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Title: Graviton mass bounds

Authors:
; ; ;
Publication Date:
Sponsoring Org.:
USDOE
OSTI Identifier:
1355117
Grant/Contract Number:
SC0009946; SC0010600
Resource Type:
Journal Article: Publisher's Accepted Manuscript
Journal Name:
Reviews of Modern Physics
Additional Journal Information:
Journal Volume: 89; Journal Issue: 2; Related Information: CHORUS Timestamp: 2017-05-03 22:12:35; Journal ID: ISSN 0034-6861
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English

Citation Formats

de Rham, Claudia, Deskins, J. Tate, Tolley, Andrew J., and Zhou, Shuang-Yong. Graviton mass bounds. United States: N. p., 2017. Web. doi:10.1103/RevModPhys.89.025004.
de Rham, Claudia, Deskins, J. Tate, Tolley, Andrew J., & Zhou, Shuang-Yong. Graviton mass bounds. United States. doi:10.1103/RevModPhys.89.025004.
de Rham, Claudia, Deskins, J. Tate, Tolley, Andrew J., and Zhou, Shuang-Yong. Wed . "Graviton mass bounds". United States. doi:10.1103/RevModPhys.89.025004.
@article{osti_1355117,
title = {Graviton mass bounds},
author = {de Rham, Claudia and Deskins, J. Tate and Tolley, Andrew J. and Zhou, Shuang-Yong},
abstractNote = {},
doi = {10.1103/RevModPhys.89.025004},
journal = {Reviews of Modern Physics},
number = 2,
volume = 89,
place = {United States},
year = {Wed May 03 00:00:00 EDT 2017},
month = {Wed May 03 00:00:00 EDT 2017}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record at 10.1103/RevModPhys.89.025004

Citation Metrics:
Cited by: 22works
Citation information provided by
Web of Science

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  • Recently LIGO collaboration discovered gravitational waves [1] predicted 100 years ago by A. Einstein. Moreover, in the key paper reporting about the discovery, the joint LIGO and VIRGO team presented an upper limit on graviton mass such as m {sub g} < 1.2 × 10{sup −22} eV [2] (see also more details in another LIGO paper [3] dedicated to a data analysis to obtain such a small constraint on a graviton mass). Since the graviton mass limit is so small the authors concluded that their observational data do not show violations of classical general relativity. We consider another opportunity tomore » evaluate a graviton mass from phenomenological consequences of massive gravity and show that an analysis of bright star trajectories could bound graviton mass with a comparable accuracy with accuracies reached with gravitational wave interferometers and expected with forthcoming pulsar timing observations for gravitational wave detection. It gives an opportunity to treat observations of bright stars near the Galactic Center as a wonderful tool not only for an evaluation specific parameters of the black hole but also to obtain constraints on the fundamental gravity law such as a modifications of Newton gravity law in a weak field approximation. In particular, we obtain bounds on a graviton mass based on a potential reconstruction at the Galactic Center.« less
  • If large extra dimensions exist in nature, supernova (SN) cores will emit large fluxes of Kaluza-Klein gravitons, producing a cosmic background of these particles with energies and masses up to about 100MeV. Radiative decays then give rise to a diffuse cosmic {gamma} -ray background with E{sub {gamma}}{approx}<100 MeV which is well in excess of the observations if more than 0.5%--1% of the SN energy is emitted into the new channel. For two extra dimensions we derive a conservative bound on their radius of R{approx}<0.9 x 10{sup -4} mm ; for three extra dimensions it is R{approx}<1.9 x 10{sup -7} mmmore » .« less
  • This paper examines a graviton rest mass (m) introduced in the framework of the relativistic theory of gravitation and obtains equations that describe a massive gravitational field. Under the assumption that the entire hidden mass of the matter in the Universe is due to the existence of a massive gravitational field, an upper bound on the rest mass is obtained: m less than or equal to 0.64 x 10/sup - -65/ g.