Energy conditions in f(Q) gravity

被引:212
作者
Mandal, Sanjay [1 ]
Sahoo, P. K. [1 ]
Santos, J. R. L. [2 ]
机构
[1] Birla Inst Technol & Sci Pilani, Dept Math, Hyderabad Campus, Hyderabad 500078, India
[2] UFCG Univ Fed Campina Grande, Unidade Acad Fis, BR-58429900 Campina Grande, PB, Brazil
关键词
D O I
10.1103/PhysRevD.102.024057
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A complete theory of gravity impels us to go beyond Einstein's general relativity. One promising approach lies in a new class of teleparallel theory of gravity named f(Q), where the nonmetricity Q is responsible for the gravitational interaction. The important roles any of these alternative theories should obey are the energy condition constraints. Such constraints establish the compatibility of a given theory with the causal and geodesic structure of space-time. In this work, we present a complete test of energy conditions for f(Q) gravity models. The energy conditions allowed us to fix our free parameters, restricting the families of f(Q) models compatible with the accelerated expansion our Universe passes through. Our results strengthen the viability of f(Q) theory, leading us close to the dawn of a complete theory for gravitation.
引用
收藏
页数:8
相关论文
共 33 条
  • [1] Abbott BP, 2018, PHYS REV LETT, V121, DOI [10.1103/PhysRevLett.123.011102, 10.1103/PhysRevLett.121.129902]
  • [2] Observation of Gravitational Waves from a Binary Black Hole Merger
    Abbott, B. P.
    Abbott, R.
    Abbott, T. D.
    Abernathy, M. R.
    Acernese, F.
    Ackley, K.
    Adams, C.
    Adams, T.
    Addesso, P.
    Adhikari, R. X.
    Adya, V. B.
    Affeldt, C.
    Agathos, M.
    Agatsuma, K.
    Aggarwal, N.
    Aguiar, O. D.
    Aiello, L.
    Ain, A.
    Ajith, P.
    Allen, B.
    Allocca, A.
    Altin, P. A.
    Anderson, S. B.
    Anderson, W. G.
    Arai, K.
    Arain, M. A.
    Araya, M. C.
    Arceneaux, C. C.
    Areeda, J. S.
    Arnaud, N.
    Arun, K. G.
    Ascenzi, S.
    Ashton, G.
    Ast, M.
    Aston, S. M.
    Astone, P.
    Aufmuth, P.
    Aulbert, C.
    Babak, S.
    Bacon, P.
    Bader, M. K. M.
    Baker, P. T.
    Baldaccini, F.
    Ballardin, G.
    Ballmer, S. W.
    Barayoga, J. C.
    Barclay, S. E.
    Barish, B. C.
    Barker, D.
    Barone, F.
    [J]. PHYSICAL REVIEW LETTERS, 2016, 116 (06)
  • [3] Ade P.A.R., 2014, Astron. Astrophys., V571, pA16, DOI [10.1051/ 0004-6361/201423811, DOI 10.1051/0004-6361/201423811]
  • [4] Akiyama K., 2019, Astrophys. J. Lett, V875, DOI DOI 10.3847/2041-8213/AB0EC7
  • [5] Atazadeh K, 2014, GEN RELAT GRAVIT, V46, DOI 10.1007/s10714-014-1664-8
  • [6] Energy conditions in modified f(G) gravity
    Bamba, Kazuharu
    Ilyas, M.
    Bhatti, M. Z.
    Yousaf, Z.
    [J]. GENERAL RELATIVITY AND GRAVITATION, 2017, 49 (08)
  • [7] Coincident general relativity
    Beltran Jimenez, Jose
    Heisenberg, Lavinia
    Koivisto, Tomi
    [J]. PHYSICAL REVIEW D, 2018, 98 (04)
  • [8] Energy conditions and stability in f(R) theories of gravity with nonminimal coupling to matter
    Bertolami, Orfeu
    Sequeira, Miguel Carvalho
    [J]. PHYSICAL REVIEW D, 2009, 79 (10):
  • [9] Calcagni G, 2017, GRAD TEXTS PHYS, P1, DOI 10.1007/978-3-319-41127-9
  • [10] The role of energy conditions in f(R) cosmology
    Capozziello, S.
    Nojiri, S.
    Odintsov, S. D.
    [J]. PHYSICS LETTERS B, 2018, 781 : 99 - 106