scholarly journals CHEMICAL EVOLUTION OF STRONGLY MAGNETIZED QUARK CORE IN A NEWBORN NEUTRON STAR

2001 ◽  
Vol 10 (01) ◽  
pp. 89-106 ◽  
Author(s):  
TANUSRI GHOSH ◽  
SOMENATH CHAKRABARTY

The chemical evolution of nascent quark matter core in a newborn compact neutron star is studied in presence of a strong magnetic field. The effective rate of strange quark production in degenerate quark matter core in presence of strong magnetic fields is obtained. The investigations show that in presence of strong magnetic field the quark matter core becomes energetically unstable and hence a first/higher order deconfinement transition to quark matter at the centre of a compact neutron star under such circumstances is absolutely impossible. The critical strength of magnetic field at the central core to make the system energetically unstable with respect to dense nuclear matter is found to be ~4.4 × 1013 G. This is the typical strength at which the Landau levels for electrons are populated. The other kind of phase transformations at such high density and ultra strong magnetic field environment are discussed.

2018 ◽  
Vol 171 ◽  
pp. 20001 ◽  
Author(s):  
V. S. Timóteo ◽  
R. L. S. Farias ◽  
S. S. Avancini ◽  
M. B. Pinto ◽  
W. R. Tavares

In this work, we improve our model by adding the strange quark and the Polyakov loop. We then build a thermo-magnetic dependence for the G and K couplings of the SU(3) PNJL model by fitting lattice QCD calculations for the average and the difference of u and d quark condensates under a strong magnetic field.


2014 ◽  
Vol 62 (6) ◽  
pp. 859-863
Author(s):  
Meng Ding ◽  
Xin-Jian Wen ◽  
Fu-Hu Liu ◽  
Bao-Chun Li

1994 ◽  
Vol 09 (39) ◽  
pp. 3611-3618 ◽  
Author(s):  
SOMENATH CHAKRABARTY ◽  
ASHOK GOYAL

Using conventional MIT bag model of confinement, the stability of bulk strange quark matter (SQM) in the presence of a strong magnetic field at zero temperature and zero pressure has been investigated. The binding energy of SQM increases in the presence of strong magnetic field greater than or of the order of some critical value at which the cyclotron lines begin to occur. At finite temperature the pressure dependence of the system has also been presented, which differs significantly from zero magnetic field case.


2001 ◽  
Vol 16 (13) ◽  
pp. 2435-2445 ◽  
Author(s):  
P. K. SAHU ◽  
S. K. PATRA

We study the effect of a strong magnetic field on interacting quark matter and apply the same to strange star. We find that interacting strange matter is less stable than noninteracting strange matter in the presence of a strong magnetic field. We then calculate strange star structure parameters such as mass and radius and find that the strange star is less compact for interacting quark matter than for free quark matter in presence of strong magnetic field. The maximum masses of strange stars are found to be within the recent observational limit.


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