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- W3100449657 abstract "Isolated millisecond pulsars (IMSPs) are a topic of academic contention. There are various models to explain their formation. We explore the formation of IMSP via quark novae (QN). During this formation process, low-mass X-ray binaries (LMXBs) are disrupted when the mass of the neutron star (NS) reaches 1.8 $rm M_odot$. Using population synthesis, this work estimates that the Galactic birthrate of QN-produced IMSPs lies between $sim 9.5times10^{-6}$ and $sim1.7times10^{-4}$ $rm yr^{-1}$. The uncertainties shown in our experiment model is due to the QN's kick velocity. Furthermore, our findings not only show that QN-produced IMSPs are statistically more significant than those produced by mergers, but also that millisecond pulsar binaries with a high eccentricity may originate from LMXBs that have been involved in, yet not disrupted by, a QN." @default.
- W3100449657 created "2020-11-23" @default.
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- W3100449657 date "2019-08-01" @default.
- W3100449657 modified "2023-10-18" @default.
- W3100449657 title "Quark novae: An alternative channel for the formation of isolated millisecond pulsars" @default.
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- W3100449657 doi "https://doi.org/10.1007/s12036-019-9596-z" @default.
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