[en] As we are going to show, some self-interacting dark matter models may provide an intriguing solution to the ”cosmic antiparticle excess vs. isotropic diffuse gamma-ray background” problem (an overproduction of diffuse gamma rays, arising in any reasonable decaying or annihilating dark matter model explaining high-energy charged cosmic antiparticles anomalous abundance).
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Alekseev, V. V.
Belotsky, K. M.
Bogomolov, Yu V.
Budaev, R. I.
Dunaeva, O. A.
Kirillov, A. A.
Kuznetsov, A. V.
Laletin, Maxim ; Université de Liège > Département d'astrophys., géophysique et océanographie (AGO) > Inter. fondamentales en physique et astrophysique (IFPA)
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