Abstract
In this paper, we constructed the three-layered gravastar model in cylindrical space–time. We considered one of the modified gravity theories to investigate the structural progression of the celestial object. The matter we considered in this model is effective, which further constituted the perfect fluid and extra degrees of freedom due to the modification of Einstein gravity. For the modelling of the three regions of gravastar, we used a specific barotropic equation of state. We then evaluated the subsequent field equations, hydrostatic equilibrium condition and gravitational mass. Furthermore, the metric coefficients for the three regions of the system were determined. Eventually, we discussed the important features of the gravastar and deduced its physical significance along with its graphical representations.
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P O Mazur and E Mottola, Proc. Natl Acad. Sci. USA 101, 9545 (2004)
C Cattoen, T Faber and M Visser, Class. Quantum Gravity 22, 4189 (2005)
M Visser and D L Wiltshire, Class. Quantum Gravity 21, 1135 (2004)
A DeBenedictis, D Horvat, S Ilijić, S Kloster and K Viswanathan, Class. Quantum Gravity 23, 2303 (2006)
C B Chirenti and L Rezzolla, Class. Quantum Gravity 24, 4191 (2007)
N Sakai, H Saida and T Tamaki, Phys. Rev. D 90, 104013 (2014)
S Fay, S Nesseris and L Perivolaropoulos, Phys. Rev. D 76, 063504 (2007)
N J Poplawski, preprint arXiv:gr-qc/0608031 (2006)
T Harko, F S N Lobo, S Nojiri and S D Odintsov, Phys. Rev. D 84, 024020 (2011)
A Das, S Ghosh, D Deb, F Rahaman and S Ray, Nucl. Phys. B 954, 114986 (2020)
U Debnath, Eur. Phys. J. C 79, 499 (2019)
Z Haghani, T Harko, F S N Lobo, H R Sepangi and S Shahidi, Phys. Rev. D 88, 044023 (2013)
S D Odintsov and D Sáez-Gómez, Phys. Lett. 725, 437 (2013)
E Baffou, M Houndjo and J Tosssa, Astrophys. Space Sci. 361, 376, (2016)
I Ayuso, J B Jiménez and Á de la Cruz-Dombriz, Phys. Rev. D 91, 104003 (2015)
Z Yousaf, M Bhatti and T Naseer, Eur. Phys. J. Plus 135, 323 (2020)
Z Yousaf, M Bhatti and T Naseer, Phys. Dark Universe 28, 100535 (2020)
M Z Bhatti, Z Yousaf and M Nawaz, Int. J. Geom. Meth. Mod. Phys. 17, 2050017 (2020)
M Z Bhatti, K Bamba, Z Yousaf and M Nawaz, J. Cosmol. Astropart. Phys. 09, 011 (2019)
Z Yousaf, M Bhatti and H Asad, Phys. Dark Universe 28, 100527 (2020)
Z Yousaf, Phys. Scr. 97, 025301 (2022)
Z Yousaf, Universe 8, 131 (2022)
S Ghosh et al, Phys. Lett. B 767, 380 (2017)
S Ghosh, S Ray, F Rahaman and B Guha, Ann. Phys. 394, 230 (2018)
S Ghosh, D Shee, S Ray, F Rahaman and B K Guha, Results Phys. 14, 102473 (2019)
S Ghosh, D Shee, S Ray, F Rahaman and B K Guha, Ann. Phys. 411, 167968 (2019)
M Bhatti, Z Yousaf and M Ajmal, Int. J. Mod. Phys. D 28, 1950123 (2019)
A Das, S Ghosh, B Guha, S Das, F Rahaman and S Ray, Phys. Rev. D 95, 124011 (2017)
R Sengupta, S Ghosh, S Ray, B Mishra and S Tripathy, Phys. Rev. D 102, 024037 (2020)
S Ray, R Sengupta and H Nimesh, Int. J. Mod. Phys. D 29, 2030004 (2020)
Y B Zeldovich, Mon. Not. R. Astron. Soc. 160, 1P (1972)
B J Carr, Astrophys. J. 201, 1 (1975)
M S Madsen, J P Mimoso, J A Butcher and G F Ellis, Phys. Rev. D 46, 1399 (1992)
P S Wesson, Vistas Astron. 29, 281 (1986)
T M Braje and R W Romani, Astrophys. J. 580, 1043 (2002)
L P Linares, M Malheiro and S Ray, Int. J. Mod. Phys. D 13, 1355 (2004)
W Israel, Nuovo Cimento B 44, 1 (1966)
G Darmois, Memorial des Sciences Mathématiques (Gauthier Villars, Paris, 1927) Vol. 25
Z Yousaf, M Z-u-H Bhatti and U Farwa, Eur. Phys. J. C 77 359 (2017)
K Lanczos, Ann. Phys. (Berlin) 379, 518 (1924)
N Sen, Ann. Phys. (Berlin) 378, 365 (1924)
G Perry and R B Mann, Gen. Relativ. Gravit. 24, 305 (1992)
P Musgrave and K Lake, Class. Quantum Gravity 13, 1885 (1996)
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Appendix
Appendix
The values of \(\delta _{i}\)’s where \(i=\)1–10 and that of \(D_{j}\)’s where \(j=\)6,7,8 appeared in eqs (9), (10) and (11) are discussed as follows:
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Yousaf, Z., Bhatti, M.Z. & Asad, H. Matter–curvature gravity modification and the formation of cylindrical isotropic systems. Pramana - J Phys 96, 111 (2022). https://doi.org/10.1007/s12043-022-02356-5
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DOI: https://doi.org/10.1007/s12043-022-02356-5