Numerical solutions of general-relativistic field equations for rapidly rotating neutron stars

DOI10.1007/BF03182869zbMath0894.35117OpenAlexW1988294105MaRDI QIDQ1368223

Chongming Xu, Xuejun Wu

Publication date: 28 September 1997

Published in: Science in China. Series A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf03182869

zbMATH Keywords

Einstein equationsrotational effectsNeugebauer's minimal surfacerapidly rotating relativistic neutron starsstructures of neutron stars

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) PDEs in connection with relativity and gravitational theory (35Q75) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Cites Work

• Einstein-Maxwell fields inside and outside rotating sources as minimal surfaces

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