2007
DOI: 10.1007/s00114-007-0235-1
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Cosmic vacuum energy decay and creation of cosmic matter

Abstract: In the more recent literature on cosmological evolutions of the universe, the cosmic vacuum energy has become a nonrenouncable ingredient. The cosmological constant Lambda, first invented by Einstein, but later also rejected by him, presently experiences an astonishing revival. Interestingly enough, it acts like a constant vacuum energy density would also do. Namely, it has an accelerating action on cosmic dynamics, without which, as it appears, presently obtained cosmological data cannot be conciliated with t… Show more

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Cited by 20 publications
(27 citation statements)
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“…Under cosmic perspectives binding energy is an absolutely necessary quanity to be brought into the thermodynamical energy balance. As worked out in quantitative terms by Fahr & Heyl (2007a; this then leads to the following completed relation…”
Section: The Concept Of Absolutely Empty Spacementioning
confidence: 98%
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“…Under cosmic perspectives binding energy is an absolutely necessary quanity to be brought into the thermodynamical energy balance. As worked out in quantitative terms by Fahr & Heyl (2007a; this then leads to the following completed relation…”
Section: The Concept Of Absolutely Empty Spacementioning
confidence: 98%
“…k = 0) and Λ put equal to zero, the first Friedmann equation (see Equ. (13)) simplifies into the formṘ 2 =( 8πG/3)ρR 2 = Φ(R) and thus allows to identify a relevant cosmic gravitational potential Φ(R) in analogy to the one in Hamilton-Lagrangian dynamics (see Fahr & Heyl (2007a;). Therefore at the cosmic expansion permanently work has to be done by cosmic matter against an intermaterial force per mass which for ρ ∼ R −3 is given by…”
Section: The Standard Cosmology Based On Five Cosmic Scalar Quantitiesmentioning
confidence: 99%
“…If we include the negatively valued gravitational self-binding energy (see Fahr & Heyl 2007a, 2007b into the total internal energy of a cosmic sphere with radius R, then instead of the above relation one obtains the following more complicate thermodynamic equation:…”
Section: Thermodynamics Of the Cosmic Vacuummentioning
confidence: 99%
“…Requiring a universe where in every instant the positively valued vacuum energy is compensated by its gravitationally induced self-binding energy, then , in addition to the above thermodynamic requirement, one has to also fullfill the following relation (see Fahr & Heyl 2007a, 2007b) for a vanishing total vacuum energy…”
Section: Do There Exist Two Competing Solutions?mentioning
confidence: 99%
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