pith. sign in

arxiv: 1708.07599 · v1 · pith:4MAWCWNNnew · submitted 2017-08-25 · 🌌 astro-ph.IM · astro-ph.HE

POEMMA: Probe Of Extreme Multi-Messenger Astrophysics

A. V. Olinto , J. H. Adams , R. Aloisio , L. A. Anchordoqui , D. R. Bergman , M. E. Bertaina , P. Bertone , M. Bustamante
show 33 more authors
M. J. Christl S. E. Csorna J. B. Eser F. Fenu C. Gu\'epin E. A. Hays S. Hunter E. Judd I. Jun K. Kotera J. F. Krizmanic E. Kuznetsov S. Mackovjak L. M. Martinez-Sierra M. Mastafa J. N. Matthews J. McEnery J. W. Mitchell A. Neronov A. N. Otte E. Parizot T. C. Paul J. S. Perkins G. Prevot P. Reardon M. H. Reno F. Sarazin K. Shinozaki F. Stecker R. Streitmatter T. Venters L. Wiencke R. M. Young
This is my paper
classification 🌌 astro-ph.IM astro-ph.HE
keywords uhecrsctnsenergiesastrophysicscosmogenicenergyextremehighest
0
0 comments X
read the original abstract

The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) mission is being designed to establish charged-particle astronomy with ultra-high energy cosmic rays (UHECRs) and to observe cosmogenic tau neutrinos (CTNs). The study of UHECRs and CTNs from space will yield orders-of-magnitude increase in statistics of observed UHECRs at the highest energies, and the observation of the cosmogenic flux of neutrinos for a range of UHECR models. These observations should solve the long-standing puzzle of the origin of the highest energy particles ever observed, providing a new window onto the most energetic environments and events in the Universe, while studying particle interactions well beyond accelerator energies. The discovery of CTNs will help solve the puzzle of the origin of UHECRs and begin a new field of Astroparticle Physics with the study of neutrino properties at ultra-high energies.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Ultra-High-Energy Tau Neutrinos as Probes of Lorentz Invariance

    hep-ph 2026-04 unverdicted novelty 5.0

    Ultra-high-energy tau neutrino detections at GRAND and POEMMA are projected to constrain Lorentz invariance violation parameters orders of magnitude more stringently than current lower-energy probes.

  2. Development of a Cherenkov Telescope for the Detection of Ultrahigh Energy Neutrinos with EUSO-SPB2 and POEMMA

    astro-ph.IM 2019-07 unverdicted novelty 4.0

    Design and component qualification for a silicon-photomultiplier Cherenkov telescope intended for tau-neutrino detection via the Earth-skimming technique on EUSO-SPB2 and POEMMA.

  3. Fundamental physics with high-energy cosmic neutrinos today and in the future

    astro-ph.HE 2019-07 unverdicted novelty 2.0

    High-energy astrophysical neutrinos enable stringent tests of physics beyond the Standard Model at energies and baselines unreachable by other means.