Distinguishing gravitational and emission physics in black hole imaging: spherical symmetry
@article{Kocherlakota2022DistinguishingGA, title={Distinguishing gravitational and emission physics in black hole imaging: spherical symmetry}, author={Prashant Kocherlakota and Luciano Rezzolla}, journal={Monthly Notices of the Royal Astronomical Society}, year={2022} }
Imaging a supermassive black hole and extracting physical information requires good knowledge of both the gravitational and the astrophysical conditions near the black hole. When the geometrical properties of the black hole are well understood, extracting information on the emission properties is possible. Similarly, when the emission properties are well understood, extracting information on the black hole geometry is possible. At present however, uncertainties are present both in theβ¦Β
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