The MeV Background

Marco Ajello,Yoshiyuki Inoue,Peter F. Bloser, Wozniak T. Vestrand,Dieter H. Hartmann,Justin D. Finke,Zorawar Wadiasingh,Chanda Prescod-Weinstein,Uwe Oberlack,Francesco Longo,Chris Shrader,Volker Beckmann,Ivan Agudo,Maria Petropoulou, Andrew W. Strong,Eugenio Bottacini,John W. Hewitt,Alexander Moiseev,Sean Griffin,Dario Gasparrini,John A. Tomsick

Bulletin of the American Astronomical Society（2019）

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摘要

The emission of our Universe at MeV energies is unknown. New measurements of the intensity and the angular fluctuations of the MeV background will allow us to constrain models of SNIa formation, the evolution of radio-loud and radio-quiet AGN, the growth of the most massive black holes and to constrain the cross-section for dark matter interaction

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