Testing General Relativity with the Shadow Size of Sgr

Testing General Relativity with the Shadow Size of Sgr

In general relativity, the angular radius of the shadow of a black hole is primarily determined by its mass-to-distance ratio and depends only weakly on its spin and inclination. If general relativity is violated, however, the shadow size may also depend strongly on parametric deviations from the Ke...

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Bibliographic Details
Main Authors: Johannsen, Tim (Author), Broderick, Avery E. (Author), Plewa, Philipp M. (Author), Chatzopoulos, Sotiris (Author), Eisenhauer, Frank (Author), Genzel, Reinhard (Author), Gerhard, Ortwin (Author), Johnson, Michael D. (Author), Doeleman, Sheperd Samuel (Contributor), Fish, Vincent L. (Contributor)
Other Authors: Haystack Observatory (Contributor)
Format: Article
Language:English
Published: American Physical Society, 2018-06-26T15:59:36Z.
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