Effective mass of free neutrons in neutron star crust-Reference-Cited by-同舟云学术

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Effective mass of free neutrons in neutron star crust

Published:2006-07 Issue:3-4 Volume:773 Page:263-278
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Chamel Nicolas

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference46 articles.

1. Neutron star crusts;Haensel,2001

2. Spin up in neutron stars: The future of the Vela pulsar;Baym;Nature,1969

3. Three velocity hydrodynamics of superfluid solutions;Andreev;Sov. Phys. JETP,1976

4. Effect of entrainment on stress and pulsar glitches in stratified neutron star crust;Chamel;Mon. Not. R. Astron. Soc.,2006

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1. Couplings of torsional and shear oscillations in a neutron star crust;Physical Review D;2024-07-23

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3. Superfluid extension of the self-consistent time-dependent band theory for neutron star matter: Anti-entrainment versus superfluid effects in the slab phase;Physical Review C;2024-06-17

4. Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. V. Improved parametrization of the nucleon density distributions;Physical Review C;2024-05-03

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