Bianchi type-I cosmological model in the scale covariant theory
- 1 May 1986
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 3 (3), 481-486
- https://doi.org/10.1088/0264-9381/3/3/021
Abstract
The author derives Bianchi type-I cosmological models in the scale covariant theory. Raychaudhuri type equations are written and it is pointed out that a big bang type of singularity may not always occur, in contrast to the general relativistic Bianchi type-I model. The behaviour of the solutions near the initial singularity, when it occurs, is discussed, as is that at late stages.This publication has 5 references indexed in Scilit:
- Can the big-bang singularity be avoided in the scale-covariant theory?Astrophysics and Space Science, 1985
- Power law singularities in orthogonal spatially homogeneous cosmologiesGeneral Relativity and Gravitation, 1984
- Scale covariance and G-varying cosmology. III - The /m, z/, /theta[SUB]m,[/SUB] z/, /theta[SUB]i,[/SUB] z/, and /N/m/, m/ testsThe Astrophysical Journal Supplement Series, 1979
- Scale-covariant theory of gravitation and astrophysical applicationsPhysical Review D, 1977
- Long range forces and broken symmetriesProceedings of the Royal Society of London. Series A - Mathematical and Physical Sciences, 1973