On the change of old neutron star masses with galactocentric distance

Publication date: Available online 30 January 2020Source: Physics of the Dark UniverseAuthor(s): Antonino Del Popolo, Maksym Deliyergiyev, Morgan Le Delliou, Laura Tolos, Fiorella BurgioAbstractWe show that the pulsar mass depends on the environment, and that it decreases going towards the center of the Milky Way. This is due to two combined effects, the capture and accumulation of self-interacting, non-annihilating dark matter by pulsars, and the increase of the dark matter density going towards the galactic center. We show that mass decrease depends both on the density profile of dark matter, steeper profiles producing a faster and larger decrease of the pulsar mass, and on the strength of self-interaction. Once future observations will provide the pulsar mass in a dark matter rich environment, close to the galactic center, the present result will be able to put constraints on the characteristics of our Galaxy halo dark matter profile, on the nature of dark matter, namely on its annihilating or non-annihilating nature, on its strength of self-interaction, and on the particle mass.

Source: Physics of the Dark Universe - January 31, 2020 Category: Physics Source Type: research