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Origin of the matter-antimatter asymmetry

Michael Dine and Alexander Kusenko

Michael Dine

  • Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA

Alexander Kusenko

  • Department of Physics and Astronomy, University of California, Los Angeles, California 90095-1547, USA
  • RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973, USA

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Rev. Mod. Phys. 76, 1 – Published 16 December, 2003

DOI: https://doi.org/10.1103/RevModPhys.76.1

Abstract

Although the origin of matter-antimatter asymmetry remains unknown, continuing advances in theory and improved experimental limits have ruled out some scenarios for baryogenesis, for example, sphaleron baryogenesis at the electroweak phase transition in the Standard Model. At the same time, the success of cosmological inflation and the prospects for discovering supersymmetry at the Large Hadron Collider have put some other models in sharper focus. We review the current state of our understanding of baryogenesis with emphasis on those scenarios that we consider most plausible.

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Rev. Mod. Phys. 76, 1– Published 16 December, 2003

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