New Insight into Magnetic Monopoles in Astrophysical Application

Abstract

In this paper, we mainly review our previous works on a magnetic-monopole toy model, in which the energy resources come from nucleon decay catalyzed by magnetic monopoles. Utilizing this unified model, we have explained various supernova explosion and gamma ray bursts, extra heat at the centers of white dwarfs and the earth. The unusually strong radial magnetic field near the Galactic Center (GC) is quantitatively consistent with our theoretical prediction in 2001. It may be strong astronomical observational evidence of the presence of magnetic monopoles predicted by particle physics. Using the masses of 100,000 quasars observed by SLOAN with various red-shifts due to the black hole, according to the popular black hole accretion model, we estimate the initial mass of quasars when they born in early universe. It is found that most low-red-shifting quasars have an initial mass of negative or very small values. However, based on our proposed model of super massive stars with magnetic monopoles, the statistical distribution of the initial mass for these quasars should be a reasonable Gaussian distribution. This suggests that the modern model of black holes in the quasars and active galactic nucleus may be unreasonable.