Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations
The Askaryan Radio Array (ARA) is an ultra-high energy (UHE, $>10^{17}$ eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic ice. In this paper, we present constraints on the diffuse...
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ftdatacite:10.48550/arxiv.1912.00987 2023-05-15T14:03:41+02:00 Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations ARA Collaboration Allison, P. Archambault, S. Beatty, J. J. Beheler-Amass, M. Besson, D. Z. Beydler, M. Chen, C. C. Chen, C. H. Chen, P. Clark, B. A. Clay, W. Connolly, A. Cremonesi, L. Davies, J. de Kockere, S. de Vries, K. D. Deaconu, C. Duvernois, M. Friedman, E. Gaior, R. Hanson, J. Hanson, K. Hoffman, K. D. Hokanson-Fasig, B. Hong, E. Hsu, S. Y. Hu, L. Huang, J. J. Huang, M. -H. Hughes, K. Ishihara, A. Karle, A. Kelley, J. L. Khandelwal, R. Kim, K. -C. Kim, M. -C. Kravchenko, I. Kurusu, K. Landsman, H. Latif, U. A. Laundrie, A. Li, C. -J. Liu, T. -C. Lu, M. -Y. Madison, B. Mase, K. Meures, T. Nam, J. Nichol, R. J. Nir, G. Novikov, A. Nozdrina, A. Oberla, E. O'Murchadha, A. Osborn, J. Pan, Y. Pfendner, C. Roth, J. Sandstrom, P. Seckel, D. Shiao, Y. -S. Shultz, A. Smith, D. Torres, J. Touart, J. van Eijndhoven, N. Varner, G. S. Vieregg, A. G. Wang, M. -Z. Wang, S. -H. Wissel, S. A. Yoshida, S. Young, R. 2019 https://dx.doi.org/10.48550/arxiv.1912.00987 https://arxiv.org/abs/1912.00987 unknown arXiv https://dx.doi.org/10.1103/physrevd.102.043021 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences article-journal Article ScholarlyArticle Text 2019 ftdatacite https://doi.org/10.48550/arxiv.1912.00987 https://doi.org/10.1103/physrevd.102.043021 2022-03-10T16:33:19Z The Askaryan Radio Array (ARA) is an ultra-high energy (UHE, $>10^{17}$ eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic ice. In this paper, we present constraints on the diffuse flux of ultra-high energy neutrinos between $10^{16}-10^{21}$ eV resulting from a search for neutrinos in two complementary analyses, both analyzing four years of data (2013-2016) from the two deep stations (A2, A3) operating at that time. We place a 90 % CL upper limit on the diffuse all flavor neutrino flux at $10^{18}$ eV of $EF(E)=5.6\times10^{-16}$ $\textrm{cm}^{-2}$$\textrm{s}^{-1}$$\textrm{sr}^{-1}$. This analysis includes four times the exposure of the previous ARA result, and represents approximately 1/5 the exposure expected from operating ARA until the end of 2022. : 12 pages, 7 figures; Accepted to PRD Article in Journal/Newspaper Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
spellingShingle |
High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences ARA Collaboration Allison, P. Archambault, S. Beatty, J. J. Beheler-Amass, M. Besson, D. Z. Beydler, M. Chen, C. C. Chen, C. H. Chen, P. Clark, B. A. Clay, W. Connolly, A. Cremonesi, L. Davies, J. de Kockere, S. de Vries, K. D. Deaconu, C. Duvernois, M. Friedman, E. Gaior, R. Hanson, J. Hanson, K. Hoffman, K. D. Hokanson-Fasig, B. Hong, E. Hsu, S. Y. Hu, L. Huang, J. J. Huang, M. -H. Hughes, K. Ishihara, A. Karle, A. Kelley, J. L. Khandelwal, R. Kim, K. -C. Kim, M. -C. Kravchenko, I. Kurusu, K. Landsman, H. Latif, U. A. Laundrie, A. Li, C. -J. Liu, T. -C. Lu, M. -Y. Madison, B. Mase, K. Meures, T. Nam, J. Nichol, R. J. Nir, G. Novikov, A. Nozdrina, A. Oberla, E. O'Murchadha, A. Osborn, J. Pan, Y. Pfendner, C. Roth, J. Sandstrom, P. Seckel, D. Shiao, Y. -S. Shultz, A. Smith, D. Torres, J. Touart, J. van Eijndhoven, N. Varner, G. S. Vieregg, A. G. Wang, M. -Z. Wang, S. -H. Wissel, S. A. Yoshida, S. Young, R. Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
description |
The Askaryan Radio Array (ARA) is an ultra-high energy (UHE, $>10^{17}$ eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic ice. In this paper, we present constraints on the diffuse flux of ultra-high energy neutrinos between $10^{16}-10^{21}$ eV resulting from a search for neutrinos in two complementary analyses, both analyzing four years of data (2013-2016) from the two deep stations (A2, A3) operating at that time. We place a 90 % CL upper limit on the diffuse all flavor neutrino flux at $10^{18}$ eV of $EF(E)=5.6\times10^{-16}$ $\textrm{cm}^{-2}$$\textrm{s}^{-1}$$\textrm{sr}^{-1}$. This analysis includes four times the exposure of the previous ARA result, and represents approximately 1/5 the exposure expected from operating ARA until the end of 2022. : 12 pages, 7 figures; Accepted to PRD |
format |
Article in Journal/Newspaper |
author |
ARA Collaboration Allison, P. Archambault, S. Beatty, J. J. Beheler-Amass, M. Besson, D. Z. Beydler, M. Chen, C. C. Chen, C. H. Chen, P. Clark, B. A. Clay, W. Connolly, A. Cremonesi, L. Davies, J. de Kockere, S. de Vries, K. D. Deaconu, C. Duvernois, M. Friedman, E. Gaior, R. Hanson, J. Hanson, K. Hoffman, K. D. Hokanson-Fasig, B. Hong, E. Hsu, S. Y. Hu, L. Huang, J. J. Huang, M. -H. Hughes, K. Ishihara, A. Karle, A. Kelley, J. L. Khandelwal, R. Kim, K. -C. Kim, M. -C. Kravchenko, I. Kurusu, K. Landsman, H. Latif, U. A. Laundrie, A. Li, C. -J. Liu, T. -C. Lu, M. -Y. Madison, B. Mase, K. Meures, T. Nam, J. Nichol, R. J. Nir, G. Novikov, A. Nozdrina, A. Oberla, E. O'Murchadha, A. Osborn, J. Pan, Y. Pfendner, C. Roth, J. Sandstrom, P. Seckel, D. Shiao, Y. -S. Shultz, A. Smith, D. Torres, J. Touart, J. van Eijndhoven, N. Varner, G. S. Vieregg, A. G. Wang, M. -Z. Wang, S. -H. Wissel, S. A. Yoshida, S. Young, R. |
author_facet |
ARA Collaboration Allison, P. Archambault, S. Beatty, J. J. Beheler-Amass, M. Besson, D. Z. Beydler, M. Chen, C. C. Chen, C. H. Chen, P. Clark, B. A. Clay, W. Connolly, A. Cremonesi, L. Davies, J. de Kockere, S. de Vries, K. D. Deaconu, C. Duvernois, M. Friedman, E. Gaior, R. Hanson, J. Hanson, K. Hoffman, K. D. Hokanson-Fasig, B. Hong, E. Hsu, S. Y. Hu, L. Huang, J. J. Huang, M. -H. Hughes, K. Ishihara, A. Karle, A. Kelley, J. L. Khandelwal, R. Kim, K. -C. Kim, M. -C. Kravchenko, I. Kurusu, K. Landsman, H. Latif, U. A. Laundrie, A. Li, C. -J. Liu, T. -C. Lu, M. -Y. Madison, B. Mase, K. Meures, T. Nam, J. Nichol, R. J. Nir, G. Novikov, A. Nozdrina, A. Oberla, E. O'Murchadha, A. Osborn, J. Pan, Y. Pfendner, C. Roth, J. Sandstrom, P. Seckel, D. Shiao, Y. -S. Shultz, A. Smith, D. Torres, J. Touart, J. van Eijndhoven, N. Varner, G. S. Vieregg, A. G. Wang, M. -Z. Wang, S. -H. Wissel, S. A. Yoshida, S. Young, R. |
author_sort |
ARA Collaboration |
title |
Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations |
title_short |
Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations |
title_full |
Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations |
title_fullStr |
Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations |
title_full_unstemmed |
Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations |
title_sort |
constraints on the diffuse flux of ultra-high energy neutrinos from four years of askaryan radio array data in two stations |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1912.00987 https://arxiv.org/abs/1912.00987 |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_relation |
https://dx.doi.org/10.1103/physrevd.102.043021 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1912.00987 https://doi.org/10.1103/physrevd.102.043021 |
_version_ |
1766274495898714112 |