2D simulation of NS-to-HS combustion via central shock-initiated deconfining front yields GW signals of amplitude 10^{-22} lasting tens of microseconds with high-frequency spectral peaks.
The star merger has revealed itself in the form of GW, neutrino production and also in other various spectra of electromagnetic range
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Gravitational waves from phase transition of NS to QS
2D simulation of NS-to-HS combustion via central shock-initiated deconfining front yields GW signals of amplitude 10^{-22} lasting tens of microseconds with high-frequency spectral peaks.