Local inhomogeneities in a Robertson-Walker background. II - Flux conditions at boundary surfaces

Details Local inhomogeneities in a Robertson-Walker background. II - Flux conditions at boundary surfaces Local inhomogeneities in a Robertson-Walker background. II - Flux conditions at boundary surfaces

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...242.1238l&link_type=abstract

Astrophysical Journal, Part 1, vol. 242, Dec. 15, 1980, p. 1238-1242. Research supported by the Queen's University and Natural

Astronomy and Astrophysics

Astronomy

10

Astronomical Models, Cosmology, Einstein Equations, Energy Transfer, Inhomogeneity, Relativity, Black Holes (Astronomy), Boundary Value Problems, Galactic Evolution, Gravitational Waves, Spheres

Scientific paper

Energy flux conditions imposed on spherical boundary surfaces are
examined. The zero-flux restriction, which is the hallmark of the
standard Swiss cheese type construction, is relaxed. A class of locally
inhomogeneous exact solutions to the Einstein equations which admit an
effectively Newtonian accretion model is discussed.

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