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

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/158554· OSTI ID:6536504
Energy flux doncitions imposed on spherical boundary surfaces are examined. The zero flux restriction which is the hallmark of the standard ''Swiss cheese'' type construction, is relaxed. We discuss a class of locally inhomogeneous exact solutions to the Einstein equations which admit an effectively Newtonian accretion mode.
Research Organization:
Astronomy Group, Department of Physics, Queen's University at Kingston, Ontario, Canada
OSTI ID:
6536504
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 242:3; ISSN ASJOA
Country of Publication:
United States
Language:
English

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Related Subjects

640106* -- Astrophysics & Cosmology-- Cosmology
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BOUNDARY CONDITIONS
CONFIGURATION
COSMIC DUST
COSMOLOGICAL MODELS
COSMOLOGY
DUSTS
EINSTEIN FIELD EQUATIONS
EQUATIONS
FIELD EQUATIONS
FIELD THEORIES
GENERAL RELATIVITY THEORY
MATHEMATICAL MODELS
SPHERICAL CONFIGURATION