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
University of Maryland, Baltimore County
The University of Chicago
University of Alabama in Huntsville
Gran Sasso Science Institute
City University of New York
National Institute for Astrophysics
National Institute for Nuclear Physics
INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palemo
Georgia Institute of Technology
University of Turin
University of Utah
NASA Marshall Space Flight Center
National Aeronautics and Space Administration
University of Copenhagen
University of Catania
RIKEN
RIIKEN
Joint Laboratory of Optics
Karlsruhe Institute of Technology
Kavli Institute for Particle Astrophysics and Cosmology
Colorado School of Mines
University of Maryland, College Park
University of Tübingen
University of California at Berkeley
Lomonosov Moscow State University
Slovak Academy of Sciences
Czech Academy of Sciences
Universidad Nacional Autónoma de México
University of Geneva
National Astronomical Observatory of Japan
Norwegian University of Science and Technology
The University of Tokyo
Université de Paris
Institute de Recherche en Astrophysique et Planétologie
University of Warsaw
National Centres for Nuclears Research
Hokkaido University
National Centre for Nuclear Research
Fairfield University
Abou Bakr Belkaïd University of Tlemcen
Nihon University
Technical University of Madrid
Badji Mokhtar University
Center for Development of Advanced Technologies
University of Alcalá
University of Rome Tor Vergata
Instituto Nacional de Tecnica Aeroespacial
University of Bari
Centro Mesoamericano de Física Teórica (MCTP)
Joint Institute for Nuclear Research
CSEM SA
Sofia University St. Kliment Ohridski
Universidad Autonoma de Chiapas
Shinshu University
Technical University of Munich
Institute of Space Science ISS
KTH Royal Institute of Technology
Kindai University
Osaka Metropolitan University
University of M'sila
University of Naples Federico II
Konan University
International Telematic University Uninettuno
National Institutes for Quantum Science and Technology
University of Leon
Instituto de Astrofísica de Canarias
Center of Research in Astronomy, Astrophysics and Geophysics
Kyoto University
Technical University of Kosice
Saitama University
Nagoya University
Sungkyunkwan University
Chiba University
Korea Astronomy and Space Science Institute
Friedrich-Alexander University Erlangen-Nürnberg
Osaka Electro-Communication University
High Energy Accelerator Research Organization, Tsukuba
Research Unit on Optics and Photonics
Universidad Michoacana de San Nicolas de Hidalgo
Benemerita Universidad Autonoma de Puebla
Frères Mentouri Constantine 1 University
JAXA Institute of Space and Astronautical Science
Institute for Atmospheric and Climate Science
Kanazawa University
Space Regatta Consortium

Research output: Contribution to journal › Conference article › peer-review

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.

Original language	English
Article number	1201
Journal	Proceedings of Science
Volume	395
State	Published - 18 Mar 2022
Externally published	Yes
Event	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Germany Duration: 12 Jul 2021 → 23 Jul 2021

Cite this

@article{64d7e6b194074f839c58c09dfcf8e746,

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 T. Kajino",

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 = "英语",

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 - Kajino, T.

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 - 会议文章

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

Abstract

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