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J. B. Hartle and K. S. Thorne, “Slowly Rotating Relativistic Stars—II. Models for Neutron Stars and Supemassive Stars,” The Astrophysical Journal, Vol. 153, 1968, pp. 807-834. doi:10.1086/149707

has been cited by the following article:

• TITLE: Computing Differentially Rotating Neutron Stars Obeying Realistic Equations of State by Using Hartle’s Perturbation Method

  AUTHORS: Anastasios Katelouzos, Vassilis Geroyannis

  KEYWORDS: Change in Mass; Differential Rotation; General-Relativistic Models; Neutron Stars; Numerical Methods; Realistic Equations of State

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.3 No.3, September 3, 2013

  ABSTRACT: In this paper, we use the well-known Hartle’s perturbation method in order to compute models of differentially rotating neutron stars obeying realistic equations of state. In our numerical treatment, we keep terms up to third order in the angular velocity. We present indicative numerical results for models satisfying a particular differential rotation law. We emphasize on computing the change in mass owing to this differential rotation law.