Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
arxiv(2024)
摘要
We present the results of two searches for gravitational waves from the
post-merger remnants of the binary neutron star coalescence events GW170817 and
GW190425. The searches are fully coherent over 1800 s of data from the 2nd (for
GW170817) and 3rd (for GW190425) observing runs of the LIGO and Virgo
observatories. The searches compute the matched filter ℱ-statistic,
and use a piecewise model of the rapidly changing frequency evolution
appropriate for young neutron stars. No detection is claimed. The peak
root-sum-squared strain upper limit at 50% detection probability
(h_rss^50%) of both searches occurs at 1700 Hz and is estimated
at 1.64 × 10^-22 Hz^-1/2 for GW170817, and 1.0 ×
10^-22 Hz^-1/2 for GW190425. This is the first gravitational wave
search for a neutron star remnant of GW190425.
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