Opening the window to the cogenesis with Affleck-Dine mechanism in gravity mediation
arXiv:1211.6813 · doi:10.1016/j.physletb.2013.01.017
Abstract
The observed baryon and dark matter densities are equal up to a factor of 5. This observation indicates that the baryon asymmetry and dark matter have the same origin. The Affleck-Dine baryogenesis is one of the most promising mechanisms in this context. Q balls, which are often formed in the early Universe associated with the Affleck-Dine baryogenesis, decay both into supersymmetric particles and into quarks. Recently, it was pointed out that annihilation of squarks into quarks gives a dominant contribution to the Q-ball decay rate and the branching ratio of Q-ball decay into supersymmetric particles changes from the previous estimate. In this paper, the scenario of baryon and dark matter cogenesis from Q ball in gravity mediation is revisited in respect of the improved Q-ball decay rates. It is found that the successful cogenesis takes place when a wino with mass 0.3-1 TeV is dark matter.
5 pages, 3 figures
References in corpus (3)
Cited by in corpus (13)
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- A solution to the baryon-DM coincidence problem in the CMSSM with a 126-GeV Higgs boson
- Cosmic perturbations, baryon asymmetry and dark matter from the minimal supersymmetric standard model
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- Scattering of fermions on a one-dimensional Q-ball
- Affleck-Dine leptogenesis and its backreaction to inflaton dynamics
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