Sterne Und Weltraum
DOI: 10.1515/9783110221596.439
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6 Kosmologie

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“…In the following cosmological considerations we treat the cosmic vacuum by quantities denoting its vacuum energy density ε vac and its associated vacuum pressure p vac , like done in case of a hydrodynamic fluid which in general relativity theory is described by the following fluid-type hydrodynamical energy-momentum tensor (see e.g Goenner 1996;Overduin & Fahr 2001;Blome, Hoell & Priester 2002;Fahr 2004)…”
Section: Thermodynamics Of the Cosmic Vacuummentioning
confidence: 99%
“…In the following cosmological considerations we treat the cosmic vacuum by quantities denoting its vacuum energy density ε vac and its associated vacuum pressure p vac , like done in case of a hydrodynamic fluid which in general relativity theory is described by the following fluid-type hydrodynamical energy-momentum tensor (see e.g Goenner 1996;Overduin & Fahr 2001;Blome, Hoell & Priester 2002;Fahr 2004)…”
Section: Thermodynamics Of the Cosmic Vacuummentioning
confidence: 99%
“…Then with the help of the well-known photon temperaturescale relation T ∼ (1/R) (e.g. see [8,35]) one would furthermore find for the beginning t b and the end t e of the recombination era the relation R e /R b = t e /t b yielding where the beginning of the recombination period, as usually assumed in cosmology, was timed with t b 380000 years.…”
Section: The Process Of Recombinationmentioning
confidence: 99%
“…those with Λ ¼ 0) (for a review, see Friedmann 1922Friedmann , 1924, or those with Λ] 0 (see reviews given, e.g. by Goenner 1996;and Blome et al 2002) the actual Hubble constant is determined by:…”
Section: A Consistency Check With Cosmological Factsmentioning
confidence: 99%