All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

Abstract

This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24--4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate-density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as $\sim$10${}^{-10}{M}_{\odot }{c}^2$ in gravitational waves at $\sim$70 Hz from a distance of 10~kpc, with 50\% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f-modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.

arXiv comment23 pages, 8 figures

References in corpus (56)

• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• Advanced LIGO
• The equation of state for nucleon matter and neutron star structure
• GW170817: Measurements of Neutron Star Radii and Equation of State
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• Explosion Mechanisms of Core-Collapse Supernovae
• The mass distribution and gravitational potential of the Milky Way
• The Progenitor Stars of Gamma-Ray Bursts
• Observation of gravitational waves from two neutron star-black hole coalescences
• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
• A study of 315 glitches in the rotation of 102 pulsars
• Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
• BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
• Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
• Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
• The Milky Way total mass profile as inferred from Gaia DR2
• Gravity Spy: Integrating Advanced LIGO Detector Characterization, Machine Learning, and Citizen Science
• Models of Pulsar Glitches
• Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
• LIGO Detector Characterization in the Second and Third Observing Runs
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Observational constraints on hyperons in neutron stars
• Detection of 107 glitches in 36 southern pulsars
• The Spherical Accretion Shock Instability in the Linear Regime
• Gravitational wave asteroseismology of fast rotating neutron stars with realistic equations of state
• Constraints on cosmic strings using data from the third Advanced LIGO-Virgo observing run
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• The BayesWave analysis pipeline in the era of gravitational wave observations
• All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
• Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
• Characterization of systematic error in Advanced LIGO calibration
• Effects of Data Quality Vetoes on a Search for Compact Binary Coalescences in Advanced LIGO's First Observing Run
• Blip glitches in Advanced LIGO data
• Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies
• Three-dimensional core-collapse supernova simulations of massive and rotating progenitors
• Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms
• The distance to the Vela pulsar gauged with HST parallax oservations
• An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• Reducing Scattered Light in LIGO's Third Observing Run
• The glitch activity of neutron stars
• All-sky search for short gravitational-wave bursts in the first Advanced LIGO run
• Coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysis
• All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
• A First Targeted Search for Gravitational-Wave Bursts from Core-Collapse Supernovae in Data of First-Generation Laser Interferometer Detectors
• Real-Time Supernova Neutrino Burst Monitor at Super-Kamiokande
• A hierarchical method for vetoing noise transients in gravitational-wave detectors
• Environmental Influences on the LIGO Gravitational Wave Detectors during the 6th Science Run
• Environmental Noise in Advanced LIGO Detectors
• Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing run
• Gravitational waves from transient neutron star f-mode oscillations
• Search for nonlinear memory from subsolar mass compact binary mergers
• Leveraging waveform complexity for confident detection of gravitational waves
• All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run
• Gravitational-wave bursts and stochastic background from superfluid vortex avalanches during pulsar glitches
• Enhancing gravitational-wave burst detection confidence in expanded detector networks with the BayesWave pipeline

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• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
• Effects of Dark Matter on $f$-mode oscillations of Neutron Stars
• Constraining cosmological extra dimensions with gravitational wave standard sirens: from theory to current and future multi-messenger observations
• Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
• Search for gravitational-wave bursts in the third Advanced LIGO-Virgo run with coherent WaveBurst enhanced by Machine Learning
• An autoencoder neural network integrated into gravitational-wave burst searches to improve the rejection of noise transients
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• Utilizing Gaussian mixture models in all-sky searches for short-duration gravitational wave bursts
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Utilizing the null stream of the Einstein Telescope
• Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• The impact of selection biases on tests of general relativity with gravitational-wave inspirals
• An Isotropy Measurement with Gravitational Wave Observations
• Gravitational waves from small spin-up and spin-down events of neutron stars
• Probing hadron-quark phase transition in twin stars using $f$-modes
• Using supervised learning algorithms as a follow-up method in the search of gravitational waves from core-collapse supernovae
• Convolutional neural network search for long-duration transient gravitational waves from glitching pulsars
• Search for gravitational waves emitted from SN 2023ixf
• Observational limits on the rate of radiation-driven binary black hole capture events
• Evolution of a black hole cluster in full general relativity
• Searching for gravitational-wave bursts with space-borne detectors
• Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
• Enhancing search pipelines for short gravitational wave transients with Gaussian mixture modelling
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• Magnetically Confined Mountains on Accreting Neutron Stars in General Relativity
• Wavelet-based tools to analyze, filter, and reconstruct transient gravitational-wave signals
• Exposing Gravitational Waves below the Quantum Shot Noise
• Waveform Reconstruction of Core-Collapse Supernova Gravitational Waves with Improved Multisynchrosqueezing Transform
• Beyond the Long Wavelength Approximation: Next-generation Gravitational-Wave Detectors and Frequency-dependent Antenna Patterns
• Extended Gravity Constraints at Different Scales
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
• PycWB: A User-friendly, Modular, and Python-based Framework for Gravitational Wave Unmodelled Search
• Using t-SNE for characterizing glitches in LIGO detectors
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Hierarchical searches for subsolar-mass binaries and the third-generation gravitational wave detector era
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Methods for Estimating Neutron Star Parameters using Multiple Mechanisms for Gravitational Wave Emission Associated with Pulsar Glitches
• Extract non-Gaussian Features in Gravitational Wave Observation Data Using Self-Supervised Learning
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range
• Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts
• Astrophysical or Terrestrial: Machine learning classification of gravitational-wave candidates using multiple-search information
• Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP
• Multi-detector characterization of gravitational-wave burst tensor polarizations with the BayesWave algorithm