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- W2001043251 abstract "Fast radio bursts (FRBs) are an emerging class of short and bright radio transients whose sources remain enigmatic. Within the galactic center, the non-detection of pulsars within the inner $sim !10,{rm pc}$ has created a missing pulsar problem that has intensified with time. With all reserve, we advance the notion that the two problems could be linked by a common solution: the collapse of neutron stars (NS) due to capture and sedimentation of dark matter (DM) within their cores. Bramante & Linden (2014), Phys. Rev. Lett.~19, 191301 showed that certain DM properties allow for rapid NS collapse within the high DM density environments near galactic centers while permitting NS survival elsewhere. Each DM-induced collapse could generate an FRB as the NS magnetosphere is suddenly expelled. This scenario could explain several features of FRBs: their short time scales, large energies, locally produced scattering tails, and high event rates. We predict that FRBs are localized to galactic centers, and that our own galactic center harbors a large population of NS-mass ($Msim1.4 M_odot$) black holes. The DM-induced collapse scenario is intrinsically unlikely because it can only occur in a small region of allowable DM parameter space. However, if observed to occur, it would place tight constraints on DM properties." @default.
- W2001043251 created "2016-06-24" @default.
- W2001043251 creator A5042137136 @default.
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- W2001043251 date "2015-04-24" @default.
- W2001043251 modified "2023-09-30" @default.
- W2001043251 title "Dark matter-induced collapse of neutron stars: a possible link between fast radio bursts and the missing pulsar problem" @default.
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- W2001043251 doi "https://doi.org/10.1093/mnrasl/slv049" @default.
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