Anisotropic compact star models in Karmarkar space time continuum

[1]  K. Singh,et al.  A 4D spacetime embedded in a 5D pseudo-Euclidean space describing interior of compact stars , 2017 .

[2]  K. Singh,et al.  Physical viability of fluid spheres satisfying the Karmarkar condition , 2016, The European Physical Journal C.

[3]  Y. K. Gupta,et al.  A new exact anisotropic solution of embedding class one , 2016 .

[4]  Y. K. Gupta,et al.  A new model for spherically symmetric anisotropic compact star , 2016 .

[5]  K. Singh,et al.  A new analytic solution representing anisotropic stellar objects in embedding class I , 2016 .

[6]  K. Singh,et al.  Charged anisotropic Buchdahl solution as an embedding class I spacetime , 2016 .

[7]  Y. K. Gupta,et al.  Modelling of anisotropic compact stars of embedding class one , 2016, 1604.00531.

[8]  P. Bhar Strange star admitting Chaplygin equation of state in Finch–Skea spacetime , 2015 .

[9]  Y. K. Gupta,et al.  Spherically symmetric charged compact stars , 2015, The European Physical Journal C.

[10]  P. Bhar A new hybrid star model in Krori-Barua spacetime , 2015 .

[11]  Y. K. Gupta,et al.  Anisotropic models for compact stars , 2015, 1504.00209.

[12]  P. Bhar Singularity-free anisotropic strange quintessence star , 2014, 1412.0107.

[13]  M. Dey,et al.  Strange star equation of state fits the refined mass measurement of 12 pulsars and predicts their radii , 2013, 1303.1956.

[14]  F. C. Ragel,et al.  Exact anisotropic sphere with polytropic equation of state , 2012 .

[15]  L. Núñez,et al.  Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects , 2007, 0706.3452.

[16]  M. Gleiser,et al.  Anisotropic Stars: Exact Solutions , 2000, astro-ph/0012265.

[17]  L. Herrera,et al.  Local anisotropy in self-gravitating systems , 1997 .

[18]  A. Mehra,et al.  Anisotropic spheres with variable energy density in general relativity , 1994 .

[19]  N. O. Santos,et al.  Dynamical instability for radiating anisotropic collapse , 1993 .

[20]  L. Herrera Cracking of self-gravitating compact objects , 1992 .

[21]  Achim Weiss,et al.  Stellar Structure and Evolution , 1990 .

[22]  J. P. Leon General relativistic electromagnetic mass models of neutral spherically symmetric systems , 1987 .

[23]  S. N. Pandey,et al.  Insufficiency of Karmarkar's condition , 1982 .

[24]  G. Ruggeri,et al.  Adiabatic contraction of anisotropic spheres in general relativity , 1979 .

[25]  E. Liang,et al.  Anisotropic spheres in general relativity , 1974 .

[26]  M. Ruderman Pulsars: Structure and Dynamics , 1972 .

[27]  R. Sawyer Condensedπ−Phase in Neutron-Star Matter , 1972 .

[28]  K. Köhler Reinigung und Charakterisierung zweier Proteine des Adenovirus Typ 2 , 1965 .

[29]  H. Bondi The contraction of gravitating spheres , 1964, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.

[30]  K. R. Karmarkar Gravitational metrics of spherical symmetry and class one , 1948 .

[31]  J. Oppenheimer,et al.  On Massive neutron cores , 1939 .

[32]  R. Tolman Static Solutions of Einstein's Field Equations for Spheres of Fluid , 1939 .

[33]  A. Eddington The mathematical theory of relativity , 1924 .

[34]  Delfino Codazzi,et al.  Sulle coordinate curvilinee d’ una superficie e dello spazio , 2007 .