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Updated: Jul 23, 2025

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Cosmography Using Strongly Lensed Gravitational Waves from Binary Black Holes
Souvik Jana1, Shasvath J Kapadia1,2, Tejaswi Venumadhav1,3
1International Centre for Theoretical Science, Tata Institute of Fundamental Research, Bangalore 560089, India.
Abstract:
Third generation gravitational wave (GW) detectors are expected to detect millions of binary black hole (BBH) mergers during their operation period. A small fraction of them (∼1%) will be strongly lensed by intervening galaxies and clusters, producing multiple observable copies of the GW signals. The expected number of lensed events and the distribution of the time delay between lensed images depend on the cosmology. We develop a Bayesian analysis method for estimating cosmological parameters from the detected number of lensed events and their time delay distribution. The expected constraints are comparable to that obtained from other cosmological measurements, but probing a different redshift regime (z∼10) that is not explored by other probes.
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