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NASA NTRS · 19920008427

Axino-induced baryogenesis

Abstract

We consider the possibility that the baryon asymmetry is generated at low energies as a consequence of the axino decay. We analyze models in which the axino, the superpartner of the axion, is heavy and decays into gluinos at temperatures T approx. = 1 GeV. If CP and B violating couplings for the quark superfields are included, the subsequent decay of these out of equilibrium gluinos can act as seeds for baryogenesis. The required amount of CP violation is well consistent with the bounds on the electric dipole moment of the neutron and the mechanism works even for low reheating temperatures after inflation (T sub RH greater or approx. = 10 exp 4 GeV).

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BibTeXRIS

Mollerach, Silvia, Roulet, Esteban. 1991-11-01. Axino-induced baryogenesis. https://ntrs.nasa.gov/citations/19920008427

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