Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Baryogenesis from cosmic strings at the electroweak scale

Journal Article · · Physical Review, D
 [1]
  1. Department of Physics, Boston University, 590 Commonwealth Avenue, Boston, Massachusetts 02215 (United States)
We explore the viability of baryogenesis from light scalar decays after the electroweak phase transition. A minimal model of this kind is constructed with new CP-violating interactions involving a heavy fourth family. The departure from thermal equilibrium must come from topological defects such as cosmic strings, and we show that almost any mechanism for producing the cosmic strings at the electroweak scale results in a viable theory. Baryogenesis occurs in the fourth generation but the baryon number is later transported to the visible generations. This mechanism of indirect baryogenesis allows us to satisfy experimental limits on the proton lifetime while still having perturbative baryon number violation at low energies. The fourth family has very small mixing angles which opens the possibility of distinct observable signatures in collider experiments. {copyright} {ital 1997} {ital The American Physical Society}
Research Organization:
Boston University
DOE Contract Number:
FG02-91ER40676
OSTI ID:
517007
Journal Information:
Physical Review, D, Journal Name: Physical Review, D Journal Issue: 6 Vol. 55; ISSN 0556-2821; ISSN PRVDAQ
Country of Publication:
United States
Language:
English

Similar Records

Strong CP violation, electroweak baryogenesis, and axionic dark matter
Journal Article · Tue Jan 14 23:00:00 EST 1992 · Physical Review, D (Particles Fields); (United States) · OSTI ID:5081862

Electroweak baryogenesis with vector-like leptons and scalar singlets
Journal Article · Sun Sep 01 20:00:00 EDT 2019 · Journal of High Energy Physics (Online) · OSTI ID:1611589

{ital CP} violation for electroweak baryogenesis from mixing of standard model and heavy vector quarks
Journal Article · Sun Dec 31 23:00:00 EST 1995 · Physical Review, D · OSTI ID:277450