## 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
Extended thermodynamics in the early Universe
✍ Scribed by B. Lukács; K. Martinás; T. Pacher
- Publisher
- John Wiley and Sons
- Year
- 1986
- Tongue
- English
- Weight
- 1002 KB
- Volume
- 307
- Category
- Article
- ISSN
- 0004-6337
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✦ Synopsis
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 given, wherc, using the notion of ekaentropy, new tcrms are introduced into the Gibbs-Duheln relation for reprcsenting the deviation. Two situations are investigated in simplified modcls : the primordial tliermalisation in the syminctric phase of GUT, and the development of a nonthcrmal distribution for massive neutrinos.
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By introducing the Bose-Einstein condensation dynamics (BEC), we develop a unified model of dark energy and dark matter . The two phases of BEC (= dark energy) and normal gas (=dark matter) transform with each other through the phase transition. We study the present mild acceleration, the inflation