Abstract
In the present article, the Eiesland condition has been used to obtain a new solution for compact star model by considering a non-singular well behaved gravitational potential of the form \(e^{\lambda (r)}=1+a r ^{2} [1+\tanh (br^{2}+c)]^{n}\) in the framework of anisotropic matter distribution. The solution so obtained is physically acceptable, which is exploited to compare the predicted masses and radii of known compact object as EXO 1785-248 (\(M=1.3M_{\odot }\)) for \(n= 3\) to 15. Moreover, the obtained solution satisfies the causality condition, Herrera cracking criterion, Tolman-Oppenheimer-Volkoff (TOV) equation, and adiabatic index \(\varGamma \) including all energy conditions. It is noted that the velocity of sound is increasing at \(n=3\) and start decreasing when \(n\ge 6\) which shows that the parameter \(n\) plays an important role to describe a well-behaved solution for anisotropic compact object. The moment of inertia \((I)\) is also obtained by Bejger-Haensel formula for \(n=3\) to 15. In addition to that, the maximum mass for the compact star has been discovered via. \(M-R\) curve for different values of \(n\).
Similar content being viewed by others
References
Abreu, H., Hernandez, H., Núñez, L.A.: Class. Quantum Gravity 24, 4631 (2007)
Bejger, M., Haensel, P.: Astron. Astrophys. 396, 917 (2002)
Bondi, H.: Proc. R. Soc. Lond. A 281, 39 (1964)
Bowers, R.L., Liang, E.P.T.: Astrophys. J. 188, 657 (1974)
Buchdahl, H.A.: Phys. Rev. D 116, 1027 (1959)
Chan, R., Herrera, L., Santos, N.O.: Mon. Not. R. Astron. Soc. 265, 533 (1993)
Chattopadhyay, P.K., Paul, B.C.: Pramāna 74, 513 (2010)
Eddington, A.S.: The Mathematical Theory of Relativity, p. 149. Cambridge University Press, Cambridge (1924)
Eiesland, J.: The group of motion of an Einstein space. Trans. Am. Math. Soc. 27, 213 (1925)
Eisenhart, L.P.: Riemannian Geometry, p. 97. Princeton Univ. Press, Princeton, New Jersey (1925)
Gupta, Y.K., Kumar, J.: Astrophys. Space Sci. 336, 419 (2011)
Hansraj, S.: Gen. Relativ. Gravit. 4, 125 (2012)
Harrison, B.K., Thorne, K.S., Wakano, M., Wheeler, J.A.: University of Chicago Press, Chicago (1965)
Herrera, L.: Phys. Lett. A 165, 206 (1992)
Herrera, L., Ponce de Leon, J.: J. Math. Phys. 26, 2302 (1985)
Herrera, L., Santos, N.O.: Astrophys. J. 438, 308 (1995)
Herrera, L., Santos, N.O.: Phys. Rep. 286, 53 (1997)
Herrera, L., Jimenez, J., Leal, L., Ponce de Leon, J.: J. Math. Phys. 25, 3274–3278 (1984)
Herrera, L., Di Prisco, A., Ospino, J., Fuenmayor, E.: J. Math. Phys. 42, 2129 (2001)
Herrera, L., Martin, J., Ospino, J.: J. Math. Phys. 43, 4889 (2002)
Ivanov, B.V.: Phys. Rev. D 65, 104011 (2002)
Ivanov, B.V.: Eur. Phys. J. C 78, 332 (2018)
Jasim, M.K., Maurya, S.K., Gupta, Y.K., Dayanandan, B.: Astrophys. Space Sci. 361, 352 (2016)
Kaluza, T.: Sitz. Preuss. Acad. Wiss. F 1, 966 (1921)
Karmarkar, K.R.: Proc. Indian Acad. Sci. A 27, 56 (1948)
Kippenhahn, R., Weigert, A. (eds.): Springer, Berlin (1990)
Klein, O.: Z. Phys. 37, 895 (1926)
Kohler, M., Chao, K.L.: Z. Naturforsch. 20, 1537 (1965)
Lake, K.: Phys. Rev. D 67, 104015 (2003)
Letelier, P.S.: Phys. Rev. D 22, 807 (1980)
Letelier, P.S.: Nuovo Cimento B 69, 145 (1982)
Letelier, P.S., Machado, R.: J. Math. Phys. 22, 827 (1981)
Liddle, A.R., et al.: Class. Quantum Gravity 7, 1009 (1990)
Maharaj, S.D., Govender, M.: Aust. J. Phys. 0, 959 (1997)
Maharaj, S.D., Komathiraj, K.: Gen. Relativ. Gravit. 39, 2079 (2007)
Mak, M.K., Harko, T.: Proc. R. Soc. Lond. A 459, 393–408 (2003)
Maurya, S.K., Govender, M.: Eur. Phys. J. C 77, 347 (2017a)
Maurya, S.K., Govender, M.: Eur. Phys. J. C 77, 420 (2017b)
Maurya, S.K., et al.: Eur. Phys. J. C 75, 389 (2015a)
Maurya, S.K., Gupta, Y.K., Ray, S., Dayanandan, B.: Eur. Phys. J. C 75, 225 (2015b)
Maurya, S.K., Gupta, Y.K., Dayanandan, B., Ray, S.: Eur. Phys. J. C 76, 266 (2016a)
Maurya, S.K., Gupta, Y.K., Smitha, T.T., Rahaman, F.: Eur. Phys. J. A 52, 191 (2016b)
Maurya, S.K., et al.: Int. J. Mod. Phys. D 26, 1750002 (2017a)
Maurya, S.K., Ratanpal, B.S., Govender, M.: Ann. Phys. 382, 36 (2017b)
Maurya, S.K., Banerjee, A., Hansraj, S.: Phys. Rev. D 97, 044022 (2018)
Pandey, S.N., Sharma, S.P.: Gen. Relativ. Gravit. 14, 113 (1981)
Pani, P., Berti, E., Cardoso, V., Read, J.: Phys. Rev. D 84, 104035 (2011)
Pavsic, M., Tapia, V.: (2001). arXiv:gr-qc/0010045
Rayski, J.: Preprint. Dublin Institute for Advance Studies (1976)
Rude, R.: Astrophysics 10, 427 (1972)
Sarkar, N., et al.: Mod. Phys. Lett. A 34, 195013 (2019)
Sawyer, R.F.: Phys. Rev. Lett. 29, 382 (1972)
Schwarzschild, K.: Sitz. Deut. Akad. Wiss. Math. Phys. Berlin 24, 424 (1916)
Singh, K.N., Pant, N.: Astrophys. Space Sci. 361, 177 (2016)
Singh, K.N., et al.: Astrophys. Space Sci. 361, 173 (2016a)
Singh, K.N., et al.: Int. J. Mod. Phys. D 25, 1650099 (2016b)
Singh, K.N., et al.: Ann. Phys. 377, 256 (2016c)
Singh, K.N., et al.: Eur. Phys. J. C 77, 100 (2017a)
Singh, K.N., et al.: Eur. Phys. J. A 53, 21 (2017b)
Singh, K.N., et al.: Int. J. Mod. Phys. D 27, 1950003 (2018)
Singh, K.N., et al.: Eur. Phys. J. C 79, 381 (2019)
Sokolov, A.I.: J. Exp. Theor. Phys. 79, 1137 (1980)
Thirukkanesh, S.: Int. J. Mod. Phys. D 24, 1550002 (2014)
Zeldovich, Y.B., Novikov, I.D.: Relativistic Astrophysics Stars and Relativity, vol. 1. University of Chicago Press, Chicago (1971)
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Conflict of interest
The authors declare that there is no conflict of interest regarding the publication of this manuscript.
Additional information
Publisher’s Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Rights and permissions
About this article
Cite this article
Jasim, M.K., Maurya, S.K. & Al-Sawaii, A.S.M. A generalised embedding class one static solution describing anisotropic fluid sphere. Astrophys Space Sci 365, 9 (2020). https://doi.org/10.1007/s10509-020-3724-8
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10509-020-3724-8