Dark matter and the baryon asymmetry

Oct, 2005
Published in:
  • Phys.Rev.Lett. 96 (2006) 041302
e-Print:

Citations per year

200520102015202020240510152025
Abstract:
We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number BXB_X, and σXˉannih<σXannih\sigma^{\rm annih}_{\bar{X}} < \sigma^{\rm annih}_{X} , the Xˉ\bar{X}'s freeze out at a higher temperature and have a larger relic density than XX's. If m_X \lsi 4.5 B_X GeV and the annihilation cross sections differ by O\mathcal{O}(10%) or more, this type of scenario naturally explains the observed ΩDM5Ωb\Omega_{DM} \approx 5 \Omega_b. Two concrete examples are given, one of which can be excluded on observational grounds.
  • 98.80.Cq
  • 95.35.+d
  • cosmology
  • dark matter
  • dark matter: interaction
  • baryon: asymmetry
  • baryon number
  • H baryon
  • postulated particle