COSMOLOGICAL MODELS IN THE PRESENCE OF SCALAR FIELDS

G. H. Harutunyan; A. G. Movsissyan; A. S. Piloyan

doi:10.46991/PYSU:A/2008.42.1.047

COSMOLOGICAL MODELS IN THE PRESENCE OF SCALAR FIELDS

Authors

G. H. Harutunyan Chair of Theoretical Physics, YSU, Armenia
A. G. Movsissyan Chair of Theoretical Physics, YSU, Armenia
A. S. Piloyan Chair of Theoretical Physics, YSU, Armenia

DOI:

https://doi.org/10.46991/PYSU:A/2008.42.1.047

Keywords:

Jordan–Brans–Dicke tensor-scalar theory, cosmological scalar, cosmological model

Abstract

In the present work the construction of the cosmological model which takes into account the presence of dark energy is realized within the framework of Jordan–Brans–Dicke tensor-scalar theory with dominating minimal and non minimal coupled scalar fields in the presence of the cosmological scalar.

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Published

2023-09-06

How to Cite

Harutunyan, G. H., Movsissyan, A. G., & Piloyan, A. S. (2023). COSMOLOGICAL MODELS IN THE PRESENCE OF SCALAR FIELDS. Proceedings of the YSU A: Physical and Mathematical Sciences, 42(1 (215), 47–54. https://doi.org/10.46991/PYSU:A/2008.42.1.047