Baryon Asymmetry of the Universe (2/2)
Abstract
In two lectures, the following topics will be discussed: (1) Why baryon asymmetry is a problem at all (2) Review of the Sakharov's conditions (3) Why old models based on GUT did not work (4) Electroweak baryogenesis (5) Leptogenesis (6) Connections to the near-future experiments.
- Authors:
- Publication Date:
- OSTI Identifier:
- 1025913
- Resource Type:
- Multimedia
- Country of Publication:
- CERN
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; BARYON ASYMMETRY; GUT; BARYOGENESIS; MATTER; ANTI MATTER; STANDARD MODEL; QUARK; HIGGS
Citation Formats
Murayama, Hitoshi. Baryon Asymmetry of the Universe (2/2). CERN: N. p., 2010.
Web.
Murayama, Hitoshi. Baryon Asymmetry of the Universe (2/2). CERN.
Murayama, Hitoshi. Wed .
"Baryon Asymmetry of the Universe (2/2)". CERN. https://www.osti.gov/servlets/purl/1025913.
@article{osti_1025913,
title = {Baryon Asymmetry of the Universe (2/2)},
author = {Murayama, Hitoshi},
abstractNote = {In two lectures, the following topics will be discussed: (1) Why baryon asymmetry is a problem at all (2) Review of the Sakharov's conditions (3) Why old models based on GUT did not work (4) Electroweak baryogenesis (5) Leptogenesis (6) Connections to the near-future experiments.},
doi = {},
journal = {},
number = ,
volume = ,
place = {CERN},
year = {Wed May 26 00:00:00 EDT 2010},
month = {Wed May 26 00:00:00 EDT 2010}
}