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Constraining the range of Yukawa gravity interaction from S2 star orbits II: bounds on graviton mass

文献类型：期刊论文

作者Zakharov, A. F.3,4,5,6,7; Jovanovic, P.2; Borka, D.1; Jovanovic, V. Borka1
刊名JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
出版日期2016-05-01
期号5页码:10
关键词gravity modified gravity GR black holes gravitational waves / theory
ISSN号1475-7516
DOI10.1088/1475-7516/2016/05/045
英文摘要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 & VIRGO team presented an upper limit on graviton mass such as m(g) < 1.2 x 10(-22)eV [1] (see also more details in another LIGO paper [2] 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 to 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.
WOS关键词SUPERMASSIVE BLACK-HOLE ; GENERAL-RELATIVITY ; GALACTIC-CENTER ; STELLAR ORBITS ; MILKY-WAY ; DEFLECTION ; MODEL ; SPEED ; FIELD
资助项目Chinese Academy of Sciences ; NSF[HRD-0833184] ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.)[NNX09AVO7A] ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.)[NNX09AVO7A] ; Ministry of Education, Science and Technological Development of the Republic of Serbia[176003]
WOS研究方向Astronomy & Astrophysics ; Physics
语种英语
WOS记录号WOS:000378041500046
出版者IOP PUBLISHING LTD
资助机构Chinese Academy of Sciences ; Chinese Academy of Sciences ; NSF ; NSF ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; NSF ; NSF ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; NSF ; NSF ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; NSF ; NSF ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NASA CADRE Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; NASA at NSF CREST Center (NCCU, Durham, NC, U.S.A.) ; Ministry of Education, Science and Technological Development of the Republic of Serbia ; Ministry of Education, Science and Technological Development of the Republic of Serbia
源URL[http://ir.bao.ac.cn/handle/114a11/28964]  
专题中国科学院国家天文台
通讯作者Zakharov, A. F.
作者单位1.Univ Belgrade, Vinca Inst Nucl Sci, Atom Phys Lab 040, POB 522, Belgrade 11001, Serbia
2.Astron Observ, Volgina 7, Belgrade 11060, Serbia
3.N Carolina Cent Univ, Durham, NC 27707 USA
4.Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia
5.Natl Res Nucl Univ MEPhI, Moscow Engn Phys Inst, Moscow 115409, Russia
6.Inst Theoret & Expt Phys, Moscow 117259, Russia
7.Chinese Acad Sci, Natl Astron Observ, Datun Rd 20A, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714		 Zakharov, A. F.,Jovanovic, P.,Borka, D.,et al. Constraining the range of Yukawa gravity interaction from S2 star orbits II: bounds on graviton mass[J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,2016(5):10.
APA Zakharov, A. F.,Jovanovic, P.,Borka, D.,&Jovanovic, V. Borka.(2016).Constraining the range of Yukawa gravity interaction from S2 star orbits II: bounds on graviton mass.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(5),10.
MLA Zakharov, A. F.,et al."Constraining the range of Yukawa gravity interaction from S2 star orbits II: bounds on graviton mass".JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS .5(2016):10.

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