Horizon structure of rotating Einstein–Born–Infeld black holes and shadow

The European Physical Journal C

Sushant G. Ghosh¹  Farruh Atamurotov²  Bobomurat Ahmedov³ 

[1] Centre for Theoretical Physics, Jamia Millia Islamia, 110025, New Delhi, India;Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of Kwa-Zulu-Natal, Private Bag 54001, 4000, Durban, South Africa;Institute of Nuclear Physics, Ulughbek, 100214, Tashkent, Uzbekistan;Inha University in Tashkent, 100170, Tashkent, Uzbekistan;Ulugh Beg Astronomical Institute, Astronomicheskaya 33, 100052, Tashkent, Uzbekistan;National University of Uzbekistan, 100174, Tashkent, Uzbekistan;Institute of Nuclear Physics, Ulughbek, 100214, Tashkent, Uzbekistan;Ulugh Beg Astronomical Institute, Astronomicheskaya 33, 100052, Tashkent, Uzbekistan;National University of Uzbekistan, 100174, Tashkent, Uzbekistan;

关键词: Black Hole;    Event Horizon;    Very Long Baseline Interferometry;    Black Hole Solution;    Extremal Black Hole;   

DOI  :  10.1140/epjc/s10052-016-4122-9

来源: Springer

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