scholarly journals Quark matter and quark stars in strong magnetic fields at finite temperature within the confined-isospin-density-dependent mass model

2018 ◽  
Vol 778 ◽  
pp. 447-453 ◽  
Author(s):  
Peng-Cheng Chu ◽  
Xiao-Hua Li ◽  
Hong-Yang Ma ◽  
Bin Wang ◽  
Yu-Min Dong ◽  
...  
2020 ◽  
Vol 47 (8) ◽  
pp. 085201
Author(s):  
Peng-Cheng Chu ◽  
Yi Zhou ◽  
Chang Chen ◽  
Xiao-Hua Li ◽  
Hong-Yang Ma

2011 ◽  
Vol 83 (6) ◽  
Author(s):  
S. S. Avancini ◽  
D. P. Menezes ◽  
C. Providência

2011 ◽  
Vol 20 (supp02) ◽  
pp. 93-99
Author(s):  
DÉBORA PERES MENEZES ◽  
SIDNEY SANTOS AVANCINI ◽  
CONSTANÇA PROVIDÊNCIA

Quark matter at finite temperature and subject to strong magnetic fields is possibly present in the early stages of heavy ion collisions and in the interior of protoneutron stars. We use the mean field approximation to investigate this type of quark matter described by the Nambu–Jona-Lasinio model. The effect of the magnetic field on the effective quark masses and chemical potentials is only felt for quite strong magnetic fields, above 5 × 1018 G , with larger effects for the lower densities. Spin polarizations are more sensitive to weaker magnetic fields and are larger for lower temperatures and lower densities.


2021 ◽  
Vol 104 (4) ◽  
Author(s):  
Peng-Cheng Chu ◽  
Xiao-Hua Li ◽  
He Liu ◽  
Jia-Wei Zhang

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