We present a mean-field quantum calculation of the specific heat in the inner crust of neutron stars, taking into account the inhomogeneous character of the system, in which a lattice of neutron-rich nuclei coexists with a gas of unbound neutrons.
Superfluidity in the inner crust of neutron stars / E. Vigezzi, F. Barranco, R.A. Broglia, P.M. Pizzochero. - In: THE EUROPEAN PHYSICAL JOURNAL. A, HADRONS AND NUCLEI. - ISSN 1434-6001. - 20:1(2004 Apr), pp. 101-102. ((Intervento presentato al convegno International Conference on Nuclear Structure with Large Gamma-Arrays tenutosi a Legnaro nel 2002.
Superfluidity in the inner crust of neutron stars
R.A. BrogliaPenultimo
;P.M. PizzocheroUltimo
2004
Abstract
We present a mean-field quantum calculation of the specific heat in the inner crust of neutron stars, taking into account the inhomogeneous character of the system, in which a lattice of neutron-rich nuclei coexists with a gas of unbound neutrons.
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