Testing general relativity with amplitudes of subdominant gravitational-wave modes
Ish Gupta, Purnima Narayan, Lionel London, Shubhanshu Tiwari, Bangalore Sathyaprakash
gr-qc, astro-ph.CO, hep-th
Submitted: 2026-07-15
Updated: 2026-08-20
Comments: Accepted version. 12 pages + Appendix, 17 figures
Journal ref: Phys. Rev. D 114, 044050 (2026)
DOI: 10.1103/wg2q-gync
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
- Advanced LIGO
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Overview of KAGRA: Detector design and construction history
- Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
- Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
- Advanced LIGO detector performance in the fourth observing run
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Tests of general relativity with GW150914
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- Tests of General Relativity with GWTC-3
- GWTC-4.0: Tests of General Relativity. I. Overview and General Tests
- GWTC-4.0: Tests of General Relativity. II. Parameterized Tests
- GWTC-4.0: Tests of General Relativity. III. Tests of the Remnants
- Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
- Detection and Parameter Estimation of Gravitational Waves from Compact Binary Inspirals with Analytical Double-Precessing Templates
- Unveiling the spectrum of inspiralling binary black holes
- Inferring small neutron star spins with neutron star-black hole mergers
- TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries
- Tests of General Relativity with GW170817
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