Accès ouvert déclaré 2021 article

Seasonal variation of multiple-muon cosmic ray air showers observed in the NOvA detector on the surface

M. A. Acero, P. Adamson, L. Aliaga, Н. Анфимов, A. Antoshkin, E. Arrieta-Diaz, L. Asquith, A. Aurisano, H.O. Back, C. Backhouse, M. Baird, N. Balashov, Pierre Baldi, B. A. Bambah, S. Bashar, K. Bays, Robert Bernstein, V. Bhatnagar, B. Bhuyan, J. M. Bian, J. Blair, Andrew Booth, R. Bowles, C. Bromberg, N. J. Buchanan, A. Butkevich, S. Calvez, Timothy J. Carroll, E. Catano-Mur, B. C. Choudhary, A. Christensen, T. E. Coan, M. Colo, L. Cremonesi, G. S. Davies, P. F. Derwent, P. F. Ding, Z. Djurčić, M. Dolce, D. Doyle, D. Dueñas Tonguino, E. C. Dukes, Hongyue Duyang, S. Edayath, R. Ehrlich, M. Elkins, E. Ewart, G. J. Feldman, P. Filip, J. Franc, M. J. Frank, H. Gallagher, R. P. Gandrajula, F. Gao, A. Giri, R. A. Gomes, M. C. Goodman, V. Grichine, M. Groh, B. Guo, A. Habig, F. Hakl, A. Reinsvold Hall, J. Hartnell, R. Hatcher, Henry H. Hausner, K. Heller, J. Hewes, A. Himmel, A. Holin, B. Jargowsky, J. Jarosz, F. Jediny, C. A. Johnson, M. Judah, I. Kakorin, D. Kalra, D. M. Kaplan, A. Kalitkina, R. Keloth, O. Klimov, L. W. Koerner, L. Kolupaeva, S.K. Kotelnikov, R. Kralik, Ch. Kullenberg, M. Kubu, Arun Kumar, C. Kuruppu, V. Kus, T. Lackey, K. Lang, P. Lasorak, J. Lesmeister, S. Lin, A. Lister, Jinzhi Liu, M. Lokajı́ček, S. Magill, M. Manrique Plata, W. A. Mann, Marvin L. Marshak, M. Martinez-Casales, V. Matveev, B. Mayes, M. D. Messier, H. Meyer, T. Miao, William H. Miller, S. Mishra, A. Mislivec, Rukmani Mohanta, A. Moren, A. Morozova, W. Mu, L. Mualem, M. Muether, K. Mulder, D. Naples, N. Nayak, J. K. Nelson, R. J. Nichol, E. Niner, A. Norman, A. Norrick, T. Nosek, H. Oh, A. Olshevskiy, T. Olson, J. Ott, J. Paley, R. B. Patterson, G. Pawloski, O. Petrova, R. Petti, D. D. Phan, R. Plunkett, Joshua Porter, A. Rafique, V. Raj, M. Rajaoalisoa, B. Ramson, B. Rebel, P. Rojas, V. Ryabov, O. Samoylov, M. C. Sánchez, S. Sánchez Falero, P. Shanahan, A. Sheshukov, P. Singh, V. Singh, E. Smith, J. Smolík, P. Snopok, N. Solomey, A. Sousa, K. Soustružnı́k, M. Strait, L. Suter, A. Sutton, S. K. Swain, C. Sweeney, B. Tapia Oregui, P. Tas, T. Thakore, R. B. Thayyullathil, J. Thomas, E. Tiras, S. C. Tognini, J. Tripathi, J. Trokan-Tenorio, Y. Torun, J. Urheim, P. Vahle, Z. Vallari, J. Vasel, P. Vokáč, T. Vrba, M. Wallbank, T. K. Warburton, M. Wetstein, D. Whittington, D. A. Wickremasinghe, S. G. Wojcicki, J. Wolcott, W. Wu, Y. J. Xiao, A. Yallappa Dombara, K. Yonehara, S. Yu, Y. Yu, S. Zadorozhnyy, J. Zálešâk, Y. Zhang, R. Zwaska

8Citations signalées, ce qui n’est pas une note de qualité

51Institutions déclarées

8Pays d’affiliation déclarés

Rattachement africain : co, us, ru, gb, in, cz, br, tr. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

We report the rate of cosmic ray air showers with multiplicities exceeding 15 muon tracks recorded in the NOvA Far Detector between May 2016 and May 2018. The detector is located on the surface under an overburden of 3.6 meters water equivalent. We observe a seasonal dependence in the rate of multiple-muon showers, which varies in magnitude with multiplicity and zenith angle. During this period, the effective atmospheric temperature and surface pressure ranged between 210 K and 230 K and 940 mbar and 990 mbar, respectively; the shower rates are anticorrelated with the variation in the effective temperature. The variations are about 30% larger for the highest multiplicities than the lowest multiplicities and 20% larger for showers near the horizon than vertical showers.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref: Seasonal variation of multiple-muon cosmic ray air showers observed in the NOvA detector on the surface
Date Crossref: 30/07/2021
Éditeur: American Physical Society (APS)
Type: journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

University of Atlántico Fermi National Accelerator Laboratory Joint Institute for Nuclear Research University of Magdalena University of Sussex University of Cincinnati Iowa State University University College London Indiana University Bloomington University of Virginia University of California, Irvine University of Hyderabad Tufts University California Institute of Technology Illinois Institute of Technology Panjab University Indian Institute of Technology Guwahati University of Minnesota University of Houston Michigan State University Colorado State University Institute for Nuclear Research University of Wisconsin–Madison The University of Texas at Austin William & Mary Williams (United States)University of Delhi Southern Methodist University Queen Mary University of London University of Mississippi Argonne National Laboratory University of South Carolina Cochin University of Science and Technology Harvard University Czech Academy of Sciences FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic Czech Technical University in Prague University of South Alabama University of Pittsburgh Indian Institute of Technology Hyderabad Universidade Federal de Goiás P.N. Lebedev Physical Institute of the Russian Academy of Sciences University of Minnesota, Duluth Czech Academy of Sciences, Institute of Computer Science Wichita State University Charles University Banaras Hindu University National Institute of Science Education and Research Erciyes University Syracuse University Stanford University

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Astrophysics and Cosmic PhenomenaDark Matter and Cosmic PhenomenaNeutrino Physics Research

Lire en accès ouvert Consulter la publication primaire Ouvrir le DOI