A static stable universe

Details A static stable universe A static stable universe

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...410..488c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 410, no. 2, p. 488-492.

Statistics

Computation

8

Cosmology, Stability, Universe, Astronomical Models, Computational Astrophysics, Gravitational Effects, Relativistic Theory

Scientific paper

A static and stable solution to a Newtonian cosmological model is described where the centripetal acceleration of high-temperature particles moving in a three-sphere embedded in a 4D Euclidian space balances the gravitational acceleration. This model is used to show a possible deficiency in the equations of general relativity in that the Newtonian model contains a term corresponding to centripetal accelerations that is not present in Friedmann's equations. Together with a gravitational interaction that can explain the Hubble redshift it provides a viable cosmological model.

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