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

• Autorzy: Anton Godizov
• Języki publikacji: EN

Abstrakty

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.

Słowa kluczowe

EN

Relativistic theory of gravity; Schwarzschild problem

• Czasopismo: Open Physics
• Rocznik: 2007
• Tom: 5
• Numer: 2
• Strony: 201-206

Daty

wydano

2007-06-01

online

2007-06-01

Twórcy

autor

Anton Godizov

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

Bibliografia

• [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.

Identyfikatory

DOI

10.2478/s11534-007-0008-7