Bogolubov–Hartree–Fock mean field theory for neutron stars and other systems with attractive interactions

DOI10.1063/1.3225565zbMath1248.81277OpenAlexW1972402468MaRDI QIDQ3583600

Volker Bach, Jürg Fröhlich, Lars-Erik Jonsson

Publication date: 17 August 2010

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

Full work available at URL: https://doi.org/10.1063/1.3225565

zbMATH Keywords

neutron starsgravitational constantHF calculations

Mathematics Subject Classification ID

Many-body theory; quantum Hall effect (81V70) Quantum equilibrium statistical mechanics (general) (82B10) Galactic and stellar structure (85A15) Molecular physics (81V55)

Related Items (7)

Translation-invariant quasi-free states for fermionic systems and the BCS approximation ⋮ Bogolubov-Hartree-Fock theory for strongly interacting fermions in the low density limit ⋮ Kinetic energy estimates for the accuracy of the time-dependent Hartree-Fock approximation with Coulomb interaction ⋮ On blowup for time-dependent generalized Hartree-Fock equations ⋮ Minimizers for the Hartree-Fock-Bogoliubov theory of neutron stars and white dwarfs ⋮ Blow-up profile of neutron stars in the Hartree-Fock-Bogoliubov theory ⋮ The gap equation for spin-polarized fermions

Cites Work

• Relativistic stability of matter. I
• The Chandrasekhar theory of stellar collapse as the limit quantum mechanics
• Error bound for the Hartree-Fock energy of atoms and molecules
• General decomposition of radial functions on \(\mathbb R^n\) and applications to \(N\)-body quantum systems
• Generalized Hartree-Fock theory and the Hubbard model
• Boson stars as solitary waves
• Dynamical collapse of white dwarfs in Hartree- and Hartree-Fock theory
• Convex trace functions and the Wigner-Yanase-Dyson conjecture
• Effective dynamics for boson stars

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