Searching for eV-scale sterile neutrinos with eight years of atmospheric neutrinos at the IceCube Neutrino Telescope

Autor: Aartsen, M. G., Abbasi, R., Anderson, T., Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Grégoire, T., Ansseau, I., Griffith, Z., Griswold, S., Günder, M., Gündüz, M., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hanson, K., Anton, G., Hardin, J., Haungs, A., Hauser, S., Hebecker, D., Heereman, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Argüelles, C., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Huber, Thomas, Auffenberg, J., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jones, B. J. P., Axani, S., Jonske, F., Joppe, R., Kang, D., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Katz, U., Bagherpour, H., Kauer, M., Kellermann, M., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, Thomas, Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Bai, X., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Koundal, P., Kowalski, M., Krings, K., Krückl, G., Kulacz, N., Balagopal, A., V., Kurahashi, N., Kyriacou, A., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Li, Y., Liu, Q. R., Barbano, A., Lohfink, E., Lozano Mariscal, C. J., Lu, L., Lucarelli, F., Ludwig, A., Lünemann, J., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Ackermann, M., Barwick, S. W., Maggi, G., Mahn, K. B. M., Makino, Y., Mallik, P., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., Maunu, R., McNally, F., Bastian, B., Meagher, K., Medici, M., Medina, A., Meier, M., Meighen-Berger, S., Merz, J., Meures, T., Micallef, J., Mockler, D., Momenté, G., Basu, V., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Nagai, R., Naumann, U., Neer, G., Nguyen, L. V., Niederhausen, H., Baum, V., Nisa, M. U., Nowicki, S. C., Nygren, D. R., Obertacke Pollmann, A., Oehler, M., Olivas, A., O'Murchadha, A., O'Sullivan, E., Palczewski, T., Pandya, H., Baur, S., Pankova, D. V., Park, N., Parker, G. K., Paudel, E. N., Peiffer, P., Pérez de los Heros, C., Philippen, S., Pieloth, D., Pieper, S., Pinat, E., Bay, R., Pizzuto, A., Plum, M., Popovych, Y., Porcelli, A., Prado Rodriguez, M., Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Beatty, J. J., Rauch, L., Rawlins, K., Rea, I. C., Rehman, A., Reimann, R., Relethford, B., Renschler, M., Renzi, G., Resconi, E., Rhode, W., Becker, K.-H., Richman, M., Riedel, B., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk Cantu, D., Safa, I., Sanchez Herrera, S. E., Becker Tjus, J., Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Scharf, M., Schaufel, M., Schieler, H., Schlunder, P., BenZvi, S., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shefali, S., Silva, M., Adams, J., Berley, D., Smithers, B., Snihur, R., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Bernardini, E., Stein, Robert, Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stössl, A., Strotjohann, Nora Linn, Stürwald, T., Stuttard, T., Sullivan, G. W., Besson, D. Z., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, Andrii, Tilav, S., Tollefson, K., Tomankova, L., Tönnis, C., Toscano, S., Tosi, D., Binder, G., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Ty, B., Unger, E., Unland Elorrieta, M. A., Usner, Marcel, Bindig, D., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., Vannerom, D., Santen, Jakob van, Verpoest, S., Vraeghe, M., Walck, C., Wallace, A., Blaufuss, E., Wallraff, M., Watson, T. B., Weaver, C., Weindl, A., Weiss, M. J., Weldert, J., Wendt, C., Werthebach, J., Whelan, B. J., Whitehorn, N., Blot, S., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wills, L., Wolf, M., Wood, T. R., Woschnagg, K., Wrede, G., Wulff, J., Xu, X. W., Bohm, C., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., Zhang, Z., Zöcklein, M., IceCube Collaboration, Böser, S., Botner, O., Aguilar, J. A., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Buscher, J., Busse, R. S., Ahlers, M., Carver, T., Chen, C., Cheung, E., Chirkin, D., Choi, S., Clark, B. A., Clark, K., Classen, L., Coleman, A., Collin, G. H., Ahrens, M., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., De Clercq, C., DeLaunay, J. J., Dembinski, H., Deoskar, K., Alispach, C., De Ridder, S., Desai, A., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Dharani, S., Diaz, A., Díaz-Vélez, J. C., Amin, N. M., Dujmovic, H., Dunkman, M., DuVernois, M. A., Dvorak, E., Ehrhardt, T., Eller, P., Engel, R., Evenson, P. A., Fahey, S., Fazely, A. R., Andeen, K., Fedynitch, A., Felde, J., Fienberg, A. T., Filimonov, K., Finley, C., Fox, D., Franckowiak, Anna, Friedman, E., Fritz, A., Gaisser, T. K.
Přispěvatelé: Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, Elementary Particle Physics
Rok vydání: 2020
Předmět:
Sterile neutrino
Physics::Instrumentation and Detectors
PROTON
sterile [neutrino]
01 natural sciences
High Energy Physics - Experiment
CROSS-SECTIONS
IceCube
Subatomär fysik
High Energy Physics - Experiment (hep-ex)
High Energy Physics - Phenomenology (hep-ph)
Astronomi
astrofysik och kosmologi

neutrino: atmosphere
Subatomic Physics
Astronomy
Astrophysics and Cosmology

detector [neutrino]
Physics
oscillation [neutrino]
Astrophysics::Instrumentation and Methods for Astrophysics
hep-ph
OPTICAL-PROPERTIES
neutrino: sterile
atmosphere [neutrino]
mass difference [neutrino]
ddc
High Energy Physics - Phenomenology
neutrino: detector
Physique des particules élémentaires
SOUTH-POLE ICE
Neutrino
data analysis method
Astrophysics::High Energy Astrophysical Phenomena
Neutrino telescope
neutrino: mass difference
FOS: Physical sciences
Context (language use)
statistical analysis
0103 physical sciences
OSCILLATIONS
conservation law
ddc:530
010306 general physics
hep-ex
010308 nuclear & particles physics
High Energy Physics::Phenomenology
Astronomy
neutrino: mixing angle
CONVERSION
Physics and Astronomy
LSND
RESOLUTION
High Energy Physics::Experiment
neutrino: oscillation
GLACIAL ICE
mixing angle [neutrino]
experimental results
Zdroj: Physical review / D 102(5), 052009 (2020). doi:10.1103/PhysRevD.102.052009
Physical Review
Physical Review D, 102 (5
Physical review / D, 102 (5), Article: 052009
Aartsen, M G, Abbasi, R, Ackermann, M, Adams, J, Aguilar, J A, Ahlers, M T, Ahrens, M, Alispach, C, Amin, N M, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Arguelles, C, Auffenberg, J, Bourbeau, E, Medici, M A, Koskinen, D J, Stuttard, T S, Rameez, M & Icecube Collaboration 2020, ' Searching for eV-scale sterile neutrinos with eight years of atmospheric neutrinos at the IceCube neutrino telescope ', Physical Review D, vol. 102, 052009 . https://doi.org/10.1103/PhysRevD.102.052009
PHYSICAL REVIEW D
ISSN: 2470-0029
2470-0010
DOI: 10.1103/physrevd.102.052009
Popis: Physical review / D D102(5), 052009 (1-32) (2020). doi:10.1103/PhysRevD.102.052009
We report in detail on searches for eV-scale sterile neutrinos, in the context of a 3+1 model, using eight years of data from the IceCube neutrino telescope. By analyzing the reconstructed energies and zenith angles of 305,735 atmospheric $\nu_\mu$ and $\bar{\nu}_\mu$ events we construct confidence intervals in two analysis spaces: $\sin^2 (2\theta_{24})$ vs. $\Delta m^2_{41}$ under the conservative assumption $\theta_{34}=0$; and $\sin^2(2\theta_{24})$ vs. $\sin^2 (2\theta_{34})$ given sufficiently large $\Delta m^2_{41}$ that fast oscillation features are unresolvable. Detailed discussions of the event selection, systematic uncertainties, and fitting procedures are presented. No strong evidence for sterile neutrinos is found, and the best-fit likelihood is consistent with the no sterile neutrino hypothesis with a p-value of 8% in the first analysis space and 19% in the second.
Published by Inst.302363, Melville, NY
Databáze: OpenAIRE