scholarly journals Strange quark matter in strong magnetic fields within a confining model

2013 ◽  
Vol 88 (2) ◽  
Author(s):  
Monika Sinha ◽  
Xu-Guang Huang ◽  
Armen Sedrakian
2018 ◽  
Vol 172 ◽  
pp. 07002
Author(s):  
Daryel Manreza Paret ◽  
A. Perez Martinez ◽  
Alejandro. Ayala ◽  
G. Piccinelli ◽  
A. Sanchez

We study a model that explain neutron stars velocities due to the anisotropic emission of neutrinos. Strong magnetic fields present in neutron stars are the source of the anisotropy in the system. To compute the velocity of the neutron star we model its core as composed by strange quark matter and analice the properties of a magnetized quark gas at finite temperature and density. Specifically we have obtained the electron polarization and the specific heat of magnetized fermions as a functions of the temperature, chemical potential and magnetic field which allow us to study the velocity of the neutron star as a function of these parameters.


2019 ◽  
Vol 22 (4) ◽  
pp. 311-317
Author(s):  
Hidezumi Terazawa

New forms of matter such as super-hypernuclei (strange quark matter) and superhypernuclear stars (strange quark stars) as candidates for dark matter are discussed in some detail, based on the so-called "Bodmer–Terazawa–Witten hypothesis" assuming that they are stable absolutely or quasi-stable (decaying only weakly).


1997 ◽  
Vol 56 (1) ◽  
pp. 491-496 ◽  
Author(s):  
G. Peng ◽  
P. Ning ◽  
H. Chiang

1999 ◽  
Vol 59 (4) ◽  
pp. R1829-R1833 ◽  
Author(s):  
T. A. Armstrong ◽  
K. Barish ◽  
S. J. Bennett ◽  
A. Chikanian ◽  
S. D. Coe ◽  
...  

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