GAMMA-RAY SIGNATURES OF DARK MATTER

被引：0
|
作者：
BERGSTROM, L
机构：
来源：
TAUP 89: WORKSHOP ON THEORETICAL AND PHENOMENOLOGICAL ASPECTS OF UNDERGROUND PHYSICS | 1989年
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页码：347 / 352
页数：6
相关论文
共 50 条
  • [31] Generic dark matter signature for gamma-ray telescopes
    Barger, V.
    Gao, Y.
    Keung, W. -Y.
    Marfatia, D.
    PHYSICAL REVIEW D, 2009, 80 (06):
  • [32] Gamma-ray line constraints on coy dark matter
    Hektor, Andi
    Marzola, Luca
    Tuvi, Taavi
    PHYSICAL REVIEW D, 2017, 95 (12)
  • [33] Gamma-ray lines from dark matter decay
    Ibarra, Alejandro
    7TH INTERNATIONAL WORKSHOP ON THE DARK SIDE OF THE UNIVERSE (DSU 2011), 2012, 384
  • [34] Gamma-ray excess and the minimal dark matter model
    Michael Duerr
    Pavel Fileviez Pérez
    Juri Smirnov
    Journal of High Energy Physics, 2016
  • [35] Gamma-ray bursts and dark energy-dark matter interaction
    Barreiro, T.
    Bertolami, O.
    Torres, P.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 409 (02) : 750 - 754
  • [36] Dark matter: the connection with gamma-ray astrophysicsDiscovering dark matter particles with astrophysical observations
    Gianfranco Bertone
    Astrophysics and Space Science, 2007, 309 : 505 - 515
  • [37] Angular signatures of dark matter in the diffuse gamma ray background
    Hooper, Dan
    Serpico, Pasquale D.
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2007, (06):
  • [38] Expected LHAASO sensitivity to decaying dark matter signatures from dwarf galaxies gamma-ray emission
    何东泽
    毕效军
    林苏杰
    殷鹏飞
    张鑫
    Chinese Physics C, 2020, (08) : 176 - 183
  • [39] Expected LHAASO sensitivity to decaying dark matter signatures from dwarf galaxies gamma-ray emission*
    He, Dong-Ze
    Bi, Xiao-Jun
    Lin, Su-Jie
    Yin, Peng-Fei
    Zhang, Xin
    CHINESE PHYSICS C, 2020, 44 (08)
  • [40] Expected LHAASO sensitivity to decaying dark matter signatures from dwarf galaxies gamma-ray emission
    何东泽
    毕效军
    林苏杰
    殷鹏飞
    张鑫
    Chinese Physics C, 2020, 44 (08) : 176 - 183
12345