Cosmological Constant, Dark Matter, and Electroweak Phase Transition
arXiv:1108.5193 · doi:10.1103/PhysRevD.84.103513
Abstract
Accepting the fine tuned cosmological constant hypothesis, we have recently proposed that this hypothesis can be tested if the dark matter freeze out occurs at the electroweak scale and if one were to measure an anomalous shift in the dark matter relic abundance. In this paper, we numerically compute this relic abundance shift in the context of explicit singlet extensions of the Standard Model and explore the properties of the phase transition which would lead to the observationally most favorable scenario. Through the numerical exploration, we explicitly identify a parameter space in a singlet extension of the standard model which gives order unity observable effects. We also clarify the notion of a temperature dependence in the vacuum energy.
58 pages, 10 figures
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- Inert Doublet Dark Matter with Strong Electroweak Phase Transition
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- Improved sphaleron decoupling condition and the Higgs coupling constants in the real singlet-extended SM
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- Thermal Dark Energy
- Probing Electroweak Baryogenesis induced by extra bottom Yukawa coupling via EDMs and collider signatures
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