Effects of galactic dark halo rotation on WIMP direct detection

被引：51

作者：

Donato, F

Fornengo, N

Scopel, S

机构：

[1] Univ Turin, Dipartimento Fis Teor, I-10125 Turin, Italy

[2] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy

[3] Univ Zaragoza, Fac Ciencias, Inst Fis Nucl & Altas Energias, E-50009 Zaragoza, Spain

来源：

ASTROPARTICLE PHYSICS | 1998年 / 9卷 / 03期

关键词：

D O I：

10.1016/S0927-6505(98)00025-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The effects of a possible rotation of the galactic dark halo on the calculation of the direct detection rates for particle dark matter are analyzed, with special attention to the extraction of the upper limits on the WIMP-nucleon scalar cross section from the experimental data. We employ a model of dark halo rotation which describes the maximal possible effects. For WIMP masses above 50 GeV, the upper limit exclusion plot is modified by less than a factor of two when rotation is included. For lighter masses the effect can be stronger, suggesting the necessity to develop specific models of halo rotation in order to provide more accurate conclusions. (C) 1998 Elsevier Science B.V.

引用

页码：247 / 260

页数：14

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