| Literature DB >> 15089191 |
Takehiko Asaka1, Dmitri Grigoriev, Vadim Kuzmin, Mikhail Shaposhnikov.
Abstract
If inflaton couples very weakly to ordinary matter, the reheating temperature of the Universe can be lower than the electroweak scale. In this Letter we show that the late reheating occurs in a highly nonuniform way, within narrow areas along the jets produced by ordinary particles originated from inflaton decays. Depending on inflaton mass and decay constant, the initial temperature inside the lumps of the overheated plasma may be large enough to trigger the unsuppressed sphaleron processes with baryon number nonconservation. This allows for efficient local electroweak baryogenesis at reheating temperatures TR approximately O(10) GeV.Entities:
Year: 2004 PMID: 15089191 DOI: 10.1103/PhysRevLett.92.101303
Source DB: PubMed Journal: Phys Rev Lett ISSN: 0031-9007 Impact factor: 9.161