Neutrino oscillations in the Non-Kerr black hole with quantum phenomenon  

作　　者：Husan Alibekov Farruh Atamurotov Ahmadjon Abdujabbarov Vokhid Khamidov 

机构地区：[1]Ulugh Beg Astronomical Institute,Astronomy St.33,Tashkent 100052,Uzbekistan [2]University of Tashkent for Applied Sciences,Str.Gavhar 1,Tashkent 100149,Uzbekistan [3]New Uzbekistan University,Movarounnahr street 1,Tashkent 100000,Uzbekistan [4]Tashkent State Technical University,Tashkent 100095,Uzbekistan [5]Institute of Theoretical Physics,National University of Uzbekistan,Tashkent 100174,Uzbekistan [6]Institute of Fundamental and Applied Research,National Research University TIIAME,Kori Niyoziy 39,Tashkent 100000,Uzbekistan [7]Tashkent University of Information Technologies named after Muhammad al Khwarizmi,Amir Temur 108,Tashkent 100014,Uzbekistan

出　　处：《Chinese Physics C》2024年第7期55-66,共12页中国物理C（英文版）

基　　金：Supported by the Grants F-FA-2021-510 from the Uzbekistan Ministry for Innovative Development。

摘　　要：In this study,we have investigated the mathematical components of the Dirac equation in curved spacetime and how they can be applied to the analysis of neutrino oscillations.More specifically,we have developed a method for calculating the phase shift in flavor neutrino oscillations by utilizing a Taylor series expansion of the action that takes into account△m^(4) orders.In addition,we have used this method to assess how the phase difference in neutrino mass eigenstates changes according to the gravitational field described by the Johannsen spacetime.

关 键 词：Dirac equation neutrino flavour oscillation curved spacetime D0I:10.1088/1674-1137/ad3c2c 

分 类 号：O572.321[理学—粒子物理与原子核物理]