Seminars

Thomas Hambye ( U. Libre Bruxelles) - Supercool Dark Matter

Europe/Rome
Aula B ()

Aula B

Description
In dimension-less theories of dynamical generation of the weak scale, the Universe can undergo a period of low-scale inflation during which all particles are massless and super-cool. This leads to a new mechanism of generation of the cosmological Dark Matter (DM) relic density: super-cooling can easily suppress the amount of DM to the desired level. This is achieved for TeV-scale DM, if super-cooling ends when quark condensates form at the QCD phase transition.
Slides
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