Hot third family of compact stars and the possibility of core-collapse supernova explosions-Reference-Cited by-同舟云学术

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Hot third family of compact stars and the possibility of core-collapse supernova explosions

Published:2016-11-07 Issue:10 Volume:94 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Hempel Matthias,Heinimann Oliver,Yudin Andrey,Iosilevskiy Igor,Liebendörfer Matthias,Thielemann Friedrich-Karl

Funder

National Science Foundation

European Research Council

Seventh Framework Programme

European Cooperation in Science and Technology

Russian Scientific Fund

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.94.103001/fulltext

Reference44 articles.

1. Can phase transitions of superdense matter strengthen supernova explosions?

2. The QCD phase transition and supernova core collapse

3. Finite temperature quark matter and supernova explosion

4. Effects of QCD phase transition on gravitational radiation from two-dimensional collapse and bounce of massive stars

5. Evidence for strange matter in supernovae?

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2. Which first order phase transitions to quark matter are possible in neutron stars?;Physical Review D;2024-03-28

3. Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations;Physical Review D;2024-02-28

4. Thermal effects on the baryon–quark phase transition in hot hybrid neutron stars: a statistical mean-field baryonic model with the standard NJL model for deconfined quarks;The European Physical Journal Plus;2023-11-02

5. Detailed analysis of the special points on M−R solutions of hybrid/twin stars;Physical Review D;2022-10-14

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