Maqola

Testing General Relativity with Black Hole X-Ray Data and ABHModels

Cosimo BambiCenter for Field Theory and Particle Physics and Department of Physics, Fudan University, 200438 Shanghai, ChinaAskar B. AbdikamalovSchool of Mathematics and Natural Sciences, New Uzbekistan University, Tashkent 100007, UzbekistanH. LiuCenter for Field Theory and Particle Physics and Department of Physics, Fudan University, 200438 Shanghai, ChinaShafqat RiazTheoretical Astrophysics, Eberhard-Karls Universität Tübingen, D-72076 Tübingen, GermanySwarnim ShashankCenter for Field Theory and Particle Physics and Department of Physics, Fudan University, 200438 Shanghai, ChinaMenglei ZhouInstitut für Astronomie und Astrophysik, Eberhard-Karls Universität Tübingen, D-72076 Tübingen, Germany

2024en

Ochiq kirishGibrid

Litsenziya: cc-by-nc-nd

ABI

Annotatsiya

The past 10 years have seen tremendous progress in our capability of testing General Relativity in the strong field regime with black hole observations. 10 years ago, the theory of General Relativity was almost completely unexplored in the strong field regime. Today, we have gravitational wave data of the coalescence of stellar-mass black holes, radio images of the supermassive black holes SgrA$^*$ and M87$^*$, and high-quality X-ray data of stellar-mass black holes in X-ray binaries and supermassive black holes in active galactic nuclei. In this manuscript, we will review current efforts to test General Relativity with black hole X-ray data and we will provide a detailed description of the public codes available on ABHModels.

Hali tarjima qilinmagan

Mavzular

Relativity and Gravitational Theory Mathematical and Theoretical Analysis Computational Physics and Python Applications

Identifikatorlar

DOI: 10.22323/1.447.0016

Iqtiboslar va manbalar

0 ta iqtibos89 ta foydalanilgan manba