Physics
Scientific paper
May 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20..615g&link_type=abstract
(Astrofizika, vol. 20, May-June 1984, p. 615-629) Astrophysics (ISSN 0571-7132), vol. 20, no. 3, Nov. 1984, p. 344-353. Translat
Physics
2
Gravitation Theory, Vacuum, Celestial Bodies, Equations Of State, Field Theory (Physics), Space-Time Functions, Tensors
Scientific paper
The theoretical consequences of ascribing an energy-momentum tensor to the vacuum and assuming that the vacuum participates in forming the space-time metric are examined. The vacuum problem is investigated in the case of a centrally symmetric static field. Some important properties of the tensor are established using the symmetry of the problem and by comparisons with post-Newtonian and Newtonian limits. Exterior solutions are found, and the interior problem and a procedure for matching the solutions on the surface of a celestial body are formulated. It is argued that in celestial bodies the matter, gravitational vacuum, and metric form a unity determined by the solution of the gravitational field equations.
Grigorian Sh. L.
Saakian G. S.
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