3-8 July 2016
The University of Melbourne
Australia/Melbourne timezone

Relic density and baryogenesis from natural SUSY with mixed axion-higgsino dark matter

4 Jul 2016, 14:20
20m
Carillo Gantner Theatre ()

Carillo Gantner Theatre

Carrillo Gantner Theatre, Sidney Myer Asia Centre The University of Melbourne VIC 3010 Australia
Talk Dark Matter and Particle Astrophysics Dark Matter and Particle Astrophysics

Speaker

Howard Baer (University of Oklahoma)

Description

We describe an eight-coupled-Boltzmann equation calculation of the mixed axion-higgsino dark matter scenario which is expected from natural SUSY. Typically the relic density is axion dominated unless late decaying axinos or saxions feed the WIMP abundance. While thermal leptogenesis is barely viable, non-thermal and Affleck-Dine leptogenesis remain robust scenarios to generate the matter-anti-matter asymmetry.

Primary author

Howard Baer (University of Oklahoma)

Presentation Materials