Possible existence of dark matter admixed pulsar

Abstract

In our previous study (Molla in Eur Phys J Plus 135:362, 2020), we have discussed the possible existence of the dark matter admixed pulsars, based on Singular Isothermal Sphere density profile, located in dwarf as well as in massive spiral galaxies. In this article, we use the Universal Rotational Curve dark matter density profile to get similar results for the pulsars in the Milky Way galaxy. These findings may be treated as a useful complement to the earlier findings. Hence, we may conclude that there is a high possibility of the existence of dark matter admixed pulsars in most of the galaxies.