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Lighthouses of Gravitational Wave Astronomy
Gravitational wave detectors capable of making astronomical observations could begin to operate within the next year, and over the next 10 years they...
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Gravitomagnetic induction in the field of a gravitational wave
The interaction of a plane gravitational wave with test masses can be described in the proper detector frame, using Fermi coordinates, in terms of a...
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Numerical Relativity for Gravitational Wave Source Modeling
The first direct detection of gravitational wave has been realized by LIGO in 2015. It opens a brand new window to observe our universe and initiates...
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Environmental Noise in Gravitational-Wave Interferometers
The first 20 years of operation of gravitational-wave interferometers have shown that, despite the high degree of isolation, detectors are affected...
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Principles of the Wave Dark Matter Detection in Gravitational Redshift Experiments in the Solar System
AbstractWe explore the possibility of using measurements of the gravitational redshift effect as a means to constrain wave dark matter—a class of...
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Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications
Binary compact objects will be among the important sources for the future space-based gravitational wave detectors. Such binary compact objects...
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Gravitational wave signals from long-lasting binary–single black hole encounters
In the dense regions of star clusters, close encounters with black holes (BHs) can occur giving rise to a new class of gravitational-wave (GW)...
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Near real-time gravitational wave data analysis of the massive black hole binary with TianQin
Space-borne gravitational wave (GW) detectors can detect the merger of massive black holes. The early warning and localization of GW events before...
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Design and implementation of a seismic Newtonian noise cancellation system for the Virgo gravitational-wave detector
Terrestrial gravity perturbations caused by seismic fields produce the so-called Newtonian noise in gravitational-wave detectors, which is predicted...
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The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies
Recently, pulsar timing array (PTA) experiments have provided compelling evidence for the existence of the nanohertz stochastic gravitational wave...
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Constraints on dark energy from the gravitational wave background
Current observational data indicate that dark energy (DE) is a cosmological constant without considering its conclusiveness evidence. Considering the...
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The equivalence principle for a plane gravitational wave in torsion-based and non-metricity-based teleparallel equivalents of general relativity
We study the energy–momentum characteristics of the plane “+”-polarized gravitational wave solution of general relativity in the teleparallel...
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Symmetries and selection rules: optimising axion haloscopes for Gravitational Wave searches
In the presence of electromagnetic fields, both axions and gravitational waves (GWs) induce oscillating magnetic fields: a potentially detectable...
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Lorentz force detuning in heterodyne gravitational wave experiments
Heterodyne cavity experiments for gravitational wave (GW) detection experience a rising interest since recent studies showed that they allow to probe...
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Space-based gravitational wave signal detection and extraction with deep neural network
Space-based gravitational wave (GW) detectors will be able to observe signals from sources that are otherwise nearly impossible from current...
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Gravitational Waves
This chapter and Chap. 7 deal with two fundamental concepts in spacetime physics—gravitational...
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Introduction to Gravitational Wave Astronomy
This chapter provides an overview of gravitational wave (GW) astronomy, providing background material that underpins the other, more specialized...
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Third-Generation Gravitational-Wave Observatories
The second generation of gravitational-wave (GW) detectors has opened a new window on the cosmos, yet leaves much of the gravitational universe...
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Oscillatory amplitude of stochastic gravitational wave spectrum
Primordial gravitational waves generated from early universe are placed in the squeezed vacuum state and the resulting stochastic background is...
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Wave effect of gravitational waves intersected with a microlens field: A new algorithm and supplementary study
The increase in gravitational wave (GW) events has allowed receiving strong lensing image pairs of GWs. However, the wave effect (diffraction and...