Q-ball Evolution, B-ball Baryogenesis and the f_{B} Problem

Abstract

We consider some of the issues surrounding the formation and evolution of Q-balls in the MSSM and its extensions. The ratio of the baryon number packed into Q-balls to that outside, f_{B}, plays a fundamental role in determining the relationship of dark matter to the baryon number in the Universe at present. The final value of f_{B} will depend upon the details of the formation of Q-balls from the collapse of the Affleck-Dine condensate and upon the subsequent evolution of the ensemble of Q-balls. We discuss the implications for neutralino dark matter in the gravity-mediated scenario and show that a light neutralino is necessary in most cases to account for the baryon to dark matter ratio, with an NMSSM singlino LSP of mass m_χ \lae 20 \GeV being a favoured candidate.

26 pages, LaTeX

References in corpus (1)

• The Extragalactic Distance Scale

Cited by in corpus (5)

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• Higgsino and Wino Dark Matter from Q-ball Decay in Affleck-Dine Baryogenesis
• Affleck-Dine baryo/leptogenesis with a gauged U(1)(B-L)
• Defects composed of kinks and Q-balls: analytical solutions and stability
• Families of Q-balls in a deformed $O(4)$ linear sigma model