4.7 Article

Light dark matter and the electroweak phase transition in the NMSSM

期刊

PHYSICAL REVIEW D
卷 85, 期 3, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.85.036003

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  1. U.S. Department of Energy [DE-AC02-07CH11359]
  2. U.S. Department of Energy (DOE), Division of HEP [DE-AC02-06CH11357]
  3. DOE [DE-FGO2-96-ER40956]

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We analyze the stability of the vacuum and the electroweak phase transition in the NMSSM close to the Peccei-Quinn symmetry limit. This limit contains light dark matter (DM) particles with a mass significantly smaller than the weak scale and also light CP-even and CP-odd Higgs bosons. Such light particles lead to a consistent relic density and facilitate a large spin-independent direct DM detection cross section, that may accommodate the recently reported signatures at the DAMA and CoGeNT experiments. Studying the one-loop effective potential at finite temperature, we show that when the lightest CP-even Higgs mass is of the order of a few GeV, the electroweak phase transition tends to become first order and strong. The inverse relationship between the direct-detection cross section and the lightest CP-even Higgs mass implies that a cross section of the order of 10(-41) cm(2) is correlated with a strong first-order phase transition.

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