Abundance of Primordial Holes Produced by Cosmological First-Order Phase Transition

DOI10.1143/PTP.68.1979zbMath1098.83593OpenAlexW2015086978MaRDI QIDQ2750471

Hideo Kodama, Misao Sasaki, Katsuhiko Sato

Publication date: 18 October 2001

Published in: Progress of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1143/ptp.68.1979

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantization in field theory; cohomological methods (81T70)

Related Items (19)

The energy budget of cosmological first-order phase transitions beyond the bag equation of state ⋮ Primordial black holes from spectator field bubbles ⋮ Inflation is always semi-classical: diffusion domination overproduces Primordial Black Holes ⋮ Solitons as key parts to produce a universe in the laboratory ⋮ Phase transition dynamics and gravitational wave spectra of strong first-order phase transition in supercooled universe ⋮ Primordial black hole formation by vacuum bubbles. Part II ⋮ Primordial black holes as a probe of strongly first-order electroweak phase transition ⋮ Primordial black hole formation with full numerical relativity ⋮ Primordial black holes from strong first-order phase transitions ⋮ Probing first-order electroweak phase transition via primordial black holes in the effective field theory ⋮ Primordial black hole isocurvature modes from non-Gaussianity ⋮ From Hubble to bubble ⋮ Primordial black holes—perspectives in gravitational wave astronomy ⋮ Dark matter as dark dwarfs and other macroscopic objects: multiverse relics? ⋮ Brans-Dicke theory and primordial black holes in early matter-dominated era ⋮ Vacuum energy and primordial black holes in Brans-Dicke theory ⋮ Friction pressure on relativistic bubble walls ⋮ Primordial black hole formation by vacuum bubbles ⋮ Cosmology of strongly interacting fermions in the early universe

This page was built for publication: Abundance of Primordial Holes Produced by Cosmological First-Order Phase Transition