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Constraining the range of Yukawa gravity interaction from S2 star orbits II: bounds on graviton mass
Zakharov, A. F.1,2,3,4,5; Jovanovic, P.6; Borka, D.7; Jovanovic, V. Borka7
2016-05-01
Source PublicationJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
ISSN1475-7516
Issue5Pages:10
AbstractRecently 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.
Keywordgravity modified gravity GR black holes gravitational waves / theory
Funding OrganizationChinese 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
DOI10.1088/1475-7516/2016/05/045
WOS KeywordSUPERMASSIVE BLACK-HOLE ; GENERAL-RELATIVITY ; GALACTIC-CENTER ; STELLAR ORBITS ; MILKY-WAY ; DEFLECTION ; MODEL ; SPEED ; FIELD
Language英语
Funding ProjectChinese 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]
Funding OrganizationChinese 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
WOS Research AreaAstronomy & Astrophysics ; Physics
WOS SubjectAstronomy & Astrophysics ; Physics, Particles & Fields
WOS IDWOS:000378041500046
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/28965
Collection中国科学院国家天文台
Corresponding AuthorZakharov, A. F.
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Datun Rd 20A, Beijing 100012, Peoples R China
2.Inst Theoret & Expt Phys, Moscow 117259, Russia
3.Natl Res Nucl Univ MEPhI, Moscow Engn Phys Inst, Moscow 115409, Russia
4.Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia
5.N Carolina Cent Univ, Durham, NC 27707 USA
6.Astron Observ, Volgina 7, Belgrade 11060, Serbia
7.Univ Belgrade, Vinca Inst Nucl Sci, Atom Phys Lab 040, POB 522, Belgrade 11001, Serbia
Recommended Citation
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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