Abstract
Locally-rotationally-symmetric Bianchi-I space-time model is studied with constant Hubble parameter in \(f(R,T)=R+2\lambda T\) gravity. Although a single (primary) matter source is considered, an additional matter source appears due to the coupling between matter and \(f(R,T)\) gravity. The constraints are obtained for a realistic cosmological scenario. The solutions are also extended to the case of a scalar field (normal or phantom) model, and it is found that the model is consistent with a phantom scalar field only. The coupled matter also acts as phantom matter. The study shows that if one expects an accelerating universe from an anisotropic model, then the solutions become physically relevant only at late times when the universe enters into an accelerated phase. Placing some observational bounds on the present equation of state of dark energy, \(\omega_{0}\), the behavior of \(\omega(z)\) is depicted, which shows that the phantom field starts dominating very recently, somewhere between \(0.2\lesssim z\lesssim0.5\). The geometrical behavior of the model remains identical to the one in general relativity.
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Notes
\(\rho\geq0\), \(\rho+p\geq0\).
\(\rho+p\geq0\).
\(|\rho|\geq p\) or \(\rho\pm p\geq0\).
References
Adhav, K.S.: Astrophys. Space Sci. 339, 365–369 (2012)
Alam, U., Sahni, V., Saini, T.D., Starobinsky, A.A.: Mon. Not. R. Astron. Soc. 354, 275 (2004). arXiv:astro-ph/0311364
Alcaniz, J.S.: Phys. Rev. D 69, 083521 (2004). arXiv:astro-ph/0312424
Alhamzawi, A., Alhamzawi, R.: Int. J. Mod. Phys. D 35, 1650020 (2016)
Alvarenga, F.G., de la Cruz-Dombriz, A., Houndjo, M.J.S., Rodrigues, M.E., Sáez-Gómez, D.: Phys. Rev. D 87, 103526 (2013a). arXiv:gr-qc/1302.1866
Alvarenga, F.G., Houndjo, M.J.S., Monwanou, A.V., Oron, J.B.C.: J. Mod. Phys. 4, 130 (2013b). arXiv:gr-qc/1205.4678
Alves, M.E.S., Moraes, P.H.R.S., de Araujo, J.C.N., Malheiro, M.: Phys. Rev. D 94, 024032 (2016). arXiv:gr-qc/1604.03874
Azizi, T.: Int. J. Theor. Phys. 52, 3486 (2013). arXiv:gr-qc/1205.6957
Baffou, E.H., Kpadonou, A.V., Rodrigues, M.E., Houndjo, M.J.S., Tossa, J.: Astrophys. Space Sci. 356, 173–180 (2015). arXiv:gr-qc/1312.7311
Baffou, E.H., Houndjo, M.J.S., Kanfon, D.A., Salako, I.G.: Phys. Rev. D 98, 124037 (2018). arXiv:gr-qc/1808.01917
Basilakos, S.: Astron. Astrophys. 508, 575 (2009). arXiv:astro-ph.Co/0901.3195
Chakraborty, S.: Gen. Relativ. Gravit. 45, 2039 (2013). arXiv:gen-ph/1212.3050
Das, A., Rahaman, F., Guha, B.K., Ray, S.: Eur. Phys. J. C 76, 654 (2016). arXiv:gr-qc/1608.00566
Deb, D., Guha, B.K., Rahaman, F., Ray, S.: Phys. Rev. D 97, 084026 (2018). arXiv:gr-qc/1810.01409
Deb, D., et al.: Mon. Not. R. Astron. Soc. 485, 5652 (2019). arXiv:gr-qc/1810.07678
Debnath, P.S.: Int. J. Geom. Methods Mod. Phys. 16, 1950005 (2019). arXiv:gr-qc/1907.02238
Elizalde, E., Khurshudyan, M.: Phys. Rev. D 98, 123525 (2018). arXiv:gr-qc/1811.11499
Esmaeili, F.M.: J. High Energy Phys. Gravit. Cosmol. 4, 716 (2018)
Fisher, S.B., Carlson, E.D.: Phys. Rev. D 100, 064059 (2019)
Hannestad, S., Morstell, E.: Phys. Rev. D 66, 063508 (2002). arXiv:astro-ph/0205096
Harko, T., Moraes, P.H.R.S.:. arXiv:gr-qc/2003.08107
Harko, T., Lobo, F.S.N., Nojiri, S., Odintsov, S.D.: Phys. Rev. D 84, 024020 (2011). arXiv:gr-qc/1104.2669
Houndjo, M.J.S., Batista, C.E.M., Campos, J.P., Piattella, O.F.: Can. J. Phys. 91, 548 (2013). arXiv:gr-qc/1203.6084
Jamil, M., Momeni, D., Raza, M., Myrzakulov, R.: Eur. Phys. J. C 72, 1999 (2012). arXiv:gen-ph/1107.5807
Kumar, P., Singh, C.P.: Astrophys. Space Sci. 357, 120 (2015)
Lobato, R.V., Carvalho, G.A., Martins, A.G., Moraes, P.H.R.S.: Eur. Phys. J. Plus 134, 132 (2019). arXiv:gr-qc/1803.08630
Maurya, S.K., Tello-Ortizb, F.: J. Cosmol. Astropart. Phys. 28, 1950056 (2019). arXiv:gr-qc/1905.13519
Melchiorri, A., Mersini, L., Odman, C.J., Trodden, M.: Phys. Rev. D 68, 043509 (2003). arXiv:astro-ph/021152
Momeni, D., Moraes, P.H.R.S., Myrzakulov, R.: Astrophys. Space Sci. 361, 228 (2016). arXiv:gr-qc/1512.04755
Moraes, P.H.R.S., Correa, R.A.C., Ribeiro, G.: Eur. Phys. J. C 78, 192 (2018). arXiv:gr-qc/1606.07045
Moraes, P.H.R.S., de Paula, W., Correa, R.A.C.: Int. J. Mod. Phys. D 28, 1950098 (2019). arXiv:gr-qc/1710.07680
Noureen, I., Zubair, M., Bhatti, A.A., Abbas, G.: Eur. Phys. J. C 75, 323 (2015). arXiv:gr-qc/1504.01251
Ordines, T.M., Carlson, E.D.: Phys. Rev. D 99, 104052 (2019). arXiv:gr-qc/1902.05858
Pasqua, A., Chattopadhyay, S., Khomenkoc, I.: Can. J. Phys. 91, 632 (2013). arXiv:gen-ph1305.1873
Rajabi, F., Nozari, K.: Phys. Rev. D 96, 084061 (2017). arXiv:gr-qc/1710.01910
Ram, S. Priyanka: Astrophys. Space Sci. 347, 389 (2013)
Reddy, D.R.K., Naidu, R.L., Satyanarayana, B.: Int. J. Theor. Phys. 51, 3222 (2013)
Saha, B.: Int. J. Theor. Phys. 54, 3776 (2015)
Sahoo, P.K., Moraes, P.H.R.S., Sahoo, P.: Eur. Phys. J. C 78, 46 (2018). arXiv:gr-qc/1709.07774
Salehi, A., Aftabi, S.: J. High Energy Phys. 09, 140 (2016). arXiv:gr-qc/1502.04507
Santos, A.F., Ferst, C.J.: Mod. Phys. Lett. A 30, 1550214 (2015)
Shabani, H., Ziaie, A.H.: Eur. Phys. J. C 78, 397 (2018). arXiv:gr-qc/1708.07874
Shamir, M.F.: J. Exp. Theor. Phys. 119, 242 (2014)
Shamir, M.F.: Eur. Phys. J. C 75, 354 (2015). arXiv:gen-ph/1507.08175
Sharif, M., Anwar, A.: Astrophys. Space Sci. 363, 123 (2018)
Sharif, M., Rani, S., Myrzakulov, R.: Eur. Phys. J. Plus 128, 123 (2013). arXiv:gr-qc/1210.2714
Singh, V., Beesham, A.: Eur. Phys. J. C 78, 564 (2018)
Singh, V., Beesham, A.: Gen. Relativ. Gravit. 51, 166 (2019). arXiv:gr-qc/1912.05850
Singh, V., Beesham, A.: Eur. Phys. J. Plus 135, 319 (2020). arXiv:gr-qc/2003.08665
Singh, C.P., Singh, V.: Gen. Relativ. Gravit. 46, 1696 (2014)
Singh, C.P., Singh, V.: Astrophys. Space Sci. 356, 153 (2015)
Singh, V., Singh, C.P.: Int. J. Theor. Phys. 55, 1257 (2016)
Sofuoglu, D.: Astrophys. Space Sci. 361, 12 (2016)
Srivastava, M., Singh, C.P.: Astrophys. Space Sci. 363, 117 (2018)
Tiwari, R.K., Beesham, A.: Astrophys. Space Sci. 363, 234 (2018)
Tretyakov, P.V.: Eur. Phys. J. C 78, 896 (2018). arXiv:gr-qc/1810.11313
Yousaf, Z., Bamba, K., Bhatti, M.Z.: Phys. Rev. D 93, 124048 (2016). arXiv:gr-qc/1606.00147
Zubair, M., Waheed, S., Ahmad, Y.: Eur. Phys. J. C 76, 444 (2016). arXiv:gr-qc/1607.05998
Acknowledgements
We are thankful to the reviewer for his suggestions which help to provide a descriptive motivation of the work. Vijay Singh expresses his sincere thank to the University of Zululand, South Africa, for providing a postdoctoral fellowship and necessary facilities. This work is based on the research supported wholly / in part by the National Research Foundation of South Africa (Grant Numbers: 118511).
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Singh, V., Beesham, A. LRS Bianchi I model with constant expansion rate in \(f(R,T)\) gravity. Astrophys Space Sci 365, 125 (2020). https://doi.org/10.1007/s10509-020-03839-w
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DOI: https://doi.org/10.1007/s10509-020-03839-w