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Cosmic Matter Creation from Viscous Energy Dissipation: A Resurrection of Fred Hoyle’s Dream
Publication year - 2019
Publication title -
advances in theoretical and computational physics
Language(s) - English
Resource type - Journals
ISSN - 2639-0108
DOI - 10.33140/atcp.02.01.02
Subject(s) - physics , equation of state , universe , classical mechanics , stress–energy tensor , metric expansion of space , dark energy , cosmology , astrophysics , quantum mechanics , exact solutions in general relativity
Fred Hoyle is known as creator of the so-called “steady state universe” which latter, although permanently expanding,does not change its state of matter, especially keeping its density constant. To achieve this virtue Hoyle introducedinto the energy-momentum tensor of the GRT field equations a term derived from a so-called ad-hoc creation fieldastonishingly leading to field equations very similar to the ones already developed by Tolman when introducingenergy sources connected with viscous dissipation forces acting upon dust-like cosmic matter [1]. In this article herewe shall again study the action of viscous forces in cosmic baryonic matter and shall boil it down to volume viscositycontributions to the viscous stress tensor in a universe with a compressible Hubble flow. Assuming that by collisionsof any kind the energy of the differential Hubble drift between two collision points of cosmic matter particles, seenin the non-inertial rest frames of moving particles, is randomized and converted into thermal energy, one can thenshow with the help of a kinetic transport equation that during the cosmic expansion permanently thermal energy isgenerated leading to the result that the matter temperature, instead of falling-off, is linearly increasing with the scaleof the universe. This not only questions the standard use of the model of pressure-free, dust-like matter in the universe,but furthermore indicates the possibility of an asymptotic cosmic-ray-like matter state including the possibility ofmatter creation by pair production.

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