Three-dimensional accelerating AdS black holes in F(R) gravity

被引:0
|
作者
B. Eslam Panah
M. Khorasani
J. Sedaghat
机构
[1] University of Mazandaran,Department of Theoretical Physics, Faculty of Science
[2] University of Mazandaran,ICRANet
[3] ICRANet,Mazandaran
[4] Shiraz University,Department of Physics, School of Science
来源
The European Physical Journal Plus | / 138卷
关键词
D O I
暂无
中图分类号
学科分类号
摘要
Considering a three-dimensional C-\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$C-$$\end{document}metric, we obtain the exact accelerating black holes in the F(R) theory of gravity coupled with and without a matter field. First, we extract uncharged accelerating AdS black hole solutions in F(R) gravity. Then, we study the effects of various parameters on metric function, roots, and the temperature of these black holes. The temperature is always positive for the radii less than 1α\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\frac{1}{ \alpha }$$\end{document}, and it is negative for the radii more than 1α\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\frac{1}{\alpha }$$\end{document}. We extend our study by coupling nonlinear electrodynamics as a matter filed to F(R) gravity to obtain charged black holes in this theory. Next, we evaluate the effects of different parameters such as the electrical charge, accelerating parameter, angular, F(R) gravity, and scalar curvature on the obtained solutions, roots, and temperature of three-dimensional charged accelerating AdS black holes. The results indicate that there is a root in which it depends on various parameters. The temperature of these black holes is positive after this root.
引用
收藏
相关论文
共 50 条
  • [31] Stability analysis of f(R)-AdS black holes
    Moon, Taeyoon
    Myung, Yun Soo
    Son, Edwin J.
    EUROPEAN PHYSICAL JOURNAL C, 2011, 71 (10): : 1 - 8
  • [32] Rotating and accelerating AdS black holes in Einstein-Gauss-Bonnet gravity
    Anabalon, Andres
    Astefanesei, Dumitru
    Cisterna, Adolfo
    Izaurieta, Fernando
    Oliva, Julio
    Quijada, Constanza
    Quinzacara, Cristian
    PHYSICS LETTERS B, 2024, 857
  • [33] Stability analysis of f(R)-AdS black holes
    Taeyoon Moon
    Yun Soo Myung
    Edwin J. Son
    The European Physical Journal C, 2011, 71
  • [34] Black holes and their shadows in F(R) gravity
    Nojiri, Shin'ichi
    Odintsov, S. D.
    PHYSICS OF THE DARK UNIVERSE, 2025, 47
  • [35] Charged Taub-NUT-AdS Black Holes in f(R) Gravity and Holographic Complexity
    Chen, Sen
    Pei, Yili
    Li, Li
    Yang, Taotao
    INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2023, 62 (02)
  • [36] Thermodynamic topology of Kiselev-AdS black holes within f (R, T) gravity
    Gashti, Saeed Noori
    Afshar, Mohammad Ali S.
    Alipoury, Mohammad Reza
    Sekhmani, Yassine
    Sadeghi, Jafar
    Rayimbaeva, Javlon
    CHINESE PHYSICS C, 2025, 49 (03)
  • [37] Charged Taub-NUT-AdS Black Holes in f(R) Gravity and Holographic Complexity
    Sen Chen
    Yili Pei
    Li Li
    Taotao Yang
    International Journal of Theoretical Physics, 62
  • [38] Notes on black holes and three dimensional gravity
    Bañados, M
    PARTICLES AND FIELDS, 1999, 490 : 198 - 216
  • [39] On boundary conditions in three-dimensional AdS gravity
    Miskovic, Olivera
    Olea, Rodrigo
    PHYSICS LETTERS B, 2006, 640 (03) : 101 - 107
  • [40] Charged accelerating black hole in f(R) gravity
    Zhang, Ming
    Mann, Robert B.
    PHYSICAL REVIEW D, 2019, 100 (08)