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The formation of primary galactic nuclei during phase transitions in the early universe

✍ Scribed by S. G. Rubin; A. S. Sakharov; M. Yu. Khlopov

Book ID
110127370
Publisher
Springer
Year
2001
Tongue
English
Weight
94 KB
Volume
92
Category
Article
ISSN
1063-7761

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The isothermal coniinement transition in the early Universc is trcatcd. For the bag model equation of state a very large entropy production is found at sufficiently large supercooling. This trcnicndous entropy increase can signiiicantly dilute the primordial monopole or baryon to cntropy ratio.