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Constraining Light Dark Matter with Diffuse X-Ray and Gamma-Ray Observations

机译:用漫射X射线和伽马射线约束光暗物质   意见

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摘要

We present constraints on decaying and annihilating dark matter (DM) in the 4keV to 10 GeV mass range, using published results from the satellites HEAO-1,INTEGRAL, COMPTEL, EGRET, and the Fermi Gamma-ray Space Telescope. We deriveanalytic expressions for the gamma-ray spectra from various DM decay modes, andfind lifetime constraints in the range 10^24-10^28 sec, depending on the DMmass and decay mode. We map these constraints onto the parameter space for avariety of models, including a hidden photino that is part of a kineticallymixed hidden sector, a gravitino with R-parity violating decays, a sterileneutrino, DM with a dipole moment, and a dark pion. The indirect constraints onsterile-neutrino and hidden-photino DM are found to be more powerful than otherexperimental or astrophysical probes in some parts of parameter space. Whileour focus is on decaying DM, we also present constraints on DM annihilation toelectron-positron pairs. We find that if the annihilation is p-wave suppressed,the galactic diffuse constraints are, depending on the DM mass and velocity atrecombination, more powerful than the constraints from the Cosmic MicrowaveBackground.
机译:我们使用从HEAO-1,INTEGRAL,COMPTEL,EGRET和费米伽马射线太空望远镜发布的结果,提出了在4keV至10 GeV质量范围内衰减和消除暗物质(DM)的约束。我们从各种DM衰减模式中导出了伽马射线谱的解析表达式,并根据DMmass和衰减模式,确定了10 ^ 24-10 ^ 28sec范围内的寿命约束。我们将这些约束映射到各种模型的参数空间上,包括作为动态混合隐藏扇区一部分的隐藏光子,具有R-parity违规衰减的引力子,不育中微子,具有偶极矩的DM和深色介子。发现在参数空间的某些部分,对不育中微子和隐性光合DM的间接约束比其他实验或天体探测探头更强大。尽管我们的重点是衰减DM,但我们也提出了对DM hil灭到电子-正电子对的约束。我们发现,如果the灭被p波抑制,则取决于DM的质量和速度复合,银河扩散约束比来自宇宙微波背景的约束更强大。

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