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• W4379051567 endingPage "95" @default.
• W4379051567 startingPage "95" @default.
• W4379051567 abstract "Compact-object binaries including a white dwarf component are unique among gravitational-wave sources because their evolution is governed not just by general relativity and tides, but also by mass transfer. While the black hole and neutron star binaries observed with ground-based gravitational-wave detectors are driven to inspiral due to the emission of gravitational radiation--manifesting as a chirp-like gravitational-wave signal--the astrophysical processes at work in double white dwarf (DWD) systems can cause the inspiral to stall and even reverse into an outspiral. The dynamics of the DWD outspiral thus encode information about tides, which tell us about the behaviour of electron-degenerate matter. We carry out a population study to determine the effect of the strength of tides on the distributions of the DWD binary parameters that the Laser Interferometer Space Antenna (LISA) will be able to constrain. We find that the strength of tidal coupling parameterized via the tidal synchronization timescale at the onset of mass transfer affects the distribution of gravitational-wave frequencies and frequency derivatives for detectably mass-transferring DWD systems. Using a hierarchical Bayesian framework informed by binary population synthesis simulations, we demonstrate how this parameter can be inferred using LISA observations. By measuring the population properties of DWDs, LISA will be able to probe the behavior of electron-degenerate matter." @default.
• W4379051567 created "2023-06-02" @default.
• W4379051567 creator A5050742735 @default.
• W4379051567 creator A5082607890 @default.
• W4379051567 creator A5088976307 @default.
• W4379051567 date "2023-06-01" @default.
• W4379051567 modified "2023-10-01" @default.
• W4379051567 title "Probing the Efficiency of Tidal Synchronization in Outspiralling Double White Dwarf Binaries with LISA" @default.
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