Imbedding a Schwarzschild mass into cosmology

Details Imbedding a Schwarzschild mass into cosmology Imbedding a Schwarzschild mass into cosmology

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvd..29.3002v&link_type=abstract

Physical Review D (Particles and Fields), Volume 29, Issue 12, 15 June 1984, pp.3002-3003

Mathematics

Logic

5

Scientific paper

The recent method of Gautreau of imbedding a Schwarzschild mass into a cosmological perfect fluid with equation of state p=p(ρ) is discussed. It is shown that the application of the method to a geodesic fluid with p≠0 necessarily reproduces an exact Friedmann-Robertson-Walker solution in the outer region. It is claimed that physically realistic exterior regions necessarily must have acceleration as well as shear.

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