Vacuum Bianchi type V and VI(0) cosmological models in a new scalar-tensor theory of gravitation

Details Vacuum Bianchi type V and VI(0) cosmological models in a new scalar-tensor theory of gravitation Vacuum Bianchi type V and VI(0) cosmological models in a new scalar-tensor theory of gravitation

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..125v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 1, Nov. 1989, p. 125-131. Research supported by the Council of Sc

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Astronomical Models, Cosmology, Gravitation Theory, Scalars, Tensor Analysis, Computational Astrophysics, Field Theory (Physics)

Scientific paper

Using the new scalar-tensor theory of gravitation proposed by Schmidt at
al. (1981), the Bianchi type V and VI(0) vacuum cosmological models are
studied for the special case when the scalar field is massless and
conformally invariant. Some physical properties of these models are also
discussed.

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