Issue of the spherically symmetric static vacuum metric in the relativistic theory of gravity

• Authors: Vladimir Kalashnikov
• Languages of publication: EN

Abstracts

EN

The spherically symmetric vacuum metric in the relativistic theory of gravity is analyzed numerically. It is found that there is no deviation of the numerical solution from that of general relativity except in the near-horizon range. The solution obtained has the well-established analytical asymptotics for both the near-and far-horizon limits. It satisfies the causality principle and does not impose a lower limit on the graviton mass.

Keywords

EN

relativistic theory of gravity; Schwarzschild problem

Discipline

• 04.20.-q: Classical general relativity(see also 02.40.-k Geometry, differential geometry, and topology)
• 04.25.dg: Numerical studies of black holes and black-hole binaries
• 04.20.Ex: Initial value problem, existence and uniqueness of solutions

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2008
• Volume: 6
• Issue: 1
• Pages: 80-83

Dates

published

1 - 3 - 2008

online

26 - 3 - 2008

Contributors

author

Vladimir Kalashnikov

• Institut für Photonik, TU Wien, Gusshausstr. 27/387, A-1040, Vienna, Austria

References

• [1] A.A. Logunov, Relativistic theory of gravity, Nova Sc. Publ., 1998
• [2] A.A. Godizov, Cent. Eur. J. Phys. 5, 201 (2007) http://dx.doi.org/10.2478/s11534-007-0008-7[Crossref]
• [3] V.L. Kalashnikov, arXiv:astro-ph/0304466
• [4] V.L. Kalashnikov, arXiv:gr-qc/0405032 [WoS]
• [5] V.L. Kalashnikov, arXiv:gr-qc/0208070 [WoS]
• [6] V. Fock, Rev. Mod. Phys. 29, 325 (1957) http://dx.doi.org/10.1103/RevModPhys.29.325[Crossref]

Identifiers

DOI

10.2478/s11534-008-0017-1