Numerical spherically symmetric static solution of the RTG equations outside of matter

• Authors: Anton Godizov
• Languages of publication: EN

Abstracts

EN

There was obtained a numerical external solution for the exact system of the RTG equations using natural boundary conditions in the static spherically symmetric case. The properties of the solution are discussed.

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)
• 04.20.Ha: Asymptotic structure

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2007
• Volume: 5
• Issue: 2
• Pages: 201-206

Dates

published

1 - 6 - 2007

online

1 - 6 - 2007

Contributors

author

Anton Godizov

• Institute for High Energy Physics, 142281, Protvino, Russia

References

• [1] C.W. Misner, K.S. Thorn and J.A. Wheeler: Gravitation, W.H. Freeman & Co., San Francisco, 1973.
• [2] A.A. Logunov: The Theory of Gravity, Nauka, Moscow, 2001.
• [3] V.A. Fock: The theory of space, time and gravitation, Pergamon Press, Oxford, 1964.
• [4] V.L. Kalashnikov: Proc. XXV Int. Workshop on Fundamental Problems of High Energy Physics and Field Theory, 25–28 June 2002, Protvino, Russia; V.L. Kalashnikov: “Quintessential cosmological scenarios in the relativistic theory of gravitation”, Preprint: arXiv:gr-qc/0208070.
• [5] V.L. Kalashnikov: “Static spherically symmetric collapsar in the relativistic theory of gravitation: numerical approach and stability analysis”, Preprint: arXiv:astroph/0304466; V.L. Kalashnikov: “Perturbations of the spherically symmetric collapsar in the relativistic theory of gravitation: axial perturbations. I”, Preprint: arXiv:gr-qc/0405032.

Identifiers

DOI

10.2478/s11534-007-0008-7