𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Neutron superfluidity and unusual nuclear shapes in neutron stars crusts

✍ Scribed by G. Lazzari; F. V. De Blasio

Publisher
Springer
Year
1994
Tongue
English
Weight
171 KB
Volume
350
Category
Article
ISSN
0939-7922

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Superfluidity in nuclear and neutron mat
Superfluidity in nuclear and neutron matter
✍ M. Baldo; E.E. Saperstein; S.V. Tolokonnikov πŸ“‚ Article πŸ“… 2005 πŸ› Elsevier Science 🌐 English βš– 234 KB

The di erent super uid states that can occur inside neutron stars are reviewed, both in the crust region and in the core. The role of correlations in determining the values of the pairing gaps is emphasized. Comparison is made on one hand with pairing in nuclear structure calculations in ordinary (t

Thermodynamic properties of nuclear β€œpas
Thermodynamic properties of nuclear β€œpasta” in neutron star crusts
✍ Gentaro Watanabe; Kei Iida; Katsuhiko Sato πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 232 KB

Equilibrium phase diagrams for neutron star matter at subnuclear densities are obtained at zero temperature. Spherical, rod-like and slab-like nuclei as well as spherical and rod-like nuclear bubbles are taken into account by using a compressible liquid-drop model. This model is designed to incorpor

Strongly Coupled Coulomb and Nuclear Pla
Strongly Coupled Coulomb and Nuclear Plasma in Inner Crusts of Neutron Stars
✍ D.G. Yakovlev; O.Y. Gnedin; A.Y. Potekhin πŸ“‚ Article πŸ“… 2001 πŸ› John Wiley and Sons 🌐 English βš– 138 KB πŸ‘ 2 views

Matter of subnuclear density in the inner crusts of neutron stars consists of neutron-rich atomic nuclei immersed in strongly degenerate relativistic gas of electrons and strongly nonideal liquid of neutrons. Thermodynamic and kinetic properties of this matter are greatly affected by Coulomb and nuc