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- W2071597816 abstract "White dwarf-neutron star binaries generate detectable gravitational radiation. We construct Newtonian equilibrium models of corotational white dwarf-neutron star (WDNS) binaries in circular orbit and find that these models terminate at the Roche limit. At this point the binary will undergo either stable mass transfer (SMT) and evolve on a secular time scale, or unstable mass transfer (UMT), which results in the tidal disruption of the WD. The path a given binary will follow depends primarily on its mass ratio. We analyze the fate of known WDNS binaries and use population synthesis results to estimate the number of LISA-resolved galactic binaries that will undergo either SMT or UMT. We model the quasistationary SMT epoch by solving a set of simple ordinary differential equations and compute the corresponding gravitational waveforms. Finally, we discuss in general terms the possible fate of binaries that undergo UMT and construct approximate Newtonian equilibrium configurations of merged WDNS remnants. We use these configurations to assess plausible outcomes of our future, fully relativistic simulations of these systems. If sufficient WD debris lands on the NS, the remnant may collapse, whereby the gravitational waves from the inspiral, merger, and collapse phases will sweep from LISA through LIGO frequency bands. If the debris forms a disk about the NS, it may fragment and form planets." @default.
- W2071597816 created "2016-06-24" @default.
- W2071597816 creator A5034590981 @default.
- W2071597816 creator A5058066370 @default.
- W2071597816 creator A5081703282 @default.
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- W2071597816 date "2009-07-07" @default.
- W2071597816 modified "2023-10-17" @default.
- W2071597816 title "Merger of white dwarf-neutron star binaries: Prelude to hydrodynamic simulations in general relativity" @default.
- W2071597816 cites W1964427975 @default.
- W2071597816 cites W1967911913 @default.
- W2071597816 cites W1971068715 @default.
- W2071597816 cites W1971332238 @default.
- W2071597816 cites W1971424001 @default.
- W2071597816 cites W1981759665 @default.
- W2071597816 cites W1986992319 @default.
- W2071597816 cites W1989170879 @default.
- W2071597816 cites W1989996162 @default.
- W2071597816 cites W1994336951 @default.
- W2071597816 cites W1994477072 @default.
- W2071597816 cites W1996902696 @default.
- W2071597816 cites W1997367763 @default.
- W2071597816 cites W2003000933 @default.
- W2071597816 cites W2006290403 @default.
- W2071597816 cites W2007884385 @default.
- W2071597816 cites W2011659854 @default.
- W2071597816 cites W2012201695 @default.
- W2071597816 cites W2013280355 @default.
- W2071597816 cites W2014874393 @default.
- W2071597816 cites W2015034160 @default.
- W2071597816 cites W2016260496 @default.
- W2071597816 cites W2016911950 @default.
- W2071597816 cites W2023148293 @default.
- W2071597816 cites W2024411983 @default.
- W2071597816 cites W2024680894 @default.
- W2071597816 cites W2031388907 @default.
- W2071597816 cites W2037771611 @default.
- W2071597816 cites W2042607720 @default.
- W2071597816 cites W2043601233 @default.
- W2071597816 cites W2043702737 @default.
- W2071597816 cites W2047735585 @default.
- W2071597816 cites W2049712818 @default.
- W2071597816 cites W2050470132 @default.
- W2071597816 cites W2056528333 @default.
- W2071597816 cites W2056875281 @default.
- W2071597816 cites W2056926899 @default.
- W2071597816 cites W2057866251 @default.
- W2071597816 cites W2065210329 @default.
- W2071597816 cites W2067369325 @default.
- W2071597816 cites W2067618271 @default.
- W2071597816 cites W2074240506 @default.
- W2071597816 cites W2076313694 @default.
- W2071597816 cites W2078124225 @default.
- W2071597816 cites W2079104852 @default.
- W2071597816 cites W2081050835 @default.
- W2071597816 cites W2081334450 @default.
- W2071597816 cites W2082839315 @default.
- W2071597816 cites W2085335800 @default.
- W2071597816 cites W2089551452 @default.
- W2071597816 cites W2104943477 @default.
- W2071597816 cites W2105539313 @default.
- W2071597816 cites W2105635519 @default.
- W2071597816 cites W2115834307 @default.
- W2071597816 cites W2118461079 @default.
- W2071597816 cites W2123552795 @default.
- W2071597816 cites W2126106500 @default.
- W2071597816 cites W2132755951 @default.
- W2071597816 cites W2133684002 @default.
- W2071597816 cites W2134255669 @default.
- W2071597816 cites W2137702713 @default.
- W2071597816 cites W2141103204 @default.
- W2071597816 cites W2148657506 @default.
- W2071597816 cites W2149573451 @default.
- W2071597816 cites W2150507559 @default.
- W2071597816 cites W2154945574 @default.
- W2071597816 cites W2157017092 @default.
- W2071597816 cites W2169835170 @default.
- W2071597816 cites W2498126760 @default.
- W2071597816 cites W3098598948 @default.
- W2071597816 cites W3099116106 @default.
- W2071597816 cites W3099742379 @default.
- W2071597816 cites W3100059635 @default.
- W2071597816 cites W3103211142 @default.
- W2071597816 cites W3103497811 @default.
- W2071597816 cites W3103875883 @default.
- W2071597816 cites W3104089750 @default.
- W2071597816 cites W3105024626 @default.
- W2071597816 cites W3105526734 @default.
- W2071597816 cites W3121253124 @default.
- W2071597816 cites W3123716683 @default.
- W2071597816 cites W4242337283 @default.
- W2071597816 doi "https://doi.org/10.1103/physrevd.80.024006" @default.
- W2071597816 hasPublicationYear "2009" @default.
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