A Study on Charged Neutron Star in
arXiv:1011.5362 · doi:10.1007/JHEP04(2011)111
Abstract
Motivated by an open question raised in recent times regarding the phase transition during the collapse of a neutron star to form a black hole and related stability issues, we have constructed charged neutron stars in and show that these stars become unstable at a particular value of their radius, regarded as the Chandrasekhar radius. We reproduced the calculations recently done in [20] in our charged star. The analysis shows that the non-Fermi liquid behavior found there in is still true in this higher dimensional case with the presence of Kosevich-Lifshitz oscillations.
20 pages, 6 figures