The sensitivity of accretion disk models with respect to its inner boundary conditions, being located in the strong gravity region of a highly compact central body, is used t o discuss a possibility of strong field tests of gravitation via compact source observations. Within the bimetric theory of g
โฆ LIBER โฆ
Accretion disks in the bimetric theory of gravitation: Strong gravity sensitivity of the inner disk edge
โ Scribed by E. V. Chubaryan; H. G. Paul; A. V. Sarkisyan
- Publisher
- Springer
- Year
- 1988
- Tongue
- English
- Weight
- 545 KB
- Volume
- 27
- Category
- Article
- ISSN
- 0571-7256
No coin nor oath required. For personal study only.
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In Rosen's "bimetric" theory of gravity the (local) speed of gravitational radiation u. is determined by the combined effects of cosmological boundary values and nearby concentrations of matter. It is possible for v. to be less than the speed of light. I show here that emission of gravitational radi