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Slowly rotating superdense configurations in Rosen's bimetric theory of gravitation

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Publication:799140
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DOI10.1007/BF00651948zbMath0547.70011OpenAlexW2047439926MaRDI QIDQ799140

Armen V. Sarkissian, Edward V. Chubarian

Publication date: 1984

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00651948


zbMATH Keywords

gravitational fieldbimetric theory of gravitationrotating configurations


Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Differential geometric methods (tensors, connections, symplectic, Poisson, contact, Riemannian, nonholonomic, etc.) for problems in mechanics (70G45) Software, source code, etc. for problems pertaining to mechanics of particles and systems (70-04)


Related Items (1)

The millisecond pulsar and neutron star structure




Cites Work

  • A bi-metric theory of gravitation




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