Solar-bound weakly interacting massive particles: A no-frills phenomenology

被引：12

作者：

Collar, JI ^{[2
]}

机构：

[1] Univ Paris 07, Phys Solides Grp, F-75251 Paris, France

[2] CERN, Div EP, CH-1211 Geneva 23, Switzerland

来源：

PHYSICAL REVIEW D | 1999年 / 59卷 / 06期

关键词：

D O I：

10.1103/PhysRevD.59.063514

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The case for a stable population of solar-bound Earth-crossing weakly interacting massive particles (WIMPs) is reviewed. If such a population exists, even with a conservative phase-space density, the next generation of large-mass, low-threshold underground bolometers should bring about a sizable enhancement in WIMP sensitivity. A practical general expression for their speed distribution in the laboratory frame is derived under basic model-independent assumptions, and a characteristic yearly modulation in their recoil signal, arising from the ellipticity of the Earth's orbit, is presented. [S0556-2821(99)04706-2].

引用

页数：5

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