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Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens
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Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens
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We prose a new measurement strategy of the estimation of the lens mass, as well as the actual amplification, of the lens through the modulation patten of lensed gravitational wave signals alone. This can be done by measuring the frequency and amplitude ratio of peaks and valleys of the modulation pattern of CBC signals, known as "beat", which is a time domain phenomenon of strong lens effect.
Forward citations
Cited by 2 Pith papers
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Detection of Lensed Gravitational Waves in the Millihertz Band Using Frequency-Domain Lensing Feature Extraction Network
DCL-xLSTM neural network detects lensed GW events with AUC over 0.99 using training on PM and SIS lens models in the millihertz band.
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Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy
Self-lensing of a moving GW chirp by an orbiting black hole yields a curve width and interference beats that together give the orbital distance and the black hole mass.
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