Dissipative cosmology with decaying vacuum energy

A closed cosmological model that begins with a phase of generalized inflation followed by a Friedmann-like period is proposed.

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Bibliographische Detailangaben
Veröffentlicht in:	Physical review. D, Particles and fields Particles and fields, 1992-05, Vol.45 (10), p.3869-3872
Hauptverfasser:	CALVAO, M. O, DE OLIVEIRA, H. P, PAVON, D, SALIM, J. M
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy ASTROPHYSICS BLACK HOLES COSMOLOGICAL MODELS Cosmology Earth, ocean, space EINSTEIN FIELD EQUATIONS ENERGY DENSITY ENERGY LOSSES EQUATIONS Exact sciences and technology FIELD EQUATIONS HYDROSTATICS INFLATIONARY UNIVERSE LOSSES MATHEMATICAL MODELS Origin and formation of the universe PARTICLE MODELS PARTICLE PRODUCTION PHASE TRANSFORMATIONS PHYSICS OF ELEMENTARY PARTICLES AND FIELDS STANDARD MODEL Stellar systems. Galactic and extragalactic objects and systems. The universe THERMODYNAMICS UNIFIED GAUGE MODELS 662110 > General Theory of Particles & Fields-- Theory of Fields & Strings-- (1992-) UNIVERSE VACUUM STATES VISCOSITY
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Beschreibung
Zusammenfassung:	A closed cosmological model that begins with a phase of generalized inflation followed by a Friedmann-like period is proposed.
ISSN:	0556-2821 1089-4918
DOI:	10.1103/PhysRevD.45.3869