Secluded WIMP dark matter

被引:880
作者
Pospelov, Maxim [1 ,2 ]
Ritz, Adam [1 ]
Voloshin, Mikhail [3 ,4 ]
机构
[1] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
[2] Perimeter Inst Theoret Phys, Waterloo, ON N2J 2W9, Canada
[3] Univ Minnesota, William I Fine Theoret Phys Inst, Minneapolis, MN 55455 USA
[4] Inst Theoret & Expt Phys, Moscow 117218, Russia
关键词
D O I
10.1016/j.physletb.2008.02.052
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a generic mechanism via which thermal relic WIMP dark matter may be decoupled from the Standard Model, namely through a combination of WIMP annihilation to metastable mediators with subsequent delayed decay to Standard Model states. We illustrate this with explicit examples of WIMPs connected to the Standard Model by metastable bosons or fermions. In all models, provided the WIMP mass is greater than that of the mediator, it can be secluded from the Standard Model with an extremely small elastic scattering cross-section on nuclei and rate for direct collider production. In contrast, indirect signatures from WIMP annihilation are consistent with a weak scale cross-section and provide potentially observable gamma-ray signals. We also point out that gamma-ray constraints and flavor physics impose severe restrictions on MeV-scale variants of secluded models, and identify limited classes that pass all the observational constraints. (c) 2008 Elsevier B.V. All rights reserved.
引用
收藏
页码:53 / 61
页数:9
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