EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors

the POEMMA; JEM-EUSO Collaborations

EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors

the POEMMA
, JEM-EUSO Collaborations

University of Iowa
NASA Goddard Space Flight Center
Biochemical and Environmental Engineering
University of Chicago
University of Alabama in Huntsville
Gran Sasso Science Institute
Lehman College
Istituto di Astrofisica e Planetologia Spaziali (IAPS)
INFN Sezione di Catania
INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palemo
College of Computing
University of Turin
INFN Sezione di Torino
University of Utah
NASA Marshall Space Flight Center
GSFC Laboratory for Atmopsheres
Niels Bohr Institutet
INFN Sezione di Bari
Università degli Studi di Catania
Riken
Sezione di Roma
INFN Roma Tor Vergata
RIIKEN
Joint Laboratory of Optics
Institute of Meteorology and Climate Research
Kavli Institute for Particle Astrophysics and Cosmology
Colorado School of Mines
University of Maryland
University of Tübingen
University of California, Space Sciences Laboratory
Moscow State University
Institute of Experimental Physics Slovak Academy of Sciences
Institute of Physics of the Czech Academy of Sciences
of Sciences
Instituto de Ciencias Nucleares de la UNAM
Universidad Nacional Autónoma de México
University of Geneva
Astroparticule and Cosmol APC
Norwegian University of Science and Technology
INFN Sezione di Napoli
University of Tokyo
IRAP/CNRS
University of Warsaw
National Centres for Nuclears Research
Hokkaido University
LNF-INFN
Astrophysics Division
Fairfield University
Tlemcen University
Nihon University
Universidad Politécnica de Madrid
Université Badji Mokhtar - Annaba
Centre de Développement des Technologies Avancées
Universidad de Alcalá
University of Rome “Tor Vergata”
Instituto Nacional de Técnica Aeroespacial (CSIC/INTA)
Università degli studi di Bari Aldo Moro
Centro Mesoamericano de Física Teórica (MCTP)
Joint Institute for Nuclear Research, Dubna
Centre Suisse d'Electronique et de Microtechnique SA
University of Sofia
Universidad Autónoma de Chiapas
Shinshu University
Technical University of Munich
Institute of Space Sciences
KTH Royal Institute of Technology
Kindai University
Osaka City University
University of M’sila
University of Naples Federico II
Konan University
UTIU
National Institutes for Quantum and Radiological Science and Technology
University of León
Instituto de Astrofisica de Canarias
Algiers Observatory
Kyoto University
Technical University of Kosice
Saitama University
Nagoya University
Sungkyunkwan University
National Astronomical Observatory
Chiba University
Korea Astronomy and Space Science Institute
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
Osaka Electro-Communication University
High Energy Accelerator Research Organization (KEK)
Research Unit on Optics and Photonics
Universidad Michoacana de San Nicolás de Hidalgo
Benemerita Universidad Autonoma de Puebla
Univ. Mentouri de Constantine
ISAS/JAXA
ETH Zurich
Kanazawa University
Space Regatta Consortium

Résultats de recherche: Contribution à un journal › Article de conférence › Revue par des pairs

Résumé

Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth-interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.

langue originale	Anglais
Numéro d'article	1201
journal	Proceedings of Science
Volume	395
état	Publié - 18 mars 2022
Modification externe	Oui
Evénement	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Allemagne Durée: 12 juil. 2021 → 23 juil. 2021

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Contient cette citation

@article{74ff2fc3bde54958b9d56cc5c165fc66,

title = "EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors",

abstract = "Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth-interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.",

author = "\{the POEMMA\} and \{JEM-EUSO Collaborations\} and Reno, \{Mary Hall\} and Venters, \{Tonia M.\} and Krizmanic, \{John F.\} and Olinto, \{A. V.\} and J. Krizmanic and Adams, \{J. H.\} and R. Aloisio and Anchordoqui, \{L. A.\} and A. Anzalone and M. Bagheri and D. Barghini and M. Battisti and Bergman, \{D. R.\} and Bertaina, \{M. E.\} and Bertone, \{P. F.\} and F. Bisconti and M. Bustamante and F. Cafagna and R. Caruso and M. Casolino and K. {\v C}ern{\'y} and Christl, \{M. J.\} and Cummings, \{A. L.\} and \{De Mitri\}, I. and R. Diesing and R. Engel and J. Eser and K. Fang and F. Fenu and G. Filippatos and E. Gazda and C. Guepin and A. Haungs and Hays, \{E. A.\} and Judd, \{E. G.\} and P. Klimov and V. Kungel and E. Kuznetsov and Mackovjak and D. Mand{\'a}t and L. Marcelli and J. McEnery and G. Medina-Tanco and Merenda, \{K. D.\} and Meyer, \{S. S.\} and Mitchell, \{J. W.\} and H. Miyamoto and Nachtman, \{J. M.\} and A. Neronov and \{de la Taille\}, C.",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s).; 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "English",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors

AU - the POEMMA

AU - JEM-EUSO Collaborations

AU - Reno, Mary Hall

AU - Venters, Tonia M.

AU - Krizmanic, John F.

AU - Olinto, A. V.

AU - Krizmanic, J.

AU - Adams, J. H.

AU - Aloisio, R.

AU - Anchordoqui, L. A.

AU - Anzalone, A.

AU - Bagheri, M.

AU - Barghini, D.

AU - Battisti, M.

AU - Bergman, D. R.

AU - Bertaina, M. E.

AU - Bertone, P. F.

AU - Bisconti, F.

AU - Bustamante, M.

AU - Cafagna, F.

AU - Caruso, R.

AU - Casolino, M.

AU - Černý, K.

AU - Christl, M. J.

AU - Cummings, A. L.

AU - De Mitri, I.

AU - Diesing, R.

AU - Engel, R.

AU - Eser, J.

AU - Fang, K.

AU - Fenu, F.

AU - Filippatos, G.

AU - Gazda, E.

AU - Guepin, C.

AU - Haungs, A.

AU - Hays, E. A.

AU - Judd, E. G.

AU - Klimov, P.

AU - Kungel, V.

AU - Kuznetsov, E.

AU - Mackovjak,

AU - Mandát, D.

AU - Marcelli, L.

AU - McEnery, J.

AU - Medina-Tanco, G.

AU - Merenda, K. D.

AU - Meyer, S. S.

AU - Mitchell, J. W.

AU - Miyamoto, H.

AU - Nachtman, J. M.

AU - Neronov, A.

AU - de la Taille, C.

PY - 2022/3/18

Y1 - 2022/3/18

N2 - Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth-interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.

AB - Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth-interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.

UR - https://www.scopus.com/pages/publications/85145570521

M3 - Conference article

AN - SCOPUS:85145570521

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1201

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors

Résumé

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