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dc.contributor.authorJohannsen, Tim
dc.contributor.authorWang, Carlos
dc.contributor.authorBroderick, Avery E.
dc.contributor.authorDoeleman, Sheperd S.
dc.contributor.authorFish, Vincent L.
dc.contributor.authorLoeb, Abraham
dc.contributor.authorPsaltis, Dimitrios
dc.date.accessioned2019-09-26T15:01:51Z
dc.date.issued2016
dc.identifier.citationJohannsen, Tim, Carlos Wang, Avery E. Broderick, Sheperd S. Doeleman, Vincent L. Fish, Abraham Loeb, and Dimitrios Psaltis. 2016. “Testing General Relativity with Accretion-Flow Imaging of SgrA*.” Physical Review Letters 117 (9). https://doi.org/10.1103/physrevlett.117.091101.
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.issn1092-0145
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41412217*
dc.description.abstractThe Event Horizon Telescope is a global, very long baseline interferometer capable of probing potential deviations from the Kerr metric, which is believed to provide the unique description of astrophysical black holes. Here, we report an updated constraint on the quadrupolar deviation of Sagittarius A* within the context of a radiatively inefficient accretion flow model in a quasi-Kerr background. We also simulate near-future constraints obtainable by the forthcoming eight-station array and show that in this model already a one-day observation can measure the spin magnitude to within 0.005, the inclination to within 0.09 degrees, the position angle to within 0.04 degrees, and the quadrupolar deviation to within 0.005 at 3 sigma confidence. Thus, we are entering an era of high-precision strong gravity measurements.
dc.language.isoen_US
dc.publisherAmerican Physical Society
dash.licenseOAP
dc.titleTesting General Relativity with Accretion-Flow Imaging of Sgr A *
dc.typeJournal Article
dc.description.versionAccepted Manuscript
dc.relation.journalPhysical Review Letters
dash.depositing.authorLoeb, Abraham::e022a3952362350ac8a0138f128a8be7::600
dc.date.available2019-09-26T15:01:51Z
dash.workflow.comments1Science Serial ID 78958
dc.identifier.doi10.1103/PhysRevLett.117.091101
dash.source.volume117;9


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