Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state-Reference-Cited by-同舟云学术

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Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state

Published:2016-04-12 Issue:8 Volume:93 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Sourie Aurélien,Oertel Micaela,Novak Jérôme

Funder

European Cooperation in Science and Technology

SN2NS

Observatoire de Paris

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.93.083004/fulltext

Reference78 articles.

1. Neutron Stars 1

2. Superfluidity and the moments of inertia of nuclei

3. Pairing in nuclear systems: from neutron stars to finite nuclei

4. Thermal relaxation in young neutron stars

5. Pulsar glitches and restlessness as a hard superfluidity phenomenon

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1. Gapless superfluidity in neutron stars: Normal-fluid fraction;Physical Review C;2023-10-10

2. Diffusion in superfluid Fermi mixtures: General formalism;Physical Review C;2023-08-30

3. Symmetry evolution for the imperfect fluid under perturbations;International Journal of Geometric Methods in Modern Physics;2022-07-15

4. Extending Israel and Stewart hydrodynamics to relativistic superfluids via Carter’s multifluid approach;Physical Review D;2022-02-16

5. New symmetry in higher curvature spacetimes;Europhysics Letters;2022-01-01

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