FERMI CONSTRAINS DARK-MATTER ORIGIN OF HIGH-ENERGY POSITRON ANOMALY

被引:4
作者
Pohl, Martin [1 ,2 ]
Eichler, David [3 ]
机构
[1] Univ Potsdam, Inst Phys & Astron, D-14476 Potsdam, Germany
[2] DESY, D-15738 Zeuthen, Germany
[3] Ben Gurion Univ Negev, Dept Phys, IL-84105 Beer Sheva, Israel
基金
美国国家科学基金会;
关键词
cosmic rays; dark matter; gamma rays: general; COSMIC-RAY POSITRONS; GAMMA-RAY; RADIATION; PARTICLES;
D O I
10.1088/2041-8205/712/1/L53
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Fermi measurements of the high-latitude gamma-ray background strongly constrain a decaying-dark-matter origin for the 1-100 GeV Galactic positron anomaly measured with PAMELA. Inverse Compton scattering of the microwave background by the emergent positrons produces a bump in the diffuse 100-200 MeV gamma-ray background that would protrude from the observed background at these energies. The positrons are thus constrained to emerge from the decay process at a typical energy between similar to 100 GeV and similar to 250 GeV. By considering only.-ray emission of the excess positrons and electrons, we derive a minimum diffuse gamma-ray flux that, apart from the positron spectrum assumed, is independent of the actual decay modes. Any gamma-rays produced directly by the dark-matter decay leads to an additional signal that makes the observational limits more severe. A similar constraint on the energy of emergent positrons from annihilation in dark-matter substructures is argued to exist, according to recent estimates of enhancement in low-mass dark-matter substructures, and improved simulations of such substructure will further sharpen this constraint.
引用
收藏
页码:L53 / L57
页数:5
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