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相关论文: Rotating charged black holes shadow in quintessenc…

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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…

广义相对论与量子宇宙学 · 物理学 2022-06-15 Chengxiang Sun , Yunqi Liu , Wei-Liang Qian , Ruihong Yue

We study the shadow of a charged rotating black hole in $f(R)$ gravity. This black hole is characterized by mass, $M$, spin, $a$, electric charge, $Q$ and $R_{0}$ which is proportional to cosmological constant. We analyze the image of the…

广义相对论与量子宇宙学 · 物理学 2022-10-06 Sara Dastan , Reza Saffari , Saheb Soroushfar

Higher dimensional theories admit astrophysical objects like supermassive black holes, which are rather different from standard ones, and their gravitational lensing features deviate from general relativity. It is well known that a black…

广义相对论与量子宇宙学 · 物理学 2018-05-31 Muhammed Amir , Balendra Pratap Singh , Sushant G. Ghosh

We construct theoretical investigation of the black hole shadow for rotating charged black hole in an asymptotically flat, axisymmetric, and stationary spacetime with Weyl corrections. This spacetime is characterized by mass ($M$), charge…

广义相对论与量子宇宙学 · 物理学 2019-06-11 Md Sabir Ali , Muhammed Amir

We study the shadow of the rotating black hole with quintessential energy i) in vacuum and ii) in the presence of plasma with radial power-law density. For vacuum case the quintessential field parameter of the rotating black hole…

广义相对论与量子宇宙学 · 物理学 2015-12-18 Ahmadjon Abdujabbarov , Bobir Toshmatov , Zdeněk Stuchlík , Bobomurat Ahmedov

Zhang have obtained recently a twisted rotating black hole metric, which is a vacuum solution in four-dimensional Einstein gravity. This black hole solution has a rotation parameter, but without the total angular moment. Here, we have…

广义相对论与量子宇宙学 · 物理学 2016-10-21 Songbai Chen , Jiliang Jing

The rotating black holes in the quintessential dark energy correspond to three horizons: inner, outer, and quintessential horizon. The domain of outer communication is the region between outer and quintessential horizon. Here, in this work…

广义相对论与量子宇宙学 · 物理学 2023-01-04 Balendra Pratap Singh

This paper investigates the shadow of a charged rotating non-commutative black hole. For this purpose, we first formulate the null geodesics and study the effects of non-commutative charge on the photon orbit. We then explore the effect of…

广义相对论与量子宇宙学 · 物理学 2016-12-21 M. Sharif , Sehrish Iftikhar

In this paper, we discuss optical properties of the topologically charged rotating black hole. We study the horizon, the photon region, the shadow of the black hole and other observables. The results show that in addition to the black hole…

广义相对论与量子宇宙学 · 物理学 2022-11-09 Hao-Ran Zhang , Peng-Zhang He , Lei-Shao , Yuan Chen , Xian-Ru Hu

In this paper, the shadows cast by non-rotating and rotating modified gravity black holes are investigated. In addition to the black hole spin parameter $a$ and the inclination angle $\theta$ of observer, another parameter $\alpha$…

广义相对论与量子宇宙学 · 物理学 2019-04-08 Hui-Min Wang , Yu-Meng Xu , Shao-Wen Wei

The motion of photons around the Kerr-Newman-dS black hole surrounded by quintessence and a cloud of strings is investigated. The existence of the Carter constant leads to that of unstable circular photon orbits on a two-dimensional plane…

广义相对论与量子宇宙学 · 物理学 2023-10-31 Wen-Fu Cao , Wen-Fang Liu , Xin Wu

The existence of quintessential dark energy around a black hole has considerable consequences on its spacetime geometry. Hence, in this article, we explore its effect on horizons and the silhouette generated by a Kerr-Newman black hole in…

广义相对论与量子宇宙学 · 物理学 2020-06-23 Saeed Ullah Khan , Jingli Ren

In this paper, we mainly investigate the shadow of a rotating charged black hole with a cosmological constant immersed in perfect fluid dark matter. We first obtain the charged spherically symmetric black hole with a cosmological constant…

广义相对论与量子宇宙学 · 物理学 2025-03-13 Zheng-Long Ban , Xiao-Jun Gao , Jinsong Yang

A black hole casts a shadow as an optical appearance because of its strong gravitational field. We study the shadow cast by the five-dimensional Myers-Perry black hole with equal rotation parameters. We demonstrate that the null geodesic…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Uma Papnoi , Farruh Atamurotov , Sushant G. Ghosh , Bobomurat Ahmedov

We study the shadows cast by the different types of rotating regular black holes viz. Ay\'on-Beato-Garc\'ia {(ABG)}, Hayward, and Bardeen. These black holes have in addition to the total mass ($M$) and rotation parameter ($a$), different…

广义相对论与量子宇宙学 · 物理学 2016-05-25 Ahmadjon Abdujabbarov , Muhammed Amir , Bobomurat Ahmedov , Sushant G. Ghosh

One of the most important and actual issues in relativistic astrophysics is testing gravity theories and obtaining constraint values for the parameters of black holes using observational data. In this research, we aimed to explore the…

广义相对论与量子宇宙学 · 物理学 2024-06-14 Saeed Ullah Khan , Javlon Rayimbaev , Furkat Sarikulov , Ozodbek Abdurakhmonov

We present the shape of the black hole shadow on the standard background screen as it is registered by the distant observer. The screen is an infinite plane, emitting the quanta uniformly distributed to a hemisphere. The source of emission…

广义相对论与量子宇宙学 · 物理学 2018-02-14 Serge V. Repin , Dmitry A. Kompaneets , Igor D. Novikov , Valeriya A. Mityagina

We discuss the horizon properties, shadow cast, and the weak gravitational lensing of charged rotating regular black holes, which in addition to mass ($M$) and rotation parameter ($a$) have an electric charge ($Q$) and magnetic charge…

广义相对论与量子宇宙学 · 物理学 2019-12-12 Rahul Kumar , Sushant G. Ghosh , Anzhong Wang

We have studied the shadows of a circular disformal Kerr black hole with a deformation parameter, which represents a rotating solution within a generalized scalar-tensor framework of Horndeski gravity that characterized by second-order…

广义相对论与量子宇宙学 · 物理学 2026-01-06 Fen Long , Songbai Chen , Jiliang Jing

We study analytically the shadow cast by the rotating black hole in the perfect fluid dark matter. The apparent shape of the shadow depends upon the black hole spin $a$ and the perfect fluid dark matter intensity parameter $k$ ($k>0$). In…

广义相对论与量子宇宙学 · 物理学 2018-12-26 Xian Hou , Zhaoyi Xu , Jiancheng Wang
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