Blow-up profile of neutron stars in the Chandrasekhar theory
DOI10.1063/1.5085277zbMath1423.85010arXiv1710.00538OpenAlexW3098908243WikidataQ127499198 ScholiaQ127499198MaRDI QIDQ5228046
Publication date: 8 August 2019
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1710.00538
Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) 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) Blow-up in context of PDEs (35B44)
Related Items (2)
Cites Work
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- The concentration-compactness principle in the calculus of variations. The locally compact case. I
- The Chandrasekhar theory of stellar collapse as the limit quantum mechanics
- The multiconfiguration equations for atoms and molecules: charge quantization and existence of solutions
- The semi-classical limit of large fermionic systems
- Ground states of pseudo-relativistic boson stars under the critical stellar mass
- On blow-up profile of ground states of boson stars with external potential
- Blow-up profile of rotating 2D focusing Bose gases
- On the mass concentration for Bose-Einstein condensates with attractive interactions
- Variational solutions of some nonlinear free boundary problems
- The Maximum Mass of Ideal White Dwarfs
- Existence and mass concentration of pseudo-relativistic Hartree equation
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