LIGO: The Laser Interferometer Gravitational-Wave Observatory

Abstract

The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves of astrophysical origin. Direct detection of gravitational waves holds the promise of testing general relativity in the strong-field regime, of providing a new probe of exotic objects such as black hole and neutron stars, and of uncovering unanticipated new astrophysics. LIGO, a joint Caltech-MIT project supported by the National Science Foundation, operates three multi-kilometer interferometers at two widely separated sites in the United States. These detectors are the result of decades of worldwide technology development, design, construction, and commissioning. They are now operating at their design sensitivity, and are sensitive to gravitational wave strains smaller than 1 part in 1E21. With this unprecedented sensitivity, the data are being analyzed to detect or place limits on gravitational waves from a variety of potential astrophysical sources.

50 pages, 14 figures

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• Results from an Einstein@Home search for continuous gravitational waves from Cassiopeia A, Vela Jr. and G347.3
• Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run
• Implementing a semicoherent search for continuous gravitational waves using optimally-constructed template banks
• Prospects of observing continuous gravitational waves from known pulsars
• A coherent method for the detection and estimation of continuous gravitational wave signals using a pulsar timing array
• Efficiency of Penrose process in spacetime of axially symmetric magnetized Reissner-Nordström black hole
• Angular instability due to radiation pressure in the LIGO gravitational wave detector
• The initial value problem as it relates to numerical relativity
• Searching for prompt signatures of nearby core-collapse supernovae by a joint analysis of neutrino and gravitational-wave data
• An Einstein@home search for continuous gravitational waves from Cassiopeia A
• Sensitivity functions for space-borne gravitational wave detectors
• Application of asymptotic expansions for maximum likelihood estimators' errors to gravitational waves from binary mergers: the network case
• Orbital Foregrounds for Ultra-Short Duration Transients
• Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project
• Faint objects in motion: the new frontier of high precision astrometry
• Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts
• A Simple method to set up low eccentricity initial data for moving puncture simulations
• Total-variation-based methods for gravitational wave denoising
• Omni-resonant optical micro-cavity
• SOAP: A generalised application of the Viterbi algorithm to searches for continuous gravitational-wave signals
• A brief history of gravitational wave research
• Characterization of the seismic environment at the Sanford Underground Laboratory, South Dakota
• Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005-2010
• All-sky search for long-duration gravitational wave transients with LIGO
• Spin-Precessing Black Hole Binaries in Dynamical Chern-Simons Gravity
• Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos
• Intermediate-mass-ratio-inspirals in the Einstein Telescope. II. Parameter estimation errors
• Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations
• Eight Millisecond Pulsars Discovered in the Arecibo PALFA Survey
• Improved Time-Domain Accuracy Standards for Model Gravitational Waveforms
• Possible High-Energy Neutrino and Photon Signals from Gravitational Wave Bursts due to Double Neutron Star Mergers
• Multimessenger astronomy with the Einstein Telescope
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Gravitational waves from supernova matter
• Effects of Mirror Aberrations on Laguerre-Gaussian Beams in Interferometric Gravitational-Wave Detectors
• Particle Swarm Optimization and gravitational wave data analysis: Performance on a binary inspiral testbed
• Implementation of the frequency-modulated sideband search method for gravitational waves from low mass X-ray binaries
• Gravitational Waveforms for Precessing, Quasicircular Compact Binaries with Multiple Scale Analysis: Small Spin Expansion
• Light curve classification with recurrent neural networks for GOTO: dealing with imbalanced data
• Practical flux-prescriptions for gamma-ray burst afterglows, from early to late times
• Strange stars in $f(\mathcal{R})$ gravity Palatini formalism and gravitational wave echoes from them
• The next detectors for gravitational wave astronomy
• High sensitivity, levitated microsphere apparatus for short-distance force measurements
• Hydraulic External Pre-Isolator System for LIGO
• Characterization of thermal effects in the Enhanced LIGO Input Optics
• Cross-correlation search for continuous gravitational waves from a compact object in SNR 1987A in LIGO Science Run 5
• Binary White Dwarfs as Laboratories for Extreme Gravity with LISA
• Application of a Hough search for continuous gravitational waves on data from the 5th LIGO science run
• Application of asymptotic expansions of maximum likelihood estimators errors to gravitational waves from binary mergers: the single interferometer case
• Interferometer Response to Geontropic Fluctuations
• Black holes in nonlinear electrodynamics: quasi-normal spectra and parity splitting
• Gravitational wave source localization for eccentric binary coalesce with a ground-based detector network
• Multivariate Classification with Random Forests for Gravitational Wave Searches of Black Hole Binary Coalescence
• Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era
• Material loss angles from direct measurements of broadband thermal noise
• Designing a cross-correlation search for continuous-wave gravitational radiation from a neutron star in the supernova remnant SNR 1987A
• High Energy Neutrinos from Choked Gamma-Ray Bursts in AGN Accretion Disks
• Swift/UVOT follow-up of Gravitational Wave Alerts in the O3 era
• A robust machine learning algorithm to search for continuous gravitational waves
• Reducing the effect of seismic noise in LIGO searches by targeted veto generation
• Optomechanically-induced-transparency cooling of massive mechanical resonators to the quantum ground state
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• Effect of interference on thermal noise and coating optimization in dielectric mirrors
• Galaxy Survey On The Fly: Prospects of Rapid Galaxy Cataloging to Aid the Electromagnetic Follow-up of Gravitational-wave Observations
• Bayesian parameter estimation of core collapse supernovae using gravitational wave simulations
• The Population of Eccentric Binary Black Holes: Implications for mHz Gravitational Wave Experiments
• Astrophysical motivation for directed searches for a stochastic gravitational wave background
• Black hole science with the Laser Interferometer Space Antenna
• Gravitational wave echoes from compact stars in $f(\mathcal{R},T)$ gravity
• Pulsar revival in neutron star mergers: multi-messenger prospects for the discovery of pre-merger coherent radio emission
• Panoramic optical and near-infrared SETI instrument: overall specifications and science program
• Multiparameter Quantum Estimation Theory in Quantum Gaussian states
• Prospects for joint observations of gravitational waves and gamma rays from merging neutron star binaries
• Optimizing Vetoes for Gravitational-wave Transient Searches
• Empirically extending the range of validity of parameter-space metrics for all-sky searches for gravitational-wave pulsars
• Optimal Networks of Future Gravitational-Wave Telescopes
• Multi-color Cavity Metrology
• Harvesting energy driven by Comisso-Asenjo process from Kerr-MOG black holes
• A search of the Orion spur for continuous gravitational waves using a "loosely coherent" algorithm on data from LIGO interferometers
• Gravitational waves from intermediate-mass black holes in young clusters
• Magnetic-distortion-induced ellipticity and gravitational wave radiation of neutron stars: millisecond magnetars in short GRBs, Galactic pulsars, and magnetars
• Non-adiabatic elimination of auxiliary modes in continuous quantum measurements
• Testing general relativity with compact coalescing binaries: comparing exact and predictive methods to compute the Bayes factor
• Status of GEO 600
• Analytic Investigation of the Branch Cut of the Green Function in Schwarzschild Space-time
• Instrumental vetoes for transient gravitational-wave triggers using noise-coupling models: The bilinear-coupling veto
• How serious can the stealth bias be in gravitational wave parameter estimation?
• A novel scheme for hundred-hertz linewidth measurements with self-heterodyne method
• Utilizing the null stream of the Einstein Telescope
• Tetrads in SU(N) Yang-Mills geometrodynamics
• Search for transient gravitational waves in coincidence with short duration radio transients during 2007-2013
• Locking the frequency of lasers to an optical cavity at the $1.6\times 10^{-17}$ relative instability level
• Application of Artificial Neural Network to Search for Gravitational-Wave Signals Associated with Short Gamma-Ray Bursts
• Technology for the next gravitational wave detectors
• Likelihood-ratio ranking of gravitational-wave candidates in a non-Gaussian background
• PTF11agg as the First Evidence for Reverse Shock Emission from a Postmerger Millisecond Magnetar
• First results and future prospects for dual-harmonic searches for gravitational waves from spinning neutron stars
• Alternatives to standard puncture initial data for binary black hole evolution
• A fully-coherent all-sky search for gravitational-waves from compact binary coalescences
• Inspiralling, Non-Precessing, Spinning Black Hole Binary Spacetime via Asymptotic Matching
• Interpolation in waveform space: enhancing the accuracy of gravitational waveform families using numerical relativity
• Weakly-Gravitating Objects in dynamical Chern-Simons gravity and Constraints with Gravity Probe B
• Bounds on graviton mass using weak lensing and SZ effect in galaxy clusters
• Minimum Noise Optical Coatings for Interferometric Detectors of Gravitational Waves
• Suppression of quantum-radiation-pressure noise in an optical spring
• Gravitational wave detector response in terms of spacetime Riemann curvature
• Data Quality Studies of Enhanced Interferometric Gravitational Wave Detectors
• Arm locking performance with the new LISA design
• Multibaseline gravitational wave radiometry
• Vacuum Beam Guide for Large-Scale Quantum Networks
• Searching for Gamma-Ray counterparts to Gravitational Waves from merging binary neutron stars with the Cherenkov Telescope Array
• A combinatorial algebraic approach for the modified second-generation time-delay interferometry
• Accurate calibration of test mass displacement in the LIGO interferometers
• Simulation of underground gravity gradients from stochastic seismic fields
• Identification of noise artifacts in searches for long-duration gravitational-wave transients
• Sliding coherence window technique for hierarchical detection of continuous gravitational waves
• Optimising the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
• Optimum quantum resource distribution for phase measurement and quantum information tapping in a dual-beam SU(1,1) interferometer
• Search for Long-duration Gravitational-wave Signals Associated with Magnetar Giant Flares
• Upper Limits from Counting Experiments with Multiple Pipelines
• Outlook for detection of GW inspirals by GRB-triggered searches in the Advanced detector era
• Feasibility of measuring the Shapiro time delay over meter-scale distances
• The Advanced LIGO Gravitational Wave Detector
• Searching for Signatures of Cosmic String Wakes in 21cm Redshift Surveys using Minkowski Functionals
• Hierarchical Bayesian method for detecting continuous gravitational waves from an ensemble of pulsars
• Using ISS Telescopes for Electromagnetic Follow-up of Gravitational Wave Detections of NS-NS and NS-BH Mergers
• Hybrid black-hole binary initial data
• Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform
• Detectability of Primordial Black Hole Binaries at High Redshift
• How photon astronomy affects searches for continuous gravitational waves
• Stochastic gravitational wave background from newly born massive magnetars: The role of a dense matter equation of state
• Novel directed search strategy to detect continuous gravitational waves from neutron stars in low- and high-eccentricity binary systems
• A New Bound on Excess Frequency Noise in Second Harmonic Generation in PPKTP at the 10^-19 Level
• Sensitivity study using machine learning algorithms on simulated r-mode gravitational wave signals from newborn neutron stars
• Fast marginalization algorithm for optimizing gravitational wave detection, parameter estimation and sky localization
• Liverpool Telescope 2: a new robotic facility for rapid transient follow-up
• Bayesian approach to radio frequency interference mitigation
• Multi-messenger astronomy of gravitational-wave sources with flexible wide-area radio transient surveys
• Many-Task Computing and Blue Waters
• Enhancing phase sensitivity in Mach-Zehnder interferometer with various detection schemes using SU(1,1) coherent states
• Cavity-immune features in the spectra of superradiant crossover laser pulses
• High-order perturbations of a spherical collapsing star
• Status of advanced ground-based laser interferometers for gravitational-wave detection
• Sensitivity Comparison of Searches for Binary Black Hole Coalescences with Ground-based Gravitational-Wave Detectors
• What can PSR J1640-4631 tell us about the internal physics of this neutron star?
• Towards a direct measurement of the quantum vacuum Lagrangian coupling coefficients using two counter propagating super-intense laser pulses
• Accurate evaluation of self-heterodyne laser linewidth measurements using Wiener filters
• Using Gravitational Wave Parallax to Measure the Hubble Parameter with Pulsar Timing Arrays
• Enhancing the significance of gravitational wave bursts through signal classification
• Results of an all-sky high-frequency Einstein@Home search for continuous gravitational waves in LIGO's fifth science run
• Detecting transient gravitational waves in non-Gaussian noise with partially redundant analysis methods
• LIGO-Virgo searches for gravitational waves from coalescing binaries: a status update
• On Investigating EMD Parameters to Search for Gravitational Waves
• Doppler effect in TianQin time-delay interferometry
• Improved Coincident and Coherent Detection Statistics for Searches for Gravitational Wave Ringdown Signals
• All-reflective coupling of two optical cavities with 3-port diffraction gratings
• Evolution of scalar fields surrounding black holes on compactified constant mean curvature hypersurfaces
• Signatures of linearized gravity in atom interferometers: A simplified computational framework
• Ultrahigh-energy Gamma Rays and Gravitational Waves from Primordial Exotic Stellar Bubbles
• Method for estimation of gravitational-wave transient model parameters in frequency-time maps
• A fifty-fold improvement of thermal noise limited inertial sensitivity by operating at cryogenic temperatures
• Reconstruction of the gravitational wave signal $h(t)$ during the Virgo science runs and independent validation with a photon calibrator
• A Technique for In-situ Measurement of Free Spectral Range and Transverse Mode Spacing of Optical Cavities
• Search for gravitational waves associated with the InterPlanetary Network short gamma ray bursts
• First stage of LISA data processing II: Alternative filtering dynamic models for LISA
• Note on Possible Emergence Time of Newtonian Gravity
• Detection of Einstein Telescope gravitational wave signals from binary black holes using deep learning
• Rapid alerts for following up gravitational wave event candidates
• Detection of gravitational waves in circular particle accelerators
• Detecting Long-Duration Narrow-Band Gravitational Wave Transients Associated with Soft Gamma Repeater Quasi-Periodic Oscillations
• Composite gravitational-wave detection of compact binary coalescence
• The Effects of Minimal Length in Entropic Force Approach
• An independent search of gravitational waves in the first observation run of advanced LIGO using cross-correlation
• Constraining the Break of Spatial Diffeomorphism Invariance with Planck Data
• GRB 191016A: The onset of the forward shock and evidence of late energy injection
• Upper limit on the amplitude of gravitational waves around 0.1Hz from the Global Positioning System
• Precision Measurement of a low-loss Cylindrical Dumbbell-Shaped Sapphire Mechanical Oscillator using Radiation Pressure
• Towards thermal noise free optomechanics
• Application of a Zero-latency Whitening Filter to Compact Binary Coalescence Gravitational-wave Searches
• Current status of gravitational-wave observations
• Identification of long-duration noise transients in LIGO and Virgo
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Newtonian noise limit in atom interferometers for gravitational wave detection
• Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity
• Vacuum-defect wormholes and a mirror world
• Distinguishing between evidence and its explanations in the steering of atomic clocks
• Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
• Monopolar and quadrupolar gravitational radiation from magnetically deformed neutron stars in modified gravity
• Classifying Lensed Gravitational Waves in the Geometrical Optics Limit with Machine Learning
• Astronomy and astrophysics with gravitational waves in the Advanced Detector Era
• Prospects for joint radio telescope and gravitational wave searches for astrophysical transients
• Gravitational waves generated by laser accelerated relativistic ions
• A boosted Kerr black hole solution and the structure of a general astrophysical black hole
• Searching for gravitational waves with the LIGO and Virgo interferometers
• The Evryscope Fast Transient Engine: Real-Time Detection for Rapidly Evolving Transients
• Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline
• Obtaining Gravitational Waves from Inspiral Binary Systems using LIGO data
• A mirrorless spinwave resonator
• Slow-rotating charged black hole solution in dynamical Chern-Simons modified gravity
• Optimizing StackSlide setup and data selection for continuous-gravitational-wave searches in realistic detector data
• On the use of black hole binaries as probes of local dark energy properties
• Identifying thermal effects in neutron star merger remnants with model-agnostic waveform reconstructions and third-generation detectors
• A Michelson-type Radio Interferometer for University Education
• Analysis of parametric oscillatory instability in Fabry-Perot cavity with Gauss and Laguerre-Gauss main mode profile
• Global Optimization for Future Gravitational Wave Detectors' Sites
• Creep events and creep noise in gravitational-wave interferometers: basic formalism and stationary limit
• Time-domain properties of electromagnetic signals in a dynamical axion background
• Multi-messenger observations of double neutron stars in Galactic disk with gravitational and radio waves
• Enabling entanglement distillation via optomechanics
• Can we discern millilensed gravitational-wave signals from signals produced by precessing binary black holes with ground-based detectors?
• Magnetically Induced Optical Transparency With Ultra-Narrow Spectrum
• The probe readout and quantum limited measurements
• The Virtual Research Environment: towards a comprehensive analysis platform
• Coherently combining short data segments for all-sky semi-coherent continuous gravitational wave searches
• Compact, robust, and spectrally pure diode-laser system with a filtered output and a tunable copy for absolute referencing
• Astroseismology of neutron stars from gravitational waves in the limit of perfect measurement
• Nonclassical states of levitated macroscopic objects beyond the ground state
• Prospects for intermediate mass black hole binary searches with advanced gravitational-wave detectors
• A New Class of Optical Beams for Large Baseline Interferometric Gravitational Wave Detectors
• Low temperature and high magnetic field performance of a commercial piezo-actuator probed $via$ laser interferometry
• Future targets for light gauge bosons from cosmic strings
• Proper Time Observables of General Gravitational Perturbations in Laser Interferometry-based Gravitational Wave Detectors
• Phenomenological gravitational waveforms from spinning coalescing binaries
• Hubble without the Hubble: cosmology using advanced gravitational-wave detectors alone
• Mechanical Squeezing in Quadratically-coupled Optomechanical Systems
• Boosted Kerr black holes in general relativity
• Stable optical spring in aLIGO detector with unbalanced arms and in Michelson-Sagnac interferometer
• Are different approaches to constructing initial data for binary black hole simulations of the same astrophysical situation equivalent?
• Improving parameter estimation accuracy with torsion-bar antennas
• Electromagnetic waves from neutron stars and black holes driven by polar gravitational perturbations
• Sensitivity improvement of a laser interferometer limited by inelastic back-scattering, employing dual readout
• Multi-mode Heterodyne Laser Interferometry Realized via Software Defined Radio
• Optical counterpart of the Foucault pendulum
• Numerical relativity simulations in the era of the Einstein Telescope
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors
• Gravitational Wave Astronomy: Needle in a Haystack
• Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
• Exploring the Use of Numerical Relativity Waveforms in Burst Analysis of Precessing Black Hole Mergers
• Numerical simulations of interfaces in relativistic hydrodynamics
• A Bayesian parameter estimation approach to pulsar time-of-arrival analysis
• Stochastic backgrounds of gravitational waves from cosmological sources - The role of dark energy
• Michelson interferometer with diffractively-coupled arm resonators in second-order Littrow configuration
• Reanalysis of F-statistic gravitational-wave searches with the higher criticism statistic
• Multidimensional optical trapping of a mirror
• GRB-triggered searches for gravitational waves in LIGO data
• The Dawn of Multi-Messenger Astronomy
• Directed graphs and interferometry
• Quantum metrology enhanced by the $XY$ spin interaction in a generalized Tavis-Cummings model
• Satellites promise global-scale quantum networks
• Recent astrophysical observations reproduced by a short-range correlated van der Waals-type model?
• The RTApipe framework for the gamma-ray real-time analysis software development
• Hierarchical Hough all-sky search for periodic gravitational waves in LIGO S5 data
• Spinning (A)dS Black Holes with Slow-Rotation Approximation in Dynamical Chern-Simons Modified Gravity
• Liverpool Telescope 2: a new robotic facility for time domain astronomy in 2020+
• Likelihood smoothing using gravitational wave surrogate models
• Un-modeled search for black hole binary systems in the NINJA project
• Gravitational-wave astronomy: Observational results and their impact
• Gravitational Waves and Time Domain Astronomy
• Omni-resonant imaging across the visible
• Diffractively coupled Fabry-Perot resonator with power-recycling
• Quasi-normal acoustic oscillations in the transonic Bondi flow
• A search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar
• An Archival Search for Neutron-Star Mergers in Gravitational Waves and Very-High-Energy Gamma Rays
• Unifying supervised learning and VAEs -- coverage, systematics and goodness-of-fit in normalizing-flow based neural network models for astro-particle reconstructions
• Orbital effects of a monochromatic plane gravitational wave with ultra-low frequency incident on a gravitationally bound two-body system
• Avenues for Analytic exploration in Axisymmetric Spacetimes. Foundations and the Triad Formalism
• Unified laboratory-frame analysis of atomic gravitational-wave sensors
• Spontaneous crystallization noise in mirrors of gravitational wave detectors
• Photon counting for axion interferometry
• Parametric Oscillatory Instability in a Fabry-Perot Cavity of the Einstein Telescope with different mirror's materials
• Decoherence from Long-Range Forces in Atom Interferometry
• On the role of magnetic fields into the dynamics and gravitational wave emission of binary neutron stars
• Influence of separating distance between atomic sensors for gravitational wave detection
• The road to gravitational-wave astronomy
• Mirror Coating Thermal Noise Mitigation Using Multi-Spatial Mode Cavity Readout
• Of Mountains and Molehills : Gravitational Waves from Neutron Stars
• A nonparametric method to assess significance of events in search for gravitational waves with false discovery rate
• Gravitational and electromagnetic perturbations of a charged black hole in a general gauge condition
• Gravitational Wave Strain and Orbital Dynamics of Binary Pulsars from LIGO-Virgo to LISA
• Squeezing of optomechanical modes in detuned Fabry-Perot interferometer
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• The Einstein Toolkit: A Student's Guide
• Probing Dark Matter Clumps, Strings and Domain Walls with Gravitational Wave Detectors
• Study on Gravitational Waves from Binary Mergers and Constraints on the Hubble Parameter
• Searches for continuous gravitational waves with the LIGO and Virgo detector
• Approaching the double-Heisenberg scaling sensitivity in the Tavis-Cummings model
• Glitch veto based on unphysical gravitational wave binary inspiral templates
• Testing the Braneworld Theory with Identical Particles
• Bayesian Estimation of Laser Linewidth from Delayed Self-Heterodyne Measurements
• The Future of low Energy Photon Experiments
• Matters of Gravity, The Newsletter of the Topical Group in Gravitation of the American Physical Society, Volume 32, Fall 2008
• Cavity locking with spatial modulation of optical phase front for laser stabilization
• Data Analysis of Massive Gravitational Waves from Gamma Ray Bursts
• Statistical Analyses for NANOGrav 5-year Timing Residuals
• Precision studies of Casimir force and short-range gravity employing prototypes of interferometric gravitational wave detectors
• Implications of the binary coalescence events found in O1 and O2 for the stochastic background of gravitational events
• Cost-benefit analysis for commissioning decisions in GEO600
• Determination of mass of an isolated neutron star using continuous gravitational waves with two frequency modes: an effect of a misalignment angle
• All-sky coherent search for continuous gravitational waves in 6-7 Hz band with a torsion-bar antenna
• Role of Modern Optical Techniques in Gravitational Wave Detection
• Partial compensation of thermal noise in the fundamental mode of an optical cavity
• Constraining Primordial Black Hole Dark Matter with CHIME Fast Radio Bursts
• Advanced LIGO Two-Stage Twelve-Axis Vibration Isolation and Positioning Platform. Part 2: Experimental Investigation and Tests Results
• Testing f(R) gravity using gravitational-wave signals from binary mergers
• Extending the micro-Hertz detection horizons via orbital resonance effect for geocentric gravitational wave antennas
• Search for gravitational waves from binary black hole inspiral, merger and ringdown
• Search for gravitational-wave bursts in the first year of the fifth LIGO science run
• Identification of Noise-Associated Glitches in KAGRA O3GK with Hveto
• MaxWave: Rapid maximum likelihood wavelet reconstruction of non-Gaussian features in gravitational wave data
• Squeezing and quantum control of antiferromagnetic magnon pseudospin
• A singlet scalar assisted $N_2$ Leptogenesis and Pseudo-Scalar Dark Matter
• The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
• Inverse compton scattered merger-nova: late X-ray counterpart of gravitational wave signals from NS-NS/BH mergers
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Logical synchronization: how evidence and hypotheses steer atomic clocks