Gravitational Wave Interference via Gravitational Lensing: Measurements of Luminosity Distance, Lens Mass, and Cosmological Parameters
arXiv:1911.02798 · doi:10.1103/PhysRevD.101.064011
Abstract
The gravitational lensing of gravitational waves might cause beat patterns detectable by interferometers. The feature of this kind of signal is the existence of the beat pattern in the early inspiral phase, followed by a seemingly randomly changing profile. After the strain peaks for the first time, the signal takes the usual waveform and the strain peaks for the second time. Once this signal is detected, the actual magnification factors can be obtained, so the true luminosity distance of the binary system is known. If the lens can be described by a point mass or a singular isothermal sphere, the functional forms of the time delay and the magnification factors are simple enough, so we can infer the mass of the lens or the cosmological parameters.
9 pages, 4 figures
References in corpus (21)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Confrontation between General Relativity and Experiment
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Implementing a search for aligned-spin neutron star -- black hole systems with advanced ground based gravitational wave detectors
- Probing non-tensorial polarizations of stochastic gravitational-wave backgrounds with ground-based laser interferometers
- Search for gravitational lensing signatures in LIGO-Virgo binary black hole events
- Multiband gravitational-wave event rates and stellar physics
- Observational signatures of microlensing in gravitational waves at LIGO/Virgo frequencies
- Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
- Strong lensing of gravitational waves as seen by LISA
- The effect of matter structure on the gravitational waveform
- Frequency response of space-based interferometric gravitational-wave detectors
- The wave nature of continuous gravitational waves from microlensing
- Strong lensing statistics in large, z~<0.2 surveys: bias in the lens galaxy population
- LISA detection of massive black hole binaries: imprint of seed populations and of exterme recoils
- How does the Earth's rotation affect predictions of gravitational wave strong lensing rates?
- Complementary constraints on dark energy equation of state from strongly lensed gravitational wave
- Pattern of lensed chirp gravitational wave signal and its implication on the mass and position of lens
- Gravitational Waves in Scalar-Tensor-Vector Gravity Theory
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- Discovering gravitationally lensed gravitational waves: predicted rates, candidate selection, and localization with the Vera Rubin Observatory
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- Compact Binaries through a Lens: Silent vs. Detectable Microlensing for the LIGO-Virgo-KAGRA Gravitational Wave Observatories
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- Parameter estimation of microlensed gravitational waves with Conditional Variational Autoencoders
- Searching for wormholes with gravitational wave scattering
- Gravitational Lensing in More Realistic Dark Matter Halo Models
- Challenges and Opportunities for time-delay cosmography with multi-messenger gravitational lensing
- Corrections to the gravitational wave phasing
- Toward Gravitational Lensing in Modified Theories of Gravity
- Lensing by primordial black holes: constraints from gravitational wave observations
- Understanding the predication mechanism of deep learning through error propagation among parameters in strong lensing case
- Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations
- Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
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