Quantum size effects in the inner crust of neutron stars

F. Barranco; Ricardo Americo Broglia; E. Vigezzi

doi:10.1088/0954-3899/37/6/064023

Quantum size effects in the inner crust of neutron stars

F. Barranco, Ricardo Americo Broglia, E. Vigezzi

4 Citationer (Scopus)

Abstract

It is generally accepted that the inner crust of neutron stars is formed by a Coulomb lattice of nuclei immersed in a gas of quasi-free neutrons. We discuss the implications of the inhomogeneity of the crust and of nuclear shell effects on the linear response and on the superfluid properties of the system, as well as on the structure of vortices.

Originalsprog	Engelsk
Tidsskrift	Journal of Physics G: Nuclear and Particle Physics
Vol/bind	37
Udgave nummer	6
Sider (fra-til)	064023
ISSN	0954-3899
DOI	https://doi.org/10.1088/0954-3899/37/6/064023
Status	Udgivet - 9 apr. 2010

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10.1088/0954-3899/37/6/064023

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title = "Quantum size effects in the inner crust of neutron stars",

abstract = "It is generally accepted that the inner crust of neutron stars is formed by a Coulomb lattice of nuclei immersed in a gas of quasi-free neutrons. We discuss the implications of the inhomogeneity of the crust and of nuclear shell effects on the linear response and on the superfluid properties of the system, as well as on the structure of vortices.",

author = "F. Barranco and Broglia, {Ricardo Americo} and E. Vigezzi",

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T1 - Quantum size effects in the inner crust of neutron stars

AU - Barranco, F.

AU - Broglia, Ricardo Americo

AU - Vigezzi, E.

PY - 2010/4/9

Y1 - 2010/4/9

N2 - It is generally accepted that the inner crust of neutron stars is formed by a Coulomb lattice of nuclei immersed in a gas of quasi-free neutrons. We discuss the implications of the inhomogeneity of the crust and of nuclear shell effects on the linear response and on the superfluid properties of the system, as well as on the structure of vortices.

AB - It is generally accepted that the inner crust of neutron stars is formed by a Coulomb lattice of nuclei immersed in a gas of quasi-free neutrons. We discuss the implications of the inhomogeneity of the crust and of nuclear shell effects on the linear response and on the superfluid properties of the system, as well as on the structure of vortices.

U2 - 10.1088/0954-3899/37/6/064023

DO - 10.1088/0954-3899/37/6/064023

M3 - Journal article

SN - 0954-3899

VL - 37

SP - 064023

JO - Journal of Physics G: Nuclear and Particle Physics

JF - Journal of Physics G: Nuclear and Particle Physics

IS - 6

ER -

Quantum size effects in the inner crust of neutron stars

Abstract

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