Nuclear-matter—quark-matter phase diagram with strangeness

1989 ◽  
Vol 40 (1) ◽  
pp. 157-164 ◽  
Author(s):  
H. W. Barz ◽  
B. L. Friman ◽  
J. Knoll ◽  
H. Schulz
1983 ◽  
Vol 313 (4) ◽  
pp. 369-370 ◽  
Author(s):  
H. Schulz ◽  
G. R�pke ◽  
M. Schmidt

2008 ◽  
Author(s):  
D. Zablocki ◽  
D. Blaschke ◽  
R. Anglani ◽  
Joseph Cugnon ◽  
Lansberg Jean-Philippe ◽  
...  

2013 ◽  
Vol 413 ◽  
pp. 012018 ◽  
Author(s):  
M Colonna ◽  
V Baran ◽  
M Di Toro ◽  
C Rizzo

2019 ◽  
Vol 204 ◽  
pp. 01023
Author(s):  
Alexey Stavinskiy

Opportunities to study unexplored domains of nuclear matter phase diagram with BM@N and SPD-NICA is discussed. Since the optimal initial energy range depends on the phase diagram domain, the subject and experimental methods for its study have a lot of opportunities both for the fixed target and collider experiments. Fixed target experiments provide an access to the laboratory study of nuclear matter with the unprecedented density as high as the one for the neutron star core and even larger. A specialised kinematic trigger for relativistic ion-ion collisions can be used for this study. On the other hand, the NICA collider energy range will provide unique opportunities to study interactions between multi-quark states. The article discusses the importance of experimental study of the diquark component of nuclear structure function and diquark-diquark interactions. It is important to develop neutron identification methods both for the fixed target and collider experiments.


2022 ◽  
Vol 258 ◽  
pp. 07004
Author(s):  
Niko Jokela

The holographic models for dense QCD matter work surprisingly well. A general implication seems that the deconfinement phase transition dictates the maximum mass of neutron stars. The nuclear matter phase turns out to be rather stiff which, if continuously merged with nuclear matter models based on effective field theories, leads to the conclusion that neutron stars do not have quark matter cores in the light of all current astrophysical data. We comment that as the perturbative QCD results are in stark contrast with strong coupling results, any future simulations of neutron star mergers incorporating corrections beyond ideal fluid should proceed cautiously. For this purpose, we provide a model which treats nuclear and quark matter phases in a unified framework at strong coupling.


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