High-energy cosmic antiparticle excess vs. isotropic gamma-ray background problem in decaying dark matter Universe

[en] We are going to show that any conventional decaying dark matter model, providing an explanation of cosmic antiparticle excess observed by PAMELA and AMS-02, inevitably faces the contradiction with isotropic diffuse gamma-ray background, measured by FERMI/LAT.

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)

Lukyanov, A. D.

Malakhov, V. V.

More authors (6 more)

Language :

English

Title :

High-energy cosmic antiparticle excess vs. isotropic gamma-ray background problem in decaying dark matter Universe

Publication date :

2016

Journal title :

Journal of Physics. Conference Series

ISSN :

1742-6588

eISSN :

1742-6596

Publisher :

Institute of Physics, Bristol, United Kingdom

Volume :

675

Issue :

Pages :

012023

Peer reviewed :

Peer Reviewed verified by ORBi

Additional URL :

http://stacks.iop.org/1742-6596/675/i=1/a=012023

Available on ORBi :

since 08 February 2017

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Bibliography

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