Constraints on millicharged particles by neutron stars
arXiv:1509.07620 · doi:10.1103/PhysRevD.91.123513
Abstract
We have constrained the charge-mass () phase space of millicharged particles through the simulation of the rotational evolution of neutron stars, where an extra slow-down effect due to the accretions of millicharged dark matter particles is considered. For a canonical neutron star of and with typical magnetic field strength G, we have shown an upper limit of millicharged particles, which is compatible with recently experimental and observational bounds. Meanwhile, we have also explored the influences on the phase space of millicharged particles for different magnetic fields and dark matter density in the vicinity of the neutron star.
5 pages, 3 figures
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