Shadow and quasinormal modes of rotating charged black holes in Kalb–Ramond gravity and implications from EHT data
Muhammad ZahidSchool of Science, Harbin Institute of Technology, ShenZhen, 518055, ChinaFurkat SarikulovUlugh Beg Astronomical Institute, Astronomy str. 33, Tashkent 100052, UzbekistanChao ShenSchool of Science, Harbin Institute of Technology, ShenZhen, 518055, ChinaJavlon RayimbaevInstitute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, UzbekistanKodir BadalovInstitute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, Tashkent 100000, UzbekistanSokhibjan MuminovUrgench State University, Kh. Alimjan str. 14, Urgench 221100, Uzbekistan
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Аннотация
Аннотация мавжуд эмас.