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Talk43 min

Scale invariance: super-cooling and Dark Matter

Satoshi Iso and Daniele Teresi · CERN

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About

If the electroweak sector of the Standard Model is described by classically conformal dynamics, the early Universe evolution can be substantially altered. In particular, one generically has a significant period of super-cooling, often ended when quark condensates form at the QCD phase transition. This scenario is potentially rich in cosmological consequences, such as renewed possibilities for electroweak baryogenesis and gravitational-wave production. In the second part of the talk we will focus on Super-cool Dark Matter, a new mechanism of generation of the cosmological Dark-Matter relic density: super-cooling can easily suppress the amount of Dark Matter down to the desired level. This mechanism generically takes place in old and new scale-invariant models..

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The talk

  1. Scale invariance: super-cooling and Dark Matter 2019-01-29 · 43 min · CERN's player

Credits and licence

Institution
CERN
Department
TH institutes
Taught by
Satoshi Iso, Daniele Teresi
Year
2019
Language
English
Subjects
Physics, Astronomy and space
Source
CERN
Licence
CERN, as CERN states it. CERN's terms
Attribution
© CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
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