2002
DOI: 10.1142/s0218271802002372
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Effect of Muons on the Phase Transition in Magnetized Proto-Neutron Star Matter

Abstract: We study the effect of inclusion of muons and the muon neutrinos on the phase transition from nuclear to quark matter in a magnetised proto-neutron star and compare our results with those obtained by us without the muons. We find that the inclusion of muons changes slightly the nuclear density at which transition occurs.However the dependence of this transition density on various chemical potentials, temperature and the magnetic field remains quantitatively the same.

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Cited by 2 publications
(2 citation statements)
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“…The rays, as mentioned earlier, are confined in the plane of bending as shown in figure 1. The power distribution of rays guided in the fibre with θ as the angle of the ray with the normal to the corecladding interface is given by [18] dP…”
Section: Transmitted Powermentioning
confidence: 99%
“…The rays, as mentioned earlier, are confined in the plane of bending as shown in figure 1. The power distribution of rays guided in the fibre with θ as the angle of the ray with the normal to the corecladding interface is given by [18] dP…”
Section: Transmitted Powermentioning
confidence: 99%
“…QMDTD model is a non-permanent quark confinement model [16] because it is based on the Friedberg-Lee model [21]. It has been used to study the thermodynamic properties of strangelets [15,17,18] and the photo strange star [22]. The detail of this model can be found in [15][16][17][18].…”
Section: Qmdtd Modelmentioning
confidence: 99%