D. Page, M. Prakash, J. M. Lattimer and A. W. Steiner, “Rapid Cooling of the Neutron Star in Cassiopeia A Triggered by Neutron Superfluidity in Dense Matter,” Physical Review Letters, Vol. 106, No. 8, 2011, pp. 081101-081104. doi:10.1103/PhysRevLett.106.081101

has been cited by the following article:

• TITLE: The Fractional Hydrogen Atom: A Paradigm for Astrophysical Phenomena

  AUTHORS: A. I. Arbab

  KEYWORDS: Hydrogen Atom; Fractional Quantum Number; Neutron Stars; White Dwarfs; Perfect Conductors

  JOURNAL NAME: Journal of Modern Physics, Vol.3 No.11, November 20, 2012

  ABSTRACT: We have found that fractional principal quantum numbers are permitted in hydrogen atom which yield the conditions for neutron and white dwarf stars evolution. The number densities of neutron and white dwarf stars reveal that these systems have the maximal conductivity of 1.37×1010Ω-1m-1. They are giant perfect conductors at very high temperature and magnetic field.