Matter and Antimatter in the Universe
arXiv:1204.4186 · doi:10.1088/1367-2630/14/9/095012
Abstract
We review observational evidence for a matter-antimatter asymmetry in the early universe, which leads to the remnant matter density we observe today. We also discuss observational bounds on the presence of antimatter in the present day universe, including the possibility of a large lepton asymmetry in the cosmic neutrino background. We briefly review the theoretical framework within which baryogenesis, the dynamical generation of a matter-antimatter asymmetry, can occur. As an example, we discuss a testable minimal model that simultaneously explains the baryon asymmetry of the universe, neutrino oscillations and dark matter.
Invited contribution to the New Journal of Physics Focus Issue "Origin of Matter" (New J. Phys. 14 (2012) 095012); this version is identical to the published article up to a few updates in the references
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Cited by in corpus (25)
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- Experimental searches for the chiral magnetic effect in heavy-ion collisions
- Cosmological Phase Transitions and their Properties in the NMSSM
- CMB constraints on the inflaton couplings and reheating temperature in -attractor inflation
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- Leptogenesis in crossing and runaway regimes
- The effects of the U(1) Chern-Simons term and its baryonic contribution on matter asymmetries and hypermagnetic fields
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- On the Minimal Mixing of Heavy Neutrinos
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- Frequency domain method of the search for the deuteron electric dipole moment in a storage ring with imperfections
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