4.7 Article

Impact of LIGO-Virgo black hole binaries on gravitational wave background searches

相关参考文献

注意:仅列出部分参考文献,下载原文获取全部文献信息。
Article Multidisciplinary Sciences

Prospective sensitivities of atom interferometers to gravitational waves and ultralight dark matter

Leonardo Badurina et al.

Summary: This study surveys the sensitivities of terrestrial and space-borne atom interferometers to gravitational waves and ultralight dark matter. The article compares the sensitivities of different detectors and discusses the impact of various background noises. It also explores the potential sources of these phenomena.

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES (2022)

Article Astronomy & Astrophysics

Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects

Arianna I. Renzini et al.

Summary: This review provides an overview of stochastic gravitational wave (GW) signals, including their generation processes, observational properties, and detection strategies. The article discusses the application of interferometric measurements using ground-based and space-based laser interferometers, as well as timing-residuals analyses with pulsar timing arrays. The review also discusses future observations with third generation detectors, space-based interferometers, and potential non-interferometric detection methods proposed in the literature.

GALAXIES (2022)

Article Astronomy & Astrophysics

Low latency detection of massive black hole binaries

Neil J. Cornish

Summary: In the next decade, the launch of space-based gravitational wave detectors such as Taiji and TianQin is expected. These detectors aim to detect the merger of black holes with masses between 103 M0 and 108 M0, which may produce electromagnetic signals in addition to gravitational waves. Low latency detection of gravitational wave signals is crucial for capturing all phases of the emission and guiding the search for counterparts.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Ability of LISA to detect a gravitational-wave background of cosmological origin: The cosmic string case

Guillaume Boileau et al.

Summary: We investigate the ability of the Laser Interferometer Space Antenna (LISA) to detect a stochastic gravitational-wave background (GWB) produced by cosmic strings, and to subsequently estimate the string tension G mu in the presence of instrument noise, an astrophysical background from compact binaries, and the galactic foreground from white dwarf binaries. We demonstrate the importance of including the galactic foreground as well as the astrophysical background for LISA to detect a cosmic string produced GWB and estimate the string tension.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Observational prospects for phase transitions at LISA: Fisher matrix analysis

Chloe Gowling et al.

Summary: This study investigates LISA's sensitivity to the thermodynamic parameters encoded in the stochastic background produced by a phase transition using the sound shell model to characterize the gravitational wave power spectrum and the Fisher matrix to estimate uncertainties. The power spectrum in the sound shell model can be well approximated by a four-parameter double broken power law, and the peak power and frequency can be measured to approximately 10% accuracy for signal-to-noise ratios (SNRs) above 20. The phase boundary speed is found to be the best constrained parameter, with potential for good prospects in combinations of parameters.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Article Astronomy & Astrophysics

Improved reconstruction of a stochastic gravitational wave background with LISA

Raphael Flauger et al.

Summary: A data analysis methodology was proposed for model-independent reconstruction of the spectral shape of a stochastic gravitational wave background with LISA; The improved algorithm includes a complete set of TDI channels, reducing uncertainties, avoiding local extrema in likelihood maximization, and breaking degeneracies between signal and instrumental noise; Testing with case studies showed that additional channels are helpful in various ways for the reconstruction process.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Article Astronomy & Astrophysics

One Channel to Rule Them All? Constraining the Origins of Binary Black Holes Using Multiple Formation Pathways

Michael Zevin et al.

Summary: The study analyzed the second batch of LIGO-Virgo gravitational wave catalog using five binary black hole population models, finding that multiple formation channels contribute to the observed sample of binary black holes and no single channel dominates the detections. Results also showed a preference for natal spins of isolated black holes less than or equal to 0.1 and common-envelope efficiencies of around 2.0.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

R. Abbott et al.

Summary: The study reveals unique characteristics of the merging binary black hole (BBH) population, including a specific primary mass spectrum and misaligned component spins leading to precession of the orbital plane. The research also estimates merger rates, indicating potential correlation between BBH rate and redshift but not exceeding the star formation rate. Additionally, recent exceptional events are examined in relation to population models, with GW190814 being identified as an outlier due to its low secondary mass.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Two populations of LIGO-Virgo black holes

Gert Hutsi et al.

Summary: The study suggests that a population consisting solely of primordial black holes is unlikely, with the best fit being a combination of astrophysical and primordial merger rates. The data also indicates the possibility of two distinct astrophysical black hole populations.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

Article Physics, Multidisciplinary

Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run

Alba Romero et al.

Summary: Constraints on the normalized energy density in gravitational waves from first-order strong phase transitions are placed using data from Advanced LIGO and Virgo, with upper limits determined at a 95% confidence level for different models. The study considers astrophysical signals as foreground and discusses the background due to bubble collisions and sound waves from phase transitions occurring at temperatures above 10(8) GeV.

PHYSICAL REVIEW LETTERS (2021)

Article Quantum Science & Technology

Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100)

Mahiro Abe et al.

Summary: MAGIS-100 is a next-generation quantum sensor being constructed at Fermilab, aiming to explore fundamental physics through atom interferometry over a 100 m baseline. This novel detector will search for ultralight dark matter, test quantum mechanics in new regimes, and pave the way for future gravitational wave detectors.

QUANTUM SCIENCE AND TECHNOLOGY (2021)

Article Astronomy & Astrophysics

Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground

Guillaume Boileau et al.

Summary: LISA will observe orbital modulated waveforms from Galactic white dwarf binaries, a binary black hole produced gravitational-wave background, and potentially a cosmologically created stochastic gravitational-wave background (SGWB) within its observational band. Through simulations, the complex waveform from the Galactic foreground with 3.5 x 10(7) binaries has been determined, and a data analysis strategy has been presented to address it.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Physics, Multidisciplinary

Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run

R. Abbott et al.

Summary: The study searches for gravitational-wave signals produced by cosmic strings in the O3 dataset and constrains the cosmic string tension using upper limits derived from the stochastic gravitational-wave background energy density. The constraints on G mu are improved upon previous studies, challenging simple inflationary models in the case of cosmic strings formed within the context of grand unified theories.

PHYSICAL REVIEW LETTERS (2021)

Article Physics, Multidisciplinary

GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run

R. Abbott et al.

Summary: This report presents 39 candidate gravitational-wave events detected by Advanced LIGO and Advanced Virgo during the first half of the third observing run (O3a) between April 1, 2019 and October 1, 2019. The events include black hole binary mergers up to a redshift of approximately 0.8 and events where the components cannot be unambiguously identified. The range of candidate event masses has expanded compared to previous catalogs, with the inclusion of binary systems with asymmetric mass ratios.

PHYSICAL REVIEW X (2021)

Article Astronomy & Astrophysics

Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo's third observing run

R. Abbott et al.

Summary: This study reports the results of a search for an isotropic gravitational-wave background using data from advanced detectors, placing upper limits on the strength of different types of gravitational-wave backgrounds. The study also explores the potential sources of correlated noise and compares the results to a fiducial model for the gravitational-wave background. Additionally, the study demonstrates the potential of combining results from individual mergers to provide stronger constraints on the merger rate of binary black holes.

PHYSICAL REVIEW D (2021)

Article Physics, Multidisciplinary

The TianQin project: Current progress on science and technology

Jianwei Mei et al.

Summary: The TianQin project aims to detect gravitational waves using three Earth-orbiting satellites forming an equilateral triangle constellation, with the goal of detecting a wide range of astrophysical and cosmological sources. The project is utilizing the 0123 plan to develop key technologies and ground research facilities in order to start science operations by 2035. Major milestones have already been achieved, such as the launch of a new-generation retro-reflector and successful ranging to all five retro-reflectors on the Moon.

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS (2021)

Article Astronomy & Astrophysics

Impact of a midband gravitational wave experiment on detectability of cosmological stochastic gravitational wave backgrounds

Barry C. Barish et al.

Summary: This study forecasts the impact of a future midband space-based gravitational wave experiment on potential detections of cosmological stochastic gravitational wave backgrounds (SGWBs), proposes a combined power-law integrated sensitivity (CPLS) curve, and models various SGWB sources, showing that the midband can significantly improve sensitivities to cosmological SGWBs.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Spectral separation of the stochastic gravitational-wave background for LISA: Observing both cosmological and astrophysical backgrounds

Guillaume Boileau et al.

Summary: This study aims to observe a stochastic gravitational-wave background with LISA, emphasizing the importance of spectral separability between cosmological and astrophysical backgrounds. Using adaptive Markov chain Monte Carlo methods, the detectable limits for future LISA measurements of SGWB are estimated, along with calculating the Cramer-Rao lower bound. Based on the expected astrophysical background level, LISA can detect a specific cosmological SGWB energy density after 4 years of observation.

PHYSICAL REVIEW D (2021)

Article Astronomy & Astrophysics

Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors

Katarina Martinovic et al.

Summary: The recent joint observing runs of Advanced LIGO and Advanced Virgo have not claimed a stochastic gravitational-wave background detection, but it is expected to change as the detectors' sensitivity improves. The study shows that third-generation detectors can reduce astrophysical signals through subtraction of individual sources and potentially reveal cosmological backgrounds.

PHYSICAL REVIEW D (2021)

Article Quantum Science & Technology

AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space

Yousef Abou El-Neaj et al.

EPJ QUANTUM TECHNOLOGY (2020)

Article Astronomy & Astrophysics

AION: an atom interferometer observatory and network

L. Badurina et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

Article Astronomy & Astrophysics

Probing the gravitational wave background from cosmic strings with LISA

Pierre Auclair et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

Article Astronomy & Astrophysics

Detecting gravitational waves from cosmological phase transitions with LISA: an update

Chiara Caprini et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

Article Astronomy & Astrophysics

ELGAR-a European Laboratory for Gravitation and Atom-interferometric Research

B. Canuel et al.

CLASSICAL AND QUANTUM GRAVITY (2020)

Article Physics, Nuclear

Taiji program: Gravitational-wave sources

Wen-Hong Ruan et al.

INTERNATIONAL JOURNAL OF MODERN PHYSICS A (2020)

Article Astronomy & Astrophysics

Foreground cleaning and template-free stochastic background extraction for LISA

Mauro Pieroni et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2020)

Article Physics, Multidisciplinary

Measuring the Primordial Gravitational-Wave Background in the Presence of Astrophysical Foregrounds

Sylvia Biscoveanu et al.

PHYSICAL REVIEW LETTERS (2020)

Article Physics, Multidisciplinary

Gravitational-wave astronomy with an uncertain noise power spectral density

Colm Talbot et al.

PHYSICAL REVIEW RESEARCH (2020)

Article Astronomy & Astrophysics

Identifying and addressing nonstationary LISA noise

Matthew C. Edwards et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

Global analysis of the gravitational wave signal from Galactic binaries

Tyson B. Littenberg et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

COSMIC Variance in Binary Population Synthesis

Katelyn Breivik et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

Subtracting compact binary foreground sources to reveal primordial gravitational-wave backgrounds

Surabhi Sachdev et al.

PHYSICAL REVIEW D (2020)

Article Astronomy & Astrophysics

The construction and use of LISA sensitivity curves

Travis Robson et al.

CLASSICAL AND QUANTUM GRAVITY (2019)

Article Astronomy & Astrophysics

Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers

Katerina Chatziioannou et al.

PHYSICAL REVIEW D (2019)

Article Astronomy & Astrophysics

Multiband gravitational-wave event rates and stellar physics

Davide Gerosa et al.

PHYSICAL REVIEW D (2019)

Review Astronomy & Astrophysics

Cosmological backgrounds of gravitational waves

Chiara Caprini et al.

CLASSICAL AND QUANTUM GRAVITY (2018)

Article Physics, Multidisciplinary

Optimal Search for an Astrophysical Gravitational-Wave Background

Rory Smith et al.

PHYSICAL REVIEW X (2018)

Article Physics, Multidisciplinary

Multiband gravitational-wave astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO

Soichiro Isoyama et al.

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS (2018)

Article Multidisciplinary Sciences

Exploring gravity with the MIGA large scale atom interferometer

B. Canuel et al.

SCIENTIFIC REPORTS (2018)

Article Astronomy & Astrophysics

Probing non-Gaussian stochastic gravitational wave backgrounds with LISA

Nicola Bartolo et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2018)

Proceedings Paper Astronomy & Astrophysics

Galactic binary science with the new LISA design

Neil Cornish et al.

11TH INTERNATIONAL LISA SYMPOSIUM (2017)

Article Astronomy & Astrophysics

Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries

Piero Madau et al.

ASTROPHYSICAL JOURNAL (2017)

Article Astronomy & Astrophysics

Science with the space-based interferometer eLISA. II: gravitational waves from cosmological phase transitions

Chiara Caprini et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Astronomy & Astrophysics

Science with the space-based interferometer LISA. IV:probing inflation with gravitational waves

Nicola Bartolo et al.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2016)

Article Astronomy & Astrophysics

Advanced LIGO

J. Aasi et al.

CLASSICAL AND QUANTUM GRAVITY (2015)

Article Astronomy & Astrophysics

Bayesian inference for spectral estimation of gravitational wave detector noise

Tyson B. Littenberg et al.

PHYSICAL REVIEW D (2015)

Article Astronomy & Astrophysics

SCIENTIFIC POTENTIAL OF DECIGO PATHFINDER AND TESTING GR WITH SPACE-BORNE GRAVITATIONAL WAVE INTERFEROMETERS

Kent Yagi

INTERNATIONAL JOURNAL OF MODERN PHYSICS D (2013)

Article Astronomy & Astrophysics

The influence of star formation history on the gravitational wave signal from close double degenerates in the thin disc

Shenghua Yu et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2013)

Article Astronomy & Astrophysics

On the gravitational wave background from compact binary coalescences in the band of ground-based interferometers

Xing-Jiang Zhu et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2013)

Article Astronomy & Astrophysics

Fortifying the characterization of binary mergers in LIGO data

Tyson B. Littenberg et al.

PHYSICAL REVIEW D (2013)

Article Astronomy & Astrophysics

Sensitivity curves for searches for gravitational-wave backgrounds

Eric Thrane et al.

PHYSICAL REVIEW D (2013)

Article Astronomy & Astrophysics

GRAVITATIONAL-WAVE EMISSION FROM COMPACT GALACTIC BINARIES

Samaya Nissanke et al.

ASTROPHYSICAL JOURNAL (2012)

Article Astronomy & Astrophysics

Modelling coloured residual noise in gravitational-wave signal processing

Christian Roever et al.

CLASSICAL AND QUANTUM GRAVITY (2011)

Article Astronomy & Astrophysics

Sensitivity studies for third-generation gravitational wave observatories

S. Hild et al.

CLASSICAL AND QUANTUM GRAVITY (2011)

Article Astronomy & Astrophysics

Student-t based filter for robust signal detection

Christian Roever

PHYSICAL REVIEW D (2011)

Review Astronomy & Astrophysics

The astrophysical gravitational wave stochastic background

Tania Regimbau

RESEARCH IN ASTRONOMY AND ASTROPHYSICS (2011)

Article Astronomy & Astrophysics

THE LISA GRAVITATIONAL WAVE FOREGROUND: A STUDY OF DOUBLE WHITE DWARFS

Ashley J. Ruiter et al.

ASTROPHYSICAL JOURNAL (2010)

Article Astronomy & Astrophysics

Subtraction-noise projection in gravitational-wave detector networks

Jan Harms et al.

PHYSICAL REVIEW D (2008)

Article Astronomy & Astrophysics

Tests of Bayesian model selection techniques for gravitational wave astronomy

Neil J. Cornish et al.

PHYSICAL REVIEW D (2007)

Article Astronomy & Astrophysics

Big Bang Observer and the neutron-star-binary subtraction problem

C Cutler et al.

PHYSICAL REVIEW D (2006)

Article Astronomy & Astrophysics

Beyond LISA: Exploring future gravitational wave missions

J Crowder et al.

PHYSICAL REVIEW D (2005)

Article Astronomy & Astrophysics

The gravitational wave background from cosmological compact binaries

AJ Farmer et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2003)

Article Astronomy & Astrophysics

Space missions to detect the cosmic gravitational-wave background

NJ Cornish et al.

CLASSICAL AND QUANTUM GRAVITY (2001)

Article Astronomy & Astrophysics

The gravitational wave signal from the Galactic disk population of binaries containing two compact objects

G Nelemans et al.

ASTRONOMY & ASTROPHYSICS (2001)

Article Astronomy & Astrophysics

Population synthesis for double white dwarfs - I. Close detached systems

G Nelemans et al.

ASTRONOMY & ASTROPHYSICS (2001)