menary, P. C. de Holanda, J. Hugon, C. Brizzolari, M. Kirby, E. Kearns, A. C. Ezeribe, T. Lord, L. Zazueta, Daijin Kim, G.D. Barr, Junwei Huang, V. De Romeri, F. Piastra, C. Girerd, Christopher L. Marshall, A. Bitadze, Yichen Li, Alexander Deisting, H. Carranza, Milos Lokajicek, Roberto Gutiérrez, J. Pinzino, Janice L. Thompson, F. Kamiya, M. Wetstein, A. Cervera Villanueva, Robert Svoboda, L. C. J. Rice, L. Pasqualini, L. Di Giulio, J. Martin-Albo, H. Muramatsu, Z. Pavlovic, A. Falcone, R. Gran, A. A. Machado, R. Petti, M. Roda, Jianbei Liu, C. Vignoli, B. Rebel, Joleen Pater, David H. Adams, D. Caratelli, S. Martynenko, Ph. Lebrun, R. Staley, J. L. 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A., Lazanu I., LaZur R., Le T., Learned J., LeBrun P., Miotto G.L., Lehnert R., de Oliveira M.A.L., Leitner M., Leyton M., Li L., Li S., Li S.W., Li T., Li Y., Liao H., Lin C.S., Lin S., Lister A., Littlejohn B.R., Liu J., Lockwitz S., Loew T., Lokajicek M., Lomidze I., Long K., Loo K., Lorca D., Lord T., LoSecco J.M., Louis W.C., Luk K.B., Luo X., Lurkin N., Lux T., Luzio V.P., MacFarland D., Machado A.A., Machado P., Macias C.T., Macier J.R., Maddalena A., Madigan P., Magill S., Mahn K., Maio A., Maloney J.A., Mandrioli G., Maneira J., Manenti L., Manly S., Mann A., Manolopoulos K., Plata M.M., Marchionni A., Marciano W., Marfatia D., Mariani C., Maricic J., Marinho F., Marino A.D., Marshak M., Marshall C., Marshall J., Marteau J., Martin-Albo J., Martinez N., Caicedo D.A.M., Martynenko S., Mason K., Mastbaum A., Masud M., Matsuno S., Matthews J., Mauger C., Mauri N., Mavrokoridis K., Mazza R., Mazzacane A., Mazzucato E., McCluskey E., McConkey N., McFarland K.S., McGrew C., McNab 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Shaevitz M.H., Shafaq S., Shamma M., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Smargianaki D., Smith A., Smith E., Smith P., Smolik J., Smy M., Snopok P., Nunes M.S., Sobel H., Soderberg M., Salinas C.J.S., Soldner-Rembold S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Oregui B.T., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Tonazzo A., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Trevor J., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Vallari Z., Valle J.W.F., Vallecorsa S., Van Berg R., Van de Water R.G., Forero D.V., Varanini F., Vargas D., Varner G., Vasel J., Vasseur G., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., de Souza H.V., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., 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D., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Rigaut, Y., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. R., Rondon, J. R., Roeth, A. J., Rogers, H., Rosauro-Alcaraz, S., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Russell, B., Russell, J., Ruterbories, D., Saakyan, R., Sacerdoti, S., Safford, T., Sahu, N., Sala, P., Samios, N., Sanchez, M. C., Sanders, D. A., Sankey, D., Santana, S., Santos-Maldonado, M., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Savinov, V., Scaramelli, A., Scarff, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schmitz, D., Scholberg, K., Schukraft, A., Segreto, E., Sensenig, J., Seong, I., Sergi, A., Sergiampietri, F., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shamma, M., Sharma, H. R., Sharma, R., Shaw, T., Shepherd-Themistocleous, C., Shin, S., Shooltz, D., Shrock, R., Simard, L., Simos, N., Sinclair, J., Sinev, G., Singh, J., Singh, V., Sipos, R., Sippach, F. W., Sirri, G., Sitraka, A., Siyeon, K., Smargianaki, D., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snopok, P., Nunes, M. S., Sobel, H., Soderberg, M., Salinas, C. J. S., Soldner-Rembold, S., Solomey, N., Solovov, V., Sondheim, W. E., Sorel, M., Soto-Oton, J., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Spurgeon, K., Staley, R., Stancari, M., Stanco, L., Steiner, H. M., Stewart, J., Stillwell, B., Stock, J., Stocker, F., Stokes, T., Strait, M., Strauss, T., Striganov, S., Stuart, A., Summers, D., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Talaga, R., Tanaka, H. A., Oregui, B. T., Tapper, A., Tariq, S., Tatar, E., Tayloe, R., Teklu, A. M., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, J. L., Thorn, C., Timm, S. C., Tonazzo, A., Torti, M., Tortola, M., Tortorici, F., Totani, D., Toups, M., Touramanis, C., Trevor, J., Trzaska, W. H., Tsai, Y. T., Tsamalaidze, Z., Tsang, K. V., Tsverava, N., Tufanli, S., Tull, C., Tyley, E., Tzanov, M., Uchida, M. A., Urheim, J., Usher, T., Vagins, M. R., Vahle, P., Valdiviesso, G. A., Valencia, E., Vallari, Z., Valle, J. W. F., Vallecorsa, S., Van Berg, R., Van de Water, R. G., Forero, D. V., Varanini, F., Vargas, D., Varner, G., Vasel, J., Vasseur, G., Vaziri, K., Ventura, S., Verdugo, A., Vergani, S., Vermeulen, M. A., Verzocchi, M., de Souza, H. V., Vignoli, C., Vilela, C., Viren, B., Vrba, T., Wachala, T., Waldron, A. V., Wallbank, M., Wang, H., Wang, J., Wang, Y., Warburton, K., Warner, D., Wascko, M., Waters, D., Watson, A., Weatherly, P., Weber, A., Weber, M., Wei, H., Weinstein, A., Wenman, D., Wetstein, M., While, M. R., White, A., Whitehead, L. H., Whittington, D., Wilking, M. J., Wilkinson, C., Williams, Z., Wilson, F., Wilson, R. J., Wolcott, J., Wongjirad, T., Wood, K., Wood, L., Worcester, E., Worcester, M., Wret, C., Wu, W., Xiao, Y., Yang, G., Yang, T., Yershov, N., Yonehara, K., Young, T., Yu, B., Yu, J., Zaki, R., Zalesak, J., Zambelli, L., Zamorano, B., Zani, A., Zazueta, L., Zeller, G. P., Zennamo, J., Zeug, K., Zhang, C., Zhao, M., Zhivun, E., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., and Zwaska, R.
Subjects: Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, 01 natural sciences, Particle detector, Physics, Particles & Fields, Nuclear physics, neutrino, 0103 physical sciences, Neutrino oscillations, neutrino physiscs, Deep Underground Neutrino Experiment, Deep Underground Neutrino Experiment, Neutrino oscillation experiment, DISTRIBUTIONS, Fermilab, High Energy Physics, LEPTON SCATTERING, 010306 general physics, Neutrino oscillation, Engineering (miscellaneous), Physics, Science & Technology, 010308 nuclear & particles physics, Detector, High Energy Physics::Phenomenology, Neutrino detector, Physical Sciences, High Energy Physics::Experiment, Neutrino, Lepton
Abstract: The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation is determined, based on a full simulation, reconstruction, and event selection of the far detector and a full simulation and parameterized analysis of the near detector. Detailed uncertainties due to the flux prediction, neutrino interaction model, and detector effects are included. DUNE will resolve the neutrino mass ordering to a precision of 5$$\sigma $$ σ , for all $$\delta _{\mathrm{CP}}$$ δ CP values, after 2 years of running with the nominal detector design and beam configuration. It has the potential to observe charge-parity violation in the neutrino sector to a precision of 3$$\sigma $$ σ (5$$\sigma $$ σ ) after an exposure of 5 (10) years, for 50% of all $$\delta _{\mathrm{CP}}$$ δ CP values. It will also make precise measurements of other parameters governing long-baseline neutrino oscillation, and after an exposure of 15 years will achieve a similar sensitivity to $$\sin ^{2} 2\theta _{13}$$ sin 2 2 θ 13 to current reactor experiments.
Published: 2020

22. Jovian Auroral Ion Precipitation: Field‐Aligned Currents and Ultraviolet Emissions

Author: Thomas E. Cravens, N. Ozak, J. T. Young, S. J. Houston, and David R. Schultz
Subjects: Physics, 010504 meteorology & atmospheric sciences, Field (physics), Astrophysics, medicine.disease_cause, 01 natural sciences, Jovian, Ion, Jupiter, Geophysics, Space and Planetary Science, 0103 physical sciences, medicine, Precipitation, 010303 astronomy & astrophysics, Ultraviolet, 0105 earth and related environmental sciences
Published: 2018

23. Mode coupling at avoided crossings in slab waveguides with comparison to optical fibers: tutorial

Author: Jonathan Hu, Curtis R. Menyuk, Chengli Wei, and J. T. Young
Subjects: Physics, Optical fiber, business.industry, Physics::Optics, Statistical and Nonlinear Physics, 02 engineering and technology, 021001 nanoscience & nanotechnology, Cladding (fiber optics), Coupled mode theory, 01 natural sciences, Atomic and Molecular Physics, and Optics, law.invention, 010309 optics, Core (optical fiber), Optics, law, 0103 physical sciences, Mode coupling, Slab, 0210 nano-technology, Leaky mode, business, Waveguide
Abstract: Avoided crossings are important in many waveguides and resonators. That is particularly the case in modern-day solid-core and air-core optical fibers that often have a complex geometry. The study of mode coupling at avoided crossings often leads to a complicated analysis. In this tutorial, we aim to explain the basic features of avoided crossings in a simple slab waveguide structure so that the modes can be found analytically with simple sinusoidal and exponential forms. We first review coupled-mode theory for the guided mode in a slab waveguide, which has a higher index in the core. We study the effective index of the guided true mode for a five-layer slab waveguide including two core layers with higher indices compared to the indices in the three cladding layers. Then, we study the same structure by using the overlap between approximate modes confined in the two individual core slabs. When the two individual core slabs are not near each other, the avoided crossing using the true modes within the two-slab waveguide agrees well with the results using the overlap between the two approximate modes. We also study coupled-mode theory and avoided crossings for leaky modes in an antiresonant slab waveguide. We obtain good agreement between the results using the true leaky mode and the results using the overlap between approximate modes. We then discuss examples of avoided crossings in solid-core and air-core optical fibers. We describe the similarities and differences between the optical fibers and simple slab waveguides that we have analyzed in detail.
Published: 2021

24. Nondestructive Cooling of an Atomic Quantum Register via State-Insensitive Rydberg Interactions

Author: Jeremy T. Young, Adam Kaufman, Peter Zoller, Zachary Eldredge, Ron Belyansky, Przemyslaw Bienias, and Alexey V. Gorshkov
Subjects: Atomic Physics (physics.atom-ph), Phonon, Quantum register, FOS: Physical sciences, General Physics and Astronomy, 01 natural sciences, Article, Physics - Atomic Physics, symbols.namesake, 0103 physical sciences, Physics::Atomic and Molecular Clusters, Physics::Atomic Physics, Quantum information, 010306 general physics, Quantum, Computer Science::Databases, Condensed Matter::Quantum Gases, Coupling, Physics, Quantum Physics, Energetic neutral atom, 3. Good health, Heat transfer, Rydberg formula, symbols, Atomic physics, Quantum Physics (quant-ph)
Abstract: We propose a protocol for sympathetically cooling neutral atoms without destroying the quantum information stored in their internal states. This is achieved by designing state-insensitive Rydberg interactions between the data-carrying atoms and cold auxiliary atoms. The resulting interactions give rise to an effective phonon coupling, which leads to the transfer of heat from the data atoms to the auxiliary atoms, where the latter can be cooled by conventional methods. This can be used to extend the lifetime of quantum storage based on neutral atoms and can have applications for long quantum computations. The protocol can also be modified to realize state-insensitive interactions between the data and the auxiliary atoms but tunable and non-trivial interactions among the data atoms, allowing one to simultaneously cool and simulate a quantum spin-model., Comment: 6 + 8 pages, 4 + 1 figures
Published: 2019

25. Probing ISM Structure in Trumpler 14 and Carina I Using the Stratospheric Terahertz Observatory 2

Author: Alexander G. G. M. Tielens, William L. Peters, Paul F. Goldsmith, Mark Wolfire, Shinji Horiuchi, Craig Kulesa, Gary J. Melnick, Thomas B. H. Kuiper, Jorge L. Pineda, Abram Young, Young Min Seo, David Rebolledo, Graeme F Wong, Pietro N. Bernasconi, Jian-Rong Gao, William D. Langer, Christopher K. Walker, Christopher Groppi, Kristina Davis, Floris van der Tak, Erick T. Young, U. Kavak, Harold W. Yorke, Jonathan H. Kawamura, Volker Tolls, Russ Shipman, Antony A. Stark, Michael G. Burton, David Hollenbach, and Astronomy
Subjects: ISM: kinematics and dynamics-ISM: structure-photon-dominated region (PDR)-stars: formation-surveys-H II regions, 010504 meteorology & atmospheric sciences, Milky Way, ISM: structure, Astrophysics, Photodissociation region, 01 natural sciences, Luminosity, surveys, Observatory, 0103 physical sciences, H II regions, 010303 astronomy & astrophysics, photon-dominated region: PDR, 0105 earth and related environmental sciences, Physics, ISM: kinematics and dynamics, Nebula, stars: formation, Molecular cloud, Astronomy and Astrophysics, Photoevaporation, Astrophysics - Astrophysics of Galaxies, Cover (topology), 13. Climate action, Space and Planetary Science
Abstract: We present observations of the Trumpler 14/Carina I region carried out using the Stratospheric Terahertz Observatory 2 (STO2). The Trumpler 14/Carina I region is in the west part of the Carina Nebula Complex, which is one of the most extreme star-forming regions in the Milky Way. We observed Trumpler 14/Carina I in the 158 $\mu$m transition of [C\,{\sc ii}] with a spatial resolution of 48$''$ and a velocity resolution of 0.17 km s$^{-1}$. The observations cover a 0.25$^\circ$ by 0.28$^\circ$ area with central position {\it l} = 297.34$^\circ$, {\it b} = -0.60$^\circ$. The kinematics show that bright [C\,{\sc ii}] structures are spatially and spectrally correlated with the surfaces of CO clouds, tracing the photodissociation region and ionization front of each molecular cloud. Along 7 lines of sight that traverse Tr 14 into the dark ridge to the southwest, we find that the [C\,{\sc ii}] luminosity from the HII region is 3.7 times that from the PDR. In same los we find in the PDRs an average ratio of 1:4.1:5.6 for the mass in atomic gas:dark-CO gas: molecular gas traced by CO. Comparing multiple gas tracers including HI 21cm, [C\,{\sc ii}], CO, and radio recombination lines, we find that the HII regions of the Carina Nebula Complex are well-described as HII regions with one-side freely expanding towards us, consistent with the champagne model of ionized gas evolution. The dispersal of the GMC in this region is dominated by EUV photoevaporation; the dispersal timescale is 20-30 Myr., Comment: ApJ accepted
Published: 2019

26. Seeding fiber amplifiers with piecewise parabolic phase modulation for high SBS thresholds and compact spectra

Author: Jeffrey O. White, Joshua T. Young, Jonathan Hu, Curtis R. Menyuk, and Chengli Wei
Subjects: Physics, business.industry, Amplifier, Bandwidth (signal processing), Phase (waves), 02 engineering and technology, 021001 nanoscience & nanotechnology, 01 natural sciences, Atomic and Molecular Physics, and Optics, 010309 optics, Optics, Brillouin scattering, 0103 physical sciences, Piecewise, Waveform, 0210 nano-technology, business, Frequency modulation, Phase modulation
Abstract: We propose using piecewise parabolic phase modulation of the seed laser for suppressing stimulated Brillouin scattering (SBS) in a fiber amplifier. Simulations are run with a 9 m passive fiber. Compared with random phase modulation and 0-π pseudo-random phase modulation, the piecewise parabolic phase waveform yields a higher SBS threshold per unit bandwidth. If the bandwidth is defined as the range of frequencies containing 85% of the total power, the threshold for parabolic phase modulation is 1.4 times higher than the threshold for the five- or seven-bit pseudo-random modulation format. If the bandwidth is defined more tightly, e.g., the range of frequencies containing 95% of the total power, the threshold for parabolic phase modulation is three times higher. For both cases, achieving a bandwidth of 1.5 GHz requires a maximum phase shift of ~30 radians. All of the waveforms are compared on the basis of the bandwidth required of the phase moduator. The coherence functions are calculated in order to compare their suitability for coherent combining.
Published: 2019

27. The Apache Point Observatory Galactic Evolution Experiment (APOGEE) Spectrographs

Author: W. Richardson, Paul Harding, Paul Maseman, Bo Zhao, Ben Breslauer, A. Uomoto, D. C. Nguyen, Suvrath Mahadevan, Stephen A. Smee, Al Harding, Stephen A. Shectman, Larry N. Carey, R. Stoll, Daniel J. Eisenstein, Joseph Huehnerhoff, J. P. Colque, Michael L. Evans, James W. Davidson, D. Skinner, J. D. Trujillo, Matthew J. Nelson, G. J. Damke, Jon A. Holtzman, Thomas P. O'Brien, J. Karakla, Nicholas MacDonald, Basil Blank, Steve Majewski, Russell Owen, John C. Wilson, B. Anthony-Brumfield, James A. Arns, Matthew Shetrone, T. Mitcheltree, Dmitry Bizyaev, Robert H. Barkhouser, David L. Nidever, José R. Sánchez-Gallego, Conor Sayres, Janice D. R. Dean, Elena Malanushenko, Calen B. Henderson, Samuel Halverson, M. Vernieri, Jeff Crane, Sophia Brunner, E. Walker, Alexandre Roman-Lopes, Mita Tembe, Ricardo P. Schiavon, Stephane Beland, T. Stolberg, Frederick R. Hearty, James E. Gunn, J. Barr, E. Leon, N. De Lee, Michael R. Blanton, S. Melton, Dan Long, Charles R. Lam, Mark A. Klaene, Bruce Gillespie, Erick T. Young, N. Shane, D. Hancock, Rosemarie W. Hammond, J. Matsunari, Alim Y. Patten, Mike Skrutskie, Matthew A. Bershady, David H. Weinberg, George H. Rieke, Marcia J. Rieke, Matthew Hall, K. W. Don, Greg Fitzgerald, Fritz Stauffer, T. Horne, F. Di Mille, Michael A. Carr, Stephen C. Hope, C. Harrison, J. Downey, F. Leger, Andrew J. Burton, Garrett Ebelke, Jennifer Sobeck, and Robert W. O'Connell
Subjects: 010504 meteorology & atmospheric sciences, Red giant, Milky Way, media_common.quotation_subject, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, law.invention, Telescope, law, Observatory, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Spectrograph, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, media_common, Physics, Instrument control, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Galaxy, Space and Planetary Science, Sky, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We describe the design and performance of the near-infrared (1.51--1.70 micron), fiber-fed, multi-object (300 fibers), high resolution (R = lambda/delta lambda ~ 22,500) spectrograph built for the Apache Point Observatory Galactic Evolution Experiment (APOGEE). APOGEE is a survey of ~ 10^5 red giant stars that systematically sampled all Milky Way populations (bulge, disk, and halo) to study the Galaxy's chemical and kinematical history. It was part of the Sloan Digital Sky Survey III (SDSS-III) from 2011 -- 2014 using the 2.5 m Sloan Foundation Telescope at Apache Point Observatory, New Mexico. The APOGEE-2 survey is now using the spectrograph as part of SDSS-IV, as well as a second spectrograph, a close copy of the first, operating at the 2.5 m du Pont Telescope at Las Campanas Observatory in Chile. Although several fiber-fed, multi-object, high resolution spectrographs have been built for visual wavelength spectroscopy, the APOGEE spectrograph is one of the first such instruments built for observations in the near-infrared. The instrument's successful development was enabled by several key innovations, including a "gang connector" to allow simultaneous connections of 300 fibers; hermetically sealed feedthroughs to allow fibers to pass through the cryostat wall continuously; the first cryogenically deployed mosaic volume phase holographic grating; and a large refractive camera that includes mono-crystalline silicon and fused silica elements with diameters as large as ~ 400 mm. This paper contains a comprehensive description of all aspects of the instrument including the fiber system, optics and opto-mechanics, detector arrays, mechanics and cryogenics, instrument control, calibration system, optical performance and stability, lessons learned, and design changes for the second instrument., 81 pages, 67 figures, PASP, accepted
Published: 2019

28. Non-equilibrium fixed points of coupled Ising models

Author: Jeremy T. Young, Alexey V. Gorshkov, Mohammad F. Maghrebi, and Michael Foss-Feig
Subjects: Phase transition, QC1-999, General Physics and Astronomy, Non-equilibrium thermodynamics, FOS: Physical sciences, Fixed point, 01 natural sciences, Article, 010305 fluids & plasmas, 0103 physical sciences, Statistical physics, 010306 general physics, Condensed Matter - Statistical Mechanics, Physics, Quantum Physics, Statistical Mechanics (cond-mat.stat-mech), Statistical Physics, Multicritical point, Renormalization group, Scale invariance, Photonics, Quantum Gases (cond-mat.quant-gas), Ising model, Condensed Matter - Quantum Gases, Quantum Physics (quant-ph), Critical exponent
Abstract: Driven-dissipative systems are expected to give rise to non-equilibrium phenomena that are absent in their equilibrium counterparts. However, phase transitions in these systems generically exhibit an effectively classical equilibrium behavior in spite of their non-equilibrium origin. In this paper, we show that multicritical points in such systems lead to a rich and genuinely non-equilibrium behavior. Specifically, we investigate a driven-dissipative model of interacting bosons that possesses two distinct phase transitions: one from a high- to a low-density phase---reminiscent of a liquid-gas transition---and another to an antiferromagnetic phase. Each phase transition is described by the Ising universality class characterized by an (emergent or microscopic) $\mathbb{Z}_2$ symmetry. They, however, coalesce at a multicritical point, giving rise to a non-equilibrium model of coupled Ising-like order parameters described by a $\mathbb{Z}_2 \times \mathbb{Z}_2$ symmetry. Using a dynamical renormalization-group approach, we show that a pair of non-equilibrium fixed points (NEFPs) emerge that govern the long-distance critical behavior of the system. We elucidate various exotic features of these NEFPs. In particular, we show that a generic continuous scale invariance at criticality is reduced to a discrete scale invariance. This further results in complex-valued critical exponents and spiraling phase boundaries, and it is also accompanied by a complex Liouvillian gap even close to the phase transition. As direct evidence of the non-equilibrium nature of the NEFPs, we show that the fluctuation-dissipation relation is violated at all scales, leading to an effective temperature that becomes "hotter" and "hotter" at longer and longer wavelengths. Finally, we argue that this non-equilibrium behavior can be observed in cavity arrays with cross-Kerr nonlinearities., Comment: 19+11 pages, 7+9 figures
Published: 2019
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29. Identifying features predictive of faculty integrating computation into physics courses

Author: Grant Allen, John M. Aiken, Marcos D. Caballero, Rachel Henderson, and Nicholas T. Young
Subjects: Science instruction, ComputingMilieux_THECOMPUTINGPROFESSION, LC8-6691, 4. Education, Computation, Teaching method, Physics, QC1-999, 05 social sciences, Physics - Physics Education, 050301 education, General Physics and Astronomy, FOS: Physical sciences, 01 natural sciences, Special aspects of education, 010305 fluids & plasmas, Education, Physics Education (physics.ed-ph), 0103 physical sciences, Mathematics education, ComputingMilieux_COMPUTERSANDEDUCATION, 0503 education, Value (mathematics)
Abstract: Computation is a central aspect of 21st century physics practice; it is used to model complicated systems, to simulate impossible experiments, and to analyze mountains of data. Physics departments and their faculty are increasingly recognizing the importance of teaching computation to their students. We recently completed a national survey of faculty in physics departments to understand the state of computational instruction and the factors that underlie that instruction. The data collected from the faculty responding to the survey included a variety of scales, binary questions, and numerical responses. We then used Random Forest, a supervised learning technique, to explore the factors that are most predictive of whether a faculty member decides to include computation in their physics courses. We find that experience using computation with students in their research, or lack thereof and various personal beliefs to be most predictive of a faculty member having experience teaching computation. Interestingly, we find demographic and departmental factors to be less useful factors in our model. The results of this study inform future efforts to promote greater integration of computation into the physics curriculum as well as comment on the current state of computational instruction across the United States.
Published: 2019

30. Stable reconnection at the dusk flank magnetopause

Author: Paul Cassak, K. J. Trattner, Craig J. Pollock, J. Mukherjee, James L. Burch, Sarah K. Vines, S. A. Fuselier, Robert J. Strangeway, S. M. Petrinec, R. G. Gomez, Christopher T. Russell, Roy B. Torbert, D. T. Young, and W. S. Lewis
Subjects: Physics, Flank, 010504 meteorology & atmospheric sciences, Magnetometer, Magnetic reconnection, Geophysics, Plasma, 01 natural sciences, law.invention, Solar wind, Magnetosheath, Physics::Plasma Physics, law, Physics::Space Physics, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, General Earth and Planetary Sciences, Magnetopause, Interplanetary magnetic field, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: The dusk flank magnetopause was surveyed with instruments on board the Magnetospheric Multiscale (MMS) spacecraft on 28 August 2015 between 13:55 UT and 14:15 UT during a period of persistent southward interplanetary magnetic field (IMF) with varying dawn-dusk component. Plasma measurements (500 eV electrons are greater than 2 keV ions) revealed the existence of at least one active reconnection region that persisted throughout the interval. The reconnection region convected equatorward despite the poleward and tailward magnetosheath flow, which ranged from slightly sub-Alfvenic to slightly super-Alfvenic throughout the interval. These results suggest that magnetic reconnection moved in response to changes in the IMF clock angle rather than the magnetosheath flow, which is corroborated using predictions of the maximum magnetic shear model.
Published: 2016

31. Magnetic reconnection and modification of the Hall physics due to cold ions at the magnetopause

Author: John C. Dorelli, Mats André, Göran Marklund, James L. Burch, Christopher T. Russell, Michael O. Chandler, Yoshitaka Saito, T. E. Moore, Per-Arne Lindqvist, Wenya Li, Daniel J. Gershman, William R. Paterson, Cecilia Norgren, Sergio Toledo-Redondo, Andris Vaivads, Barbara L. Giles, Levon A. Avanov, Benoit Lavraud, Robert E. Ergun, D. T. Young, Craig J. Pollock, Werner Magnes, Yuri V. Khotyaintsev, Daniel B. Graham, and Roy Torbert
Subjects: Physics, Ohm's law, 010504 meteorology & atmospheric sciences, Condensed matter physics, Thermal Hall effect, Magnetic reconnection, Electron, 01 natural sciences, symbols.namesake, Geophysics, Physics::Plasma Physics, Hall effect, Electric field, Physics::Space Physics, 0103 physical sciences, symbols, General Earth and Planetary Sciences, Magnetopause, Electric current, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: Observations by the four Magnetospheric Multiscale spacecraft are used to investigate the Hall physics of a magnetopause magnetic reconnection separatrix layer. Inside this layer of currents and st ...
Published: 2016

32. Comparison of Magnetospheric Multiscale ion jet signatures with predicted reconnection site locations at the magnetopause

Author: C. Schiff, W. S. Lewis, Christopher T. Russell, Robert J. Strangeway, Robert E. Ergun, T. D. Phan, R. G. Gomez, Craig J. Pollock, Barry Mauk, D. T. Young, James L. Burch, S. M. Petrinec, K. J. Trattner, and S. A. Fuselier
Subjects: Physics, Jet (fluid), 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Conjunction (astronomy), Magnetosphere, Magnetic reconnection, Plasma, Geophysics, 01 natural sciences, Ion, Solar wind, Physics::Plasma Physics, Physics::Space Physics, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, General Earth and Planetary Sciences, Magnetopause, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: Magnetic reconnection at the Earths magnetopause is the primary process by which solar wind plasma and energy gains access to the magnetosphere. One indication that magnetic reconnection is occurring is the observation of accelerated plasma as a jet tangential to the magnetopause. The direction of ion jets along the magnetopause surface as observed by the Fast Plasma Instrument (FPI) and the Hot Plasma Composition Analyzer (HPCA) instrument on board the recently launched Magnetospheric Multiscale (MMS) set of spacecraft is examined. For those cases where ion jets are clearly discerned, the direction of origin compares well statistically with the predicted location of magnetic reconnection using convected solar wind observations in conjunction with the Maximum Magnetic Shear model.
Published: 2016

33. The response time of the magnetopause reconnection location to changes in the solar wind: MMS case study

Author: Robert E. Ergun, S. A. Fuselier, K. J. Trattner, Craig J. Pollock, Eric Grimes, D. T. Young, T. D. Phan, W. S. Lewis, R. G. Gomez, Frederick Wilder, Barry Mauk, S. M. Petrinec, James L. Burch, and Sarah K. Vines
Subjects: Physics, 010504 meteorology & atmospheric sciences, Field (physics), Magnetosphere, Magnetic reconnection, Geophysics, 01 natural sciences, Nanoflares, Magnetic field, Solar wind, Physics::Space Physics, 0103 physical sciences, General Earth and Planetary Sciences, Magnetopause, Interplanetary magnetic field, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: Reconnection at the Earth's magnetopause is the mechanism by which magnetic fields in different regions change topology to create open magnetic field lines that allow energy, mass, and momentum to flow into the magnetosphere. It is the primary science goal of the recently launched MMS mission to unlock the mechanism of magnetic reconnection with a novel suite of plasma and field instruments. This study investigates several magnetopause crossings in the vicinity of the X-line on 19 September 2015 and compares the observed X-line location with predictions from the Maximum Magnetic Shear model. Rotations of the interplanetary magnetic field OMF) during the magnetopause crossings together with the close proximity of the four MMS satellites are used to determine the response time of the reconnection X-line location to changes in the IMF. The reconnection location exhibits a continuous motion during slow changes in the IMF but a delayed response to sudden changes in the IMF.
Published: 2016

34. Exploration of Configurational and Topological Properties of Minichromosomes using Elastic Energy Optimizations at the DNA Base-Pair Level

Author: Robert T. Young and Wilma K. Olson
Subjects: Physics, Base pair, Biophysics, Elastic energy, Molecular physics
Published: 2020

35. Integration of mathematics and communication in physics-intensive workplaces

Author: Benjamin M. Zwickl, Nicholas T. Young, Anna E. Leak, Kelly Norris Martin, and Brianna Santangelo
Subjects: Physics, Mathematics education, Mathematics
Published: 2018

36. Observed hierarchy of student proficiency with period, frequency, and angular frequency

Author: Andrew F. Heckler and Nicholas T. Young
Subjects: Hierarchy, Angular frequency, LC8-6691, Item analysis, 4. Education, Teaching method, Physics, QC1-999, 05 social sciences, 050301 education, General Physics and Astronomy, Mastery learning, 01 natural sciences, Special aspects of education, Education, Item tree analysis, Categorization, 0103 physical sciences, Mathematics education, ComputingMilieux_COMPUTERSANDEDUCATION, 010306 general physics, 0503 education, Period (music)
Abstract: In the context of a generic harmonic oscillator, we investigated students’ accuracy in determining the period, frequency, and angular frequency from mathematical and graphical representations. In a series of studies including interviews, free response tests, and multiple choice tests developed in an iterative process, we assessed students in both algebra-based and calculus-based, traditionally instructed university-level introductory physics courses. Using the results, we categorized nine skills necessary for proficiency in determining period, frequency, and angular frequency. Overall results reveal that, postinstruction, proficiency is quite low: only about 20%–40% of students mastered most of the nine skills. Next, we used a semiquantitative, intuitive method to investigate the hierarchical structure of the nine skills. We also employed the more formal item tree analysis method to verify this structure and found that the skills form a multilevel, nonlinear hierarchy, with mastery of some skills being prerequisite for mastery in other skills. Finally, we implemented a targeted, 30-min group-work activity to improve proficiency in these skills and found a 1 standard deviation gain in accuracy. Overall, the results suggest that many students currently lack these essential skills, targeted practice may lead to required mastery, and that the observed hierarchical structure in the skills suggests that instruction should especially attend to the skills lower in the hierarchy.
Published: 2018

37. Dissipation-induced dipole blockade and antiblockade in driven Rydberg systems

Author: Elizabeth A. Goldschmidt, T. Boulier, Alexey V. Gorshkov, Jeremy T. Young, Steven L. Rolston, Eric Magnan, James V. Porto, and Ryan Wilson
Subjects: Atomic Physics (physics.atom-ph), Population, FOS: Physical sciences, 01 natural sciences, 010305 fluids & plasmas, Physics - Atomic Physics, symbols.namesake, 0103 physical sciences, Physics::Atomic Physics, 010306 general physics, education, Scaling, Physics, education.field_of_study, Quantum Physics, Rate equation, Dissipation, 3. Good health, Dipole, Quantum Gases (cond-mat.quant-gas), Rydberg atom, Rydberg formula, symbols, Atomic physics, Quantum Physics (quant-ph), Condensed Matter - Quantum Gases, Rabi frequency
Abstract: We study theoretically and experimentally the competing blockade and anti-blockade effects induced by spontaneously generated contaminant Rydberg atoms in driven Rydberg systems. These contaminant atoms provide a source of strong dipole-dipole interactions and play a crucial role in the system's behavior. We study this problem theoretically using two different approaches. The first is a cumulant expansion approximation, in which we ignore third-order and higher connected correlations. Using this approach for the case of resonant drive, a many-body blockade radius picture arises, and we find qualitative agreement with previous experimental results. We further predict that as the atomic density is increased, the Rydberg population's dependence on Rabi frequency will transition from quadratic to linear dependence at lower Rabi frequencies. We study this behavior experimentally by observing this crossover at two different atomic densities. We confirm that the larger density system has a smaller crossover Rabi frequency than the smaller density system. The second theoretical approach is a set of phenomenological inhomogeneous rate equations. We compare the results of our rate equation model to the experimental observations in [E. A. Goldschmidt, et al., PRL 116, 113001 (2016)] and find that these rate equations provide quantitatively good scaling behavior of the steady-state Rydberg population for both resonant and off-resonant drive., 16 pages, 13 figures
Published: 2018
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38. Effect of Tetrameric Base-Pair Context on the Sequence-Dependent Configurations of DNA Minicircles

Author: Pamela J. Perez, Robert T. Young, Wilma K. Olson, Luke Czapla, and Benjamin Cohen
Subjects: Physics, chemistry.chemical_compound, Sequence dependent, chemistry, Base pair, Biophysics, Context (language use), Computational biology, Minicircle, DNA
Published: 2019

39. A Revised Sensitivity Model for Cassini INMS: Results at Titan

Author: Gregory Fletcher, A. Y. Lee, E. L. Patrick, David A. Gell, Brian Magee, D. T. Young, Rebecca Perryman, J. Grimes, Wayne Kasprzak, Greg Miller, Hasso B. Niemann, B. D. Teolis, Véronique Vuitton, Roger V. Yelle, Jared Bell, Kathleen Mandt, F. J. Pelletier, and J. H. Waite
Subjects: Physics, Spacecraft, business.industry, Monte Carlo method, Detector, Astronomy and Astrophysics, Atmospheric sciences, Computational physics, Ion, Constant factor, symbols.namesake, Planetary science, Space and Planetary Science, symbols, Enceladus, Titan (rocket family), business
Abstract: Cassini Ion Neutral Mass Spectrometer (INMS) measurements from roughly a hundred Titan encounters over the Cassini mission yield neutral and ion densities systematically lower, by factors approximately 2 to 3, than estimates from several other spacecraft systems, including the Attitude and Articulation Control System, and Navigation system. In this paper we present a new INMS instrument sensitivity model, obtained by re-analyzing (1) the capture and transmission of neutral gas through the instrument, and (2) the detector gain reduction during pre-launch testing. By correcting for an under-estimation of gas leakage out of the instrument into space by the original calibration model, and adjusting for the gain change, the new model brings INMS densities into much closer agreement with the other Cassini systems. Accordingly, the INMS ion densities are revised upward by a constant detector sensitivity correction factor of 1.55±21 %, while the neutral sensitivities have a complex instrument pointing direction dependence, due (mostly) to the effect of the INMS vent and antechamber-to-closed source tube. In the special case of on-ram pointing the neutral densities are revised upward by a constant factor of 2.2±23 %. The corrected neutral and ion sensitivities given here are applicable to all previously published INMS results at Titan, Enceladus and elsewhere in the Saturn system. The new model gives reliable densities at high ram angles, in some cases above 90 degrees, thereby expanding the list of Titan flybys from which INMS densities may be extracted. We apply the model to obtain accurate densities from several off-ram Titan flybys which gave unusual neutral density vs. altitude profiles, or unreasonably high densities, with the original calibration.
Published: 2015

40. Fast Quantum State Transfer and Entanglement Renormalization Using Long-Range Interactions

Author: Michael Foss-Feig, Zhe-Xuan Gong, Ali Hamed Moosavian, Jeremy T. Young, Zachary Eldredge, and Alexey V. Gorshkov
Subjects: Physics, Quantum Physics, Degree (graph theory), Atomic Physics (physics.atom-ph), FOS: Physical sciences, General Physics and Astronomy, Quantum entanglement, State (functional analysis), 01 natural sciences, Upper and lower bounds, Article, Physics - Atomic Physics, 010305 fluids & plasmas, Renormalization, Quantum state, Quantum mechanics, 0103 physical sciences, Tensor, Quantum Physics (quant-ph), 010306 general physics, Ansatz
Abstract: In short-range interacting systems, the speed at which entanglement can be established between two separated points is limited by a constant Lieb-Robinson velocity. Long-range interacting systems are capable of faster entanglement generation, but the degree of the speed-up possible is an open question. In this paper, we present a protocol capable of transferring a quantum state across a distance $L$ in $d$ dimensions using long-range interactions with strength bounded by $1/r^\alpha$. If $\alpha < d$, the state transfer time is asymptotically independent of $L$; if $\alpha = d$, the time is logarithmic in distance $L$; if $d < \alpha < d+1$, transfer occurs in time proportional to $L^{\alpha - d}$; and if $\alpha \geq d + 1$, it occurs in time proportional to $L$. We then use this protocol to upper bound the time required to create a state specified by a MERA (multiscale entanglement renormalization ansatz) tensor network, and show that, if the linear size of the MERA state is $L$, then it can be created in time that scales with $L$ identically to state transfer up to multiplicative logarithmic corrections., Comment: 6 pages, 4 figures
Published: 2017

41. Dynamics robustness of cascading systems

Author: Jonathan T. Young, Tetsuhiro S. Hatakeyama, and Kunihiko Kaneko
Subjects: 0301 basic medicine, Proteome, Computer science, Biochemistry, Systems Science, 0302 clinical medicine, Cell Signaling, Invariant (mathematics), Post-Translational Modification, Phosphorylation, lcsh:QH301-705.5, Ecology, Protein Kinase Signaling Cascade, Physics, Invariant (physics), Signaling Cascades, Dynamical Systems, Enzymes, Computational Theory and Mathematics, Cascade, Modeling and Simulation, Physical Sciences, Response Duration, Biological system, Network Analysis, Research Article, Signal Transduction, Computer and Information Sciences, MAPK signaling cascades, Dynamical systems theory, Systems biology, ENCODE, Models, Biological, Cell Physiological Phenomena, 03 medical and health sciences, Cellular and Molecular Neuroscience, Robustness (computer science), Multienzyme Complexes, Genetics, Animals, Humans, Computer Simulation, Kinase activity, Molecular Biology, Temporal information, Relaxation (Physics), Ecology, Evolution, Behavior and Systematics, Simulation, Homeorhesis, Phosphatases, Biology and Life Sciences, Proteins, Cell Biology, Signaling Networks, 030104 developmental biology, lcsh:Biology (General), Enzymology, 030217 neurology & neurosurgery, Mathematics
Abstract: A most important property of biochemical systems is robustness. Static robustness, e.g., homeostasis, is the insensitivity of a state against perturbations, whereas dynamics robustness, e.g., homeorhesis, is the insensitivity of a dynamic process. In contrast to the extensively studied static robustness, dynamics robustness, i.e., how a system creates an invariant temporal profile against perturbations, is little explored despite transient dynamics being crucial for cellular fates and are reported to be robust experimentally. For example, the duration of a stimulus elicits different phenotypic responses, and signaling networks process and encode temporal information. Hence, robustness in time courses will be necessary for functional biochemical networks. Based on dynamical systems theory, we uncovered a general mechanism to achieve dynamics robustness. Using a three-stage linear signaling cascade as an example, we found that the temporal profiles and response duration post-stimulus is robust to perturbations against certain parameters. Then analyzing the linearized model, we elucidated the criteria of when signaling cascades will display dynamics robustness. We found that changes in the upstream modules are masked in the cascade, and that the response duration is mainly controlled by the rate-limiting module and organization of the cascade’s kinetics. Specifically, we found two necessary conditions for dynamics robustness in signaling cascades: 1) Constraint on the rate-limiting process: The phosphatase activity in the perturbed module is not the slowest. 2) Constraints on the initial conditions: The kinase activity needs to be fast enough such that each module is saturated even with fast phosphatase activity and upstream changes are attenuated. We discussed the relevance of such robustness to several biological examples and the validity of the above conditions therein. Given the applicability of dynamics robustness to a variety of systems, it will provide a general basis for how biological systems function dynamically., Author summary Cells use signaling pathways to transmit information received on its membrane to DNA, and many important cellular processes are tied to signaling networks. Past experiments have shown that cells’ internal signaling networks are sophisticated enough to process and encode temporal information such as the length of time a ligand is bound to a receptor. However, little research has been done to verify whether information encoded onto temporal profiles can be made robust. We examined mathematical models of linear signaling networks and found that the relaxation of the response to a transient stimuli can be made robust to certain parameter fluctuations. Robustness is a key concept in biological systems—it would be disastrous if a cell could not operate if there was a slight change in its environment or physiology. Our research shows that such dynamics robustness is a property of linear signaling cascades, and we outline the design principles needed to generate such robustness. We discovered that two conditions regarding the speed of the internal chemical reactions and concentration levels are needed to generate dynamics robustness.
Published: 2017

42. Cold Ionospheric Ions in the Magnetic Reconnection Outflow Region

Author: Per-Arne Lindqvist, Cunguo Wang, Thomas E. Moore, Binbin Tang, Yuri V. Khotyaintsev, Michael O. Chandler, James L. Burch, Cecilia Norgren, Roy Torbert, S. A. Fuselier, Drew Turner, Wenya Li, Barbara L. Giles, D. T. Young, Christopher T. Russell, Mats André, Benoit Lavraud, Daniel B. Graham, Sergio Toledo-Redondo, Robert E. Ergun, Andris Vaivads, Craig J. Pollock, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, cold ion, reconnection outflow, 010504 meteorology & atmospheric sciences, Magnetic reconnection, Plasma, Geophysics, 01 natural sciences, MMS, Physics::Geophysics, Ion, Magnetosheath, Space and Planetary Science, Physics::Plasma Physics, [SDU]Sciences of the Universe [physics], 0103 physical sciences, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Magnetopause, Outflow, Astrophysics::Earth and Planetary Astrophysics, Ionosphere, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: International audience; Magnetosheath plasma usually determines properties of asymmetric magnetic reconnection at the subsolar region of Earth's magnetopause. However, cold plasma that originated from the ionosphere can also reach the magnetopause and modify the kinetic physics of asymmetric reconnection. We present a magnetopause crossing with high-density (10-60 cm-3) cold ions and ongoing reconnection from the observation of the Magnetospheric Multiscale (MMS) spacecraft. The magnetopause crossing is estimated to be 300 ion inertial lengths south of the X line. Two distinct ion populations are observed on the magnetosheath edge of the ion jet. One population with high parallel velocities (200-300 km/s) is identified to be cold ion beams, and the other population is the magnetosheath ions. In the deHoffman-Teller frame, the field-aligned magnetosheath ions are Alfvénic and move toward the jet region, while the field-aligned cold ion beams move toward the magnetosheath boundary layer, with much lower speeds. These cold ion beams are suggested to be from the cold ions entering the jet close to the X line. This is the first observation of the cold ionospheric ions in the reconnection outflow region, including the reconnection jet and the magnetosheath boundary layer.
Published: 2017

43. A solvable family of driven-dissipative many-body systems

Author: Michael Foss-Feig, Victor V. Albert, Mohammad F. Maghrebi, Jeremy T. Young, and Alexey V. Gorshkov
Subjects: Thermal equilibrium, Physics, Quantum Physics, Quantum decoherence, General Physics and Astronomy, Non-equilibrium thermodynamics, FOS: Physical sciences, 01 natural sciences, Article, 010305 fluids & plasmas, symbols.namesake, Classical mechanics, Quantum Gases (cond-mat.quant-gas), Quantum mechanics, 0103 physical sciences, Rydberg atom, Dissipative system, symbols, Ising model, Condensed Matter - Quantum Gases, 010306 general physics, Hamiltonian (quantum mechanics), Quantum Physics (quant-ph), Quantum computer
Abstract: Exactly solvable models have played an important role in establishing the sophisticated modern understanding of equilibrium many-body physics. And conversely, the relative scarcity of solutions for non-equilibrium models greatly limits our understanding of systems away from thermal equilibrium. We study a family of non-equilibrium models, some of which can be viewed as dissipative analogues of the transverse-field Ising model, in that an effectively classical Hamiltonian is frustrated by dissipative processes that drive the system toward states that do not commute with the Hamiltonian. Surprisingly, a broad and experimentally relevant subset of these models can be solved efficiently in any number of spatial dimensions. We leverage these solutions to prove a no-go theorem on steady-state phase transitions in a many-body model that can be realized naturally with Rydberg atoms or trapped ions, and to compute the effects of decoherence on a canonical trapped-ion-based quantum computation architecture., Comment: 8 pages, 3 figures
Published: 2017
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44. The Effect of Atmospheric Cooling on Vertical Velocity Dispersion and Density Distribution of Brown Dwarfs

Author: Sarah J. Schmidt, Nimish P. Hathi, Erick T. Young, Seth H. Cohen, Nor Pirzkal, Russell E. Ryan, Rogier A. Windhorst, Paul Thorman, Jonathan I. Lunine, Benne W. Holwerda, Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Milky Way, Brown dwarf, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Galaxy: disk, Mass transfer, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Disc, Galaxy: structure, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], Astronomy and Astrophysics, Scale height, Astrophysics - Astrophysics of Galaxies, Galaxy, Stars, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics::Earth and Planetary Astrophysics, Dispersion (chemistry), stars: mass-loss, brown dwarfs
Abstract: We present a Monte Carlo simulation designed to predict the vertical velocity dispersion of brown dwarfs in the Milky Way. We show that since these stars are constantly cooling, the velocity dispersion has a noticeable trend with spectral type. With realistic assumptions for the initial-mass function, star-formation history, and the cooling models, we show that the velocity dispersion is roughly consistent with what is observed for M dwarfs, decreases to cooler spectral types, and increases again for the coolest types in our study ($\sim$T9). We predict a minimum in the velocity dispersions for L/T transition objects, however the detailed properties of the minimum predominately depend on the star-formation history. Since this trend is due to brown dwarf cooling, we expect the velocity dispersion as a function of spectral type should deviate from constancy around the hydrogen-burning limit. We convert from velocity dispersion to vertical scale height using standard disk models, and present similar trends in disk thickness as a function of spectral type. We suggest that future, wide-field photometric and/or spectroscopic missions may collect sizable samples of distant ($\sim\!1$ kpc) of dwarfs that span the hydrogen-burning limit. As such, we speculate that such observations may provide a unique way of constraining the average spectral type of hydrogen-burning., 12 pages, 6 figures, 2 tables. Accepted to ApJ
Published: 2017

45. Topology of spin meron pairs in coupled Ni/Fe/Co/Cu(001) disks

Author: A. T. Young, J. Li, Elke Arenholz, Andreas Scholl, Qian Li, A. Tan, Chanyong Hwang, and Z. Q. Qiu
Subjects: Physics, Meron, High Energy Physics::Lattice, Skyrmion, Fluids & Plasmas, 02 engineering and technology, Condensed Matter::Mesoscopic Systems and Quantum Hall Effect, 021001 nanoscience & nanotechnology, Topology, 01 natural sciences, Helicity, Inductive coupling, Vortex, Engineering, Pairing, 0103 physical sciences, Physical Sciences, Chemical Sciences, 010306 general physics, 0210 nano-technology, Topological quantum number, Spin-½
Abstract: The meron is a special topological object that carries only one-half of the topological charge unit. In condensed matter physics, a spin meron corresponds to one-half of a spin skyrmion. As compared to the many fascinating topological properties of skyrmion materials, little is known of the properties of spin merons especially about their formation. It was confirmed only recently that hedgehog merons could exist in pairs with opposite helicities via a spin flux closure. However, it is unclear whether a single hedgehog meron could ever exist by pairing with another type of meron. Using element-resolved magnetic imaging measurements on epitaxial trilayer disks, we show that a spin meron with a full range of helicity, including the hedgehog meron, can be stabilized by pairing with another vortex meron with a fine tuning of the magnetic coupling between the two merons. Furthermore, the meron divergence is fully controlled by the polarity of the vortex meron, independent of the vortex helicity.
Published: 2016

46. Electron-scale measurements of magnetic reconnection in space

Author: Rumi Nakamura, Drew Turner, Michael Shay, Yu. V. Khotyaintsev, J. F. Fennell, K. A. Goodrich, Ian J. Cohen, Michael O. Chandler, Per-Arne Lindqvist, Göran Marklund, Klaus Torkar, Shan Wang, Martin V. Goldman, Allison Jaynes, J. H. Clemmons, James Drake, D. T. Young, J. B. Blake, Daniel J. Gershman, K. J. Trattner, M. Steller, S. M. Petrinec, Frederick Wilder, Barry Mauk, Tai Phan, Wolfgang Baumjohann, John C. Dorelli, Jonathan Eastwood, Levon A. Avanov, Yoshifumi Saito, Benoit Lavraud, Matthew R. Argall, T. E. Moore, L. J Chen, Jerry Goldstein, David Newman, Mitsuo Oka, Craig J. Pollock, James L. Burch, Christopher T. Russell, Robert E. Ergun, Michael Hesse, Patricia H. Reiff, Roy B. Torbert, Daniel N. Baker, Stephen A. Fuselier, W. S. Lewis, Barbara L. Giles, Paul Cassak, Robert J. Strangeway, Werner Magnes, Victoria N. Coffey, Science and Technology Facilities Council (STFC), and Science and Technology Facilities Council [2006-2012]
Subjects: 010504 meteorology & atmospheric sciences, General Science & Technology, Magnetosphere, Astrophysics, ACCELERATION, 01 natural sciences, Physics::Plasma Physics, DIFFUSION REGION, 0103 physical sciences, EARTHS MAGNETOPAUSE, Interplanetary magnetic field, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, MULTISCALE MMS MISSION, Physics, Science & Technology, Multidisciplinary, Magnetic energy, Demagnetizing field, Magnetic reconnection, MAGNETOSPHERIC MULTISCALE, Magnetic field, Computational physics, Multidisciplinary Sciences, Physics::Space Physics, Science & Technology - Other Topics, Astrophysical plasma, Magnetospheric Multiscale Mission
Abstract: 著者人数: 52名, 資料番号: SA1160034000
Published: 2016

47. Emergent equilibrium in many-body optical bistability

Author: Alexey V. Gorshkov, Jeremy T. Young, Pradeep Niroula, Mohammad F. Maghrebi, Mohammad Hafezi, Ryan Wilson, and Michael Foss-Feig
Subjects: Quantum optics, Physics, Collective behavior, Phase transition, Quantum Physics, Quantum dynamics, FOS: Physical sciences, Observable, 01 natural sciences, Article, 010305 fluids & plasmas, Optical bistability, symbols.namesake, Quantum Gases (cond-mat.quant-gas), 0103 physical sciences, Rydberg formula, symbols, Ising model, Statistical physics, 010306 general physics, Condensed Matter - Quantum Gases, Quantum Physics (quant-ph)
Abstract: Many-body systems constructed of quantum-optical building blocks can now be realized in experimental platforms ranging from exciton-polariton fluids to ultracold gases of Rydberg atoms, establishing a fascinating interface between traditional many-body physics and the driven-dissipative, non-equilibrium setting of cavity-QED. At this interface, the standard techniques and intuitions of both fields are called into question, obscuring issues as fundamental as the role of fluctuations, dimensionality, and symmetry on the nature of collective behavior and phase transitions. Here, we study the driven-dissipative Bose-Hubbard model, a minimal description of numerous atomic, optical, and solid-state systems in which particle loss is countered by coherent driving. Despite being a lattice version of optical bistability---a foundational and patently non-equilibrium model of cavity-QED---the steady state possesses an emergent equilibrium description in terms of a classical Ising model. We establish this picture by identifying a limit in which the quantum dynamics is asymptotically equivalent to non-equilibrium Langevin equations, which support a phase transition described by model A of the Hohenberg-Halperin classification. Numerical simulations of the Langevin equations corroborate this picture, producing results consistent with the behavior of a finite-temperature Ising model., Comment: 11 pages + appendices, 8 figures
Published: 2016
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48. Protoplanetary and Transitional Disks in the Open Stellar Cluster IC 2395

Author: George H. Rieke, Cameron P. M. Bell, Nick Siegler, Erick T. Young, Andras Gaspar, Jozsef Vinko, Zoltan Balog, Kate Y. L. Su, Robert A. Gutermuth, James Muzerolle, and László L. Kiss
Subjects: Physics, ComputingMilieux_THECOMPUTINGPROFESSION, 010504 meteorology & atmospheric sciences, Foundation (engineering), Astronomy, FOS: Physical sciences, ComputerApplications_COMPUTERSINOTHERSYSTEMS, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, 01 natural sciences, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), 0103 physical sciences, ComputingMilieux_COMPUTERSANDEDUCATION, Cluster (physics), 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), 0105 earth and related environmental sciences
Abstract: We present new deep UBVRI images and high-resolution multi-object optical spectroscopy of the young (~ 6 - 10 Myr old), relatively nearby (800 pc) open cluster IC 2395. We identify nearly 300 cluster members and use the photometry to estimate their spectral types, which extend from early B to middle M. We also present an infrared imaging survey of the central region using the IRAC and MIPS instruments on board the Spitzer Space Telescope, covering the wavelength range from 3.6 to 24 microns. Our infrared observations allow us to detect dust in circumstellar disks originating over a typical range of radii ~ 0.1 to ~ 10AU from the central star. We identify 18 Class II, 8 transitional disk, and 23 debris disk candidates, respectively 6.5%, 2.9%, and 8.3% of the cluster members with appropriate data. We apply the same criteria for transitional disk identification to 19 other stellar clusters and associations spanning ages from ~ 1 to ~ 18 Myr. We find that the number of disks in the transitional phase as a fraction of the total with strong 24 micron excesses ([8] - [24] > 1.5) increases from 8.4 +\- 1.3% at ~ 3 Myr to 46 +\- 5% at ~ 10 Myr. Alternative definitions of transitional disks will yield different percentages but should show the same trend., accepted by the Astrophysical Journal
Published: 2016
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49. Analysis of energetic electron drop-outs in the upper atmosphere of Titan during flybys in the dayside magnetosphere of Saturn

Author: Markus Fränz, D. G. Mitchell, Zoltán Németh, G. Erdos, M. K. Dougherty, Norbert Krupp, Karoly Szego, D. T. Young, Stamatios M. Krimigis, and Z. Bebesi
Subjects: Physics, Magnetosphere, Astronomy and Astrophysics, Electron, Astrophysics, Charged particle, Astrobiology, symbols.namesake, Space and Planetary Science, Local time, Physics::Space Physics, symbols, Magnetopause, Astrophysics::Earth and Planetary Astrophysics, Atmosphere of Titan, Ionosphere, Titan (rocket family)
Abstract: We discuss the high energy electron absorption signatures at Titan during the Cassini dayside magnetospheric encounters. We use the electron measurements of the Low Energy Measurement System of the Magnetospheric Imaging Instrument. We also examine the mass loading boundary based on the ion data of the Ion Mass Spectrometer sensor of the Cassini Plasma Spectrometer. The dynamic motion of the Kronian magnetopause and the periodic charged particle flux and magnetic field variations – associated with the magnetodisk of Saturn – of the subcorotating magnetospheric plasma creates a unique and complex environment at Titan. Most of the analysed flybys (like T25–T33 and T35–T51) cluster at similar Saturn Local Time positions. However the instantaneous direction of the incoming magnetospheric particles may change significantly from flyby to flyby due to the very different magnetospheric field conditions which are found upstream of Titan within the sets of encounters. The energetic magnetospheric electrons gyrate along the magnetic field lines of Saturn, and at the same time bounce between the mirror points of the magnetosphere. This motion is combined with the drift of the magnetic field lines. When these flux tubes interact with the upper atmosphere of Titan, their content is depleted over approximately an electron bounce period. These depletion signatures are observed as sudden drop-outs of the electron fluxes. We examined the altitude distribution of these drop-outs and concluded that these mostly detected in the exo-ionosphere of Titan and sometimes within the ionosphere. However there is a relatively significant scatter in the orbit to orbit data, which can be attributed to the which can be attributed to the variability of the plasma environment and as a consequence, the induced magnetosphere of Titan. A weak trend between the incoming electron fluxes and the measured drop-out altitudes has also been observed.
Published: 2012

50. Computing in Thermal Equilibrium With Dipole-Coupled Nanomagnets

Author: Paul D. Ashby, Brian Lambson, A. T. Young, Jeffrey Bokor, Andreas Scholl, Eduard Tuchfeld, David Carlton, and Scott Dhuey
Subjects: Thermal equilibrium, Physics, Work (thermodynamics), business.industry, Electrical engineering, Computer Science Applications, Magnetic field, Computational physics, Dipole, Logic gate, Thermal, Digital signal, Electrical and Electronic Engineering, business, Micromagnetics
Abstract: In the 1970s, work at IBM by Charles Bennett suggested the possibility of a computer operating near thermal equilibrium and dissipating energy near the thermodynamic limits. Here, we demonstrate experimentally that a computing architecture based on dipole-coupled nanomagnets can operate near thermal equilibrium without the assistance of externally applied magnetic fields. The dynamics of digital signal propagation is demonstrated with micromagnetic simulation and then verified experimentally using time-lapse photoemission electron microscopy. A logic gate that computes using energy from the thermal bath without external fields is also demonstrated. Nanomagnetic logic circuits operating under these conditions are expected to dissipate energy near the fundamental thermodynamic limits of computation.
Published: 2011

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