Constraints on millicharged dark matter and axion-like particles from timing of radio waves
arXiv:1902.02695 · doi:10.1103/PhysRevD.100.063515
Abstract
We derive novel constraints on millicharged dark matter and ultralight axion-like particles using pulsar timing and fast radio burst observations. Millicharged dark matter affects the dispersion measure of the time of arrival of radio pulses in a way analogous to free electrons. Light pseudo-scalar dark matter, on the other hand, causes the polarization angle of radio signals to oscillate. We show that current and future data can set strong constraints in both cases. For dark matter particles of charge , these constraints are , for masses eV. For axion-like particles, the analysis of signals from pulsars yields constraints in the axial coupling of the order of . Both bounds scale as if the energy density of the components is a fraction of the total dark matter energy density . We do a detailed study of both effects using data from two samples of pulsars in the galaxy and in globular clusters, as well as data from FRB 121102 and PSR J04374715. We show that in both cases actual pulsar data constrain a new region of the parameter space for these models, and will improve with future pulsar-timing observations.
arXiv comment6 pages, 2 figures; v3: to appear on PRD
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