Mathematics – Logic
Scientific paper
Apr 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993gregr..25..327c&link_type=abstract
General Relativity and Gravitation, Volume 25, Issue 4, pp.327-341
Mathematics
Logic
Scientific paper
The dynamics of the production of relative high frequency gravitational waves by astrophysical events taking place within the galaxies in the cosmological context can be well represented by a phenomenological description of the generating processes through a “radiation energy profile” that contains two adjustable parameters. This profile gives a relation between the total pressure and energy density of the matter generating gravitational radiation together with the “waves” themselves, both treated as ordinary hydrodynamic fluids. The resulting cosmological models then represent, in a descriptive way only, universes filled with two interacting fluids: on the one hand gravitational radiation, and the matter which emits it but does not reabsorb it, on the other. It is shown that the dynamic effects of the model can be significant, even if the conversion rate of matter into gravitational radiation is relatively small.
Cervantes-Cota Jorge
Chauvet Pablo
Klapp Jaime
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