Sensitivity of supersymmetric dark matter to the b quark mass -: art. no. 035014

被引:40
作者
Gómez, ME
Ibrahim, T
Nath, P
Skadhauge, S
机构
[1] Inst Super Tecn, Dept Fis, P-1049001 Lisbon, Portugal
[2] Univ Alexandria, Fac Sci, Dept Phys, Alexandria, Egypt
[3] Northeastern Univ, Dept Phys, Boston, MA 02115 USA
来源
PHYSICAL REVIEW D | 2004年 / 70卷 / 03期
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.70.035014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An analysis of the sensitivity of supersymmetric dark matter to variations in the b quark mass is given. Specifically we study the effects on the neutralino relic abundance from supersymmetric loop corrections to the mass of the b quark. It is known that these loop corrections can become significant for large tan beta. The analysis is carried out in the framework of MSUGRA and we focus on the region where the relic density constraints are satisfied by resonant annihilation through the s-channel Higgs poles. We extend the analysis to include CP phases taking into account the mixing of the CP-even and CP-odd Higgs boson states which play an important role in determining the relic density. Implications of the analysis for the neutralino relic density consistent with the recent WMAP relic density constraints are discussed.
引用
收藏
页数:18
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