scholarly journals Hot quark matter and (proto-) neutron stars

2019 ◽  
Vol 100 (1) ◽  
Author(s):  
Germán Malfatti ◽  
Milva G. Orsaria ◽  
Gustavo A. Contrera ◽  
Fridolin Weber ◽  
Ignacio F. Ranea-Sandoval
Keyword(s):  
Neutron Stars ◽  
Quark Matter ◽  
Hot Quark Matter

scholarly journals Light Front Approach to Correlations in Hot Quark Matter

2006 ◽  
Vol 27 (2-3) ◽  
pp. 379-382
Author(s):  
S. Strauß ◽  
M. Beyer ◽  
S. Mattiello
Keyword(s):  
Quark Matter ◽  
Light Front ◽  
Hot Quark Matter

Quark matter in neutron stars

2004 ◽  
Vol 19 (S1) ◽  
pp. 189-196
Author(s):  
Marcello Baldo
Keyword(s):  
Neutron Stars ◽  
Quark Matter

scholarly journals Converting neutron stars into strange stars: Instanton model

2014 ◽  
Vol 23 (09) ◽  
pp. 1450078
Author(s):  
Victor Ts. Gurovich ◽  
Leonid G. Fel
Keyword(s):  
Field Theory ◽  
Quantum Field Theory ◽  
Detonation Wave ◽  
Neutron Stars ◽  
Quark Matter ◽  
Quantum Fluctuation ◽  
The Self ◽  
Quantum Field ◽  
Spherical Detonation ◽  
Self Similar

We calculate the quasiclassical probability to emerge the quantum fluctuation which gives rise to the quark-matter drop with interface propagating as the self-similar spherical detonation wave (DN) in the ambient nuclear matter. For this purpose, we make use of instanton method which is known in the quantum field theory.

Phase transition to quark matter in neutron stars

1981 ◽  
Vol 98 (1-2) ◽  
pp. 140-144 ◽  
Author(s):  
Enrique Alvarez
Keyword(s):  
Phase Transition ◽  
Neutron Stars ◽  
Quark Matter

Quark Clustering and Chiral Symmetry Breaking in Nuclear Matter

2003 ◽  
Vol 18 (32) ◽  
pp. 2255-2264 ◽  
Author(s):  
O. A. Battistel ◽  
G. Krein
Keyword(s):  
Symmetry Breaking ◽  
Neutron Stars ◽  
Nuclear Matter ◽  
Chiral Symmetry ◽  
Quark Matter ◽  
Traditional Approach ◽  
Chiral Symmetry Breaking ◽  
Quark Condensate ◽  
Baryon Density ◽  
Hadronic Matter

Chiral symmetry breaking at finite baryon density is usually discussed in the context of quark matter, i.e. a system of deconfined quarks. Many systems like stable nuclei and neutron stars however have quarks confined within nucleons. In this paper we construct a Fermi sea of three-quark nucleon clusters and investigate the change of the quark condensate as a function of baryon density. We study the effect of quark clustering on the in-medium quark condensate and compare results with the traditional approach of modeling hadronic matter in terms of a Fermi sea of deconfined quarks.

Neutron stars' quark matter not so strange

Science ◽  
2018 ◽  
Vol 360 (6390) ◽  
pp. 697-697 ◽  
Author(s):  
Adrian Cho
Keyword(s):  
Neutron Stars ◽  
Quark Matter
Sign in / Sign up

Export Citation Format

Share Document