Rapidly rotating stars

DOI10.1007/s00220-019-03414-7zbMath1419.83017arXiv1907.13155OpenAlexW3099491185MaRDI QIDQ2415341

Walter A. Strauss, Yilun Wu

Publication date: 21 May 2019

Published in: Communications in Mathematical Physics, Nonlinearity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1907.13155

zbMATH Keywords

Euler-Poisson equationsequation of stateEuler-Poisson systemglobal continuationrotating starrapid rotationwhite dwarf star

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) PDEs in connection with astronomy and astrophysics (35Q85)

Related Items (11)

Continua of steadily rotating stars ⋮ Global existence for the \(N\) body Euler-Poisson system ⋮ On uniformly rotating binary stars and galaxies ⋮ Rapidly rotating stars ⋮ Global continuation of a Vlasov model of rotating galaxies ⋮ Stability of rotating gaseous stars ⋮ Existence of Rotating Stars with Variable Entropy ⋮ The uniqueness of the slowly uniformly rotating supermassive star for a given total mass ⋮ Global finite-energy solutions of the compressible Euler-Poisson equations for general pressure laws with large initial data of spherical symmetry ⋮ Global continuation and the theory of rotating stars ⋮ Variational rotating solutions to non-isentropic Euler-Poisson equations with prescribed total mass

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