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作 者:Chengxiang Sun Yunqi Liu Wei-Liang Qian Ruihong Yue 孙呈祥;刘云旗;钱卫良;岳瑞宏(Center for Gravitation and Cosmology,College of Physical Science and Technology,Yangzhou University,Yangzhou 225009,China;Escola de Engenharia de Lorena,Universidade de Sao Paulo,12602-810,Lorena,SP,Brazil;School of Aeronautics and Astronautics,Shanghai Jiao Tong University,Shanghai 200240,China;Faculdade de Engenharia de Guaratingueta,Universidade Estadual Paulista,12516-410,Guaratingueia,SP,Brazil)
机构地区:[1]Center for Gravitation and Cosmology,College of Physical Science and Technology,Yangzhou University,Yangzhou 225009,China [2]Escola de Engenharia de Lorena,Universidade de Sao Paulo,12602-810,Lorena,SP,Brazil [3]School of Aeronautics and Astronautics,Shanghai Jiao Tong University,Shanghai 200240,China [4]Faculdade de Engenharia de Guaratingueta,Universidade Estadual Paulista,12516-410,Guaratingueia,SP,Brazil
出 处:《Chinese Physics C》2022年第6期246-256,共11页中国物理C(英文版)
基 金:Supported by the National Key R&D Program of China(2020YFC2201400);the Major Program of the National Natural Science Foundation of China(11690021);the National Natural Science Foundation of China(11505066)。
摘 要:In this work,we study the optical properties of a class of magnetically charged rotating black hole spacetimes.The black holes in question are assumed to be immersed in the quintessence field,and subsequently,the resulting black hole shadows are expected to be modified by the presence of dark energy.We investigate the photon region and the black hole shadow,especially their dependence on the relevant physical conditions,such as the quintessence state parameter,angular momentum,and magnetic charge magnitude.The photon regions depend sensitively on the horizon structure and possess intricate features.Moreover,from the viewpoint of a static observer,we explore a few observables,especially those associated with the distortion of the observed black hole shadows.
关 键 词:black hole shadow QUINTESSENCE magnetically charged rotating black hole
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