Full Paper View Go Back
Anisotropic String Cosmological Model for Perfect Fluid Distribution in f(T) Gravity
Kalpana Pawar1 , A.K. Dabre2 , N.T. Katre3
Section:Research Paper, Product Type: Journal-Paper
Vol.10 ,
Issue.6 , pp.1-7, Dec-2022
Online published on Dec 31, 2022
Copyright © Kalpana Pawar, A.K. Dabre, N.T. Katre . This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
View this paper at Google Scholar | DPI Digital Library
How to Cite this Paper
- IEEE Citation
- MLA Citation
- APA Citation
- BibTex Citation
- RIS Citation
IEEE Style Citation: Kalpana Pawar, A.K. Dabre, N.T. Katre, “Anisotropic String Cosmological Model for Perfect Fluid Distribution in f(T) Gravity,” International Journal of Scientific Research in Physics and Applied Sciences, Vol.10, Issue.6, pp.1-7, 2022.
MLA Style Citation: Kalpana Pawar, A.K. Dabre, N.T. Katre "Anisotropic String Cosmological Model for Perfect Fluid Distribution in f(T) Gravity." International Journal of Scientific Research in Physics and Applied Sciences 10.6 (2022): 1-7.
APA Style Citation: Kalpana Pawar, A.K. Dabre, N.T. Katre, (2022). Anisotropic String Cosmological Model for Perfect Fluid Distribution in f(T) Gravity. International Journal of Scientific Research in Physics and Applied Sciences, 10(6), 1-7.
BibTex Style Citation:
@article{Pawar_2022,
author = {Kalpana Pawar, A.K. Dabre, N.T. Katre},
title = {Anisotropic String Cosmological Model for Perfect Fluid Distribution in f(T) Gravity},
journal = {International Journal of Scientific Research in Physics and Applied Sciences},
issue_date = {12 2022},
volume = {10},
Issue = {6},
month = {12},
year = {2022},
issn = {2347-2693},
pages = {1-7},
url = {https://www.isroset.org/journal/IJSRPAS/full_paper_view.php?paper_id=3001},
publisher = {IJCSE, Indore, INDIA},
}
RIS Style Citation:
TY - JOUR
UR - https://www.isroset.org/journal/IJSRPAS/full_paper_view.php?paper_id=3001
TI - Anisotropic String Cosmological Model for Perfect Fluid Distribution in f(T) Gravity
T2 - International Journal of Scientific Research in Physics and Applied Sciences
AU - Kalpana Pawar, A.K. Dabre, N.T. Katre
PY - 2022
DA - 2022/12/31
PB - IJCSE, Indore, INDIA
SP - 1-7
IS - 6
VL - 10
SN - 2347-2693
ER -
Abstract :
The present study deals with a spatially homogeneous and anisotropic Bianchi type VI0 space-time in the presence of string of clouds and perfect fluid distribution within the context of gravity. The analytic relation and the hybrid exponential form of the average scale factor have been considered to obtain the exact solutions of highly non-linear field equations. Some physical and kinematical parameters of the constructed model along with the behavior of the equation of state parameter for string fluid are discussed and presented graphically.
Key-Words / Index Term :
Bianchi-type VI0 space-time, Cosmic String, Perfect Fluid, Gravity.
References :
[1] G. Cognola, E. Elizalde, S. Nojiri, S. D. Odintsov, and S. Zerbini, “String-inspired Gauss-Bonnet gravity reconstructed from the universe expansion history and yielding the transition from matter dominance to dark energy,” Phys. Rev. D - Part. Fields, Gravit. Cosmol., vol. 75, no. 8, Apr. 2007.
[2] S. Nojiri, S. D. Odintsov, and M. Sami, “Dark energy cosmology from higher-order, string-inspired gravity, and its reconstruction,” vol. 74, no. 4, p. 046004, Aug. 2006.
[3] P.-M. Zhang, Y.-S. Duan, and L.-M. Cao, “The Order Parameter Field For Cosmic String, Inflation And Dark Energy,” Mod. Phys. Lett. A, vol. 18, no. 36, pp. 2587–2597, Nov. 2003.
[4] P. F. Gonzalez-Diaz and J. A. Jimenez Madrid, “Wiggly Cosmic Strings Accrete Dark Energy,” Int. J. Mod. Phys. D, vol. 15, no. 04, pp. 603–613, Apr. 2006.
[5] Y. Cui and D. E. Morrissey, “Nonthermal dark matter from cosmic strings,” Phys. Rev. D, vol. 79, no. 8, p. 083532, Apr. 2009.
[6] H. Bernardo, R. Brandenberger, and G. Franzmann, “String cosmology backgrounds from classical string geometry,” Phys. Rev. D, vol. 103, no. 4, p. 43540, 2021.
[7] T. Kibble, “Topology of cosmic domains and strings,” J. Phys. A Gen. Phys., vol. 9, no. 8, pp. 1387–1398, 1976.
[8] N. Turok, “The evolution of cosmic density perturbations around grand unified strings,” Phys. Lett. B, vol. 126, no. 6, pp. 437–440, Jul. 1983.
[9] P. S. Letelier, “Fluids of strings in general relativity,” Nuovo Cim. B, vol. 63, no. 2, pp. 519–528, 1981.
[10] P. S. Letelier, “String cosmologies,” Phys. Rev. D, vol. 28, no. 10, pp. 2414–2419, Nov. 1983.
[11] J. Stachel, “Thickening the string. I. The string perfect dust,” Phys. Rev. D, vol. 21, no. 8, pp. 2171–2181, 1980.
[12] A. Vilenkin, “Cosmic strings and domain walls,” Phys. Rep., vol. 121, no. 5, pp. 263–315, 1985.
[13] B. Hartmann and F. Arbabzadah, “Cosmic strings interacting with dark strings,” J. High Energy Phys., vol. 2009, no. 07, pp. 068–068, Jul. 2009.
[14] T. Vinutha, V. U. M. Rao, and M. Mengesha, “Anisotropic dark energy cosmological model with cosmic strings,” Can. J. Phys., vol. 99, no. 3, pp. 168–175, Mar. 2021.
[15] R. Bali and D. K. Singh, “Bianchi type-V bulk viscous fluid string dust cosmological model in general relativity,” Astrophys. Space Sci., vol. 300, no. 4, pp. 387–394, 2005.
[16] S. P. Hatkar, S. V. Gore, and S. D. Katore, “Kasner type magnetized string cosmological models in F(R, T) gravity,” Serbian Astron. J., vol. 197, no. 197, pp. 1–11, 2018.
[17] T. Vinutha, V. U. M. Rao, B. Getaneh, and M. Mengesha, “Dark energy cosmological models with cosmic string,” Astrophys. Space Sci., vol. 363, no. 9, p. 188, Sep. 2018.
[18] D. R. K. Reddy, R. L. Naidu, K. Dasu Naidu, and T. Ram Prasad, “Kaluza-Klein universe with cosmic strings and bulk viscosity in f(R,T) gravity,” Astrophys. Space Sci., vol. 346, no. 1, pp. 261–265, 2013.
[19] P. Berglund, T. Hübsch, and D. Mini?, “Dark energy and string theory,” Phys. Lett. B, vol. 798, p. 134950, Nov. 2019.
[20] M. Kiran and D. R. K. Reddy, “Non-existence of Bianchi type-III bulk viscous string cosmological model in f(R,T) gravity,” Astrophys. Space Sci., vol. 346, no. 2, pp. 521–524, Aug. 2013.
[21] B. Mishra, S. Tarai, and S. K. Tripathy, “Anisotropic cosmological reconstruction in f (R, T) gravity,” Mod. Phys. Lett. A, vol. 33, no. 29, 2018.
[22] R. Bali and Anjali, “Bianchi type I magnetized string cosmological model in general relativity,” Astrophys. Space Sci., vol. 302, no. 1–4, pp. 201–205, 2006.
[23] R. Bali and U. K. Pareek, “Bianchi Type I string dust cosmological model with magnetic field in general relativity,” Astrophys. Space Sci., vol. 312, no. 3–4, pp. 305–310, 2007.
[24] R. Bali and A. Pradhan, “Bianchi type-III string cosmological models with time dependent bulk viscosity,” Chinese Phys. Lett., vol. 24, no. 2, pp. 585–588, 2007.
[25] R. Ferraro, “f(R) and f(T) theories of modified gravity,” AIP Conf. Proc., vol. 1471, no. 2012, pp. 103–110, 2012.
[26] C. G. Böhmer, A. Mussa, and N. Tamanini, “Existence of relativistic stars in f(T) gravity,” Class. Quantum Gravity, vol. 28, no. 24, Dec. 2011.
[27] A. Moreira, J. Silva, D. Veras, and C. A. S. Almeida, “Thick string-like braneworlds in f(T) gravity,” Int. J. Mod. Phys. D, vol. 30, no. 07, p. 2150047, May 2021.
[28] V. R. Chirde, S. P. Hatkar, and S. D. Katore, “Bianchi type I cosmological model with perfect fluid and string in f(T) theory of gravitation,” Int. J. Mod. Phys. D, vol. 29, no. 08, p. 2050054, Jun. 2020.
[29] N. P. Gaikwad, M. S. Borkar, and S. S. Charjan, “Bianchi type-I massive string magnetized barotropic perfect fluid cosmological model in the bimetric theory of gravitation,” Chinese Phys. Lett., vol. 28, no. 8, 2011.
[30] A. Pradhan, H. Amirhashchi, and H. Zainuddin, “Exact solution of perfect fluid massive string cosmology in Bianchi type III space-time with decaying vacuum energy density ?,” Astrophys. Space Sci., vol. 331, no. 2, pp. 679–687, Feb. 2011.
[31] S. Rani, J. K. Singh, and N. K. Sharma, “Bianchi Type-III Magnetized String Cosmological Models for Perfect Fluid Distribution in f (R,T) Gravity,” Int. J. Theor. Phys., vol. 54, no. 5, pp. 1698–1710, May 2015.
[32] R. Bali and U. K. Pareek, “Bianchi Type III magnetized massive string cosmological model for perfect fluid distribution in general relativity,” Astrophys. Space Sci., vol. 318, no. 3–4, pp. 237–242, Dec. 2008.
[33] P. S. Letelier, “Clouds of strings in general relativity,” Phys. Rev. D, vol. 20, no. 6, pp. 1294–1302, Sep. 1979.
[34] J. Baro and K. P. Singh, “Higher Dimensional Bianchi Type-Iii String Universe With Bulk Viscous Fluid And Constant Deceleration Parameter,” Adv. Math. Sci. J., vol. 9, no. 10, pp. 8779–8787, Oct. 2020.
[35] A. Dixit, R. Zia, and A. Pradhan, “Anisotropic bulk viscous string cosmological models of the Universe under a time-dependent deceleration parameter,” Pramana, vol. 94, no. 1, p. 25, Dec. 2020.
[36] K. D. Krori, T. Chaudhury, C. R. Mahanta, and A. Mazumdar, “Some exact solutions in string cosmology,” Gen. Relativ. Gravit., vol. 22, no. 2, pp. 123–130, Feb. 1990.
You do not have rights to view the full text article.
Please contact administration for subscription to Journal or individual article.
Mail us at support@isroset.org or view contact page for more details.