Astrophysical implications of equation of state for hadron-quark mixed phase: Compact stars and stellar collapses-Reference-Cited by-同舟云学术

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Astrophysical implications of equation of state for hadron-quark mixed phase: Compact stars and stellar collapses

Published:2008-05-16 Issue:10 Volume:77 Page:
ISSN:1550-7998
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Nakazato Ken’ichiro,Sumiyoshi Kohsuke,Yamada Shoichi

Publisher

American Physical Society (APS)

Subject

Nuclear and High Energy Physics

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.77.103006/fulltext

Reference51 articles.

1. Hydrostatic Equilibrium of Hypothetical Quark Stars

2. Cosmic separation of phases

3. Strange quark matter and compact stars

4. First-order phase transitions with more than one conserved charge: Consequences for neutron stars

5. Finite temperature quark matter and supernova explosion

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1. Exploring thermal effects of the hadron-quark matter transition in neutron star mergers;Physical Review D;2023-09-28

2. Impact of pions on binary neutron star mergers;Physical Review D;2023-07-26

3. Nuclei in core-collapse supernovae engine;Progress in Particle and Nuclear Physics;2023-03

4. Equation of State in Neutron Stars and Supernovae;Handbook of Nuclear Physics;2023

5. Equation of State in Neutron Stars and Supernovae;Handbook of Nuclear Physics;2023

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