Cosmic Gas Thermodynamics at z = 1089
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Abstract The Universe at z = 1089 is treated as an expanding ideal gas. Its internal kinetic energy loss exceeds the amount absorbed by gravity and drives further expansion. A Hubble relation (Hg) is derived and compared to the value found by the ΛCDM model (HΛ) over the range z = 1089 to 0. The results suggest that the adiabatic release of energy from cosmic gas accounts for about half of present-day Universal expansion.
2011 ◽
Vol 234
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pp. 116-119
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1989 ◽
Vol 42
(2)
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pp. 290-292
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2008 ◽
Vol 6
(35)
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pp. 549-559
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2015 ◽
Vol 20
(6)
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pp. 2297-2307
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1990 ◽
Vol 12
(4)
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pp. 926-946
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