Noether symmetries and some exact solutions inf(R, T2) Theory
- 作者: Sharif M.1, Gul M.1
-
隶属关系:
- The University of Lahore
- 期: 卷 163, 编号 4 (2023)
- 页面: 496-502
- 栏目: Articles
- URL: https://journals.rcsi.science/0044-4510/article/view/145387
- DOI: https://doi.org/10.31857/S0044451023040065
- EDN: https://elibrary.ru/LRECZQ
- ID: 145387
如何引用文章
详细
The main objective of this article is to examine some physically viable solutions through the Noether symmetry technique in f ( R, T 2) theory. In order to investigate Noether equations, symmetry generators and conserved quantities, we use a speci c model of this modi ed theory. We nd exact solutions and examine the behavior of various cosmological quantities. It is found the behavior these quantities is consistent with current observations indicating that this theory describes the cosmic accelerated expansion. We conclude that generators of Noether symmetry and conserved quantities exist in this theory.
作者简介
M. Sharif
The University of Lahore
Email: jetp@kapitza.ras.ru
Lahore-54000, Pakistan
M. Gul
The University of Lahore
编辑信件的主要联系方式.
Email: jetp@kapitza.ras.ru
Lahore-54000, Pakistan
参考
- A.V. Filippenko and A.G. Riess, Phys. Rep. 307, 31 (1998)
- M. Tegmark, M.A. Strauss, M.R. Blanton, K. Abazajian, S. Dodelson, H. Sandvik, X. Wang, D.H. Weinberg, I. Zehavi, N.A. Bahcall, and F. Hoyle, Phys. Rev. D 69, 103501 (2004).
- A.D. Felice and S.R. Tsujikawa, Living Rev. Relativ. 13, 3 (2010)
- S. Nojiri and S.D. Odintsov, Phys. Rep. 505, 59 (2011).
- N. Katirci and M. Kavuk, Eur. Phys. J. Plus 129, 163 (2014).
- M. Roshan and F. Shojai, Phys. Rev. D 94, 044002 (2016).
- C.V.R. Board and J.D. Barrow, Phys. Rev. D 96, 123517 (2017).
- S. Bahamonde, M. Marciu, and P.Rudra, Phys. Rev. D 100, 083511 (2019).
- M. Sharif and M.Z. Gul, Phys. Scr. 96, 025002 (2021)
- Phys. Scr. 96, 125007 (2021)
- Chin. J. Phys. 80, 58 (2022).
- M. Sharif and M.Z. Gul, Int. J. Mod. Phys. A 36, 2150004 (2021)
- Universe 7, 154 (2021)
- Int. J. Geom. Methods Mod. Phys. 19, 2250012 (2021)
- Chin. J. Phys. 71, 365 (2021)
- Mod. Phys. Lett. A 37, 2250005 (2022).
- E. Noether, Tramp. Th. Stat, Phys 1, 189 (1918)
- T. Feroze, F.M. Mahomed, and A. Qadir, Nonlinear Dyn. 45, 65 (2006).
- S. Capozziello, M. De Laurentis, and S.D. Odintsov, Eur. Phys. J. C 72, 1434 (2012).
- S. Capozziello, R.D. Ritis, and A.A. Marino, Class. Quantum Gravity 14, 3259 (1997).
- S. Capozziello, G. Marmo, and C.P.Rubano, Int. J. Mod. Phys. D 6, 491 (1997).
- A.K. Sanyal, Phys. Lett. B 524, 177 (2002).
- U. Camci and Y. Kucukakca,: Phys. Rev. D 76, 084023 (2007).
- D. Momeni and H. Gholizade, Int. J. Mod. Phys. D 18, 1 (2009).
- Y. Kucukakca, U. Camci, and I. Semiz, Gen. Relat. Gravit. 44, 1893 (2012).
- S. Basilakos, S. Capozziello, M. De Laurentis, A. Paliathanasis, and M. Tsamparlis, Phys. Rev. D 88, 103526 (2013).
- U. Camci, Eur. Phys. J. C 74, 3201 (2014)
- J. Cosmol. Astropart. Phys. 07, 002 (2014).
- U. Camci and J. Cosmol, J. Cosmol. Astropart. Phys. 2014, 2 (2014).
- U. Camci, A. Yildirim, and I. Basaran, Astropart. Phys. 76, 29 (2016).
- S. Capozziello, S.J.G. Gionti, and D. Vernieri, J. Cosmol. Astropart. Phys. 1601, 015 (2016).