Browsing by Subject "General relativity"

Now showing items 1-5 of 5

    • A class of relativistic anisotropic charged stellar models in isotropic coordinates 

      Pant, Neeraj; Pradhan, Nirakar; Murad, Mohammad Hassan (© 2014, Springer Science+Business Media Dordrecht., 2014)
      In this present paper, we present a class of static, spherically symmetric charged anisotropic fluid models of super dense stars in isotropic coordinates by considering a particular type of metric potential, a specific ...

    • A class of super dense stars models using charged analogues of Hajj-Boutros type relativistic fluid solutions 

      Pant, Neeraj; Pradhan, Nirakar; Murad, Mohammad Hassan (© 2014, Springer Science+Business Media New York, 2014-10)
      We present a spherically symmetric solution of the general relativistic field equations in isotropic coordinates for perfect charged fluid, compatible with a super dense star modeling. The solution is well behaved for all ...

    • Relativistic anisotropic stellar models with Tolman VII spacetime 

      Bhar, Piyali; Murad, Mohammad Hassan; Pant, Neeraj (© 2015, Springer Science+Business Media Dordrecht, 2015-09)
      In this paper we have studied the behavior of static spherically symmetric relativistic objects with locally anisotropic matter distribution considering the Tolman VII form for the gravitational potential grr in curvature ...

    • Relativistic compact anisotropic charged stellar models with Chaplygin equation of state 

      Bhar, Piyali; Murad, Mohammad Hassan (© Springer Science+Business Media Dordrecht 2016, 2016)
      This paper presents a new model of static spherically symmetric relativistic charged stellar objects with locally anisotropic matter distribution together with the Chaplygin equation of state. The interior spacetime has ...

    • Some analytical models of anisotropic strange stars 

      Murad, Mohammad Hassan (© Springer Science+Business Media Dordrecht 2015, 2016)
      Over the years of the concept of local isotropy has become a too stringent condition in modeling relativistic self-gravitating objects. Taking local anisotropy into consideration, in this work, some analytical models of ...