INTERACTING SCALAR FIELD IN THE THEORY OF GRAVITY
Abstract
In the framework of the scalar-tensor theory of gravitation, a scalar field is considered, whose source is the trace of own energy-momentum tensor and the trace of the energy-momentum tensor of matter. The potential that enters the Lagrangian of a scalar field depends on three parameters: scalar interaction constant, scalar field mass, and constant that determines the minimum of the field energy. The representation of the scalar-tensor theory on the Minkowski background with a linear connection between the metric and the tensor gravitational potential is considered, and the additional conditions for field equations are obtained that restriction a tensor field over its spin states. For a cosmological problem, it is shown that additional conditions lead to a spatially flat universe according to observations. Numerical solutions of field equations are obtained and on their basis it is shown that the cosmological parameters of the model well describe modern observational data and the scalar field under consideration can then successfully simulate dark energy. The area of variation of parameters of the cosmological solution was studied and a cosmological scalar-tensor solution was compared with the ΛCDM-model of General Relativity. Depending on the model parameters for cosmological evolution, possible scenarios are analyzed.
Keywords
About the Authors
Yu. P. VyblyiBelarus
Ph. D. (Physics and Mathematics), Leading Researcher of the Theoretical Physics Laboratory
68, Nezavisimosti Ave., 220072, Minsk
A. A. Leonovich
Belarus
Ph. D. (Physics and Mathematics), Assistant Professor of the Department of Physics
6, P. Brovka Str., 220013, Minsk
References
1. Riess A. G., Filippenko A. V., Challis P., Clocchiatti A, Diercks A., Garnavich P. M., Gilliland R. L., Hogan C. J., Jha S., Kirshner R. P. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Comstant. Astronomy Journal, 1998, vol. 116, no. 3, pp. 1009–1012. Doi: 10.1086/300499
2. Perlmutter S., Aldering G., Goldhaber G., Knop R. A., Nugent P., Castro P. G., Deustua S., Fabbro S., Goobar A., Groom D. E., Hook I. M. Measurement of Ω and Λ from 42 High-redshift Supernovae. Astronomy Journal, 1999, vol. 517, no. 2, pp. 565–586.
3. Matos, T., Guzman F. S., Nunez D. Spherical scalar field halo in galaxies. Physical Review D, 2000, vol. 62, pp. 061301. Doi: 10.1103/PhysRevD.62.061301
4. Perlmutter S., Schmidt B. P. Supernovaand Gamma Ray Bursts. Ed. K. Weiler, Springer, 2003.
5. Matos T., Guzman F. S. Dynavical Approach to the Cosmological Constant. Classical and Quantum Gravity, 2001, vol. 18, no. 23. pp. 5055–5064. Doi: 10.1088/0264-9381/18/23/303
6. Peebles P. J., Ratra B. The cosmological constant and dark energy. Reviews of Modern Physics, 2003, vol. 75, no. 2, pp. 559–606. Doi: 10.1103/revmodphys.75.559
7. Scherrer R. J., Sen A. A. Thawing quintessence with a nearly flat potential. Physical Review D, 2008, vol. 77, no. 8, p. 083515.
8. Deser S. Self-interaction and gauge invariance. General Relativity and Gravitation, 1970, vol. 1, no. 1, pp. 9–15. Doi: 10.1007/bf00759198
9. Weinberg S. Gravitation and Cosmology. New-York, London, Sydney, Toronto, J. Wiley and Sons Inc., 1972. 657 p.
10. Logunov A. A. Relativistic Theory of Gravitation. Moscow, Nauka Publ., 2011. 351 p. (in Russian).
11. Vyblyi Yu. P., Tarasenko A. N. Scalar field with the source being the trace of the stress-energy tensor as a model of the dark energy. Kovariantnye metody v teoreticheskoi fizike: sb. nauch. tr. [Covariant methods in theoretical physics: Collection of Scientific Works]. Minsk, 2011, no. 7, pp. 36–44 (in Russian).
12. Freund P., Nambu Y. Scalar field coupled to the trace of the energy-momentum tensor. Physical Review, 1968, vol. 174, no. 5, pp. 1741–1743. Doi: 10.1103/physrev.174.1741
13. Gorbunov D. S., Rubakov V. A. Interaction to Theory of Early Universe, Moscow, Krasand Publ., 2008. 568 p. (in Russian).
14. Dudko I. G., Vyblyi Yu. P. Scalar field with the source in the form of the stress-energy tensor trace as a dark-energy model. Gravitation and Cosmology, 2016, vol. 22, no. 4, pp. 368–373. Doi: 10.1134/s020228931604006x