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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2004, Volume 80, Issue 8, Pages 595–599
(Mi jetpl2145)
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This article is cited in 9 scientific papers (total in 9 papers)
GRAVITY, ASTROPHYSICS
Effect of superfluidity on the structure of the inner crust of neutron stars
M. Baldoa, U. Lombardoab, È. E. Sapershteinc, S. V. Tolokonnikovc a National Institute of Nuclear Physics, Sezione di Catania, Italy
b Università degli Studi di Catania, Italy
c Russian Research Centre "Kurchatov Institute", Moscow
Abstract:
A self-consistent, completely quantum calculation of the structure of the inner crust of neutron stars is carried out in the Wigner-Seitz approximation with a realistic phenomenological nuclear energy functional, where pair correlations of neutrons and protons are included in the explicit form. It has been shown that the superfluidity of neutrons and protons affects the structure of the ground state of the crust.
Received: 04.08.2004 Revised: 13.09.2004
Citation:
M. Baldo, U. Lombardo, È. E. Sapershtein, S. V. Tolokonnikov, “Effect of superfluidity on the structure of the inner crust of neutron stars”, Pis'ma v Zh. Èksper. Teoret. Fiz., 80:8 (2004), 595–599; JETP Letters, 80:8 (2004), 523–526
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https://www.mathnet.ru/eng/jetpl2145 https://www.mathnet.ru/eng/jetpl/v80/i8/p595
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Abstract page: | 187 | Full-text PDF : | 61 | References: | 23 |
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