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1. High-energy and ultra-high-energy neutrinos: A Snowmass white paper

Author

Ackermann, Markus, Bustamante, Mauricio, Lu, Lu, Otte, Nepomuk, Reno, Mary Hall, Wissel, Stephanie, Agarwalla, Sanjib K., Alvarez-Muñiz, Jaime, Alves Batista, Rafael, Argüelles, Carlos A., Clark, Brian A., Cummings, Austin, Das, Sudipta, Decoene, Valentin, Denton, Peter B., Dornic, Damien, Dzhilkibaev, Zhan-Arys, Farzan, Yasaman, Garcia, Alfonso, Garzelli, Maria Vittoria, Glaser, Christian, Heijboer, Aart, Hörandel, Jörg R., Illuminati, Giulia, Seon Jeong, Yu, Kelley, John L., Kelly, Kevin J., Kheirandish, Ali, Klein, Spencer R., Krizmanic, John F., Larson, Michael J., Murase, Kohta, Narang, Ashish, Prechelt, Remy L., Prohira, Steven, Resconi, Elisa, Santander, Marcos, Valera, Victor B., Vandenbroucke, Justin, Vasil'evna Suvorova, Olga, Wiencke, Lawrence, Yoshida, Shigeru, Yuan, Tianlu, Zas, Enrique, Zhelnin, Pavel, Zhou, Bei, Anchordoqui, Luis A., Ashida, Yosuke, Bagheri, Mahdi, Balagopal, Aswathi, V, Basu, Vedant, Beatty, James, Bechtol, Keith, Bell, Nicole, Bishop, Abigail, Book, Julia, Brown, Anthony, Burgman, Alexander, Campana, Michael, Chau, Nhan, Chen, Thomas Y., Coleman, Alan, Connolly, Amy, Conrad, Janet M., Correa, Pablo, Creque-Sarbinowski, Cyril, Curtis-Ginsberg, Zachary, Dasgupta, Paramita, De Kockere, Simon, de Vries, Krijn, Deaconu, Cosmin, Desai, Abhishek, DeYoung, Tyce, di Matteo, Armando, Elsaesser, Dominik, Fürst, Phillip, Fan, Kwok Lung, Fedynitch, Anatoli, Fox, Derek, Ganster, Erik, Minh, Martin Ha, Haack, Christian, Hallman, Steffen, Halzen, Francis, Haungs, Andreas, Ishihara, Aya, Judd, Eleanor, Karg, Timo, Karle, Albrecht, Katori, Teppei, Kochocki, Alina, Kopper, Claudio, Kowalski, Marek, Kravchenko, Ilya, Kurahashi, Naoko, Lamoureux, Mathieu, León Vargas, Hermes, Lincetto, Massimiliano, Liu, Qinrui, Madsen, Jim, Makino, Yuya, Mammo, Joseph, Marka, Zsuzsa, Mayotte, Eric, Meagher, Kevin, Meier, Maximilian, Miramonti, Lino, Moulai, Marjon, Mulrey, Katharine, Muzio, Marco, Naab, Richard, Nelles, Anna, Nichols, William, Nozdrina, Alisa, O'Sullivan, Erin, OD́ell, Vivian, Osborne, Jesse, Pandey, Vishvas, Paudel, Ek Narayan, Pizzuto, Alex, Plum, Mattias, Pobes Aranda, Carlos, Pyras, Lilly, Raab, Christoph, Rechav, Zoe, Rojo, Juan, Romero Matamala, Oscar, Savina, Pierpaolo, Schroeder, Frank, Schumacher, Lisa, Sciutto, Sergio, Sclafani, Stephen, Ful Hossain Seikh, Mohammad, Silva, Manuel, Singh, Rajeev, Smith, Daniel, Spencer, Samuel Timothy, Springer, Robert Wayne, Stachurska, Juliana, Suvorova, Olga, Taboada, Ignacio, Toscano, Simona, Tueros, Matias, Twagirayezu, Jean Pierre, van Eijndhoven, Nick, Veres, Péter, Vieregg, Abigail, Wang, Winnie, Whitehorn, Nathan, Winter, Walter, Yildizci, Emre, and Yu, Shiqi

Published
2022
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2. In-situ estimation of ice crystal properties at the South Pole using LED calibration data from the IceCube Neutrino Observatory

Author

Abbasi, Rasha, Ackermann, Markus, Adams, Jenni, Aggarwal, Nakul, Aguilar, Juanan, Ahlers, Markus, Ahrens, Maryon, Alameddine, Jean-Marco, Alves Junior, Antonio Augusto, Amin, Najia Moureen Binte, Andeen, Karen, Anderson, Tyler, Anton, Gisela, Argüelles, Carlos, Ashida, Yosuke, Athanasiadou, Sofia, Axani, Spencer, Bai, Xinhua, Balagopal V, Aswathi, Baricevic, Moreno, Barwick, Steve, Basu, Vedant, Bay, Ryan, Beatty, James, Becker, Karl Heinz, Becker Tjus, Julia, Beise, Jakob, Bellenghi, Chiara, Benda, Samuel, BenZvi, Segev, Berley, David, Bernardini, Elisa, Besson, Dave, Binder, Gary, Bindig, Daniel, Blaufuss, Erik, Blot, Summer, Bontempo, Federico, Book, Julia, Borowka, Jürgen, Boscolo Meneguolo, Caterina, Böser, Sebastian, Botner, Olga, Böttcher, Jakob, Bourbeau, Etienne, Braun, Jim, Brinson, Bennett, Brostean-Kaiser, Jannes, Burley, Ryan, Busse, Raffaela, Campana, Michael, Carnie-Bronca, Erin, Chen, Chujie, Chen, Zheyang, Chirkin, Dmitry, Choi, Koun, Clark, Brian, Classen, Lew, Coleman, Alan, Collin, Gabriel, Connolly, Amy, Conrad, Janet, Coppin, Paul, Correa, Pablo, Countryman, Stefan, Cowen, Doug, Cross, Robert, Dappen, Christian, Dave, Pranav, De Clercq, Catherine, DeLaunay, James, Delgado López, Diyaselis, Dembinski, Hans, Deoskar, Kunal, Desai, Abhishek, Desiati, Paolo, de Vries, Krijn, de Wasseige, Gwenhael, DeYoung, Tyce, Diaz, Alejandro, Díaz-Vélez, Juan Carlos, Dittmer, Markus, Dujmovic, Hrvoje, DuVernois, Michael, Ehrhardt, Thomas, Eller, Philipp, Engel, Ralph, Erpenbeck, Hannah, Evans, John, Evenson, Paul, Fan, Kwok Lung, Fazely, Ali, Fedynitch, Anatoli, Feigl, Nora, Fiedlschuster, Sebastian, Fienberg, Aaron, Finley, Chad, Fischer, Leander, Fox, Derek, Franckowiak, Anna, Friedman, Elizabeth, Fritz, Alexander, Fürst, Philipp, Gaisser, Tom, Gallagher, Jay, Ganster, Erik, Garcia, Alfonso, Garrappa, Simone, Gerhardt, Lisa, Ghadimi, Ava, Glaser, Christian, Glüsenkamp, Thorsten, Glauch, Theo, Goehlke, Noah, Gonzalez, Javier, Goswami, Sreetama, Grant, Darren, Gray, Shannon, Grégoire, Timothée, Griswold, Spencer, Günther, Christoph, Gutjahr, Pascal, Haack, Christian, Hallgren, Allan, Halliday, Robert, Halve, Lasse, Halzen, Francis, Hamdaoui, Hassane, Ha Minh, Martin, Hanson, Kael, Hardin, John, Harnisch, Alexander, Hatch, Patrick, Haungs, Andreas, Helbing, Klaus, Hellrung, Jonas, Henningsen, Felix, Heuermann, Lars, Hickford, Stephanie, Hill, Colton, Hill, Gary, Hoffman, Kara, Hoshina, Kotoyo, Hou, Wenjie, Huber, Thomas, Hultqvist, Klas, Hünnefeld, Mirco, Hussain, Raamis, Hymon, Karolin, In, Seongjin, Iovine, Nadege, Ishihara, Aya, Jansson, Matti, Japaridze, George, Jeong, Minjin, Jin, Miaochen, Jones, Ben, Kang, Donghwa, Kang, Woosik, Kang, Xinyue, Kappes, Alexander, Kappesser, David, Kardum, Leonora, Karg, Timo, Karl, Martina, Karle, Albrecht, Katz, Uli, Kauer, Matt, Kelley, John, Kheirandish, Ali, Kin, Ken'ichi, Kiryluk, Joanna, Klein, Spencer, Kochocki, Alina, Koirala, Ramesh, Kolanoski, Hermann, Kontrimas, Tomas, Köpke, Lutz, Kopper, Claudio, Koskinen, Jason, Koundal, Paras, Kovacevich, Michael, Kowalski, Marek, Kozynets, Tetiana, Krupczak, Emmett, Kun, Emma, Kurahashi, Naoko, Lad, Neha, Lagunas Gualda, Cristina, Larson, Michael, Lauber, Frederik, Lazar, Jeffrey, Lee, Jiwoong, Leonard, Kayla, Leszczyńska, Agnieszka, Lincetto, Massimiliano, Liu, Qinrui, Liubarska, Maria, Lohfink, Elisa, Love, Christina, Lozano Mariscal, Cristian Jesus, Lu, Lu, Lucarelli, Francesco, Ludwig, Andrew, Luszczak, William, Lyu, Yang, Ma, Wing Yan, Madsen, Jim, Mahn, Kendall, Makino, Yuya, Mancina, Sarah, Marie Sainte, Wenceslas, Mariş, Ioana, Marka, Szabolcs, Marka, Zsuzsa, Marsee, Matthew, Martinez-Soler, Ivan, Maruyama, Reina, McElroy, Thomas, McNally, Frank, Mead, James Vincent, Meagher, Kevin, Mechbal, Sarah, Medina, Andres, Meier, Maximilian, Meighen-Berger, Stephan, Merckx, Yarno, Micallef, Jessie, Mockler, Daniela, Montaruli, Teresa, Moore, Roger, Morse, Bob, Moulai, Marjon, Mukherjee, Tista, Naab, Richard, Nagai, Ryo, Naumann, Uwe, Nayerhoda, Amid, Necker, Jannis, Neumann, Miriam, Niederhausen, Hans, Nisa, Mehr, Nowicki, Sarah, Obertacke Pollmann, Anna, Oehler, Marie, Oeyen, Bob, Olivas, Alex, Orsoe, Rasmus, Osborn, Jesse, O'Sullivan, Erin, Pandya, Hershal, Pankova, Daria, Park, Nahee, Parker, Grant, Paudel, Ek Narayan, Paul, Larissa, Pérez de los Heros, Carlos, Peters, Lilly, Peterson, Josh, Philippen, Saskia, Pieper, Sarah, Pizzuto, Alex, Plum, Matthias, Popovych, Yuiry, Porcelli, Alessio, Prado Rodriguez, Maria, Pries, Brandon, Procter-Murphy, Rachel, Przybylski, Gerald, Raab, Christoph, Rack-Helleis, John, Rameez, Mohamed, Rawlins, Katherine, Rechav, Zoe, Rehman, Abdul, Reichherzer, Patrick, Renzi, Giovanni, Resconi, Elisa, Reusch, Simeon, Rhode, Wolfgang, Richman, Mike, Riedel, Benedikt, Roberts, Ella, Robertson, Sally, Rodan, Steven, Roellinghoff, Gerrit, Rongen, Martin, Rott, Carsten, Ruhe, Tim, Ruohan, Li, Ryckbosch, Dirk, Rysewyk Cantu, Devyn, Safa, Ibrahim, Saffer, Julian, Salazar-Gallegos, Daniel, Sampathkumar, Pranav, Sanchez Herrera, Sebastian, Sandrock, Alexander, Santander, Marcos, Sarkar, Sourav, Sarkar, Subir, Schaufel, Merlin, Schieler, Harald, Schindler, Sebastian, Schlüter, Berit, Schmidt, Torsten, Schneider, Judith, Schröder, Frank, Schumacher, Lisa, Schwefer, Georg, Sclafani, Steve, Seckel, Dave, Seunarine, Surujhdeo, Sharma, Ankur, Shefali, Shefali, Shimizu, Nobuhiro, Silva, Manuel, Skrzypek, Barbara, Smithers, Ben, Snihur, Robert, Soedingrekso, Jan, Søgaard, Andreas, Soldin, Dennis, Spannfellner, Christian, Spiczak, Glenn, Spiering, Christian, Stamatikos, Michael, Stanev, Todor, Stein, Robert, Stezelberger, Thorsten, Stürwald, Timo, Stuttard, Thomas, Sullivan, Greg, Taboada, Ignacio, Ter-Antonyan, Samvel, Thompson, Will, Thwaites, Jessie, Tilav, Serap, Tollefson, Kirsten, Tönnis, Christoph, Toscano, Simona, Tosi, Delia, Trettin, Alexander, Tung, Chun Fai, Turcotte, Roxanne, Twagirayezu, Jean Pierre, Ty, Bunheng, Unland Elorrieta, Martin, Upshaw, Karriem, Valtonen-Mattila, Nora, Vandenbroucke, Justin, van Eijndhoven, Nick, Vannerom, David, van Santen, Jakob, Vara, Javi, Veitch-Michaelis, Joshua, Verpoest, Stef, Veske, Doga, Walck, Christian, Wang, Winnie, Watson, Timothy Blake, Weaver, Chris, Weigel, Philip, Weindl, Andreas, Weldert, Jan, Wendt, Chris, Werthebach, Johannes, Weyrauch, Mark, Whitehorn, Nathan, Wiebusch, Christopher, Willey, Nathan, Williams, Dawn, Wolf, Martin, Wrede, Gerrit, Wulff, Johan, Xu, Xianwu, Yanez, Juan Pablo, Yildizci, Emre, Yoshida, Shigeru, Yu, Shiqi, Yuan, Tianlu, Zhang, Zelong, Zhelnin, Pavel, and IceCube Collaboration

Abstract

doi:10.5194/tc-2022-174, The IceCube Neutrino Observatory instruments about 1 km3 of deep, glacial ice at the geographic South Pole using 5160 photomultipliers to detect Cherenkov light emitted by charged relativistic particles. A unexpected light propagation effect observed by the experiment is an anisotropic attenuation, which is aligned with the local flow direction of the ice. Birefringent light propagation has been examined as a possible explanation for this effect. The predictions of a first-principles birefringence model developed for this purpose, in particular curved light trajectories resulting from asymmetric diffusion, provide a qualitatively good match to the main features of the data. This in turn allows us to deduce ice crystal properties. Since the wavelength of the detected light is short compared to the crystal size, these crystal properties do not only include the crystal orientation fabric, but also the average crystal size and shape, as a function of depth. By adding small empirical corrections to this first-principles model, a quantitatively accurate description of the optical properties of the IceCube glacial ice is obtained. In this paper, we present the experimental signature of ice optical anisotropy observed in IceCube LED calibration data, the theory and parametrization of the birefringence effect, the fitting procedures of these parameterizations to experimental data as well as the inferred crystal properties.

Published
2022
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3. High-Energy and Ultra-High-Energy Neutrinos

Author

Ackermann, Markus, Agarwalla, Sanjib K., Alvarez-Muñiz, Jaime, Batista, Rafael Alves, Argüelles, Carlos A., Bustamante, Mauricio, Clark, Brian A., Cummings, Austin, Das, Sudipta, Decoene, Valentin, Denton, Peter B., Dornic, Damien, Dzhilkibaev, Zhan-Arys, Farzan, Yasaman, Garcia, Alfonso, Garzelli, Maria Vittoria, Glaser, Christian, Heijboer, Aart, Hörandel, Jörg R., Illuminati, Giulia, Jeong, Yu Seon, Kelley, John L., Kelly, Kevin J., Kheirandish, Ali, Klein, Spencer R., Krizmanic, John F., Larson, Michael J., Lu, Lu, Murase, Kohta, Narang, Ashish, Otte, Nepomuk, Prechelt, Remy L., Prohira, Steven, Reno, Mary Hall, Resconi, Elisa, Santander, Marcos, Suvorova, Olga Vasil'evna, Valera, Victor B., Vandenbroucke, Justin, Wiencke, Lawrence, Wissel, Stephanie, Yoshida, Shigeru, Yuan, Tianlu, Zas, Enrique, Zhelnin, Pavel, and Zhou, Bei

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years., Contribution to Snowmass 2021, updated to include community feedback

Published
2022

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