The Bethe homework problem for hot neutron matter in the static fluctuation approximation
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Publication:1008141
DOI10.1007/S10773-008-9666-5zbMath1160.85305OpenAlexW2053413099MaRDI QIDQ1008141
M. K. Al-Sugheir, N. M. Ghulam, Humam B. Ghassib
Publication date: 24 March 2009
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-008-9666-5
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)
Cites Work
- Hot nuclear matter in asymmetry chiral sigma model
- Normal liquid helium-3 in the static fluctuation approximation
- Renormalization group approach to neutron matter: Quasiparticle interactions, superfluid gaps and the equation of state
- Spin-polarized \(^{3}\)He-HeII mixtures in the static fluctuation approximation
- Liquid helium-4 in the static fluctuation approximation
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