Uniformly rotating, axisymmetric and triaxial quark stars in general relativity

20 Dec 2017 Zhou Enping Tsokaros Antonios Rezzolla Luciano Xu Renxin Uryū Kōji

Quasi-equilibrium models of uniformly rotating axisymmetric and triaxial quark stars are computed in general relativistic gravity scenario. The Isenberg-Wilson-Mathews (IWM) formulation is employed and the Compact Object CALculator (COCAL) code is extended to treat rotating stars with finite surface density and new equations of state (EOSs)... (read more)

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Categories


  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • GENERAL RELATIVITY AND QUANTUM COSMOLOGY