Dark matter seeding and the kinematics and rotation of neutron stars

Details Dark matter seeding and the kinematics and rotation of neutron stars Dark matter seeding and the kinematics and rotation of neutron stars

May 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012phlb..711....6p&link_type=abstract

Physics Letters B, Volume 711, Issue 1, p. 6-9.

Physics

Scientific paper

Self-annihilation of dark matter accreted from the galactic halo in the inner regions of neutron stars may significantly affect their kinematical properties, namely velocity kicks and rotation patterns. We find that if a stable long-lived single or multiple strangelet off-center seed forms leading to an asymmetric ejection of matter and radiation, there is a significant modification in linear and angular momentum observables of the star.

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