Computing rotating polytropic models in the post-Newtonian approximation: The problem revisited
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics,Instrumentation
Reference23 articles.
1. The Post-Newtonian Equations of Hydrodynamics in General Relativity.
2. A Variational Principle Governing the Equilibrium of a Uniformly Rotating Configuration in the Post-Newtonian Approximation
3. The Equilibrium of Slowly Rotating Configurations in the Post-Newtonian Approximation: Corrections to Clairaut's Equation
4. Rapidly rotating polytropes in the post-Newtonian approximation to general relativity
5. A RUNGE–KUTTA–FEHLBERG CODE FOR THE COMPLEX PLANE: COMPARING WITH SIMILAR CODES BY APPLYING TO POLYTROPIC MODELS
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1. Rotating neutron stars in the first-order post-Newtonian approximation;Astronomy and Computing;2023-07
2. Polytropic wind solutions via the Complex Plane Strategy;Astronomy and Computing;2021-07
3. A numerical method for computing optimum radii of host stars and orbits of planets, with application to Kepler-11, Kepler-90, Kepler-215, HD 10180, HD 34445 and TRAPPIST-1;International Journal of Modern Physics C;2020-11-30
4. Nonradial oscillations of neutron stars and emitted gravitational waves: Computing strongly damped normal modes;International Journal of Modern Physics C;2017-05-07
5. Critical rotation of general-relativistic polytropic models simulating neutron stars: A post-Newtonian hybrid approximative scheme;New Astronomy;2015-08
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