Binding energy for spherical stars

Details Binding energy for spherical stars Binding energy for spherical stars

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cqgra...7.1953b&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 7, Nov. 1990, p. 1953-1959.

Physics

26

Gravitational Effects, Relativistic Theory, Shell Stars, Conformal Mapping, Mass Distribution, Stellar Mass

Scientific paper

It is proved that the binding energy for a spherical distribution of
matter at rest, in general relativity, is bounded by the Newtonian value
for a shell with same mass and radius. This confirms a conjecture of
Arnowitt, et al.

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