Neutrinos, Cosmic Rays, and the MeV Band

Journal
Date Issued
2019
Author(s)
Ojha, Roopesh
•
Zhang, Haocheng
•
Kadler, Matthias
•
Neilson, Naoko K.
•
Kreter, Michael
•
McEnery, J.
•
Buson, S.
•
Caputo, R.
•
Coppi, P.
•
•
De Angelis, A.
•
Fang, K.
•
Giannios, D.
•
Guiriec, S.
•
Guo, F.
•
Kopp, J.
•
Krauss, F.
•
Li, H.
•
Meyer, M.
•
Moiseev, A.
•
Petropoulou, M.
•
Prescod-Weinstein, C.
•
Rani, B.
•
Shrader, C.
•
Venters, T.
•
Wadiasingh, Z.
Abstract
The Mev band holds the key to answering three astrophysical questions: the sites where cosmic Rays are produced and accelerated, the origins of high- energy neutrinos, and the physical mechanisms producing the high energy gamma- ray emission from blazars. Theoretical and experimental capabilities needed in the next decade are discussed.
Volume
51
Issue
3
Start page
431
Uri
Url
Issn Identifier
2330-9458
Ads BibCode
2019BAAS...51c.431O
Rights
open.access
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