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Search for strongly lensed counterpart images of binary black hole mergers in the first two LIGO observing runs

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arxiv 1912.05389 v3 pith:ZRT47O3M submitted 2019-12-11 gr-qc astro-ph.COastro-ph.HE

classification gr-qcastro-ph.COastro-ph.HE
keywords lensedeventsevidenceimagessearchadditionalbinaryblack
verification ladder T0 review T1 audit T2 compute T3 formal
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Strong gravitational lensing can produce multiple images of the same gravitational-wave signal, each arriving at different times and with different magnification. Previous work has explored if lensed pairs exist among the known high-significance events and found no evidence of this. However, the possibility remains that weaker counterparts of these events are present in the data, unrecovered by previous searches. We conduct a targeted search specifically looking for sub-threshold lensed images of known binary black hole (BBH) observations. We recover candidates matching three of the additional events first reported by Venumadhav et al. (2019), but find no evidence for additional BBH events. We also find no evidence that any of the Venumadhav et al. observations are lensed counterparts. We demonstrate how this type of counterpart search can constrain hypotheses about the overall source and lens populations and we rule out at very high confidence the extreme hypothesis that all heavy BBH detections are in fact lensed systems at high redshift with intrinsic masses < 15Msun.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Gravitational lensing of gravitational waves: universal characteristics of strongly lensed memory waveforms

    gr-qc 2025-10 conditional novelty 7.0 of 10

    Strongly lensed gravitational-wave memory waveforms acquire universal parity signatures—odd for type I/III images, even for type II—that can identify image type via a simple step-function approximation.

  2. The diffraction-lensing interpretation of GW231123 with astrophysical priors

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    GW231123 is better fit by a lower-mass merger diffracted by an isolated ~1000 M_sun lens, but astrophysical priors and a frequentist rate estimate make this lensing interpretation unlikely.

  3. Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Combining Strongly Lensed Gravitational Waves and Galaxy Surveys

    astro-ph.CO 2026-01 conditional novelty 6.0 of 10

    Simulated doubly lensed gravitational-wave events matched to galaxy surveys give a forecasted H0 precision of 0.42% with next-generation detectors.

  4. Better early than never: A new test for superluminal gravitational wave polarizations

    gr-qc 2025-01 conditional novelty 6.0 of 10

    A backward search in time from known gravitational wave detections could detect or constrain superluminal non-tensor polarizations, and the authors argue this is feasible with current detectors.

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