A wide-parameter-space search of LIGO O3 data for continuous gravitational waves from unknown binary neutron stars finds no signals and sets new upper limits excluding ellipticities above 5.2e-8 for fast rotators within 100 pc.
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ZLK oscillations in Sgr A* triples enhance dual-line GW source formation rates by a factor of 5-10.
Resampling cross-correlation search of LIGO O4a data sets Sco X-1 continuous-wave upper limits below torque balance (independent of inclination) for 50–200 Hz.
Future CE+ET detectors may detect lensed BNS kilonovae at ~0.5/yr via pointed follow-up of known galaxy lenses, while lensed sGRBs and afterglows remain rare or undetectable with current-generation facilities.
citing papers explorer
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Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems
A wide-parameter-space search of LIGO O3 data for continuous gravitational waves from unknown binary neutron stars finds no signals and sets new upper limits excluding ellipticities above 5.2e-8 for fast rotators within 100 pc.
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An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai Effect in Triples Involving Sgr A*
ZLK oscillations in Sgr A* triples enhance dual-line GW source formation rates by a factor of 5-10.
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Sub-Torque-Balance Upper Limits on Continuous Gravitational Waves from Scorpius X-1
Resampling cross-correlation search of LIGO O4a data sets Sco X-1 continuous-wave upper limits below torque balance (independent of inclination) for 50–200 Hz.
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Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers
Future CE+ET detectors may detect lensed BNS kilonovae at ~0.5/yr via pointed follow-up of known galaxy lenses, while lensed sGRBs and afterglows remain rare or undetectable with current-generation facilities.