Inflationary scenario in Bianchi type V bulk viscous cosmological model in Saez Ballester theory
Manish Khowalmanish.2410180015@muj.manipal.eduDepartment of Mathematics and StatisticsManipal University JaipurJaipur, Rajasthan, 303007, IndiaView full profile → , *Laxmi PooniaCorresponding authorLaxmi.poonia@jaipur.manipal.eduDepartment of Mathematics and StatisticsManipal University JaipurJaipur, Rajasthan, 303007, IndiaView full profile → , Manali Vijayvargiyamanali.2410180014@muj.manipal.eduDepartment of Mathematics and StatisticsManipal University JaipurJaipur, Rajasthan, 303007, IndiaView full profile → , Rakhi Mathurrakhi.221051021@muj.manipal.eduDepartment of Mathematics and StatisticsManipal University JaipurJaipur, Rajasthan, 303007, IndiaView full profile →
* Corresponding author · click or hover a name for details
- Received:
- 10 Dec 2024
- Published Online:
- 30 Sep 2025
- Article type:
- Research Article
- Language:
- EN
- Article no.:
- JIM-2372
- Pages:
- 2301–2310
Abstract
Keywords
Subject Classifications
References
[1] A. H. Guth, “Inflationary universe: A possible solution to the horizon and flatness problems,” Phys. Rev. D, vol. 23, no. 2, pp. 347–356, 1981.
[2] J. D. Barrow and M. S. Turner, “Inflation in the Universe,” Nature, vol. 292, no. 5818, pp. 35–38 (1981).
[3] L. F. Abbott and M. B. Wise, “Constraints on generalized inflationary cosmologies,” Nucl. Phys. B, vol. 244, no. 2, pp. 541–548 (1984).
[4] A. Albrecht and P. J. Steinhardt, “Cosmology for grand unified theories with radiatively induced symmetry breaking,” Phys. Rev. Lett., vol. 48, no. 17, pp. 1220–1223 (1982).
[5] A. D. Linde, “A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems,” Phys. Lett. B, vol. 108, no. 6, pp. 389–393, 1982.
[6] A. D. Linde, “Chaotic inflation,” Phys. Lett. B, vol. 129, no. 3–4, pp. 177–181 (1983).
[7] D. La and P. J. Steinhardt, “Extended inflationary cosmology,” Phys. Rev. Lett., vol. 62, no. 4, pp. 376–379 (1989).
[8] M. B. Mijić, M. S. Morris, and W. M. Suen, “The R² cosmology: Inflation without a phase transition,” Phys. Rev. D, vol. 34, no. 10, pp. 2934–2946 (1986).
[9] S. Mataresse and P. Luechin, “Power-Law Inflation,” Phys. Rev. D, vol. 32, pp. 1316–1322 (1985).
[10] C. Mathiazhagan and V. B. Johri, “An inflationary universe in Brans-Dicke theory: a hopeful sign of theoretical estimation of the gravitational constant,” Class. Quantum Grav., vol. 1, no. 2, pp. L29–L32 (1984).
[11] T. Rothman and G. F. R. Ellis, “Can inflation occur in anisotropic cosmologies?,” Phys. Lett. B, vol. 180, no. 1–2, pp. 19–24 (1986).
[12] J. A. Stein-Schabes, “Inflation in spherically symmetric inhomogeneous models,” Phys. Rev. D, vol. 35, no. 8, pp. 2345–2353 (1987).
[13] V. Maheshwari and L. Poonia, “Bianchi Type V Inflationary Cosmological Model with Bulk Viscosity in General Relativity,” (2023).
[14] L. L. Jat, D. Chhajed, and A. Tyagi, “Bianchi type-VIII inflationary universe with flat potential for perfect fluid distribution in general relativity,” J. Rajasthan Acad. Phys. Sci., vol. 21, no. 3, pp. 131–142 (2022).
[15] S. Singh and R. Bali, “Inflationary cosmological model with variable bulk viscosity in anisotropic Bianchi type VI0 space-time,” [Journal Name Missing].
[16] J. C. Fabris, S. V. B. Goncalves, and R. D. S. Ribeiro, “Bulk viscosity driving the acceleration of the Universe,” Gen. Relativ. Gravit., vol. 38, pp. 495–506 (2006).
[17] J. P. Singh and P. S. Baghel, “Bianchi type V bulk viscous cosmological models with time dependent Λ-term,” Electron. J. Theor. Phys., vol. 6, no. 22, pp. 85–96 (2009).
[18] M. Vijaya Santhi, V. U. M. Rao, and Y. Aditya, “Bianchi type-I bulk viscous string model in f(R) gravity,” J. Dyn. Syst. Geom. Theor., vol. 17, no. 1, pp. 23–38 (2019).
[19] R. Bali, P. Singh, and J. P. Singh, “Bianchi type V viscous fluid cosmological models in presence of decaying vacuum energy,” Astrophys. Space Sci., vol. 341, pp. 701–706 (2012).
[20] S. Sen, G. S. Khadekar, and S. Samdurkar, “Bulk Viscous Bianchi Type-III Cosmological Model with Modified Takabayasi String in the Presence of Varying Λ,” J. Dyn. Syst. Geom. Theor., vol. 19, no. 1, pp. 95–112 (2021).
[21] K. L. Mahanta, “Bulk viscous cosmological models in f(R, T) theory of gravity,” Astrophys. Space Sci., vol. 353, pp. 683–689 (2014).
[22] M. P. V. V. Bhaskara Rao, D. R. K. Reddy, and K. Sobhan Babu, “Bianchi type-V bulk viscous string cosmological model in a self-creation theory of gravitation,” Astrophys. Space Sci., vol. 359, pp. 1–5 (2015).
[23] L. K. Tiwari and R. K. Tiwari, “Bianchi Type-V Cosmological Models with Viscous Fluid & Varying Λ,” Prespacetime J., vol. 8, no. 14, pp. 1509–1520 (2017).
[24] S. Garg, B. Agrawal, S. Kumar, and A. Singh, “Bianchi Type I Bulk Viscous Fluid Cosmological Models with Varying Cosmological Term Λ,” Prespacetime J., vol. 15, no. 3 (2024).
[25] S. Jokweni, V. Singh, and A. Beesham, “LRS Bianchi I model with bulk viscosity in gravity,” Gravit. Cosmol., vol. 27, no. 2, pp. 169–177 (2021).
[26] D. Saez and V. J. Ballester, “A simple coupling with cosmological implications,” Phys. Lett. A, vol. 113, no. 9, pp. 467–470 (1986).
[27] C. Brans and R. H. Dicke, “Mach’s principle and a relativistic theory of gravitation,” Phys. Rev., vol. 124, no. 3, pp. 925–935 (1961).
[28] S. Capozziello, S. Carloni, and A. Troisi, “Quintessence without scalar fields,” arXiv preprint, arXiv:astro-ph/0303041, 2003.
[29] S. I. Nojiri and S. D. Odintsov, “Modified gravity with negative and positive powers of curvature: Unification of inflation and cosmic acceleration,” Phys. Rev. D, vol. 68, no. 12, pp. 123512 (2003).
[30] T. Harko, F. S. Lobo, S. I. Nojiri, and S. D. Odintsov, “f(R, T) gravity,” Phys. Rev. D, vol. 84, no. 2, pp. 024020 (2011).
[31] R. K. Mishra and H. Dua, “Evolution of FLRW universe in Brans-Dicke gravity theory,” Astrophys. Space Sci., vol. 366, no. 1, pp. 6 (2021).
[32] R. K. Mishra and H. Dua, “Bulk viscous string cosmological models in Saez–Ballester theory of gravity,” Astrophys. Space Sci., vol. 364, no. 11, pp. 195 (2019).
[33] M. V. Santhi and Y. Sobhanbabu, “Bianchi type-III Tsallis holographic dark energy model in Saez–Ballester theory of gravitation,” Eur. Phys. J. C, vol. 80, no. 12, pp. 1198 (2020).
[34] R. L. Naidu, Y. Aditya, K. D. Raju, T. Vinutha, and D. R. K. Reddy, “Kaluza-Klein FRW dark energy models in Saez–Ballester theory of gravitation,” New Astron., vol. 85, pp. 101564 (2021).
