The hadronization transition in the early universe
β Scribed by Gordon Baym
- Publisher
- Elsevier Science
- Year
- 1986
- Tongue
- English
- Weight
- 528 KB
- Volume
- 447
- Category
- Article
- ISSN
- 0375-9474
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π SIMILAR VOLUMES
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.
## Abstract We give a pedagogical introduction to two aspects of magnetic fields in the early Universe. We first focus on how to formulate electrodynamics in curved space time, defining appropriate magnetic and electric fields and writing Maxwell equations in terms of these fields. We then speciali
I t is a geiicrsl belief that iri some early stages of the evolutiou of the Uiiiversc unequilibriuni situations played importatit role. In order to iiicorporatc sonic deviations froin tlicrmal equilibrium into thc description of the cvolution. lierc an extension of the tliermodynamic formalism is gi