Thick brane in f (R) gravity with Palatini dynamics

被引:34
|
作者
Bazeia, D. [1 ]
Losano, L. [1 ]
Menezes, R. [2 ,3 ]
Olmo, Gonzalo J. [1 ,4 ]
Rubiera-Garcia, D. [1 ,5 ,6 ]
机构
[1] Univ Fed Paraiba, Dept Fis, BR-58051900 Joao Pessoa, Paraiba, Brazil
[2] Univ Fed Paraiba, Dept Ciencias Exatas, BR-58297000 Rio Tinto, PB, Brazil
[3] Univ Fed Campina Grande, Dept Fis, BR-58109970 Campina Grande, PB, Brazil
[4] Univ Valencia, Dept Fis Teor, IFIC, Ctr Mixto Univ Valencia CSIC, E-46100 Valencia, Spain
[5] Univ Lisbon, Inst Astrofis & Ciencias Espaco, Fac Ciencias, P-1749016 Lisbon, Portugal
[6] Fudan Univ, Dept Phys, Ctr Field Theory & Particle Phys, 220 Handan Rd, Shanghai 200433, Peoples R China
来源
EUROPEAN PHYSICAL JOURNAL C | 2015年 / 75卷 / 12期
关键词
EXTRA DIMENSIONS; MODELS; GEOMETRY; DEFECTS;
D O I
10.1140/epjc/s10052-015-3803-0
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
This work deals with modified gravity in five-dimensional space-time. We study a thick Palatini f (R) brane, that is, a braneworld scenario described by an anti-de Sitter warped geometry with a single extra dimension of infinite extent, sourced by a real scalar field under the Palatini approach, where the metric and the connection are regarded as independent degrees of freedom. We consider a first-order framework which we use to provide exact solutions for the scalar field and warp factor. We also investigate a perturbative scenario such that the Palatini approach is implemented through a Lagrangian f (R) = R + is an element of R-n, where the small parameter is an element of controls the deviation from the standard thick brane case. In both cases it is found that the warp factor tends to localize the extra dimension due to the nonlinear corrections.
引用
收藏
页码:1 / 10
页数:10
相关论文
共 50 条
  • [41] PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
    Olmo, Gonzalo J.
    INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2011, 20 (04): : 413 - 462
  • [42] Lookback time as a test for f(R) gravity in the Palatini approach
    Zhong-Xu Zhai and Wen-Biao Liu Department of Physics
    ResearchinAstronomyandAstrophysics, 2011, 11 (11) : 1257 - 1265
  • [43] Statefinder diagnostic and constraints on the Palatini f(R) gravity theories
    Cao, Shu-Lei
    Li, Song
    Yu, Hao-Ran
    Zhang, Tong-Jie
    RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2018, 18 (03)
  • [44] Stability criterion for white dwarfs in Palatini f(R) gravity
    Sarmah, Lupamudra
    Kalita, Surajit
    Wojnar, Aneta
    PHYSICAL REVIEW D, 2022, 105 (02)
  • [45] Numerical evolutions of boson stars in Palatini f (R) gravity
    Maso-Ferrando, Andreu
    Sanchis-Gual, Nicolas
    Font, Jose A.
    Olmo, Gonzalo J.
    PHYSICAL REVIEW D, 2024, 109 (04)
  • [46] SOLAR SYSTEM CONSTRAINTS ON ANALYTIC PALATINI f(R) GRAVITY
    Toniato, Junior D.
    ACTA PHYSICA POLONICA B PROCEEDINGS SUPPLEMENT, 2020, 13 (02) : 255 - 259
  • [47] Bianchi V cosmological model in Palatini f (R) gravity
    Banik, Debika Kangsha
    Banik, Sebika Kangsha
    Bhuyan, Kalyan
    GENERAL RELATIVITY AND GRAVITATION, 2018, 50 (01)
  • [48] Wormhole spacetimes in Palatini f(R) gravity and energy conditions
    Hamidreza Saiedi
    Indian Journal of Physics, 2022, 96 : 3039 - 3045
  • [49] Noether gauge symmetry for f(R) gravity in Palatini formalism
    Y. Kucukakca
    U. Camci
    Astrophysics and Space Science, 2012, 338 : 211 - 216
  • [50] f(R) theories of gravity in the Palatini approach matched with observations
    S. Capozziello
    V. F. Cardone
    M. Francaviglia
    General Relativity and Gravitation, 2006, 38 : 711 - 734