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This paper uses population synthesis to investigate the possible origin ofisolated millisecond pulsars (IMSPs) as born from the coalescence of a neutronstar (NS) and a white dwarf (WD). Results show that the galactic birth - rateof IMSPs is likely to lie between $5.8\times10^{-5}$ $\rm yr^{-1}$ and$2.0\times10^{-4}$ $\rm yr^{-1}$, depending on critical variables, such as thestability of mass transfer via the Roche lobe and the value of kick velocity.In addition to this, this paper estimates that the solar mass of IMSPs canrange from $1.5$ and 2.0 $M_{\odot}$, making them more massive than other'normal' pulsars. Finally, the majority of IMSPs in our simulations have spinperiods ranging from several to 20 milliseconds, which is consistent withprevious observations.

On Isolated Millisecond Pulsars Formed by the Coalescence of Neutron Stars and Massive White Dwarfs