by Roopesh Ojha, Haocheng Zhang, Matthias Kadler, Naoko K. Neilson, Michael Kreter, J. McEnery, S. Buson, R. Caputo, P. Coppi, F. D'Ammando, A. De Angelis, K. Fang, D. Giannios, S. Guiriec, F. Guo, J. Kopp, F. Krauss, H. Li, M. Meyer, A. Moiseev, M. Petropoulou, C. Prescod-Weinstein, B. Rani, C. Shrader, T. Venters, and Z. Wadiasingh
Published onMay 31, 2019
Neutrinos, Cosmic Rays, and the MeV Band
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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.
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