https://doi.org/10.1140/epjp/s13360-020-00650-y
Regular Article
Possible existence of dark matter admixed pulsar
1
Department of Physics, Aliah University, IIA/27, New Town, 700 160, Kolkata, India
2
Department of Physics, New Alipore College, L Block, New Alipore, 700053, Kolkata, India
Received:
19
June
2020
Accepted:
29
July
2020
Published online:
8
August
2020
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.
© Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2020
