TY  - CONF
AU  - Zakharov, Alexander F.
AU  - Jovanović, Predrag
AU  - Borka, Duško
AU  - Borka Jovanović, Vesna
PY  - 2017
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/7166
AB  - One could use trajectories of test particles to evaluate a gravitational potential. In particular, in the case of the Galactic Center one could use photon trajectories to analyze a shadow structure. Another way is to use bright stars near the Galactic Center to evaluate a gravitational potential and constrain parameters of a model for the Galactic Center. In particular, one could obtain constraints on parameters of black hole, stellar cluster and dark matter concentration. Earlier, we constrained parameters of Fr and a Yukawa potential from observational data for the S2 star trajectory. Now gravity theories with a massive graviton are a subject of intensive studies. People proposed different experimental ways to evaluate a graviton mass. Recently, the joint LIGO and VIRGO collaboration reported not only a discovery of gravitational waves and binary black holes, but the team claimed also that found a constraint on a graviton mass as 1.2 x 10(-22) eV. We show that an analysis of the S2 star trajectory could constrain a graviton mass with a comparable accuracy and this constraint is consistent with LIGOs one.
C3  - Journal of Physics: Conference Series
T1  - Graviton mass evaluation with trajectories of bright stars at the Galactic Center
VL  - 798
DO  - 10.1088/1742-6596/798/1/012081
ER  - 

@conference{
author = "Zakharov, Alexander F. and Jovanović, Predrag and Borka, Duško and Borka Jovanović, Vesna",
year = "2017",
abstract = "One could use trajectories of test particles to evaluate a gravitational potential. In particular, in the case of the Galactic Center one could use photon trajectories to analyze a shadow structure. Another way is to use bright stars near the Galactic Center to evaluate a gravitational potential and constrain parameters of a model for the Galactic Center. In particular, one could obtain constraints on parameters of black hole, stellar cluster and dark matter concentration. Earlier, we constrained parameters of Fr and a Yukawa potential from observational data for the S2 star trajectory. Now gravity theories with a massive graviton are a subject of intensive studies. People proposed different experimental ways to evaluate a graviton mass. Recently, the joint LIGO and VIRGO collaboration reported not only a discovery of gravitational waves and binary black holes, but the team claimed also that found a constraint on a graviton mass as 1.2 x 10(-22) eV. We show that an analysis of the S2 star trajectory could constrain a graviton mass with a comparable accuracy and this constraint is consistent with LIGOs one.",
journal = "Journal of Physics: Conference Series",
title = "Graviton mass evaluation with trajectories of bright stars at the Galactic Center",
volume = "798",
doi = "10.1088/1742-6596/798/1/012081"
}

Zakharov, A. F., Jovanović, P., Borka, D.,& Borka Jovanović, V.. (2017). Graviton mass evaluation with trajectories of bright stars at the Galactic Center. in Journal of Physics: Conference Series, 798.
https://doi.org/10.1088/1742-6596/798/1/012081

Zakharov AF, Jovanović P, Borka D, Borka Jovanović V. Graviton mass evaluation with trajectories of bright stars at the Galactic Center. in Journal of Physics: Conference Series. 2017;798.
doi:10.1088/1742-6596/798/1/012081 .

Zakharov, Alexander F., Jovanović, Predrag, Borka, Duško, Borka Jovanović, Vesna, "Graviton mass evaluation with trajectories of bright stars at the Galactic Center" in Journal of Physics: Conference Series, 798 (2017),
https://doi.org/10.1088/1742-6596/798/1/012081 . .