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140 results on '"Nelson, J."'

1. Constraints on dark photons and axionlike particles from the SuperCDMS Soudan experiment

Author

Aralis, T, Aramaki, T, Arnquist, IJ, Azadbakht, E, Baker, W, Banik, S, Barker, D, Bathurst, C, Bauer, DA, Bezerra, LVS, Bhattacharyya, R, Binder, T, Bowles, MA, Brink, PL, Bunker, R, Cabrera, B, Calkins, R, Cameron, RA, Cartaro, C, Cerdeño, DG, Chang, Y-Y, Cooley, J, Coombes, H, Corbett, J, Cornell, B, Cushman, P, De Brienne, F, di Vacri, ML, Diamond, MD, Fascione, E, Figueroa-Feliciano, E, Fink, CW, Fouts, K, Fritts, M, Gerbier, G, Germond, R, Ghaith, M, Golwala, SR, Harris, HR, Herbert, N, Hines, BA, Hollister, MI, Hong, Z, Hoppe, EW, Hsu, L, Huber, ME, Iyer, V, Jardin, D, Jastram, A, Kelsey, MH, Kennedy, A, Kubik, A, Kurinsky, NA, Lawrence, RE, Li, A, Loer, B, Asamar, E Lopez, Lukens, P, MacDonell, D, MacFarlane, DB, Mahapatra, R, Mandic, V, Mast, N, Michaud, ÉM, Michielin, E, Mirabolfathi, N, Mohanty, B, Mendoza, JD Morales, Nagorny, S, Nelson, J, Neog, H, Orrell, JL, Oser, SM, Page, WA, Pakarha, P, Partridge, R, Podviianiuk, R, Ponce, F, Poudel, S, Pyle, M, Rau, W, Ren, R, Reynolds, T, Roberts, A, Robinson, AE, Rogers, HE, Saab, T, Sadoulet, B, Sander, J, Schnee, RW, Scorza, S, Senapati, K, Serfass, B, Sincavage, DJ, Stanford, C, Stein, M, Street, J, Toback, D, Underwood, R, and Verma, S

Subjects
hep-ex, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract

We present an analysis of electron recoils in cryogenic germanium detectors operated during the SuperCDMS Soudan experiment. The data are used to set new constraints on the axioelectric coupling of axionlike particles and the kinetic mixing parameter of dark photons, assuming the respective species constitutes all of the galactic dark matter. This study covers the mass range from 40 eV/c2 to 500 keV/c2 for both candidates, excluding previously untested parameter space for masses below ∼1 keV/c2. For the kinetic mixing of dark photons, values below 10-15 are reached for particle masses around 100 eV/c2; for the axioelectric coupling of axionlike particles, values below 10-12 are reached for particles with masses in the range of a few-hundred eV/c2.

Published
2020

2. Search for low-mass dark matter with CDMSlite using a profile likelihood fit

Author

Agnese, R, Aralis, T, Aramaki, T, Arnquist, IJ, Azadbakht, E, Baker, W, Banik, S, Barker, D, Bauer, DA, Binder, T, Bowles, MA, Brink, PL, Bunker, R, Cabrera, B, Calkins, R, Cameron, RA, Cartaro, C, Cerdeño, DG, Chang, Y-Y, Cooley, J, Cornell, B, Cushman, P, De Brienne, F, Doughty, T, Fascione, E, Figueroa-Feliciano, E, Fink, CW, Fritts, M, Gerbier, G, Germond, R, Ghaith, M, Golwala, SR, Harris, HR, Herbert, N, Hong, Z, Hoppe, EW, Hsu, L, Huber, ME, Iyer, V, Jardin, D, Jastram, A, Jena, C, Kelsey, MH, Kennedy, A, Kubik, A, Kurinsky, NA, Lawrence, RE, Loer, B, Asamar, E Lopez, Lukens, P, MacDonell, D, Mahapatra, R, Mandic, V, Mast, N, Miller, E, Mirabolfathi, N, Mohanty, B, Mendoza, JD Morales, Nelson, J, Neog, H, Orrell, JL, Oser, SM, Page, WA, Partridge, R, Pepin, M, Ponce, F, Poudel, S, Pyle, M, Qiu, H, Rau, W, Reisetter, A, Ren, R, Reynolds, T, Roberts, A, Robinson, AE, Rogers, HE, Saab, T, Sadoulet, B, Sander, J, Scarff, A, Schnee, RW, Scorza, S, Senapati, K, Serfass, B, Speller, D, Stanford, C, Stein, M, Street, J, Tanaka, HA, Toback, D, Underwood, R, Villano, AN, von Krosigk, B, Watkins, SL, Wilson, JS, Wilson, MJ, Winchell, J, Wright, DH, Yellin, S, and Young, BA

Subjects
astro-ph.CO, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics
Abstract

The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) searches for interactions between dark matter particles and germanium nuclei in cryogenic detectors. The experiment has achieved a low energy threshold with improved sensitivity to low-mass (

Published
2019

3. Low-mass dark matter search with CDMSlite

Author

Agnese, R, Anderson, AJ, Aralis, T, Aramaki, T, Arnquist, IJ, Baker, W, Balakishiyeva, D, Barker, D, Basu Thakur, R, Bauer, DA, Binder, T, Bowles, MA, Brink, PL, Bunker, R, Cabrera, B, Caldwell, DO, Calkins, R, Cartaro, C, Cerdeño, DG, Chang, Y, Chagani, H, Chen, Y, Cooley, J, Cornell, B, Cushman, P, Daal, M, Di Stefano, PCF, Doughty, T, Esteban, L, Fascione, E, Figueroa-Feliciano, E, Fritts, M, Gerbier, G, Ghaith, M, Godfrey, GL, Golwala, SR, Hall, J, Harris, HR, Hong, Z, Hoppe, EW, Hsu, L, Huber, ME, Iyer, V, Jardin, D, Jastram, A, Jena, C, Kelsey, MH, Kennedy, A, Kubik, A, Kurinsky, NA, Leder, A, Loer, B, Lopez Asamar, E, Lukens, P, Macdonell, D, Mahapatra, R, Mandic, V, Mast, N, Miller, EH, Mirabolfathi, N, Moffatt, RA, Mohanty, B, Morales Mendoza, JD, Nelson, J, Orrell, JL, Oser, SM, Page, K, Page, WA, Partridge, R, Pepin, M, Peñalver Martinez, M, Phipps, A, Poudel, S, Pyle, M, Qiu, H, Rau, W, Redl, P, Reisetter, A, Reynolds, T, Roberts, A, Robinson, AE, Rogers, HE, Saab, T, Sadoulet, B, Sander, J, Schneck, K, Schnee, RW, Scorza, S, Senapati, K, Serfass, B, Speller, D, Stein, M, Street, J, Tanaka, HA, Toback, D, Underwood, R, Villano, AN, Von Krosigk, B, Welliver, B, and Wilson, JS

Subjects
astro-ph.CO, astro-ph.IM, hep-ex, physics.ins-det
Abstract

The SuperCDMS experiment is designed to directly detect weakly interacting massive particles (WIMPs) that may constitute the dark matter in our Galaxy. During its operation at the Soudan Underground Laboratory, germanium detectors were run in the CDMSlite mode to gather data sets with sensitivity specifically for WIMPs with masses

Published
2018

6. Investigating the sources of low-energy events in a SuperCDMS-HVeV detector

Author

SuperCDMS Collaboration, Albakry, M. F., Alkhatib, I., Amaral, D. W. P., Aralis, T., Aramaki, T., Arnquist, I. J., Langroudy, I. Ataee, Azadbakht, E., Banik, S., Bathurst, C., Bauer, D. A., Bhattacharyya, R., Brink, P. L., Bunker, R., Cabrera, B., Calkins, R., Cameron, R. A., Cartaro, C., Cerdeño, D. G., Chang, Y. -Y., Chaudhuri, M., Chen, R., Chott, N., Cooley, J., Coombes, H., Corbett, J., Cushman, P., De Brienne, F., Dharani, S., di Vacri, M. L., Diamond, M. D., Fascione, E., Figueroa-Feliciano, E., Fink, C. W., Fouts, K., Fritts, M., Gerbier, G., Germond, R., Ghaith, M., Golwala, S. R., Hall, J., Hassan, N., Hines, B. A., Hollister, M. I., Hong, Z., Hoppe, E. W., Hsu, L., Huber, M. E., Iyer, V., Jastram, A., Kashyap, V. K. S., Kelsey, M. H., Kubik, A., Kurinsky, N. A., Lawrence, R. E., Lee, M., Li, A., Liu, J., Liu, Y., Loer, B., Asamar, E. Lopez, Lukens, P., MacFarlane, D. B., Mahapatra, R., Mandic, V., Mast, N., Mayer, A. J., Theenhausen, H. Meyer zu, Michaud, É., Michielin, E., Mirabolfathi, N., Mohanty, B., Nagorny, S., Nelson, J., Neog, H., Novati, V., Orrell, J. L., Osborne, M. D., Oser, S. M., Page, W. A., Partridge, R., Pedreros, D. S., Podviianiuk, R., Ponce, F., Poudel, S., Pradeep, A., Pyle, M., Rau, W., Reid, E., Ren, R., Reynolds, T., Roberts, A., Robinson, A. E., Saab, T., Sadoulet, B., Saikia, I., Sander, J., Sattari, A., Schmidt, B., Schnee, R. W., Scorza, S., Serfass, B., Poudel, S. S., Sincavage, D. J., Stanford, C., Street, J., Sun, H., Thasrawala, F. K., Toback, D., Underwood, R., Verma, S., Villano, A. N., von Krosigk, B., Watkins, S. L., Wen, O., Williams, Z., Wilson, M. J., Winchell, J., Wykoff, K., Yellin, S., Young, B. A., Yu, T. C., Zatschler, B., Zatschler, S., Zaytsev, A., Zhang, E., Zheng, L., and Zuber, S.

Subjects
High Energy Physics - Experiment (hep-ex), Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, Physics, FOS: Physical sciences, ddc:530, Instrumentation and Detectors (physics.ins-det), High Energy Physics - Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Recent experiments searching for sub−GeV/c2 dark matter have observed event excesses close to their respective energy thresholds. Although specific to the individual technologies, the measured excess event rates have been consistently reported at or below event energies of a few-hundred eV, or with charges of a few electron-hole pairs. In the present work, we operated a 1-g silicon SuperCDMS-HVeV detector at three voltages across the crystal (0, 60 and 100 V). The 0 V data show an excess of events in the tens of eV region. Despite this event excess, we demonstrate the ability to set a competitive exclusion limit on the spin-independent dark matter–nucleon elastic scattering cross section for dark matter masses of O(100) MeV/c2, enabled by operation of the detector at 0 V potential and achievement of a very low O(10) eV threshold for nuclear recoils. Comparing the data acquired at 0, 60 and 100 V potentials across the crystal, we investigated possible sources of the unexpected events observed at low energy. The data indicate that the dominant contribution to the excess is consistent with a hypothesized luminescence from the printed circuit boards used in the detector holder.

Published
2022

8. Investigating the sources of low-energy events in a SuperCDMS-HVeV detector

Author

Albakry, M. F., primary, Alkhatib, I., additional, Amaral, D. W. P., additional, Aralis, T., additional, Aramaki, T., additional, Arnquist, I. J., additional, Ataee Langroudy, I., additional, Azadbakht, E., additional, Banik, S., additional, Bathurst, C., additional, Bauer, D. A., additional, Bhattacharyya, R., additional, Brink, P. L., additional, Bunker, R., additional, Cabrera, B., additional, Calkins, R., additional, Cameron, R. A., additional, Cartaro, C., additional, Cerdeño, D. G., additional, Chang, Y.-Y., additional, Chaudhuri, M., additional, Chen, R., additional, Chott, N., additional, Cooley, J., additional, Coombes, H., additional, Corbett, J., additional, Cushman, P., additional, De Brienne, F., additional, Dharani, S., additional, di Vacri, M. L., additional, Diamond, M. D., additional, Fascione, E., additional, Figueroa-Feliciano, E., additional, Fink, C. W., additional, Fouts, K., additional, Fritts, M., additional, Gerbier, G., additional, Germond, R., additional, Ghaith, M., additional, Golwala, S. R., additional, Hall, J., additional, Hassan, N., additional, Hines, B. A., additional, Hollister, M. I., additional, Hong, Z., additional, Hoppe, E. W., additional, Hsu, L., additional, Huber, M. E., additional, Iyer, V., additional, Jastram, A., additional, Kashyap, V. K. S., additional, Kelsey, M. H., additional, Kubik, A., additional, Kurinsky, N. A., additional, Lawrence, R. E., additional, Lee, M., additional, Li, A., additional, Liu, J., additional, Liu, Y., additional, Loer, B., additional, Lopez Asamar, E., additional, Lukens, P., additional, MacFarlane, D. B., additional, Mahapatra, R., additional, Mandic, V., additional, Mast, N., additional, Mayer, A. J., additional, Meyer zu Theenhausen, H., additional, Michaud, É., additional, Michielin, E., additional, Mirabolfathi, N., additional, Mohanty, B., additional, Nagorny, S., additional, Nelson, J., additional, Neog, H., additional, Novati, V., additional, Orrell, J. L., additional, Osborne, M. D., additional, Oser, S. M., additional, Page, W. A., additional, Partridge, R., additional, Pedreros, D. S., additional, Podviianiuk, R., additional, Ponce, F., additional, Poudel, S., additional, Pradeep, A., additional, Pyle, M., additional, Rau, W., additional, Reid, E., additional, Ren, R., additional, Reynolds, T., additional, Roberts, A., additional, Robinson, A. E., additional, Saab, T., additional, Sadoulet, B., additional, Saikia, I., additional, Sander, J., additional, Sattari, A., additional, Schmidt, B., additional, Schnee, R. W., additional, Scorza, S., additional, Serfass, B., additional, Poudel, S. S., additional, Sincavage, D. J., additional, Stanford, C., additional, Street, J., additional, Sun, H., additional, Thasrawala, F. K., additional, Toback, D., additional, Underwood, R., additional, Verma, S., additional, Villano, A. N., additional, von Krosigk, B., additional, Watkins, S. L., additional, Wen, O., additional, Williams, Z., additional, Wilson, M. J., additional, Winchell, J., additional, Wykoff, K., additional, Yellin, S., additional, Young, B. A., additional, Yu, T. C., additional, Zatschler, B., additional, Zatschler, S., additional, Zaytsev, A., additional, Zhang, E., additional, Zheng, L., additional, and Zuber, S., additional

Published
2022
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9. Ionization yield measurement in a germanium CDMSlite detector using photo-neutron sources

Author

Albakry, M. F., primary, Alkhatib, I., additional, Amaral, D. W. P., additional, Aralis, T., additional, Aramaki, T., additional, Arnquist, I. J., additional, Ataee Langroudy, I., additional, Azadbakht, E., additional, Banik, S., additional, Bathurst, C., additional, Bauer, D. A., additional, Bezerra, L. V. S., additional, Bhattacharyya, R., additional, Bowles, M. A., additional, Brink, P. L., additional, Bunker, R., additional, Cabrera, B., additional, Calkins, R., additional, Cameron, R. A., additional, Cartaro, C., additional, Cerdeño, D. G., additional, Chang, Y.-Y., additional, Chaudhuri, M., additional, Chen, R., additional, Chott, N., additional, Cooley, J., additional, Coombes, H., additional, Corbett, J., additional, Cushman, P., additional, De Brienne, F., additional, di Vacri, M. L., additional, Diamond, M. D., additional, Fascione, E., additional, Figueroa-Feliciano, E., additional, Fink, C. W., additional, Fouts, K., additional, Fritts, M., additional, Gerbier, G., additional, Germond, R., additional, Ghaith, M., additional, Golwala, S. R., additional, Hall, J., additional, Hines, B. A., additional, Hollister, M. I., additional, Hong, Z., additional, Hoppe, E. W., additional, Hsu, L., additional, Huber, M. E., additional, Iyer, V., additional, Jastram, A., additional, Kashyap, V. K. S., additional, Kelsey, M. H., additional, Kubik, A., additional, Kurinsky, N. A., additional, Lawrence, R. E., additional, Lee, M., additional, Li, A., additional, Liu, J., additional, Liu, Y., additional, Loer, B., additional, Lukens, P., additional, MacDonell, D., additional, MacFarlane, D. B., additional, Mahapatra, R., additional, Mandic, V., additional, Mast, N., additional, Mayer, A. J., additional, Meyer zu Theenhausen, H., additional, Michaud, É., additional, Michielin, E., additional, Mirabolfathi, N., additional, Mohanty, B., additional, Morales Mendoza, J. D., additional, Nagorny, S., additional, Nelson, J., additional, Neog, H., additional, Novati, V., additional, Orrell, J. L., additional, Osborne, M. D., additional, Oser, S. M., additional, Page, W. A., additional, Partridge, R., additional, Pedreros, D. S., additional, Podviianiuk, R., additional, Ponce, F., additional, Poudel, S., additional, Pradeep, A., additional, Pyle, M., additional, Rau, W., additional, Reid, E., additional, Ren, R., additional, Reynolds, T., additional, Roberts, A., additional, Robinson, A. E., additional, Saab, T., additional, Sadoulet, B., additional, Saikia, I., additional, Sander, J., additional, Sattari, A., additional, Scarff, A., additional, Schmidt, B., additional, Schnee, R. W., additional, Scorza, S., additional, Serfass, B., additional, Sincavage, D. J., additional, Stanford, C., additional, Street, J., additional, Thasrawala, F. K., additional, Toback, D., additional, Underwood, R., additional, Verma, S., additional, Villano, A. N., additional, von Krosigk, B., additional, Watkins, S. L., additional, Wen, O., additional, Williams, Z., additional, Wilson, M. J., additional, Winchell, J., additional, Wykoff, K., additional, Yellin, S., additional, Young, B. A., additional, Yu, T. C., additional, Zatschler, B., additional, Zatschler, S., additional, Zaytsev, A., additional, Zhang, E., additional, Zheng, L., additional, and Zuber, S., additional

Published
2022
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10. Measurement of inclusive charged-current νμ cross sections as a function of muon kinematics at ⟨Eν⟩∼6GeV on hydrocarbon

Author

Ruterbories, D., primary, Filkins, A., additional, Ahmad Dar, Z., additional, Akbar, F., additional, Andrade, D. A., additional, Ascencio, M. V., additional, Bashyal, A., additional, Bellantoni, L., additional, Bercellie, A., additional, Betancourt, M., additional, Bodek, A., additional, Bonilla, J. L., additional, Bravar, A., additional, Budd, H., additional, Caceres, G., additional, Cai, T., additional, Carneiro, M. F., additional, Díaz, G. A., additional, da Motta, H., additional, Dytman, S. A., additional, Felix, J., additional, Fields, L., additional, Fine, R., additional, Gago, A. M., additional, Gallagher, H., additional, Gran, R., additional, Harris, D. A., additional, Henry, S., additional, Jena, D., additional, Jena, S., additional, Kleykamp, J., additional, Kordosky, M., additional, Last, D., additional, Le, T., additional, Lozano, A., additional, Lu, X.-G., additional, Maher, E., additional, Manly, S., additional, Mann, W. A., additional, Mauger, C., additional, McFarland, K. S., additional, Messerly, B., additional, Miller, J., additional, Morfín, J. G., additional, Naples, D., additional, Nelson, J. K., additional, Nguyen, C., additional, Norrick, A., additional, Olivier, A., additional, Perdue, G. N., additional, Ramírez, M. A., additional, Ray, H., additional, Schellman, H., additional, Silva, G., additional, Solano Salinas, C. J., additional, Su, H., additional, Sultana, M., additional, Syrotenko, V. S., additional, Valencia, E., additional, Waldron, A. V., additional, Wret, C., additional, Yaeggy, B., additional, Yang, K., additional, and Zazueta, L., additional

Published
2021
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11. Search for slow magnetic monopoles with the NOvA detector on the surface

Author

NOvA Collaboration, Acero, M. A., Adamson, P., Aliaga, L., Alion, T., Allakhverdian, V., Anfimov, N., Antoshkin, A., Arrieta-Diaz, E., Asquith, L., Aurisano, A., Back, A., Backhouse, C., Baird, M., Balashov, N., Baldi, P., Bambah, B. A., Bashar, S., Bays, K., Bending, S., Bernstein, R., Bhatnagar, V., Bhuyan, B., Bian, J., Blair, J., Booth, A. C., Bour, P., Bowles, R., Bromberg, C., Buchanan, N., Butkevich, A., Calvez, S., Carroll, T. J., Catano-Mur, E., Childress, S., Choudhary, B. C., Coan, T. E., Colo, M., Corwin, L., Cremonesi, L., Davies, G. S., Derwent, P. F., Ding, P., Djurcic, Z., Dolce, M., Doyle, D., Tonguino, D. Dueñas, Dung, P., Dukes, E. C., Duyang, H., Edayath, S., Ehrlich, R., Elkins, M., Feldman, G. J., Filip, P., Flanagan, W., Franc, J., Frank, M. J., Gallagher, H. R., Gandrajula, R., Gao, F., Germani, S., Giri, A., Gomes, R. A., Goodman, M. C., Grichine, V., Groh, M., Group, R., Guo, B., Habig, A., Hakl, F., Hall, A., Hartnell, J., Hatcher, R., Heller, K., Hewes, V, Himmel, A., Holin, A., Huang, J., Hylen, J., Jarosz, J., Jediny, F., Johnson, C., Judah, M., Kakorin, I., Kalra, D., Kaplan, D. M., Keloth, R., Klimov, O., Koerner, L. W., Kolupaeva, L., Kotelnikov, S., Kullenberg, Ch., Kubu, M., Kumar, A., Kuruppu, C. D., Kus, V., Lackey, T., Lang, K., Li, L., Lin, S., Lister, A., Lokajicek, M., Luchuk, S., Magill, S., Mann, W. A., Marshak, M. L., Martinez-Casales, M., Matveev, V., Mayes, B., Méndez, D. P., Messier, M. D., Meyer, H., Miao, T., Miller, W. H., Mishra, S. R., Mislivec, A., Mohanta, R., Moren, A., Morozova, A., Mualem, L., Muether, M., Mufson, S., Mulder, K., Murphy, R., Musser, J., Naples, D., Nayak, N., Nelson, J. K., Nichol, R., Niner, E., Norman, A., Norrick, A., Nosek, T., Olshevskiy, A., Olson, T., Paley, J., Patterson, R. B., Pawloski, G., Petrova, O., Petti, R., Plunkett, R. K., Rafique, A., Raj, V., Ramson, B., Rebel, B., Rojas, P., Ryabov, V., Samoylov, O., Sanchez, M. C., Falero, S. Sánchez, Shanahan, P., Sheshukov, A., Singh, P., Singh, V., Smith, E., Smolik, J., Snopok, P., Solomey, N., Song, E., Sousa, A., Soustruznik, K., Strait, M., Suter, L., Sutton, A., Swain, S., Sweeney, C., Oregui, B. Tapia, Tas, P., Thayyullathil, R. B., Thomas, J., Tiras, E., Torbunov, D., Tripathi, J., Trokan-Tenorio, J., Torun, Y., Urheim, J., Vahle, P., Vallari, Z., Vasel, J., Vokac, P., Vrba, T., Wallbank, M., Wang, Z., Warburton, T. K., Wetstein, M., Whittington, D., Wickremasinghe, D. A., Wojcicki, S. G., Wolcott, J., Xiao, Y., Dombara, A. Yallappa, Yonehara, K., Yu, S., Yu, Y., Zadorozhnyy, S., Zalesak, J., Zhang, Y., and Zwaska, R.

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Detector, Magnetic monopole, FOS: Physical sciences, Flux, Instrumentation and Detectors (physics.ins-det), Electron, Nova (laser), Scintillator, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Overburden, 0103 physical sciences, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics
Abstract

We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure of the NOvA experiment's Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an upper limit on the flux of $2\times 10^{-14} \mathrm{cm^{-2}s^{-1}sr^{-1}}$ at 90% C.L. for monopole speed $6\times 10^{-4} < β< 5\times 10^{-3}$ and mass greater than $5\times 10^{8}$ GeV. Because of NOvA's small overburden of 3 meters-water equivalent, this constraint covers a previously unexplored low-mass region., 8 pages, 7 figures

Published
2021

12. Nucleon binding energy and transverse momentum imbalance in neutrino-nucleus reactions

Author

Cai, T., Lu, X. -G., Harewood, L. A., Wret, C., Akbar, F., Andrade, D. A., Ascencio, M. V., Bellantoni, L., Bercellie, A., Betancourt, M., Bodek, A., Bonilla, J. L., Bravar, A., Budd, H., Caceres, G., Carneiro, M. F., Coplowe, D., da Motta, H., Dar, Zubair Ahmad, D��az, G. A., Felix, J., Fields, L., Filkins, A., Fine, R., Gago, A. M., Gallagher, H., Ghosh, A., Gran, R., Harris, D. A., Henry, S., Jena, S., Jena, D., Kleykamp, J., Kordosky, M., Last, D., Le, T., Lozano, A., Maher, E., Manly, S., Mann, W. A., Mauger, C., McFarland, K. S., Messerly, B., Miller, J., Morf��n, J. G., Naples, D., Nelson, J. K., Nguyen, C., Norrick, A., Nuruzzaman, Olivier, A., Paolone, V., Perdue, G. N., Ram��rez, M. A., Ransome, R. D., Ruterbories, D., Schellman, H., Salinas, C. J. Solano, Su, H., Sultana, M., Syrotenko, V. S., Valencia, E., Wark, D., Weber, A., Wospakrik, M., Yaeggy, B., and Zazueta, L.

Subjects
Physics, Proton, 010308 nuclear & particles physics, Binding energy, Momentum transfer, FOS: Physical sciences, Computer Science::Digital Libraries, 01 natural sciences, High Energy Physics - Experiment, 3. Good health, Momentum, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, Neutrino, 010306 general physics, Nucleon, Fermi gas, Energy (signal processing)
Abstract

We have measured new observables based on the final state kinematic imbalances in the mesonless production of $\nu_\mu+A\rightarrow\mu^-+p+X$ in the $\text{MINER}\nu\text{A}$ tracker. Components of the muon-proton momentum imbalances parallel ($\delta p_\mathrm{Ty}$) and perpendicular($\delta p_\mathrm{Tx}$) to the momentum transfer in the transverse plane are found to be sensitive to the nuclear effects such as Fermi motion, binding energy and non-QE contributions. The QE peak location in $\delta p_\mathrm{Ty}$ is particularly sensitive to the binding energy. Differential cross sections are compared to predictions from different neutrino interaction models. The Fermi gas models presented in this study cannot simultaneously describe features such as QE peak location, width and the non-QE events contributing to the signal process. Correcting the GENIE's binding energy implementation according to theory causes better agreement with data. Hints of proton left-right asymmetry are observed in $\delta p_\mathrm{Tx}$. Better modeling of the binding energy can reduce bias in neutrino energy reconstruction and these observables can be applied in current and future experiments to better constrain nuclear effects., Comment: 14 pages, 12 figures; Added data release file in .root format

Published
2020

13. Disformally coupled quintessence

Author

Nelson J. Nunes, Elsa M. Teixeira, and Ana Nunes

Subjects
Physics, Stability parameter, Theoretical physics, Dark energy, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Cosmological model, Fixed point, Phenomenology (particle physics), Scaling, Scalar field, General Relativity and Quantum Cosmology, Quintessence
Abstract

In this work we consider a cosmological model in which dark energy is portrayed by a canonical scalar field which is allowed to couple to the other species by means of a disformal transformation of the metric. We revisit the current literature by assuming that the disformal function in the metric transformation can depend both on the scalar field itself and on its derivatives, encapsulating a wide variety of scalar-tensor theories. This generalisation also leads to new and richer phenomenology, explaining some of the features found in previously studied models. We present the background equations and perform a detailed dynamical analysis, from where new disformal fixed points emerge, that translate into novel cosmological features. These include early scaling regimes between the coupled species and broader stability parameter regions. However, viable cosmological models seem to have suppressed disformal late-time contributions., Comment: 20 pages, 6 figures. V2: Matches published version

Published
2020

14. Spherical collapse in coupled quintessence with a ΛCDM background

Author

Bruno J. Barros, Nelson J. Nunes, and Tiago Barreiro

Subjects
Physics, Cold dark matter, 010308 nuclear & particles physics, Dark matter, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Coupling (probability), 01 natural sciences, General Relativity and Quantum Cosmology, Cosmology, South Pole Telescope, 0103 physical sciences, Dark energy, Density contrast, 010306 general physics, Astrophysics - Cosmology and Nongalactic Astrophysics, Quintessence
Abstract

In this work we study the growth of cold dark matter density perturbations in the nonlinear regime on a conformally coupled quintessence model in which the background is designed to mimic a $\Lambda$CDM cosmology. The spherical collapse of overdense regions is analyzed. We highlight the role of the coupling on the overall dynamics, trace the evolution of the density contrast throughout the cosmic history and compute perturbative parameters such as the critical density contrast. We find that the coupling has the influence of delaying the collapse due to the slower growth of matter perturbations. We follow to compute the cluster number counts using the Press-Schechter and Sheth-Tormen mass functions. In both cases, the transfer of energy between the dark energy field and dark matter suppresses the number of objects at low redshifts and enhances the number at high redshifts. Finally, we compute the expected cluster number counts for the future eROSITA mission and the current South Pole Telescope survey., Comment: 11 pages, 9 figures. V2: Matches published version

Published
2020

15. Parameter Estimation for Compact Binary Coalescence Signals with the First Generation Gravitational-Wave Detector Network

Author

Aasi, J, Abadie, J, Abbott, B. P, Abbott, R, Abbott, T. D, Abernathy, M, Accadia, T, Acernese, F, Adams, C, Adams, T, Addesso, P, Adhikari, R, Affeldt, C, Agathos, M, Agatsuma, K, Ajith, P, Allen, B, Allocca, A, Ceron, E. Amador, Amariutei, D, Anderson, S. B, Anderson, W. G, Arai, K, Araya, M. C, Ast, S, Aston, S. M, Astone, P, Atkinson, D, Aufmuth, P, Aulbert, C, Aylott, B. E, Babak, S, Baker, P, Ballardin, G, Ballmer, S, Bao, Y, Barayoga, J. C. B, Barker, D, Barone, F, Barr, B, Barsotti, L, Barsuglia, M, Barton, M. A, Bartos, I, Bassiri, R, Bastarrika, M, Basti, A, Batch, J, Bauchrowitz, J, Bauer, Th. S, Bebronne, M, Beck, D, Behnke, B, Bejger, M, Beker, M. G, Bell, A. S, Bell, C, Belopolski, I, Benacquista, M, Berliner, J. M, Bertolini, A, Betzwieser, J, Beveridge, N, Beyersdorf, P. T, Bhadbade, T, Bilenko, I. A, Billingsley, G, Birch, J, Biswas, R, Bitossi, M, Bizouard, M. A, Black, E, Blackburn, J. K, Blackburn, L, Blair, D, Bland, B, Blom, M, Bock, O, Bodiya, T. P, Bogan, C, Bond, C, Bondarescu, R, Bondu, F, Bonelli, L, Bonnand, R, Bork, R, Born, M, Boschi, V, Bose, S, Bosi, L, Bouhou, B, Braccini, S, Bradaschia, C, Brady, P. R, Braginsky, V. B, Branchesi, M, Brau, J. E, Breyer, J, Briant, T, Bridges, D. O, Brillet, A, Brinkmann, M, Brisson, V, Britzger, M, Brooks, A. F, Brown, D. A, Bulik, T, Bulten, H. J, Buonanno, A, Burguet–Castell, J, Buskulic, D, Buy, C, Byer, R. L, Cadonati, L, Cagnoli, G, Calloni, E, Camp, J. B, Campsie, P, Cannon, K, Canuel, B, Cao, J, Capano, C. D, Carbognani, F, Carbone, L, Caride, S, Caudill, S, Cavaglia, M, Cavalier, F, Cavalieri, R, Cella, G, Cepeda, C, Cesarini, E, Chalermsongsak, T, Charlton, P, Chassande-Mottin, E, Chen, W, Chen, X, Chen, Y, Chincarini, A, Chiummo, A, Cho, H. S, Chow, J, Christensen, N, Chua, S. S.Y, Chung, C. T.Y, Chung, S, Ciani, G, Clara, F, Clark, D. E, Clark, J. A, Clayton, J. H, Cleva, F, Coccia, E, Cohadon, P.-F, Colacino, C. N, Colla, A, Colombini, M, Conte, A, Conte, R, Cook, D, Corbitt, T. R, Cordier, M, Cornish, N, Corsi, A, Costa, C. A, Coughlin, M, Coulon, J.-P, Couvares, P, Coward, D. M, Cowart, M, Coyne, D. C, Creighton, J. D. E, Creighton, T. D, Cruise, A. M, Cumming, A, Cunningham, L, Cuoco, E, Cutler, R. M, Dahl, K, Damjanic, M, Danilishin, S. L, D’Antonio, S, Danzmann, K, Dattilo, V, Daudert, B, Daveloza, H, Davier, M, Daw, E. J, Dayanga, T, Rosa, R. De, DeBra, D, Debreczeni, G, Degallaix, J, Pozzo, W. Del, Dent, T, Dergachev, V, DeRosa, R, Dhurandhar, S, Fiore, L. Di, Lieto, A. Di, Palma, I. Di, Emilio, M. Di Paolo, Virgilio, A. Di, Dı´az, M, Dietz, A, Donovan, F, Dooley, K. L, Doravari, S, Dorsher, S, Drago, M, Drever, R.W. P, Driggers, J. C, Du, Z, Dumas, J.-C, Dwyer, S, Eberle, T, Edgar, M, Edwards, M, Effler, A, Ehrens, P, Endro˝czi, G, Engel, R, Etzel, T, Evans, K, Evans, M, Evans, T, Factourovich, M, Fafone, V, Fairhurst, S, Farr, B. F, Farr, W. M, Favata, M, Fazi, D, Fehrmann, H, Feldbaum, D, Feroz, F, Ferrante, I, Ferrini, F, Fidecaro, F, Finn, L. S, Fiori, I, Fisher, R. P, Flaminio, R, Foley, S, Forsi, E, Forte, L. A, Fotopoulos, N, Fournier, J.-D, Franc, J, Franco, S, Frasca, S, Frasconi, F, Frede, M, Frei, M. A, Frei, Z, Freise, A, Frey, R, Fricke, T. T, Friedrich, D, Fritschel, P, Frolov, V.V, Fujimoto, M.-K, Fulda, P. J, Fyffe, M, Gair, J, Galimberti, M, Gammaitoni, L, Garcia, J, Garufi, F, Ga´spa´r, M. E, Gelencser, G, Gemme, G, Genin, E, Gennai, A, Gergely, L.A ´, Ghosh, S, Giaime, J. A, Giampanis, 6 S, Giardina, K. D, Giazotto, A, Gil-Casanova, S, Gill, C, Gleason, J, Goetz, E, Gonza´lez, G, Gorodetsky, M. L, Goßler, S, Gouaty, R, Graef, C, Graff, P. B, Granata, M, Grant, A, Gray, C, Greenhalgh, R. J. S, Gretarsson, A. M, Griffo, C, Grote, H, Grover, K, Grunewald, S, Guidi, G. M, Guido, C, Gupta, R, Gustafson, E. K, Gustafson, R, Hallam, J. M, Hammer, D, Hammond, G, Hanks, J, Hanna, C, Hanson, J, Harms, J, Harry, G. M, Harry, I.W, Harstad, E. D, Hartman, M. T, Haster, C.-J, Haughian, K, Hayama, K, Hayau, J.-F, Heefner, J, Heidmann, A, Heintze, M. C, Heitmann, H, Hello, P, Hemming, G, Hendry, M. A, Heng, I. S, Heptonstall, A.W, Herrera, V, Heurs, M, Hewitson, M, Hild, S, Hoak, D, Hodge, K. A, Holt, K, Holtrop, M, Hong, T, Hooper, S, Hough, J, Howell, E. J, Hughey, B, Husa, S, Huttner, S. H, Huynh-Dinh, T, Ingram, D. R, Inta, R, Isogai, T, Ivanov, A, Izumi, K, Jacobson, M, James, E, Jang, Y. J, Jaranowski, P, Jesse, E, Johnson, W.W, Jones, D. I, Jones, R, Jonker, R. J. G, Ju, L, Kalmus, P, Kalogera, V, Kandhasamy, S, Kang, G, Kanner, J. B, Kasprzack, M, Kasturi, R, Katsavounidis, E, Katzman, W, Kaufer, H, Kaufman, K, Kawabe, K, Kawamura, S, Kawazoe, F, Keitel, D, Kelley, D, Kells, W, Keppel, D. G, Keresztes, Z, Khalaidovski, A, Khalili, F.Y, Khazanov, E. A, Kim, B. K, Kim, C, Kim, H, Kim, K, Kim, N, Kim, Y. M, King, P. J, Kinzel, D. L, Kissel, J. S, Klimenko, S, Kline, J, Kokeyama, K, Kondrashov, V, Koranda, S, Korth, W. Z, Kowalska, I, Kozak, D, Kringel, V, Krishnan, B, Kro´lak, A, Kuehn, G, Kumar, P, Kumar, R, Kurdyumov, R, Kwee, P, Lam, P. K, Landry, M, Langley, A, Lantz, B, Lastzka, N, Lawrie, C, Lazzarini, A, Roux, A. Le, Leaci, P, Lee, C. H, Lee, H. K, Lee, H. M, Leong, J. R, Leonor, I, Leroy, N, Letendre, N, Lhuillier, V, Li, J, Li, T. G. F, Lindquist, P. E, Litvine, V, Liu, Y, Liu, Z, Lockerbie, N. A, Lodhia, D, Logue, J, Lorenzini, M, Loriette, V, Lormand, M, Losurdo, G, Lough, J, Lubinski, M, Lu¨ck, H, Lundgren, A. P, Macarthur, J, Macdonald, E, Machenschalk, B, MacInnis, M, Macleod, D. M, Mageswaran, M, Mailand, K, Majorana, E, Maksimovic, I, Malvezzi, V, Man, N, Mandel, I, Mandic, V, Mantovani, M, Marchesoni, F, Marion, F, Marka, S, Ma´rka, Z, Markosyan, A, Maros, E, Marque, J, Martelli, F, Martin, I.W, Martin, R. M, Marx, J. N, Mason, K, Masserot, A, Matichard, F, Matone, L, Matzner, R. A, Mavalvala, N, Mazzolo, G, McCarthy, R, McClelland, D. E, McGuire, S. C, McIntyre, G, McIver, J, Meadors, G. D, Mehmet, M, Meier, T, Melatos, A, Melissinos, A. C, Mendell, G, Menendez, D. F, Mercer, R. A, Meshkov, S, Messenger, C, Meyer, M. S, Miao, H, Michel, C, Milano, L, Miller, J, Minenkov, Y, Mingarelli, C. M. F, Mitrofanov, V. P, Mitselmakher, G, Mittleman, R, Moe, B, Mohan, M, Mohapatra, S. R. P, Moraru, D, Moreno, G, Morgado, N, Morgia, A, Mori, T, Morriss, S. R, Mosca, S, Mossavi, K, Mours, B, Mow–Lowry, C. M, Mueller, C. L, Mueller, G, Mukherjee, S, Mullavey, A, Muller-Ebhardt, H, Munch, J, Murphy, D, Murray, P. G, Mytidis, A, Nash, T, Naticchioni, L, Necula, V, Nelson, J, Neri, I, Newton, G, Nguyen, T, Nishizawa, A, Nitz, A, Nocera, F, Nolting, D, Normandin, M. E, Nuttall, L, Ochsner, E, O’Dell, J, Oelker, E, Ogin, G. H, Oh, J. J, Oh, S. H, Oldenberg, R. G, O’Reilly, B, O’Shaughnessy, R, Osthelder, C, Ott, C. D, Ottaway, D. J, Ottens, R. S, Overmier, H, Owen, B. J, Page, A, Palladino, L, Palomba, C, Pan, Y, Pankow, C, Paoletti, F, Paoletti, R, Papa, M. A, Parisi, M, Pasqualetti, A, Passaquieti, R, Passuello, D, Pedraza, M, Penn, S, Perreca, A, Persichetti, G, Phelps, M, Pichot, M, Pickenpack, M, Piergiovanni, F, Pierro, V, Pihlaja, M, Pinard, L, Pinto, I. M, Pitkin, M, Pletsch, H. J, Plissi, M.V, Poggiani, R, Po¨ld, J, Postiglione, F, Poux, C, Prato, M, Predoi, V, Prestegard, T, Price, L. R, Prijatelj, M, Principe, M, Privitera, S, Prodi, G. A, Prokhorov, L. G, Puncken, O, Punturo, M, Puppo, P, Quetschke, V, Quitzow-James, R, Raab, F. J, Rabeling, D. S, Ra´cz, I, Radkins, H, Raffai, P, Rakhmanov, M, Ramet, C, Rankins, B, Rapagnani, P, Raymond, V, Re, V, Reed, C. M, Reed, T, Regimbau, T, Reid, S, Reitze, D. H, Ricci, F, Riesen, R, Riles, K, Roberts, M, Robertson, N. A, Robinet, F, Robinson, C, Robinson, E. L, Rocchi, A, Roddy, S, Rodriguez, C, Rodruck, M, Rolland, L, Rollins, J. G, Romano, R, Romie, J. H, Rosinska, D, Rover, C, Rowan, S, Rudiger, A, Ruggi, P, Ryan, K, Salemi, F, Sammut, L, Sandberg, V, Sankar, S, Sannibale, V, Santamarıa, L, Santiago-Prieto, I, Santostasi, G, Saracco, E, Sassolas, B, Sathyaprakash, B. S, Saulson, P. R, Savage, R. L, Schilling, R, Schnabel, R, Schofield, R. M. S, Schulz, B, Schutz, B. F, Schwinberg, P, Scott, J, Scott, S. M, Seifert, F, Sellers, D, Sentenac, D, Sergeev, A, Shaddock, D. A, Shaltev, M, Shapiro, B, Shawhan, P, Shoemaker, D. H, Sidery, T. L, Siemens, X, Sigg, D, Simakov, D, Singer, A, Singer, L, Sintes, A. M, Skelton, G. R, Slagmolen, B. J. J, Slutsky, J, Smith, J. R, Smith, M. R, Smith, R. J. E, Smith-Lefebvre, N. D, Somiya, K, Sorazu, B, Speirits, F. C, Sperandio, L, Stefszky, M, Steinert, E, Steinlechner, J, Steinlechner, S, Steplewski, S, Stochino, A, Stone, R, Strain, K. A, Strigin, S. E, Stroeer, A. S, Sturani, R, Stuver, A. L, Summerscales, T. Z, Sung, M, Susmithan, S, Sutton, P. J, Swinkels, B, Szeifert, G, Tacca, M, Taffarello, L, Talukder, D, Tanner, D. B, Tarabrin, S. P, Taylor, R, Braack, A. P. M. ter, Thomas, P, Thorne, K. A, Thorne, K. S, Thrane, E, Thuring, A, Titsler, C, Tokmakov, K.V, Tomlinson, C, Toncelli, A, Tonelli, M, Torre, O, Torres, C.V, Torrie, C. I, Tournefier, E, Travasso, F, Traylor, G, Tse, M, Ugolini, D, Vahlbruch, H, Vajente, G, Brand, J. F. J. van den, Broeck, C. Van Den, Putten, S. van der, Veggel, A. A. van, Vass, S, Vasuth, M, Vaulin, R, Vavoulidis, M, Vecchio, A, Vedovato, G, Veitch, J, Veitch, P. J, Venkateswara, K, Verkindt, D, Vetrano, F, Vicere, A, Villar, A. E, Vinet, J.-Y, Vitale, S, Vocca, H, Vorvick, C, Vyatchanin, S. P, Wade, A, Wade, L, Wade, M, Waldman, S. J, Wallace, L, Wan, Y, Wang, M, Wang, X, Wanner, A, Ward, R. L, Was, M, Weinert, M, Weinstein, A. J, Weiss, R, Welborn, T, Wen, L, Wessels, P, West, M, Westphal, T, Wette, K, Whelan, J. T, Whitcomb, S. E, White, D. J, Whiting, B. F, Wiesner, K, Wilkinson, C, Willems, P. A, Williams, L, Williams, R, Willke, B, Wimmer, M, Winkelmann, L, Winkler, W, Wipf, C. C, Wiseman, A. G, Wittel, H, Woan, G, Wooley, R, Worden, J, Yablon, J, Yakushin, I, Yamamoto, H, Yamamoto, K, Yancey, C. C, Yang, H, Yeaton-Massey, D, Yoshida, S, Yvert, M, Zadrozny, A, Zanolin, M, Zendri, J.-P, Zhang, F, Zhang, L, Zhao, C, Zotov, N, Zucker, M. E, and Zweizig, and J

Subjects
Astrophysics
Abstract

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational-wave detectors. Gravitational radiation encodes rich information about source physics; thus parameter estimation and model selection are crucial analysis steps for any detection candidate events. Detailed models of the anticipated waveforms enable inference on several parameters, such as component masses, spins, sky location and distance, that are essential for new astrophysical studies of these sources. However, accurate measurements of these parameters and discrimination of models describing the underlying physics are complicated by artifacts in the data, uncertainties in the waveform models and in the calibration of the detectors. Here we report such measurements on a selection of simulated signals added either in hardware or software to the data collected by the two LIGO instruments and the Virgo detector during their most recent joint science run, including a blind injection where the signal was not initially revealed to the collaboration. We exemplify the ability to extract information about the source physics on signals that cover the neutron-star and black-hole binary parameter space over the component mass range 1M25M and the full range of spin parameters. The cases reported in this study provide a snapshot of the status of parameter estimation in preparation for the operation of advanced detectors.

Published
2013
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16. Constraints on low-mass, relic dark matter candidates from a surface-operated SuperCDMS single-charge sensitive detector

Author

Amaral, D. W., primary, Aralis, T., additional, Aramaki, T., additional, Arnquist, I. J., additional, Azadbakht, E., additional, Banik, S., additional, Barker, D., additional, Bathurst, C., additional, Bauer, D. A., additional, Bezerra, L. V. S., additional, Bhattacharyya, R., additional, Binder, T., additional, Bowles, M. A., additional, Brink, P. L., additional, Bunker, R., additional, Cabrera, B., additional, Calkins, R., additional, Cameron, R. A., additional, Cartaro, C., additional, Cerdeño, D. G., additional, Chang, Y.-Y., additional, Chen, R., additional, Chott, N., additional, Cooley, J., additional, Coombes, H., additional, Corbett, J., additional, Cushman, P., additional, De Brienne, F., additional, di Vacri, M. L., additional, Diamond, M. D., additional, Fascione, E., additional, Figueroa-Feliciano, E., additional, Fink, C. W., additional, Fouts, K., additional, Fritts, M., additional, Gerbier, G., additional, Germond, R., additional, Ghaith, M., additional, Golwala, S. R., additional, Harris, H. R., additional, Herbert, N., additional, Hines, B. A., additional, Hollister, M. I., additional, Hong, Z., additional, Hoppe, E. W., additional, Hsu, L., additional, Huber, M. E., additional, Iyer, V., additional, Jardin, D., additional, Jastram, A., additional, Kelsey, M. H., additional, Kubik, A., additional, Kurinsky, N. A., additional, Lawrence, R. E., additional, Li, A., additional, Loer, B., additional, Lopez Asamar, E., additional, Lukens, P., additional, MacDonell, D., additional, MacFarlane, D. B., additional, Mahapatra, R., additional, Mandic, V., additional, Mast, N., additional, Mayer, A. J., additional, Michaud, É. M., additional, Michielin, E., additional, Mirabolfathi, N., additional, Mohanty, B., additional, Morales Mendoza, J. D., additional, Nagorny, S., additional, Nelson, J., additional, Neog, H., additional, Novati, V., additional, Orrell, J. L., additional, Oser, S. M., additional, Page, W. A., additional, Pakarha, P., additional, Partridge, R., additional, Podviianiuk, R., additional, Ponce, F., additional, Poudel, S., additional, Pyle, M., additional, Rau, W., additional, Reid, E., additional, Ren, R., additional, Reynolds, T., additional, Roberts, A., additional, Robinson, A. E., additional, Rogers, H. E., additional, Saab, T., additional, Sadoulet, B., additional, Sander, J., additional, Sattari, A., additional, Schnee, R. W., additional, Scorza, S., additional, Serfass, B., additional, Sincavage, D. J., additional, Stanford, C., additional, Stein, M., additional, Street, J., additional, Toback, D., additional, Underwood, R., additional, Verma, S., additional, Villano, A. N., additional, von Krosigk, B., additional, Watkins, S. L., additional, Wills, L., additional, Wilson, J. S., additional, Wilson, M. J., additional, Winchell, J., additional, Wright, D. H., additional, Yellin, S., additional, Young, B. A., additional, Yu, T. C., additional, Zhang, E., additional, Zhang, H. G., additional, Zhao, X., additional, and Zheng, L., additional

Published
2020
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19. Conformally coupled tachyonic dark energy

Author

Nelson J. Nunes, Elsa M. Teixeira, and Ana Nunes

Subjects
Physics, 010308 nuclear & particles physics, FOS: Physical sciences, Inverse, General Relativity and Quantum Cosmology (gr-qc), Fixed point, 01 natural sciences, Omega, General Relativity and Quantum Cosmology, Theoretical physics, Tachyon, Critical point (thermodynamics), 0103 physical sciences, Attractor, Dark energy, 010306 general physics, Scaling
Abstract

We present and study a conformally coupled dark energy model, characterised by an interaction between a tachyon field $\phi$, with an inverse square potential $V (\phi)$, and the matter sector. A detailed analysis of the cosmological outcome reveals different possibilities, in contrast with the previously studied uncoupled model, for which there exists only one stable critical point that gives late-time acceleration of the Universe. The introduction of the coupling translates into an energy exchange between the fluids. We find the interesting possibility of the emergence of a new fixed point, which is a scaling solution and an attractor of the system. In this case, it is possible to describe an everlasting Universe with $\Omega_{\phi} \simeq 0.7$, therefore alleviating the cosmic coincidence problem. However, we find that, in order for the evolution to be cosmologically viable, there is the need to introduce one uncoupled matter species, dominant at early times., Comment: 18 pages, 7 figures. V3: Matches published version

Published
2019

20. Most general cubic-order Horndeski Lagrangian allowing for scaling solutions and the application to dark energy

Author

Shinji Tsujikawa, Nelson J. Nunes, Noemi Frusciante, and Ryotaro Kase

Subjects
High Energy Physics - Theory, Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010308 nuclear & particles physics, FOS: Physical sciences, Order (ring theory), Inverse, General Relativity and Quantum Cosmology (gr-qc), Fixed point, Coupling (probability), 01 natural sciences, General Relativity and Quantum Cosmology, Square (algebra), High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), High Energy Physics - Theory (hep-th), Critical point (thermodynamics), 0103 physical sciences, 010306 general physics, Scalar field, Laplace operator, Astrophysics - Cosmology and Nongalactic Astrophysics, Mathematical physics
Abstract

In cubic-order Horndeski theories where a scalar field $\phi$ is coupled to nonrelativistic matter with a field-dependent coupling $Q(\phi)$, we derive the most general Lagrangian having scaling solutions on the isotropic and homogenous cosmological background. For constant $Q$ including the case of vanishing coupling, the corresponding Lagrangian reduces to the form $L=Xg_2(Y)-g_3(Y)\square \phi$, where $X=-\partial_{\mu}\phi\partial^{\mu}\phi/2$ and $g_2, g_3$ are arbitrary functions of $Y=Xe^{\lambda \phi}$ with constant $\lambda$. We obtain the fixed points of the scaling Lagrangian for constant $Q$ and show that the $\phi$-matter-dominated-epoch ($\phi$MDE) is present for the cubic coupling $g_3(Y)$ containing inverse power-law functions of $Y$. The stability analysis around the fixed points indicates that the $\phi$MDE can be followed by a stable critical point responsible for the cosmic acceleration. We propose a concrete dark energy model allowing for such a cosmological sequence and show that the ghost and Laplacian instabilities can be avoided even in the presence of the cubic coupling., Comment: 17 pages, 3 figures, version to appear in Physical Review D

Published
2018

21. New scaling solutions in cubic Horndeski theories

Author

Shinji Tsujikawa, Noemi Frusciante, Inês S. Albuquerque, and Nelson J. Nunes

Subjects
Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010308 nuclear & particles physics, Equation of state (cosmology), FOS: Physical sciences, Scalar potential, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Kinetic term, Parameter space, 01 natural sciences, General Relativity and Quantum Cosmology, 0103 physical sciences, Dark energy, 010306 general physics, Scaling, Weak gravitational lensing, Astrophysics - Cosmology and Nongalactic Astrophysics, Quintessence, Mathematical physics
Abstract

We propose a viable dark energy scenario in the presence of cubic Horndeski interactions and a standard scalar-field kinetic term with two exponential potentials. We show the existence of new scaling solutions along which the cubic coupling $G_3$ provides an important contribution to the field density that scales in the same way as the background fluid density. The solutions finally exit to the epoch of cosmic acceleration driven by a scalar-field dominated fixed point arising from the second exponential potential. We clarify the viable parameter space in which all the theoretically consistent conditions including those for the absence of ghost and Laplacian instabilities are satisfied on scaling and scalar-field dominated critical points. In comparison to Quintessence with the same scalar potential, we find that the cubic coupling gives rise to some novel features: (i) the allowed model parameter space is wider in that a steeper potential can drive the cosmic acceleration; (ii) the dark energy equation of state $w_{\phi}$ today can be closer to $-1$ relative to Quintessence; (iii) even if the density associated with the cubic coupling dominates over the standard field density in the scaling era, the former contribution tends to be suppressed at low redshifts. We also compute quantities associated with the growth of matter perturbations and weak lensing potentials under the quasi-static approximation in the sub-horizon limit and show that the cubic coupling leads to the modified evolution of perturbations which can be distinguished from Quintessence., Comment: 15 pages, 7 figures, accepted version by PRD

Published
2018

24. Linear density perturbations in multifield coupled quintessence

Author

Karim A. Malik, Nelson J. Nunes, Alexander Leithes, and David J. Mulryne

Subjects
Physics, Linear density, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cold dark matter, 010308 nuclear & particles physics, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Python (programming language), Lambda, 01 natural sciences, General Relativity and Quantum Cosmology, Theoretical physics, Experimental uncertainty analysis, 0103 physical sciences, Cosmological perturbation theory, Statistical physics, 010306 general physics, computer, Astrophysics - Cosmology and Nongalactic Astrophysics, computer.programming_language, Quintessence
Abstract

We study the behaviour of linear perturbations in multifield coupled quintessence models. Using gauge invariant linear cosmological perturbation theory we provide the full set of governing equations for this class of models, and solve the system numerically. We apply the numerical code to generate growth functions for various examples, and compare these both to the standard $\Lambda$CDM model and to current and future observational bounds. Finally, we examine the applicability of the "small scale approximation", often used to calculate growth functions in quintessence models, in light of upcoming experiments such as SKA and Euclid. We find the deviation of the full equation results for large k modes from the approximation exceeds the experimental uncertainty for these future surveys. The numerical code, PYESSENCE, written in Python will be publicly available., Comment: 19 pages, 9 figures, version accepted for publication by PRD, refs. added, extra Consistency Test section added

Published
2017

25. Measurements of the inclusive neutrino and antineutrino charged current cross sections in MINERvA using the low- ν flux method

Author

MINERvA Collaboration, DeVan, J., Ren, L., Aliaga, L., Altinok, O., Bellantoni, L., Bercellie, A., Betancourt, M., Bodek, A., Budd, H., Cai, T., Carneiro, M. F., da Motta, H., Devan, J., Dytman, S. A., Díaz, G. A., Eberly, B., Endress, E., Felix, J., Fields, L., Fine, R., Gago, A. M., Galindo, R., Gallagher, H., Ghosh, A., Gran, R., Harris, D. A., Higuera, A., Hurtado, K., Kleykamp, J., Kordosky, M., Le, T., Maher, E., Manly, S., Mann, W. A., Marshall, C. M., Caicedo, D. A. Martinez, McFarland, K. S., McGivern, C. L., McGowan, A. M., Messerly, B., Miller, J., Mislivec, A., Morfín, J. G., Mousseau, J., Naples, D., Nelson, J. K., Norrick, A., Nuruzzaman, Paolone, V., Park, J., Patrick, C. E., Perdue, G. N., Ramirez, M. A., Ransome, R. D., Ray, H., Rimal, D., Rodrigues, P. A., Ruterbories, D., Schellman, H., Salinas, C. J. Solano, Sultana, M., Falero, S. Sánchez, Tice, B. G., Valencia, E., Wolcott, J., Wospakrik, M., and Zhang, D.

Subjects
Physics, Particle physics, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, Solar neutrino problem, 7. Clean energy, 01 natural sciences, NuMI, High Energy Physics - Experiment, Nuclear physics, Neutrino detector, 0103 physical sciences, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, Nuclear Experiment, 010306 general physics, Neutrino oscillation, Charged current
Abstract

The total cross sections are important ingredients for the current and future neutrino oscillation experiments. We present measurements of the total charged-current neutrino and antineutrino cross sections on scintillator (CH) in the NuMI low-energy beamline using an {\em in situ} prediction of the shape of the flux as a function of neutrino energy from 2--50 GeV. This flux prediction takes advantage of the fact that neutrino and antineutrino interactions with low nuclear recoil energy ($\nu$) have a nearly constant cross section as a function of incident neutrino energy. This measurement is the lowest energy application of the low-$\nu$ flux technique, the first time it has been used in the NuMI antineutrino beam configuration, and demonstrates that the technique is applicable to future neutrino beams operating at multi-GeV energies. The cross section measurements presented are the most precise measurements to date below 5 GeV., Comment: 8 pages, 6 figures, and 12 supplemental tables of fluxes, cross sections, breakdowns of their uncertainties, and their covariance matrices

Published
2016

27. Non-Gaussianity in multiple three-form field inflation

Author

João Marto, K. Sravan Kumar, David J. Mulryne, Nelson J. Nunes, Paulo Vargas Moniz, and uBibliorum

Subjects
High Energy Physics - Theory, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, δN formalism, Curvature perturbation, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Equilateral triangle, 01 natural sciences, General Relativity and Quantum Cosmology, Theoretical physics, Non-Gaussianity, 0103 physical sciences, 010306 general physics, Physics, Spectral index, 010308 nuclear & particles physics, Primordial non-Gaussianity, Cosmological model, Inflation, Formalism (philosophy of mathematics), Amplitude, High Energy Physics - Theory (hep-th), Multiple three-forms, Bispectrum, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

In this work, we present a method for implementing the $\delta N$ formalism to study the primordial non-Gaussianity produced in multiple three-form field inflation. Using a dual description relating three-form fields to noncanonical scalar fields, and employing existing results, we produce expressions for the bispectrum of the curvature perturbation in terms of three-form quantities. We study the bispectrum generated in a two three-form field inflationary scenario for a particular potential that for suitable values of the parameters was found in earlier work to give values of the spectral index and ratio of tensor to scalar perturbations compatible with current bounds. We calculate the reduced bispectrum for this model, finding an amplitude in equilateral and orthogonal configurations of ${\cal O}(1)$ and in the squeezed limit of ${\cal O}(10^{-3})$. We confirm, therefore, that this three-form inflationary scenario is compatible with present observational constraints., Comment: 14 pages, 3 figures, discussion added, references updated, version accepted in PRD

Published
2016

28. Three-form inflation in type II Randall-Sundrum

Author

Bruno J. Barros and Nelson J. Nunes

Subjects
Inflation (cosmology), Physics, 010308 nuclear & particles physics, Observable, 01 natural sciences, Gravitation, General Relativity and Quantum Cosmology, symbols.namesake, Theoretical physics, Classical mechanics, Randall–Sundrum model, 0103 physical sciences, symbols, Dark energy, Brane, Planck, 010306 general physics, Scalar field
Abstract

It has been shown in the last few years that three-form fields present viable cosmological solutions for inflation and dark energy with particular observable signatures distinct from those of canonical single scalar field inflation. The aim of this work is to explore the dynamics of a single three-form in a five-dimensional type II Randall-Sundrum braneworld scenario, in which a three-form is confined to the brane and only gravity propagates in the bulk. We compare the solutions with the standard four-dimensional case already studied in the literature. In particular, we evaluate how the spectral index and the ratio of tensor-to-scalar perturbations are influenced by the presence of the bulk and put constraints on the parameters of the models in light of the recent Planck 2015 data.

Published
2016

30. Multifield coupled quintessence

Author

Nelson J. Nunes, Tiago Barreiro, and Luca Amendola

Subjects
Physics, Nuclear and High Energy Physics, Classical mechanics, Logarithm, Scalar (mathematics), Dark matter, Scalar potential, Statistical physics, Scaling, Cosmology, Exponential function, Quintessence
Abstract

We study models of quintessence consisting of a number of scalar fields coupled to several dark matter components. In the case of exponential potentials the scaling solutions can be described in terms of a single field. The corresponding effective logarithmic slope and effective coupling can be written in a simple form in terms of the individual slopes and couplings of the original fields. We also investigate solutions where the scalar potential is negligible, in particular those leading to transient matter dominated solutions. Finally, we compute the evolution equations for the linear perturbations which will allow these models to be tested against current and future observational data.

Published
2014

33. Search for the disappearance of muon antineutrinos in the NuMI neutrino beam

Author

MINOS Collaboration, Adamson, P., Auty, D. J., Ayres, D. S., Backhouse, C., Barr, G., Bishai, M., Blake, A., Bock, G. J., Boehnlein, D. J., Bogert, D., Cao, S. V., Cavanaugh, S., Cherdack, D., Childress, S., Choudhary, B. C., Coelho, J. A. B., Coleman, S. J., Corwin, L., Cronin-Hennessy, D., Danko, I. Z., de Jong, J. K., Devenish, N. E., Diwan, M. V., Dorman, M., Escobar, C. O., Evans, J. J., Falk, E., Feldman, G. J., Frohne, M. V., Gallagher, H. R., Gomes, R. A., Goodman, M. C., Gouffon, P., Graf, N., Gran, R., Grant, N., Grzelak, K., Habig, A., Hartnell, J., Hatcher, R., Himmel, A., Holin, A., Howcroft, C., Huang, X., Hylen, J., Irwin, G. M., Isvan, Z., Jaffe, D. E., James, C., Jensen, D., Kafka, T., Kasahara, S. M. S., Koizumi, G., Kopp, S., Kordosky, M., Kreymer, A., Lang, K., Lefeuvre, G., Ling, J., Litchfield, P. J., Loiacono, L., Lucas, P., Mann, W. A., Marshak, M. L., Mathis, M., Mayer, N., Mehdiyev, R., Meier, J. R., Messier, M. D., Michael, D. G., Miller, W. H., Mishra, S. R., Mitchell, J., Moore, C. D., Mualem, L., Mufson, S., Musser, J., Naples, D., Nelson, J. K., Newman, H. B., Nichol, R. J., Nowak, J. A., Ochoa-Ricoux, J. P., Oliver, W. P., Orchanian, M., Pahlka, R., Paley, J., Patterson, R. B., Pawloski, G., Pearce, G. F., Phan-Budd, S., Plunkett, R. K., Qiu, X., Ratchford, J., Rebel, B., Rosenfeld, C., Rubin, H. A., Sanchez, M. C., Schneps, J., Schreckenberger, A., Schreiner, P., Sharma, R., Sousa, A., Strait, M., Tagg, N., Talaga, R. L., Tavera, M. A., Thomas, J., Thomson, M. A., Tinti, G., Toner, R., Torretta, D., Tzanakos, G., Urheim, J., Vahle, P., Viren, B., Walding, J. J., Weber, A., Webb, R. C., White, C., Whitehead, L., Wojcicki, S. G., Yang, T., and Zwaska, R.

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Muon, FOS: Physical sciences, NuMI, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), MINOS, Antimatter, Fermilab, Neutrino, Charged current, Lepton
Abstract

We report constraints on antineutrino oscillation parameters that were obtained by using the two MINOS detectors to measure the 7% muon antineutrino component of the NuMI neutrino beam. In the Far Detector, we select 130 events in the charged-current muon antineutrino sample, compared to a prediction of 136.4 +/- 11.7(stat) ^{+10.2}_{-8.9}(syst) events under the assumption |dm2bar|=2.32x10^-3 eV^2, snthetabar=1.0. Assuming no oscillations occur at the Near Detector baseline, a fit to the two-flavor oscillation approximation constrains |dm2bar, Accepted for publication by Phys. Rev. D Rapid Communications. 6 pages, 4 figures

Published
2011

34. Mass freezing in growing neutrino quintessence

Author

Lily Schrempp, Christof Wetterich, and Nelson J. Nunes

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Time-variation of fundamental constants, 01 natural sciences, General Relativity and Quantum Cosmology, Cosmology, Massless particle, High Energy Physics - Phenomenology, Gravitational potential, 0103 physical sciences, Dark energy, High Energy Physics::Experiment, Neutrino, 010306 general physics, Astrophysics - Cosmology and Nongalactic Astrophysics, Lepton, Quintessence
Abstract

Growing neutrino quintessence solves the coincidence problem for dark energy by a growing cosmological value of the neutrino mass which emerges from a cosmon-neutrino interaction stronger than gravity. The cosmon-mediated attraction between neutrinos induces the formation of large scale neutrino lumps in a recent cosmological epoch. We argue that the non-linearities in the cosmon field equations stop the further increase of the neutrino mass within sufficiently dense and large lumps. As a result, we find the neutrino induced gravitational potential to be substantially reduced when compared to linear extrapolations. We furthermore demonstrate that inside a lump the possible time variation of fundamental constants is much smaller than their cosmological evolution. This feature may reconcile current geophysical bounds with claimed cosmological variations of the fine structure constant., Comment: 15 pages, 12 figures. Version published in PRD

Published
2011

36. Gravitational wave background from superinflation in loop quantum cosmology

Author

David J. Mulryne, Edmund J. Copeland, Maryam Shaeri, and Nelson J. Nunes

Subjects
High Energy Physics - Theory, Physics, Nuclear and High Energy Physics, Spectral index, Gravitational wave, Astrophysics (astro-ph), FOS: Physical sciences, Spectral density, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology, Gravitational wave background, High Energy Physics - Theory (hep-th), Gravitational field, Quantum mechanics, Tensor, Scalar field, Loop quantum cosmology
Abstract

We investigate the behaviour of tensor fluctuations in Loop Quantum Cosmology, focusing on a class of scaling solutions which admit a near scale-invariant scalar field power spectrum. We obtain the spectral index of the gravitational field perturbations, and find a strong blue tilt in the power spectrum with $n_t \approx 2$. The amplitude of tensor modes are, therefore, suppressed by many orders of magnitude on large scales compared to those predicted by the standard inflationary scenario where $n_t \approx 0$., Comment: 8 pages, 3 figures

Published
2009

37. Constraints on a scale invariant power spectrum from superinflation in loop quantum cosmology

Author

Nelson J. Nunes and David J. Mulryne

Subjects
Physics, Inflation (cosmology), Nuclear and High Energy Physics, Classical mechanics, Field (physics), Quantum cosmology, Quantum field theory, Scale invariance, Scalar field, Scaling, Loop quantum cosmology
Abstract

The computation of the spectrum of primordial perturbations, generated by a scalar field during the superinflationary phase of loop quantum cosmology, is revisited. The calculation is performed for two different cases. The first considers the dynamics of a massless field and it is found that scale invariance can only be achieved under a severe fine-tuning. The second assumes that the field evolves with a constant ratio between kinetic and potential energy, i.e. in a scaling solution. In this case, near scale invariance is a generic feature of the theory if the field rolls in a steep self-interaction potential.

Published
2006

38. Reconstructing the dark energy equation of state with varying alpha

Author

Nelson J. Nunes and James E. Lidsey

Subjects
Physics, Nuclear and High Energy Physics, Field (physics), Equation of state (cosmology), Astrophysics (astro-ph), FOS: Physical sciences, Fine-structure constant, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Redshift, High Energy Physics - Phenomenology, Supernova, High Energy Physics - Phenomenology (hep-ph), Quantum mechanics, Dark energy, Dark fluid, Quintessence
Abstract

The possibility of reconstructing the dark energy equation of state from variations in the fine structure constant is investigated for a class of models where the quintessence field is non-minimally coupled to the electromagnetic field. For given classes of couplings and quintessence interaction potentials, it is typically found that variations in alpha would need to be measured to within an accuracy of at least $5 \times 10^{-7}$ to obtain a reconstructed equation of state with less than a twenty per cent deviation from the true equation of state between redshifts 0 and 3. In this case, it is argued that the sign of the first derivative of the equation of state can be uncovered from the reconstruction, thus providing unique information on how the universe developed into its present dark energy dominated phase independent of high redshift surveys. Such information would complement future observations anticipated from the Supernova Acceleration Probe., Comment: 6 pages, 4 figures. Extended discussion and bibliography. In Press, Physical Review D

Published
2004

39. Models of quintessence coupled to the electromagnetic field and the cosmological evolution of alpha

Author

Maxim Pospelov, Edmund J. Copeland, and Nelson J. Nunes

Subjects
Electromagnetic field, Physics, Nuclear and High Energy Physics, 010308 nuclear & particles physics, Astrophysics (astro-ph), Planck mass, FOS: Physical sciences, Observable, Fine-structure constant, Astrophysics, Coupling (probability), 7. Clean energy, 01 natural sciences, High Energy Physics - Phenomenology, Theoretical physics, High Energy Physics - Phenomenology (hep-ph), 13. Climate action, Quantum mechanics, 0103 physical sciences, Dark energy, 010306 general physics, Scalar field, Quintessence
Abstract

We study the change of the effective fine structure constant in the cosmological models of a scalar field with a non-vanishing coupling to the electromagnetic field. Combining cosmological data and terrestrial observations we place empirical constraints on the size of the possible coupling and explore a large class of models that exhibit tracking behavior. The change of the fine structure constant implied by the quasar absorption spectra together with the requirement of tracking behavior impose a lower bound of the size of this coupling. Furthermore, the transition to the quintessence regime implies a narrow window for this coupling around $10^{-5}$ in units of the inverse Planck mass. We also propose a non-minimal coupling between electromagnetism and quintessence which has the effect of leading only to changes of alpha determined from atomic physics phenomena, but leaving no observable consequences through nuclear physics effects. In doing so we are able to reconcile the claimed cosmological evidence for a changing fine structure constant with the tight constraints emerging from the Oklo natural nuclear reactor., Comment: 13 pages, 10 figures, RevTex, new references added

Published
2004

42. Tracking quintessential inflation from brane worlds

Author

Nelson J. Nunes and Edmund J. Copeland

Subjects
Physics, Nuclear and High Energy Physics, Astrophysics (astro-ph), Scalar (mathematics), Cosmic microwave background, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Parameter space, Astrophysics, General Relativity and Quantum Cosmology, Theoretical physics, Classical mechanics, Scale structure, Brane, Quintessence
Abstract

We analyse the mechanism of quintessential inflation in brane world scenarios for a number of particle physics inspired scalar potentials. We constrain the parameter space of those scalar potentials and comment on the likelihood that we could discriminate these models from standard inflation, based on upcoming large scale structure and cosmic microwave background observations., Comment: 8 pages, corrected typo in Eqs. (43) and (44)

Published
2002

43. Applications of scalar attractor solutions to cosmology

Author

F. Rosati, S. C. C. Ng, and Nelson J. Nunes

Subjects
High Energy Physics - Theory, Physics, Nuclear and High Energy Physics, Astrophysics (astro-ph), Scalar (mathematics), FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, General Relativity and Quantum Cosmology, Cosmology, Moduli, High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), Classical mechanics, High Energy Physics - Theory (hep-th), Phase space, Attractor, Energy density, Scalar field, Quintessence, Mathematical physics
Abstract

We develop a framework to study the phase space of a system consisting of a scalar field rolling down an arbitrary potential with varying slope and a background fluid, in a cosmological setting. We give analytical approximate solutions of the field evolution and discuss applications of its features to the issues of quintessence, moduli stabilisation and quintessential inflation., 9 pages, 7 figures. Accepted for publication in PRD

Published
2001

44. Quintessence models in supergravity

Author

Edmund J. Copeland, F. Rosati, and Nelson J. Nunes

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Supergravity, Astrophysics (astro-ph), Planck mass, FOS: Physical sciences, Context (language use), Expectation value, Astrophysics, Moduli, High Energy Physics - Phenomenology, General Relativity and Quantum Cosmology, Theoretical physics, High Energy Physics - Phenomenology (hep-ph), Higher-dimensional supergravity, Scalar field, Quintessence
Abstract

Scalar field models of quintessence typically require that the expectation value of the field today is of order the Planck mass, if we want them to explain the observed acceleration of the Universe. This suggests that we should be considering models in the context of supergravity. We discuss a particular class of supergravity models and analyze their behavior under different choices of the Kahler metric., Comment: 6 pages, revised version to appear in PRD

Published
2000

45. Quintessence arising from exponential potentials

Author

T. Barreiro, Nelson J. Nunes, and Edmund J. Copeland

Subjects
High Energy Physics - Theory, Physics, Coupling constant, Nuclear and High Energy Physics, Equation of state, Astrophysics (astro-ph), FOS: Physical sciences, Model parameters, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology, Exponential function, Range (mathematics), Classical mechanics, High Energy Physics - Theory (hep-th), Attractor, Statistical physics, Scaling, Quintessence
Abstract

We demonstrate how exponential potentials that could arise in the early Universe as a result of Kaluza-Klein type compactifications of string theory, can lead to cosmological solutions which correspond to the currently observed accelerating Universe. The idea is simple, relying solely on the known scaling properties associated with exponential potentials. In particular we show that the existence of stable attractor solutions implies that the results hold for a wide range of coupling constants and initial conditions., Comment: 4 pages, 3 figures, published version

Published
2000

46. Search for flavor-changing non-standard neutrino interactions by MINOS

Author

Adamson, P., primary, Barr, G., additional, Bishai, M., additional, Blake, A., additional, Bock, G. J., additional, Bogert, D., additional, Cao, S. V., additional, Cherdack, D., additional, Childress, S., additional, Coelho, J. A. B., additional, Corwin, L., additional, Cronin-Hennessy, D., additional, de Jong, J. K., additional, Devan, A. V., additional, Devenish, N. E., additional, Diwan, M. V., additional, Escobar, C. O., additional, Evans, J. J., additional, Falk, E., additional, Feldman, G. J., additional, Frohne, M. V., additional, Gallagher, H. R., additional, Gomes, R. A., additional, Goodman, M. C., additional, Gouffon, P., additional, Graf, N., additional, Gran, R., additional, Grzelak, K., additional, Habig, A., additional, Hartnell, J., additional, Hatcher, R., additional, Himmel, A., additional, Holin, A., additional, Hylen, J., additional, Irwin, G. M., additional, Isvan, Z., additional, James, C., additional, Jensen, D., additional, Kafka, T., additional, Kasahara, S. M. S., additional, Koizumi, G., additional, Kordosky, M., additional, Kreymer, A., additional, Lang, K., additional, Ling, J., additional, Litchfield, P. J., additional, Lucas, P., additional, Mann, W. A., additional, Marshak, M. L., additional, Mathis, M., additional, Mayer, N., additional, Medeiros, M. M., additional, Mehdiyev, R., additional, Meier, J. R., additional, Messier, M. D., additional, Miller, W. H., additional, Mishra, S. R., additional, Moed Sher, S., additional, Moore, C. D., additional, Mualem, L., additional, Mufson, S., additional, Musser, J., additional, Naples, D., additional, Nelson, J. K., additional, Newman, H. B., additional, Nichol, R. J., additional, Nowak, J. A., additional, Oliver, W. P., additional, Orchanian, M., additional, Pahlka, R. B., additional, Paley, J., additional, Patterson, R. B., additional, Pawloski, G., additional, Phan-Budd, S., additional, Plunkett, R. K., additional, Qiu, X., additional, Radovic, A., additional, Rebel, B., additional, Rosenfeld, C., additional, Rubin, H. A., additional, Sanchez, M. C., additional, Schneps, J., additional, Schreckenberger, A., additional, Schreiner, P., additional, Sharma, R., additional, Sousa, A., additional, Tagg, N., additional, Talaga, R. L., additional, Thomas, J., additional, Thomson, M. A., additional, Toner, R., additional, Torretta, D., additional, Tzanakos, G., additional, Urheim, J., additional, Vahle, P., additional, Viren, B., additional, Weber, A., additional, Webb, R. C., additional, White, C., additional, Whitehead, L., additional, Wojcicki, S. G., additional, and Zwaska, R., additional

Published
2013
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47. Erratum: Search for gravitational waves from binary black hole inspiral, merger, and ringdown [Phys. Rev. D83, 122005 (2011)]

Author

Abadie, J., primary, Abbott, B. P., additional, Abbott, R., additional, Abernathy, M., additional, Accadia, T., additional, Acernese, F., additional, Adams, C., additional, Adhikari, R., additional, Ajith, P., additional, Allen, B., additional, Allen, G. S., additional, Amador Ceron, E., additional, Amin, R. S., additional, Anderson, S. B., additional, Anderson, W. G., additional, Antonucci, F., additional, Arain, M. A., additional, Araya, M. C., additional, Aronsson, M., additional, Aso, Y., additional, Aston, S. M., additional, Astone, P., additional, Atkinson, D., additional, Aufmuth, P., additional, Aulbert, C., additional, Babak, S., additional, Baker, P., additional, Ballardin, G., additional, Ballinger, T., additional, Ballmer, S., additional, Barker, D., additional, Barnum, S., additional, Barone, F., additional, Barr, B., additional, Barriga, P., additional, Barsotti, L., additional, Barsuglia, M., additional, Barton, M. A., additional, Bartos, I., additional, Bassiri, R., additional, Bastarrika, M., additional, Bauchrowitz, J., additional, Bauer, Th. S., additional, Behnke, B., additional, Beker, M. G., additional, Belletoile, A., additional, Benacquista, M., additional, Bertolini, A., additional, Betzwieser, J., additional, Beveridge, N., additional, Beyersdorf, P. T., additional, Bilenko, I. A., additional, Billingsley, G., additional, Birch, J., additional, Birindelli, S., additional, Biswas, R., additional, Bitossi, M., additional, Bizouard, M. A., additional, Black, E., additional, Blackburn, J. K., additional, Blackburn, L., additional, Blair, D., additional, Bland, B., additional, Blom, M., additional, Boccara, C., additional, Bock, O., additional, Bodiya, T. P., additional, Bondarescu, R., additional, Bondu, F., additional, Bonelli, L., additional, Bonnand, R., additional, Bork, R., additional, Born, M., additional, Boschi, V., additional, Bose, S., additional, Bosi, L., additional, Bouhou, B., additional, Boyle, M., additional, Braccini, S., additional, Bradaschia, C., additional, Brady, P. R., additional, Braginsky, V. B., additional, Brau, J. E., additional, Breyer, J., additional, Bridges, D. O., additional, Brillet, A., additional, Brinkmann, M., additional, Brisson, V., additional, Britzger, M., additional, Brooks, A. F., additional, Brown, D. A., additional, Budzyński, R., additional, Bulik, T., additional, Bulten, H. J., additional, Buonanno, A., additional, Burguet–Castell, J., additional, Burmeister, O., additional, Buskulic, D., additional, Buy, C., additional, Byer, R. L., additional, Cadonati, L., additional, Cagnoli, G., additional, Cain, J., additional, Calloni, E., additional, Camp, J. B., additional, Campagna, E., additional, Campsie, P., additional, Cannizzo, J., additional, Cannon, K., additional, Canuel, B., additional, Cao, J., additional, Capano, C., additional, Carbognani, F., additional, Caride, S., additional, Caudill, S., additional, Cavaglià, M., additional, Cavalier, F., additional, Cavalieri, R., additional, Cella, G., additional, Cepeda, C., additional, Cesarini, E., additional, Chaibi, O., additional, Chalermsongsak, T., additional, Chalkley, E., additional, Charlton, P., additional, Chassande-Mottin, E., additional, Chelkowski, S., additional, Chen, Y., additional, Chincarini, A., additional, Christensen, N., additional, Chua, S. S. Y., additional, Chung, C. T. Y., additional, Clark, D., additional, Clark, J., additional, Clayton, J. H., additional, Cleva, F., additional, Coccia, E., additional, Colacino, C. N., additional, Colas, J., additional, Colla, A., additional, Colombini, M., additional, Conte, R., additional, Cook, D., additional, Corbitt, T. R., additional, Cornish, N., additional, Corsi, A., additional, Costa, C. A., additional, Coulon, J.-P., additional, Coward, D. M., additional, Coyne, D. C., additional, Creighton, J. D. E., additional, Creighton, T. D., additional, Cruise, A. M., additional, Culter, R. M., additional, Cumming, A., additional, Cunningham, L., additional, Cuoco, E., additional, Dahl, K., additional, Danilishin, S. L., additional, Dannenberg, R., additional, D’Antonio, S., additional, Danzmann, K., additional, Das, K., additional, Dattilo, V., additional, Daudert, B., additional, Davier, M., additional, Davies, G., additional, Davis, A., additional, Daw, E. J., additional, Day, R., additional, Dayanga, T., additional, De Rosa, R., additional, DeBra, D., additional, Debreczeni, G., additional, Degallaix, J., additional, del Prete, M., additional, Dent, T., additional, Dergachev, V., additional, DeRosa, R., additional, DeSalvo, R., additional, Devanka, P., additional, Dhurandhar, S., additional, Di Fiore, L., additional, Di Lieto, A., additional, Di Palma, I., additional, Di Paolo Emilio, M., additional, Di Virgilio, A., additional, Díaz, M., additional, Dietz, A., additional, Donovan, F., additional, Dooley, K. L., additional, Doomes, E. E., additional, Dorsher, S., additional, Douglas, E. S. D., additional, Drago, M., additional, Drever, R. W. P., additional, Driggers, J. C., additional, Dueck, J., additional, Dumas, J.-C., additional, Eberle, T., additional, Edgar, M., additional, Edwards, M., additional, Effler, A., additional, Ehrens, P., additional, Ely, G., additional, Engel, R., additional, Etzel, T., additional, Evans, M., additional, Evans, T., additional, Fafone, V., additional, Fairhurst, S., additional, Fan, Y., additional, Farr, B. F., additional, Fazi, D., additional, Fehrmann, H., additional, Feldbaum, D., additional, Ferrante, I., additional, Fidecaro, F., additional, Finn, L. S., additional, Fiori, I., additional, Flaminio, R., additional, Flanigan, M., additional, Flasch, K., additional, Foley, S., additional, Forrest, C., additional, Forsi, E., additional, Forte, L. A., additional, Fotopoulos, N., additional, Fournier, J.-D., additional, Franc, J., additional, Frasca, S., additional, Frasconi, F., additional, Frede, M., additional, Frei, M., additional, Frei, Z., additional, Freise, A., additional, Frey, R., additional, Fricke, T. T., additional, Friedrich, D., additional, Fritschel, P., additional, Frolov, V. V., additional, Fulda, P., additional, Fyffe, M., additional, Galimberti, M., additional, Gammaitoni, L., additional, Garofoli, J. A., additional, Garufi, F., additional, Gáspár, M. E., additional, Gemme, G., additional, Genin, E., additional, Gennai, A., additional, Gholami, I., additional, Ghosh, S., additional, Giaime, J. A., additional, Giampanis, S., additional, Giardina, K. D., additional, Giazotto, A., additional, Gill, C., additional, Goetz, E., additional, Goggin, L. M., additional, González, G., additional, Gorodetsky, M. L., additional, Goßler, S., additional, Gouaty, R., additional, Graef, C., additional, Granata, M., additional, Grant, A., additional, Gras, S., additional, Gray, C., additional, Greenhalgh, R. J. S., additional, Gretarsson, A. M., additional, Greverie, C., additional, Grosso, R., additional, Grote, H., additional, Grunewald, S., additional, Guidi, G. M., additional, Gustafson, E. K., additional, Gustafson, R., additional, Hage, B., additional, Hall, P., additional, Hallam, J. M., additional, Hammer, D., additional, Hammond, G., additional, Hanks, J., additional, Hanna, C., additional, Hanson, J., additional, Harms, J., additional, Harry, G. M., additional, Harry, I. W., additional, Harstad, E. D., additional, Haughian, K., additional, Hayama, K., additional, Hayau, J.-F., additional, Hayler, T., additional, Heefner, J., additional, Heitmann, H., additional, Hello, P., additional, Heng, I. S., additional, Heptonstall, A. W., additional, Hewitson, M., additional, Hild, S., additional, Hirose, E., additional, Hoak, D., additional, Hodge, K. A., additional, Holt, K., additional, Hosken, D. J., additional, Hough, J., additional, Howell, E. J., additional, Hoyland, D., additional, Huet, D., additional, Hughey, B., additional, Husa, S., additional, Huttner, S. H., additional, Huynh–Dinh, T., additional, Ingram, D. R., additional, Inta, R., additional, Isogai, T., additional, Ivanov, A., additional, Jaranowski, P., additional, Johnson, W. W., additional, Jones, D. I., additional, Jones, G., additional, Jones, R., additional, Ju, L., additional, Kalmus, P., additional, Kalogera, V., additional, Kandhasamy, S., additional, Kanner, J. B., additional, Katsavounidis, E., additional, Kawabe, K., additional, Kawamura, S., additional, Kawazoe, F., additional, Kells, W., additional, Keppel, D. G., additional, Khalaidovski, A., additional, Khalili, F. Y., additional, Khazanov, E. A., additional, Kim, H., additional, King, P. J., additional, Kinzel, D. L., additional, Kissel, J. S., additional, Klimenko, S., additional, Kondrashov, V., additional, Kopparapu, R., additional, Koranda, S., additional, Kowalska, I., additional, Kozak, D., additional, Krause, T., additional, Kringel, V., additional, Krishnamurthy, S., additional, Krishnan, B., additional, Królak, A., additional, Kuehn, G., additional, Kullman, J., additional, Kumar, R., additional, Kwee, P., additional, Landry, M., additional, Lang, M., additional, Lantz, B., additional, Lastzka, N., additional, Lazzarini, A., additional, Leaci, P., additional, Leong, J., additional, Leonor, I., additional, Leroy, N., additional, Letendre, N., additional, Li, J., additional, Li, T. G. F., additional, Liguori, N., additional, Lin, H., additional, Lindquist, P. E., additional, Lockerbie, N. A., additional, Lodhia, D., additional, Lorenzini, M., additional, Loriette, V., additional, Lormand, M., additional, Losurdo, G., additional, Lu, P., additional, Luan, J., additional, Lubinski, M., additional, Lucianetti, A., additional, Lück, H., additional, Lundgren, A. D., additional, Machenschalk, B., additional, MacInnis, M., additional, Mageswaran, M., additional, Mailand, K., additional, Majorana, E., additional, Mak, C., additional, Maksimovic, I., additional, Man, N., additional, Mandel, I., additional, Mandic, V., additional, Mantovani, M., additional, Marchesoni, F., additional, Marion, F., additional, Márka, S., additional, Márka, Z., additional, Maros, E., additional, Marque, J., additional, Martelli, F., additional, Martin, I. W., additional, Martin, R. M., additional, Marx, J. N., additional, Mason, K., additional, Masserot, A., additional, Matichard, F., additional, Matone, L., additional, Matzner, R. A., additional, Mavalvala, N., additional, McCarthy, R., additional, McClelland, D. E., additional, McGuire, S. C., additional, McIntyre, G., additional, McIvor, G., additional, McKechan, D. J. A., additional, Meadors, G., additional, Mehmet, M., additional, Meier, T., additional, Melatos, A., additional, Melissinos, A. C., additional, Mendell, G., additional, Menéndez, D. F., additional, Mercer, R. A., additional, Merill, L., additional, Meshkov, S., additional, Messenger, C., additional, Meyer, M. S., additional, Miao, H., additional, Michel, C., additional, Milano, L., additional, Miller, J., additional, Minenkov, Y., additional, Mino, Y., additional, Mitra, S., additional, Mitrofanov, V. P., additional, Mitselmakher, G., additional, Mittleman, R., additional, Moe, B., additional, Mohan, M., additional, Mohanty, S. D., additional, Mohapatra, S. R. P., additional, Moraru, D., additional, Moreau, J., additional, Moreno, G., additional, Morgado, N., additional, Morgia, A., additional, Morioka, T., additional, Mors, K., additional, Mosca, S., additional, Moscatelli, V., additional, Mossavi, K., additional, Mours, B., additional, Mow–Lowry, C. M., additional, Mueller, G., additional, Mukherjee, S., additional, Mullavey, A., additional, Müller-Ebhardt, H., additional, Munch, J., additional, Murray, P. G., additional, Nash, T., additional, Nawrodt, R., additional, Nelson, J., additional, Neri, I., additional, Newton, G., additional, Nishizawa, A., additional, Nocera, F., additional, Nolting, D., additional, Ochsner, E., additional, O’Dell, J., additional, Ogin, G. H., additional, Oldenburg, R. G., additional, O’Reilly, B., additional, O’Shaughnessy, R., additional, Osthelder, C., additional, Ottaway, D. J., additional, Ottens, R. S., additional, Overmier, H., additional, Owen, B. J., additional, Page, A., additional, Pagliaroli, G., additional, Palladino, L., additional, Palomba, C., additional, Pan, Y., additional, Pankow, C., additional, Paoletti, F., additional, Papa, M. A., additional, Pardi, S., additional, Pareja, M., additional, Parisi, M., additional, Pasqualetti, A., additional, Passaquieti, R., additional, Passuello, D., additional, Patel, P., additional, Pathak, D., additional, Pedraza, M., additional, Pekowsky, L., additional, Penn, S., additional, Peralta, C., additional, Perreca, A., additional, Persichetti, G., additional, Pichot, M., additional, Pickenpack, M., additional, Piergiovanni, F., additional, Pietka, M., additional, Pinard, L., additional, Pinto, I. M., additional, Pitkin, M., additional, Pletsch, H. J., additional, Plissi, M. V., additional, Poggiani, R., additional, Postiglione, F., additional, Prato, M., additional, Predoi, V., additional, Price, L. R., additional, Prijatelj, M., additional, Principe, M., additional, Privitera, S., additional, Prix, R., additional, Prodi, G. A., additional, Prokhorov, L., additional, Puncken, O., additional, Punturo, M., additional, Puppo, P., additional, Quetschke, V., additional, Raab, F. J., additional, Rabeling, D. S., additional, Rácz, I., additional, Radke, T., additional, Radkins, H., additional, Raffai, P., additional, Rakhmanov, M., additional, Rankins, B., additional, Rapagnani, P., additional, Raymond, V., additional, Re, V., additional, Reed, C. M., additional, Reed, T., additional, Regimbau, T., additional, Reid, S., additional, Reitze, D. H., additional, Ricci, F., additional, Riesen, R., additional, Riles, K., additional, Roberts, P., additional, Robertson, N. A., additional, Robinet, F., additional, Robinson, C., additional, Robinson, E. L., additional, Rocchi, A., additional, Roddy, S., additional, Rolland, L., additional, Rollins, J., additional, Romano, J. D., additional, Romano, R., additional, Romie, J. H., additional, Rosińska, D., additional, Röver, C., additional, Rowan, S., additional, Rüdiger, A., additional, Ruggi, P., additional, Ryan, K., additional, Sakata, S., additional, Sakosky, M., additional, Salemi, F., additional, Sammut, L., additional, Sancho de la Jordana, L., additional, Sandberg, V., additional, Sannibale, V., additional, Santamaría, L., additional, Santostasi, G., additional, Saraf, S., additional, Sassolas, B., additional, Sathyaprakash, B. S., additional, Sato, S., additional, Satterthwaite, M., additional, Saulson, P. R., additional, Savage, R., additional, Schilling, R., additional, Schnabel, R., additional, Schofield, R. M. S., additional, Schulz, B., additional, Schutz, B. F., additional, Schwinberg, P., additional, Scott, J., additional, Scott, S. M., additional, Searle, A. C., additional, Seifert, F., additional, Sellers, D., additional, Sengupta, A. S., additional, Sentenac, D., additional, Sergeev, A., additional, Shaddock, D. A., additional, Shapiro, B., additional, Shawhan, P., additional, Shoemaker, D. H., additional, Sibley, A., additional, Siemens, X., additional, Sigg, D., additional, Singer, A., additional, Sintes, A. M., additional, Skelton, G., additional, Slagmolen, B. J. J., additional, Slutsky, J., additional, Smith, J. R., additional, Smith, M. R., additional, Smith, N. D., additional, Somiya, K., additional, Sorazu, B., additional, Speirits, F. C., additional, Sperandio, L., additional, Stein, A. J., additional, Stein, L. C., additional, Steinlechner, S., additional, Steplewski, S., additional, Stochino, A., additional, Stone, R., additional, Strain, K. A., additional, Strigin, S., additional, Stroeer, A. S., additional, Sturani, R., additional, Stuver, A. L., additional, Summerscales, T. Z., additional, Sung, M., additional, Susmithan, S., additional, Sutton, P. J., additional, Swinkels, B., additional, Szokoly, G. P., additional, Tacca, M., additional, Talukder, D., additional, Tanner, D. B., additional, Tarabrin, S. P., additional, Taylor, J. R., additional, Taylor, R., additional, Thomas, P., additional, Thorne, K. A., additional, Thorne, K. S., additional, Thrane, E., additional, Thüring, A., additional, Titsler, C., additional, Tokmakov, K. V., additional, Toncelli, A., additional, Tonelli, M., additional, Torre, O., additional, Torres, C., additional, Torrie, C. I., additional, Tournefier, E., additional, Travasso, F., additional, Traylor, G., additional, Trias, M., additional, Tseng, K., additional, Turner, L., additional, Ugolini, D., additional, Urbanek, K., additional, Vahlbruch, H., additional, Vaishnav, B., additional, Vajente, G., additional, Vallisneri, M., additional, van den Brand, J. F. J., additional, Van Den Broeck, C., additional, van der Putten, S., additional, van der Sluys, M. V., additional, van Veggel, A. A., additional, Vass, S., additional, Vasuth, M., additional, Vaulin, R., additional, Vavoulidis, M., additional, Vecchio, A., additional, Vedovato, G., additional, Veitch, J., additional, Veitch, P. J., additional, Veltkamp, C., additional, Verkindt, D., additional, Vetrano, F., additional, Viceré, A., additional, Villar, A. E., additional, Vinet, J.-Y., additional, Vocca, H., additional, Vorvick, C., additional, Vyachanin, S. P., additional, Waldman, S. J., additional, Wallace, L., additional, Wanner, A., additional, Ward, R. L., additional, Was, M., additional, Wei, P., additional, Weinert, M., additional, Weinstein, A. J., additional, Weiss, R., additional, Wen, L., additional, Wen, S., additional, Wessels, P., additional, West, M., additional, Westphal, T., additional, Wette, K., additional, Whelan, J. T., additional, Whitcomb, S. E., additional, White, D., additional, Whiting, B. F., additional, Wilkinson, C., additional, Willems, P. A., additional, Williams, L., additional, Willke, B., additional, Winkelmann, L., additional, Winkler, W., additional, Wipf, C. C., additional, Wiseman, A. G., additional, Woan, G., additional, Wooley, R., additional, Worden, J., additional, Yakushin, I., additional, Yamamoto, H., additional, Yamamoto, K., additional, Yeaton-Massey, D., additional, Yoshida, S., additional, Yu, P., additional, Yvert, M., additional, Zanolin, M., additional, Zhang, L., additional, Zhang, Z., additional, Zhao, C., additional, Zotov, N., additional, Zucker, M. E., additional, and Zweizig, J., additional

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2012
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48. Measurements of atmospheric neutrinos and antineutrinos in the MINOS far detector

Author

Adamson, P., primary, Backhouse, C., additional, Barr, G., additional, Bishai, M., additional, Blake, A. S. T., additional, Bock, G. J., additional, Boehnlein, D. J., additional, Bogert, D., additional, Cao, S. V., additional, Chapman, J. D., additional, Childress, S., additional, Coelho, J. A. B., additional, Corwin, L., additional, Cronin-Hennessy, D., additional, Danko, I. Z., additional, de Jong, J. K., additional, Devenish, N. E., additional, Diwan, M. V., additional, Escobar, C. O., additional, Evans, J. J., additional, Falk, E., additional, Feldman, G. J., additional, Frohne, M. V., additional, Gallagher, H. R., additional, Gomes, R. A., additional, Goodman, M. C., additional, Gouffon, P., additional, Graf, N., additional, Gran, R., additional, Grzelak, K., additional, Habig, A., additional, Hartnell, J., additional, Hatcher, R., additional, Himmel, A., additional, Holin, A., additional, Hylen, J., additional, Irwin, G. M., additional, Isvan, Z., additional, Jaffe, D. E., additional, James, C., additional, Jensen, D., additional, Kafka, T., additional, Kasahara, S. M. S., additional, Koizumi, G., additional, Kopp, S., additional, Kordosky, M., additional, Kreymer, A., additional, Lang, K., additional, Ling, J., additional, Litchfield, P. J., additional, Loiacono, L., additional, Lucas, P., additional, Mann, W. A., additional, Marshak, M. L., additional, Mathis, M., additional, Mayer, N., additional, Medeiros, M. M., additional, Mehdiyev, R., additional, Meier, J. R., additional, Messier, M. D., additional, Miller, W. H., additional, Mishra, S. R., additional, Mitchell, J., additional, Moore, C. D., additional, Mualem, L., additional, Mufson, S., additional, Musser, J., additional, Naples, D., additional, Nelson, J. K., additional, Newman, H. B., additional, Nichol, R. J., additional, Nowak, J. A., additional, Oliver, W. P., additional, Orchanian, M., additional, Pahlka, R. B., additional, Paley, J., additional, Patterson, R. B., additional, Pawloski, G., additional, Phan-Budd, S., additional, Plunkett, R. K., additional, Qiu, X., additional, Radovic, A., additional, Ratchford, J., additional, Rebel, B., additional, Rosenfeld, C., additional, Rubin, H. A., additional, Sanchez, M. C., additional, Schneps, J., additional, Schreckenberger, A., additional, Schreiner, P., additional, Sharma, R., additional, Sousa, A., additional, Speakman, B., additional, Strait, M., additional, Tagg, N., additional, Talaga, R. L., additional, Thomas, J., additional, Thomson, M. A., additional, Toner, R., additional, Torretta, D., additional, Tzanakos, G., additional, Urheim, J., additional, Vahle, P., additional, Viren, B., additional, Walding, J. J., additional, Weber, A., additional, Webb, R. C., additional, White, C., additional, Whitehead, L., additional, Wojcicki, S. G., additional, Zhang, K., additional, and Zwaska, R., additional

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2012
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50. Search for gravitational waves from low mass compact binary coalescence in LIGO’s sixth science run and Virgo’s science runs 2 and 3

Author

Abadie, J., primary, Abbott, B. P., additional, Abbott, R., additional, Abbott, T. D., additional, Abernathy, M., additional, Accadia, T., additional, Acernese, F., additional, Adams, C., additional, Adhikari, R., additional, Affeldt, C., additional, Agathos, M., additional, Ajith, P., additional, Allen, B., additional, Allen, G. S., additional, Amador Ceron, E., additional, Amariutei, D., additional, Amin, R. S., additional, Anderson, S. B., additional, Anderson, W. G., additional, Arai, K., additional, Arain, M. A., additional, Araya, M. C., additional, Aston, S. M., additional, Astone, P., additional, Atkinson, D., additional, Aufmuth, P., additional, Aulbert, C., additional, Aylott, B. E., additional, Babak, S., additional, Baker, P., additional, Ballardin, G., additional, Ballmer, S., additional, Barker, D., additional, Barone, F., additional, Barr, B., additional, Barriga, P., additional, Barsotti, L., additional, Barsuglia, M., additional, Barton, M. A., additional, Bartos, I., additional, Bassiri, R., additional, Bastarrika, M., additional, Basti, A., additional, Batch, J., additional, Bauchrowitz, J., additional, Bauer, Th. S., additional, Bebronne, M., additional, Behnke, B., additional, Beker, M. G., additional, Bell, A. S., additional, Belletoile, A., additional, Belopolski, I., additional, Benacquista, M., additional, Berliner, J. M., additional, Bertolini, A., additional, Betzwieser, J., additional, Beveridge, N., additional, Beyersdorf, P. T., additional, Bilenko, I. A., additional, Billingsley, G., additional, Birch, J., additional, Biswas, R., additional, Bitossi, M., additional, Bizouard, M. A., additional, Black, E., additional, Blackburn, J. K., additional, Blackburn, L., additional, Blair, D., additional, Bland, B., additional, Blom, M., additional, Bock, O., additional, Bodiya, T. P., additional, Bogan, C., additional, Bondarescu, R., additional, Bondu, F., additional, Bonelli, L., additional, Bonnand, R., additional, Bork, R., additional, Born, M., additional, Boschi, V., additional, Bose, S., additional, Bosi, L., additional, Bouhou, B., additional, Braccini, S., additional, Bradaschia, C., additional, Brady, P. R., additional, Braginsky, V. B., additional, Branchesi, M., additional, Brau, J. E., additional, Breyer, J., additional, Briant, T., additional, Bridges, D. O., additional, Brillet, A., additional, Brinkmann, M., additional, Brisson, V., additional, Britzger, M., additional, Brooks, A. F., additional, Brown, D. A., additional, Brummit, A., additional, Bulik, T., additional, Bulten, H. J., additional, Buonanno, A., additional, Burguet–Castell, J., additional, Burmeister, O., additional, Buskulic, D., additional, Buy, C., additional, Byer, R. L., additional, Cadonati, L., additional, Cagnoli, G., additional, Calloni, E., additional, Camp, J. B., additional, Campsie, P., additional, Cannizzo, J., additional, Cannon, K., additional, Canuel, B., additional, Cao, J., additional, Capano, C. D., additional, Carbognani, F., additional, Caride, S., additional, Caudill, S., additional, Cavaglià, M., additional, Cavalier, F., additional, Cavalieri, R., additional, Cella, G., additional, Cepeda, C., additional, Cesarini, E., additional, Chaibi, O., additional, Chalermsongsak, T., additional, Chalkley, E., additional, Charlton, P., additional, Chassande-Mottin, E., additional, Chelkowski, S., additional, Chen, Y., additional, Chincarini, A., additional, Chiummo, A., additional, Cho, H., additional, Christensen, N., additional, Chua, S. S. Y., additional, Chung, C. T. Y., additional, Chung, S., additional, Ciani, G., additional, Clara, F., additional, Clark, D. E., additional, Clark, J., additional, Clayton, J. H., additional, Cleva, F., additional, Coccia, E., additional, Cohadon, P.-F., additional, Colacino, C. N., additional, Colas, J., additional, Colla, A., additional, Colombini, M., additional, Conte, A., additional, Conte, R., additional, Cook, D., additional, Corbitt, T. R., additional, Cordier, M., additional, Cornish, N., additional, Corsi, A., additional, Costa, C. A., additional, Coughlin, M., additional, Coulon, J.-P., additional, Couvares, P., additional, Coward, D. M., additional, Coyne, D. C., additional, Creighton, J. D. E., additional, Creighton, T. D., additional, Cruise, A. M., additional, Cumming, A., additional, Cunningham, L., additional, Cuoco, E., additional, Cutler, R. M., additional, Dahl, K., additional, Danilishin, S. L., additional, Dannenberg, R., additional, D’Antonio, S., additional, Danzmann, K., additional, Dattilo, V., additional, Daudert, B., additional, Daveloza, H., additional, Davier, M., additional, Davies, G., additional, Daw, E. J., additional, Day, R., additional, Dayanga, T., additional, De Rosa, R., additional, DeBra, D., additional, Debreczeni, G., additional, Degallaix, J., additional, Del Pozzo, W., additional, del Prete, M., additional, Dent, T., additional, Dergachev, V., additional, DeRosa, R., additional, DeSalvo, R., additional, Dhurandhar, S., additional, Di Fiore, L., additional, Di Lieto, A., additional, Di Palma, I., additional, Di Paolo Emilio, M., additional, Di Virgilio, A., additional, Díaz, M., additional, Dietz, A., additional, DiGuglielmo, J., additional, Donovan, F., additional, Dooley, K. L., additional, Dorsher, S., additional, Drago, M., additional, Drever, R. W. P., additional, Driggers, J. C., additional, Du, Z., additional, Dumas, J.-C., additional, Dwyer, S., additional, Eberle, T., additional, Edgar, M., additional, Edwards, M., additional, Effler, A., additional, Ehrens, P., additional, Endrőczi, G., additional, Engel, R., additional, Etzel, T., additional, Evans, K., additional, Evans, M., additional, Evans, T., additional, Factourovich, M., additional, Fafone, V., additional, Fairhurst, S., additional, Fan, Y., additional, Farr, B. F., additional, Farr, W., additional, Fazi, D., additional, Fehrmann, H., additional, Feldbaum, D., additional, Ferrante, I., additional, Fidecaro, F., additional, Finn, L. S., additional, Fiori, I., additional, Fisher, R. P., additional, Flaminio, R., additional, Flanigan, M., additional, Foley, S., additional, Forsi, E., additional, Forte, L. A., additional, Fotopoulos, N., additional, Fournier, J.-D., additional, Franc, J., additional, Frasca, S., additional, Frasconi, F., additional, Frede, M., additional, Frei, M., additional, Frei, Z., additional, Freise, A., additional, Frey, R., additional, Fricke, T. T., additional, Friedrich, D., additional, Fritschel, P., additional, Frolov, V. V., additional, Fulda, P. J., additional, Fyffe, M., additional, Galimberti, M., additional, Gammaitoni, L., additional, Ganija, M. R., additional, Garcia, J., additional, Garofoli, J. A., additional, Garufi, F., additional, Gáspár, M. E., additional, Gemme, G., additional, Geng, R., additional, Genin, E., additional, Gennai, A., additional, Gergely, L. Á., additional, Ghosh, S., additional, Giaime, J. A., additional, Giampanis, S., additional, Giardina, K. D., additional, Giazotto, A., additional, Gill, C., additional, Goetz, E., additional, Goggin, L. M., additional, González, G., additional, Gorodetsky, M. 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C., additional, Heitmann, H., additional, Hello, P., additional, Hendry, M. A., additional, Heng, I. S., additional, Heptonstall, A. W., additional, Herrera, V., additional, Hewitson, M., additional, Hild, S., additional, Hoak, D., additional, Hodge, K. A., additional, Holt, K., additional, Hong, T., additional, Hooper, S., additional, Hosken, D. J., additional, Hough, J., additional, Howell, E. J., additional, Hughey, B., additional, Husa, S., additional, Huttner, S. H., additional, Huynh-Dinh, T., additional, Ingram, D. R., additional, Inta, R., additional, Isogai, T., additional, Ivanov, A., additional, Izumi, K., additional, Jacobson, M., additional, Jang, H., additional, Jaranowski, P., additional, Johnson, W. W., additional, Jones, D. I., additional, Jones, G., additional, Jones, R., additional, Ju, L., additional, Kalmus, P., additional, Kalogera, V., additional, Kamaretsos, I., additional, Kandhasamy, S., additional, Kang, G., additional, Kanner, J. B., additional, Katsavounidis, E., additional, Katzman, W., additional, Kaufer, H., additional, Kawabe, K., additional, Kawamura, S., additional, Kawazoe, F., additional, Kells, W., additional, Keppel, D. G., additional, Keresztes, Z., additional, Khalaidovski, A., additional, Khalili, F. Y., additional, Khazanov, E. A., additional, Kim, B., additional, Kim, C., additional, Kim, D., additional, Kim, H., additional, Kim, K., additional, Kim, N., additional, Kim, Y.-M., additional, King, P. J., additional, Kinsey, M., additional, Kinzel, D. L., additional, Kissel, J. S., additional, Klimenko, S., additional, Kokeyama, K., additional, Kondrashov, V., additional, Kopparapu, R., additional, Koranda, S., additional, Korth, W. Z., additional, Kowalska, I., additional, Kozak, D., additional, Kringel, V., additional, Krishnamurthy, S., additional, Krishnan, B., additional, Królak, A., additional, Kuehn, G., additional, Kumar, R., additional, Kwee, P., additional, Lam, P. K., additional, Landry, M., additional, Lang, M., additional, Lantz, B., additional, Lastzka, N., additional, Lawrie, C., additional, Lazzarini, A., additional, Leaci, P., additional, Lee, C. H., additional, Lee, H. M., additional, Leindecker, N., additional, Leong, J. R., additional, Leonor, I., additional, Leroy, N., additional, Letendre, N., additional, Li, J., additional, Li, T. G. F., additional, Liguori, N., additional, Lindquist, P. E., additional, Lockerbie, N. A., additional, Lodhia, D., additional, Lorenzini, M., additional, Loriette, V., additional, Lormand, M., additional, Losurdo, G., additional, Luan, J., additional, Lubinski, M., additional, Lück, H., additional, Lundgren, A. P., additional, Macdonald, E., additional, Machenschalk, B., additional, MacInnis, M., additional, Macleod, D. M., additional, Mageswaran, M., additional, Mailand, K., additional, Majorana, E., additional, Maksimovic, I., additional, Man, N., additional, Mandel, I., additional, Mandic, V., additional, Mantovani, M., additional, Marandi, A., additional, Marchesoni, F., additional, Marion, F., additional, Márka, S., additional, Márka, Z., additional, Markosyan, A., additional, Maros, E., additional, Marque, J., additional, Martelli, F., additional, Martin, I. W., additional, Martin, R. M., additional, Marx, J. N., additional, Mason, K., additional, Masserot, A., additional, Matichard, F., additional, Matone, L., additional, Matzner, R. A., additional, Mavalvala, N., additional, Mazzolo, G., additional, McCarthy, R., additional, McClelland, D. E., additional, McGuire, S. C., additional, McIntyre, G., additional, McIver, J., additional, McKechan, D. J. A., additional, Meadors, G. D., additional, Mehmet, M., additional, Meier, T., additional, Melatos, A., additional, Melissinos, A. C., additional, Mendell, G., additional, Menendez, D., additional, Mercer, R. A., additional, Meshkov, S., additional, Messenger, C., additional, Meyer, M. S., additional, Miao, H., additional, Michel, C., additional, Milano, L., additional, Miller, J., additional, Minenkov, Y., additional, Mitrofanov, V. P., additional, Mitselmakher, G., additional, Mittleman, R., additional, Miyakawa, O., additional, Moe, B., additional, Moesta, P., additional, Mohan, M., additional, Mohanty, S. D., additional, Mohapatra, S. R. P., additional, Moraru, D., additional, Moreno, G., additional, Morgado, N., additional, Morgia, A., additional, Mori, T., additional, Mosca, S., additional, Mossavi, K., additional, Mours, B., additional, Mow-Lowry, C. M., additional, Mueller, C. L., additional, Mueller, G., additional, Mukherjee, S., additional, Mullavey, A., additional, Müller-Ebhardt, H., additional, Munch, J., additional, Murphy, D., additional, Murray, P. G., additional, Mytidis, A., additional, Nash, T., additional, Naticchioni, L., additional, Nawrodt, R., additional, Necula, V., additional, Nelson, J., additional, Newton, G., additional, Nishizawa, A., additional, Nocera, F., additional, Nolting, D., additional, Nuttall, L., additional, Ochsner, E., additional, O’Dell, J., additional, Oelker, E., additional, Ogin, G. H., additional, Oh, J. J., additional, Oh, S. H., additional, Oldenburg, R. G., additional, O’Reilly, B., additional, O’Shaughnessy, R., additional, Osthelder, C., additional, Ott, C. D., additional, Ottaway, D. J., additional, Ottens, R. S., additional, Overmier, H., additional, Owen, B. J., additional, Page, A., additional, Pagliaroli, G., additional, Palladino, L., additional, Palomba, C., additional, Pan, Y., additional, Pankow, C., additional, Paoletti, F., additional, Papa, M. A., additional, Parisi, M., additional, Pasqualetti, A., additional, Passaquieti, R., additional, Passuello, D., additional, Patel, P., additional, Pedraza, M., additional, Peiris, P., additional, Pekowsky, L., additional, Penn, S., additional, Peralta, C., additional, Perreca, A., additional, Persichetti, G., additional, Phelps, M., additional, Pickenpack, M., additional, Piergiovanni, F., additional, Pietka, M., additional, Pinard, L., additional, Pinto, I. M., additional, Pitkin, M., additional, Pletsch, H. J., additional, Plissi, M. V., additional, Poggiani, R., additional, Pöld, J., additional, Postiglione, F., additional, Prato, M., additional, Predoi, V., additional, Price, L. R., additional, Prijatelj, M., additional, Principe, M., additional, Privitera, S., additional, Prix, R., additional, Prodi, G. A., additional, Prokhorov, L., additional, Puncken, O., additional, Punturo, M., additional, Puppo, P., additional, Quetschke, V., additional, Raab, F. J., additional, Rabeling, D. S., additional, Rácz, I., additional, Radkins, H., additional, Raffai, P., additional, Rakhmanov, M., additional, Ramet, C. R., additional, Rankins, B., additional, Rapagnani, P., additional, Raymond, V., additional, Re, V., additional, Redwine, K., additional, Reed, C. M., additional, Reed, T., additional, Regimbau, T., additional, Reid, S., additional, Reitze, D. H., additional, Ricci, F., additional, Riesen, R., additional, Riles, K., additional, Robertson, N. A., additional, Robinet, F., additional, Robinson, C., additional, Robinson, E. L., additional, Rocchi, A., additional, Roddy, S., additional, Rodriguez, C., additional, Rodruck, M., additional, Rolland, L., additional, Rollins, J., additional, Romano, J. D., additional, Romano, R., additional, Romie, J. H., additional, Rosińska, D., additional, Röver, C., additional, Rowan, S., additional, Rüdiger, A., additional, Ruggi, P., additional, Ryan, K., additional, Ryll, H., additional, Sainathan, P., additional, Sakosky, M., additional, Salemi, F., additional, Samblowski, A., additional, Sammut, L., additional, Sancho de la Jordana, L., additional, Sandberg, V., additional, Sankar, S., additional, Sannibale, V., additional, Santamaría, L., additional, Santiago-Prieto, I., additional, Santostasi, G., additional, Sassolas, B., additional, Sathyaprakash, B. S., additional, Sato, S., additional, Saulson, P. R., additional, Savage, R. L., additional, Schilling, R., additional, Schlamminger, S., additional, Schnabel, R., additional, Schofield, R. M. S., additional, Schulz, B., additional, Schutz, B. F., additional, Schwinberg, P., additional, Scott, J., additional, Scott, S. M., additional, Searle, A. C., additional, Seifert, F., additional, Sellers, D., additional, Sengupta, A. S., additional, Sentenac, D., additional, Sergeev, A., additional, Shaddock, D. A., additional, Shaltev, M., additional, Shapiro, B., additional, Shawhan, P., additional, Shoemaker, D. H., additional, Sibley, A., additional, Siemens, X., additional, Sigg, D., additional, Singer, A., additional, Singer, L., additional, Sintes, A. M., additional, Skelton, G., additional, Slagmolen, B. J. J., additional, Slutsky, J., additional, Smith, J. R., additional, Smith, M. R., additional, Smith, N. D., additional, Smith, R. J. E., additional, Somiya, K., additional, Sorazu, B., additional, Soto, J., additional, Speirits, F. C., additional, Sperandio, L., additional, Stefszky, M., additional, Stein, A. J., additional, Steinert, E., additional, Steinlechner, J., additional, Steinlechner, S., additional, Steplewski, S., additional, Stochino, A., additional, Stone, R., additional, Strain, K. A., additional, Strigin, S., additional, Stroeer, A. S., additional, Sturani, R., additional, Stuver, A. 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J., additional, Van Den Broeck, C., additional, van der Putten, S., additional, van Veggel, A. A., additional, Vass, S., additional, Vasuth, M., additional, Vaulin, R., additional, Vavoulidis, M., additional, Vecchio, A., additional, Vedovato, G., additional, Veitch, J., additional, Veitch, P. J., additional, Veltkamp, C., additional, Verkindt, D., additional, Vetrano, F., additional, Viceré, A., additional, Villar, A. E., additional, Vinet, J.-Y., additional, Vitale, S., additional, Vocca, H., additional, Vorvick, C., additional, Vyatchanin, S. P., additional, Wade, A., additional, Waldman, S. J., additional, Wallace, L., additional, Wan, Y., additional, Wang, X., additional, Wang, Z., additional, Wanner, A., additional, Ward, R. L., additional, Was, M., additional, Wei, P., additional, Weinert, M., additional, Weinstein, A. 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G., additional, Wittel, H., additional, Woan, G., additional, Wooley, R., additional, Worden, J., additional, Yablon, J., additional, Yakushin, I., additional, Yamamoto, H., additional, Yamamoto, K., additional, Yang, H., additional, Yeaton-Massey, D., additional, Yoshida, S., additional, Yu, P., additional, Yvert, M., additional, Zadroźny, A., additional, Zanolin, M., additional, Zendri, J.-P., additional, Zhang, F., additional, Zhang, L., additional, Zhang, W., additional, Zhang, Z., additional, Zhao, C., additional, Zotov, N., additional, Zucker, M. E., additional, and Zweizig, J., additional

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2012
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