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- W3003451526 endingPage "100484" @default.
- W3003451526 startingPage "100484" @default.
- W3003451526 abstract "We 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." @default.
- W3003451526 created "2020-02-07" @default.
- W3003451526 creator A5010904609 @default.
- W3003451526 creator A5011035633 @default.
- W3003451526 creator A5076989248 @default.
- W3003451526 creator A5090182049 @default.
- W3003451526 creator A5091624758 @default.
- W3003451526 date "2020-05-01" @default.
- W3003451526 modified "2023-09-24" @default.
- W3003451526 title "On the change of old neutron star masses with galactocentric distance" @default.
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