Exploring the shadow of a rotating charged ModMax black hole

被引:10
|
作者
Karshiboev, Khurshid [1 ]
Atamurotov, Farruh [2 ,3 ,4 ,5 ]
Abdujabbarov, Ahmadjon [1 ,6 ,7 ]
Ovgun, Ali [8 ]
Reyimberganov, Anvar [9 ]
机构
[1] Natl Univ Uzbekistan, Inst Theoret Phys, Tashkent 100174, Uzbekistan
[2] New Uzbekistan Univ, Movarounnahr St 1, Tashkent 100000, Uzbekistan
[3] Cent Asian Univ, Milliy Bog St 264, Tashkent 111221, Uzbekistan
[4] Univ Tashkent Appl Sci, Str Gavhar 1, Tashkent 100149, Uzbekistan
[5] Tashkent State Tech Univ, Tashkent 100095, Uzbekistan
[6] Ulugh Beg Astron Inst, Astron St 33, Tashkent 100052, Uzbekistan
[7] Natl Res Univ TIIAME, Inst Fundamental & Appl Res, Kori Niyoziy 39, Tashkent 100000, Uzbekistan
[8] Eastern Mediterranean Univ, Phys Dept, via Mersin 10, TR-99628 Famagusta, North Cyprus, Turkiye
[9] Urgench State Univ, Urgench 220100, Uzbekistan
关键词
black hole; ModMax gravity; rotating black hole; black hole shadow; TELESCOPE RESULTS. I;
D O I
10.1088/1572-9494/ad1583
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The research presented in this paper discusses the impact that the parameters of charge (Q) and screening factor (gamma) have on properties of the horizon and silhouette of rotating charged ModMax black holes which were reviewed in [Eur. Phys. J. C (2022) 82:1155] recently, building upon previous findings in the field. Furthermore, the study explores the behavior of null geodesics, which can help us better understand the apparent shape of the black hole's silhouette, as well as the distortion parameter and approximate radii of the silhouette that are influenced by the aforementioned parameters, and there are some values of parameter Q which corresponds to data from the Event Horizon Telescope (EHT). Notably, we explore the distortion parameter and approximate radii of the silhouette, revealing that while an increase in gamma leads to a growth in silhouette radius (R s ), it simultaneously reduces the distortion rate (delta s ). Conversely, heightened Q charge results in a reduction of R s accompanied by an increase in delta s . Lastly, the paper analyzes the effects of the black hole's parameters on the effective potential and energy emission: the peak value of the energy emission rate experiences a decrease as the screening factor (gamma) increases, while it increases with higher values of the charge parameter (Q).
引用
收藏
页数:13
相关论文
共 50 条
  • [31] A nonsingular rotating black hole
    Sushant G. Ghosh
    The European Physical Journal C, 2015, 75
  • [32] Rotating black hole and quintessence
    Sushant G. Ghosh
    The European Physical Journal C, 2016, 76
  • [33] Dynamics of a charged particle around a slowly rotating Kerr black hole immersed in magnetic field
    Saqib Hussain
    Ibrar Hussain
    Mubasher Jamil
    The European Physical Journal C, 2014, 74
  • [34] Investigation of circular geodesics in a rotating charged black hole in the presence of perfect fluid dark matter
    Das, Anish
    Saha, Ashis
    Gangopadhyay, Sunandan
    CLASSICAL AND QUANTUM GRAVITY, 2021, 38 (06)
  • [35] Thermodynamics of a rotating and non-linear magnetic-charged black hole in the quintessence field
    Ndongmo, Ragil
    Mahamat, Saleh
    Bouetou, Thomas Bouetou
    Kofane, Timoleon Crepin
    PHYSICA SCRIPTA, 2021, 96 (09)
  • [36] Geodesic Study of a Charged Black Hole
    Mehedi Kalam
    Nur Farhad
    Sk. Monowar Hossein
    International Journal of Theoretical Physics, 2014, 53 : 339 - 349
  • [37] Geodesic Study of a Charged Black Hole
    Kalam, Mehedi
    Farhad, Nur
    Hossein, Sk. Monowar
    INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2014, 53 (01) : 339 - 349
  • [38] Charged black hole remnants at the LHC
    G. L. Alberghi
    L. Bellagamba
    X. Calmet
    R. Casadio
    O. Micu
    The European Physical Journal C, 2013, 73
  • [39] Back Reaction of Charged Black Hole
    Zhang Lichun
    Zhao Ren
    Liu Liao
    International Journal of Theoretical Physics, 1998, 37 (8) : 2273 - 2280
  • [40] Observing the shadow of modified gravity black hole
    Alhamzawi, Ahmed
    INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2017, 26 (14):