Certain vacuum Bianchi-type models in a new relativistic theory of gravitation

Details Certain vacuum Bianchi-type models in a new relativistic theory of gravitation Certain vacuum Bianchi-type models in a new relativistic theory of gravitation

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179..223s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 2, May 1991, p. 223-235.

Physics

5

Dynamic Models, Field Theory (Physics), Gravitation Theory, Relativistic Theory, Gravitational Fields, Hubble Constant, Relativity, Space-Time Functions

Scientific paper

The cosmological models of Bianchi type I, III, V, and VI(0), and Kantowski-Sachs models are investigated in a vacuum and their dynamical behavior is discussed. The solutions are consistent with the physical nature of the field quantities and are quantitatively supported by experimental evidence about the cosmological constant. Energy conservation is possible even though both the cosmological term Lambda and the gravitational constant may vary with time.

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