Abstract

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 tanβ. 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.

Notes

Originally published in Physical Review D v.70 (2004): 035014. DOI: 10.1103/PhysRevD.70.035014

Keywords

b quark mass, loop corrections, neutralino relic abundance

Subject Categories

Dark matter (Astronomy), Supersymmetry

Disciplines

Physics

Publisher

American Physical Society

Publication Date

8-30-2004

Rights Information

Copyright (2004) American Physical Society

Rights Holder

American Physical Society



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