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Testing General Relativity with the Shadow Size of Sgr A*

PHYSICAL REVIEW LETTERS, no. 3 (2016)

引用64|浏览29
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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 Kerr metric. Based on a reconstructed imag...更多

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