Different Ways to Estimate Graviton Mass

Author:

Zakharov Alexander F.12345,Jovanović Predrag6,Borka Dusko7,Jovanović Vesna Borka7

Affiliation:

1. National Astronomical Observatories of Chinese Academy of Sciences, 20A Datun Road, 100012 Beijing, China

2. Institute of Theoretical and Experimental Physics, B. Cheremushkinskaya 25, 117218 Moscow, Russia

3. Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, 141980 Dubna, Russia

4. National Research Nuclear University MEPhI, (Moscow Engineering Physics Institute), 115409, Moscow, Russia

5. North Carolina Central University, Durham, NC 27707, USA

6. Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia

7. Atomic Physics Laboratory (040), Vinča Institute of Nuclear Sciences & University of Belgrade, P. O. Box 522, 11001 Belgrade, Serbia

Abstract

An experimental detection of graviton is extremely hard problem, however, there are different ways to evaluate a graviton mass if it is non-vanishing. Theories of massive gravity or theories with non-vanishing graviton mass initially have a number of pathologies such as discontinuities, ghosts etc. In last years theorists found ways to overcome weaknesses of such theories meanwhile observational features are also discussed. In the first publication reporting about the discovery of gravitational waves from the binary black hole system the LIGO-Virgo collaboration obtained the graviton mass constraint around [Formula: see text] eV (later the estimate was improved with new data). A comparable and consistent graviton mass constraint around [Formula: see text] eV has been obtained from analysis of the bright star S2 trajectory near the Galactic Center.

Publisher

World Scientific Pub Co Pte Lt

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