On slowly rotating axisymmetric solutions of the Einstein-Euler equations

DOI10.1063/1.5026133zbMath1402.83029arXiv1705.07392OpenAlexW2617439669WikidataQ125890606 ScholiaQ125890606MaRDI QIDQ4556636

Tetu Makino

Publication date: 16 November 2018

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1705.07392

zbMATH Keywords

Euler-Poisson equationsEinstein-Euler equationsslowly rotating axisymmetric solutionsuniformly rotating gaseous stars

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (2)

The relativistic Euler equations with a physical vacuum boundary: Hadamard local well-posedness, rough solutions, and continuation criterion ⋮ On the axisymmetric metric generated by a rotating perfect fluid with the vacuum boundary

Cites Work

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