Vacuum Bianchi type-III cosmological models in Ross and Dunn theories of gravitation

Abstract Spatially-homogeneous and anisotropic-vacuum Bianchi type-III cosmological models are obtained in scalar-tensor theories of gravitation proposed by Ross and Dunn. Some physical properties of the models are also discussed.

Gespeichert in:

Autor*in:	Shanthi, K. [verfasserIn] Rao, V. U. M. Reddy, D. R. K. Venkateswarlu, R.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1991

Schlagwörter:	Cosmological Model

Anmerkung:	© Kluwer Academic Publishers 1991

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 175(1991), 2 vom: Jan., Seite 241-245
Übergeordnetes Werk:	volume:175 ; year:1991 ; number:2 ; month:01 ; pages:241-245

Links:	Volltext

DOI / URN:	10.1007/BF00644286

Katalog-ID:	OLC2066183458

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abstract	Abstract Spatially-homogeneous and anisotropic-vacuum Bianchi type-III cosmological models are obtained in scalar-tensor theories of gravitation proposed by Ross and Dunn. Some physical properties of the models are also discussed. © Kluwer Academic Publishers 1991
abstractGer	Abstract Spatially-homogeneous and anisotropic-vacuum Bianchi type-III cosmological models are obtained in scalar-tensor theories of gravitation proposed by Ross and Dunn. Some physical properties of the models are also discussed. © Kluwer Academic Publishers 1991
abstract_unstemmed	Abstract Spatially-homogeneous and anisotropic-vacuum Bianchi type-III cosmological models are obtained in scalar-tensor theories of gravitation proposed by Ross and Dunn. Some physical properties of the models are also discussed. © Kluwer Academic Publishers 1991
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Vacuum Bianchi type-III cosmological models in Ross and Dunn theories of gravitation

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