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arXiv 1206.2279hep-phastro-ph.CO
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如果暗物质Gamma-Ray线与胶子线一起出现会怎样?

What if Dark Matter Gamma-Ray Lines come with Gluon Lines?

Xiaoyong Chu, Thomas Hambye, Tiziana Scarna, Michel H. G. Tytgat

摘要:

在暗物质(DM)模型中,由DM湮灭产生的伽马线(或“盒形”伽马射线谱)通常从涉及重带电粒子的环图进行。如果环中的带电粒子也带有色荷,这将不可避免地导致DM湮灭为胶子,其速率自然更大。我们考虑的情况下,DM候选人湮灭成胶子对占主导地位,并确定(尽可能,独立于模型)从各种可观测的约束:a)的暗物质遗迹密度,b)的生产反质子,c)DM直接检测和d)胶子胶子融合过程在大型强子对撞机。除其他外,我们表明,这种情况下,连同最近的索赔可能的伽马线从银河系中心的费米-LAT数据,导致一个遗迹丰富的DM,可能是自然接近的宇宙学观测。

英文摘要:

In dark matter (DM) models, the production of a gamma line (or of a "box-shaped" gamma-ray spectrum) from DM annihilation proceeds in general from a loop diagram involving a heavy charged particle. If the charged particle in the loop carries also a color charge, this leads inevitably to DM annihilation to gluons, with a naturally larger rate. We consider a scenario in which DM candidates annihilate dominantly into gluon pairs, and determine (as far as possible, model-independent) constraints from a variety of observables: a) the dark matter relic density, b) the production of anti-protons, c) DM direct detection and d) gluon-gluon fusion processes at LHC. Among other things, we show that this scenario together with the recent claim for a possible gamma line from the Galactic center in the Fermi-LAT data, leads to a relic abundance of DM that may be naturally close to the cosmological observations.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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