Cosmological baryon-number domain structure and the first order phase transition of a vacuum

1981/02/01 by Katsuhiko Sato · 23 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Particle physics theoretical and experimental studies

paper · doi:10.1016/0370-2693(81)90805-4

crossref issued 1981/02/01 · crossref published 1981/02/01 · crossref published-print 1981/02/01 · openalex publication_date 1981/02/01 · crossref created 2002/11/12 · crossref deposited 2020/03/11 · openalex created_date 2025/10/10 · crossref indexed 2026/06/29 · openalex updated_date 2026/07/22

Cited by

• Shear viscous effects on the primordial power spectrum from warm inflation
• Could there be something rather than nothing?
• Baryogenesis, 30 years after
• Entropy and uncertainty of squeezed quantum open systems
• Universe out of a breathing bubble
• Inflationary cosmology — a dissipative quantum field theory process
• Reconstruction of inflation models
• Chaotic inflation in higher derivative gravity theories
• Inhomogeneous fluids for warm inflation
• Weakly non-Gaussian formula for the Minkowski functionals in general dimensions
• “All that Matter … in One Big Bang …”, &Other Cosmological Singularities
• A new limit on the flux of cosmic antihelium
• Generalizing the swampland: Embedding P(X,φ) inflationary theories in a curved multifield space
• Gravitational waves from first order phase transitions as a probe of an early matter domination era and its inverse problem
• Antimatter regions in the early universe and big bang nucleosynthesis
• NATURAL INFLATION: STATUS AFTER WMAP THREE-YEAR DATA
• The warm inflationary universe
• Dynamical analysis of attractor behavior in constant roll inflation
• Preheating with nonminimally coupled scalar fields in higher-curvature inflation models
• On classical stability with broken supersymmetry
• Search for GUT monopoles at Super–Kamiokande
• Natural inflation: Status after WMAP 3-year data
• Cosmic inflation [wikipedia]