Protecting the baryon asymmetry with thermal masses

S. Davidson, K. Kainulainen, K. A. Olive

Research output: Contribution to journalArticlepeer-review

18 Scopus citations

Abstract

We consider the evolution of baryon number B in the early universe under the influence of rapid sphaleron interactions and show that B will remain nonzero at all times even in the case of B - L = 0. This result arises due to thermal Yukawa interactions that cause nonidentical dispersion relations (thermal masses) for different lepton families. We point out the relevance of our result to the Affleck-Dine type baryogenesis.

Original languageEnglish (US)
Pages (from-to)339-344
Number of pages6
JournalPhysics Letters B
Volume335
Issue number3-4
DOIs
StatePublished - Sep 8 1994

Bibliographical note

Funding Information:
K.K. wishes to thank Jim Cline and S.D. wishes to thank H. Murayama and J. March-Russel for useful discussions. This research was supported by the DOE grant DE-FB02-94ER40823, by NSF grant AST 91-20005, by NSERC, KAO:s Presidential Young Investigator Award and by (K.K.) the Finnish Academy.

Fingerprint Dive into the research topics of 'Protecting the baryon asymmetry with thermal masses'. Together they form a unique fingerprint.

Cite this