Comparing Models of Rapidly Rotating Relativistic Stars Constructed by Two Numerical Methods We present the first direct comparison of codes based on two different numerical methods for constructing rapidly rotating relativistic stars. A code based on the Komatsu-Eriguchi-Hachisu (KEH) method (Komatsu et al. 1989), written by Stergioulas, is compared to the Butterworth-I

📄 Comparing Models of Rapidly Rotating Relativistic Stars Constructed b…

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Stergioulas, Nikolaos et al. (1995) · The Astrophysical Journal
Reads: 100 · Citations: 521
DOI: 10.1086/175605

#Astronomy #Astrophysics #ComputationalAstrophysics #ComputerizedSimulation #NumericalAnalysis

A Comparison of Numerical Methods for the Study of Star Cluster Dynamics We compare the results of three different numerical methods for computing the evolution of a spherical star cluster from a given initial state, under the influence of internal relaxation: the N-body integration, the Monte Carlo method, and the fluid-dynamical approach. The genera

📄 A Comparison of Numerical Methods for the Study of Star Cluster Dynam…

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Aarseth, S. J. et al. (1974) · Astronomy and Astrophysics
Reads: 5 · Citations: 254
DOI: N/A

#Astronomy #Astrophysics #AstronomicalModels #ComputerizedSimulation #NumericalAnalysis