Global continuation and the theory of rotating stars
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Publication:4972701
DOI10.1090/qam/1550zbMath1427.35285OpenAlexW2964153533WikidataQ127480099 ScholiaQ127480099MaRDI QIDQ4972701
Publication date: 26 November 2019
Published in: Quarterly of Applied Mathematics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1090/qam/1550
Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar dynamics (85A05) Euler equations (35Q31) PDEs in connection with astronomy and astrophysics (35Q85)
Related Items
Continua of steadily rotating stars, Existence of Rotating Stars with Variable Entropy, The uniqueness of the slowly uniformly rotating supermassive star for a given total mass
Cites Work
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- On rotating star solutions to the non-isentropic Euler-Poisson equations
- Existence and nonlinear stability of rotating star solutions of the compressible Euler-Poisson equations
- Symmetry and related properties via the maximum principle
- Asymptotic estimates for an axisymmetric rotating fluid
- The shape of axisymmetric rotating fluid
- A priori estimates and existence of positive solutions of semilinear elliptic equations
- Existence and dimensions of a rotating white dwarf
- On uniformly rotating stars
- The implicit function theorem and the global methods of cohomology
- On diameters of uniformly rotating stars
- Bifurcation theory. An introduction with applications of PDEs
- Untersuchungen über die Gleichgewichtsfiguren rotierender Flüssigkeiten, deren Teilchen einander nach dem Newtonschen Gesetze anziehen. III. Abh. Nichthomogene Flüssigkeiten. Figur der Erde
- On slowly rotating axisymmetric solutions of the Euler-Poisson equations
- Dual variational methods in critical point theory and applications
- Rapidly rotating stars
- Some global results for nonlinear eigenvalue problems
- Variational solutions of some nonlinear free boundary problems
- Uniqueness and nonuniqueness for positive radial solutions of Δu + f(u, r) = 0
- Steady States of Rotating Stars and Galaxies
- Ellipsoidal figures of equilibrium—an historical account
- Existence of rotating planet solutions to the Euler-Poisson equations with an inner hard core
