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Homogeneous isotropic cosmological model in a new scalar-tensor theory
Phys. Rev. D 26, 3747 – Published 15 December, 1982
DOI: https://doi.org/10.1103/PhysRevD.26.3747
Abstract
A Friedmann-Robertson-Walker (FRW) model is studied in the new scalar-tensor theory of gravitation proposed by Schmidt et al. There is an assumption of a particular functional relationship between the cosmological expansion factor of the FRW model and the scalar field. Exact solutions are given, and it is observed that at least in one case it is possible to obtain a model with oscillation between finite limits.
Original Article
Stability of massive objects in a new scalar-tensor theory
Phys. Rev. D 24, 1484 (1981)
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