Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector

Abstract

Construction of the Japanese second-generation gravitational-wave detector KAGRA has been started. In the next 6 \sim 7 years, we will be able to observe the space-time ripple from faraway galaxies. KAGRA is equipped with the latest advanced technologies. The entire 3-km long detector is located in the underground to be isolated from the seismic motion, the core optics are cooled down to 20 K to reduce thermal fluctuations, and quantum non-demolition techniques are used to decrease quantum noise. In this paper, we introduce the detector configuration of KAGRA; its design, strategy, and downselection of parameters.

Proceeding for the Amaldi conference, 2011. To be published in Classical Quantum Gravity

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• Quantum noise of white light cavity using double-pumped gain medium
• Stiffness effects on the dynamics of the bar-mode instability of Neutron Stars in full General Relativity
• Gravitational Waves from Phase Transition in Minimal SUSY $U(1{)}_{B-L}$ Model
• Searching for anisotropic stochastic gravitational-wave backgrounds with constellations of space-based interferometers
• Gravitational-Wave Detection using Multivariate Analysis
• Performance of Particle Swarm Optimization on the fully-coherent all-sky search for gravitational waves from compact binary coalescences
• Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
• Spinning compact binary dynamics and chameleon orbits
• Molecular adsorbed layer formation on cooled mirrors and its impacts on cryogenic gravitational wave telescopes
• Forecasts on interacting dark energy with standard sirens
• "Stairway to Heaven" -- Spectroscopy of Particle Couplings with Gravitational Waves
• Post-inflationary thermal histories and the refractive index of relic gravitons
• High Performance Heat Conductor with Small Spring Constant for Cryogenic Applications
• Astrophysical black holes as natural laboratories for fundamental physics and strong-field gravity
• Towards a real-time fully-coherent all-sky search for gravitational waves from compact binary coalescences using particle swarm optimization
• Core-Collapse Supernovae, Neutrinos, and Gravitational Waves
• An arm length stabilization system for KAGRA and future gravitational-wave detectors
• An implementation of Galactic white dwarf binary data analysis for MLDC-3.1
• On the primordial black hole formation in hybrid inflation
• The Linear Regime of Tachyonic Preheating
• Indication for dominating surface absorption in crystalline silicon test masses at 1550nm
• Using ISS Telescopes for Electromagnetic Follow-up of Gravitational Wave Detections of NS-NS and NS-BH Mergers
• Photo-Thermal Transfer Function of Dielectric Mirrors for Precision Measurements
• Evaluating residual acceleration noise for TianQin gravitational waves observatory with an empirical magnetic field model
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Accuracy of source localization for eccentric inspiraling binary mergers using a ground-based detector network
• An optically trapped mirror for reaching the standard quantum limit
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Using pulsar timing arrays and the quantum normalization condition to constrain relic gravitational waves
• Effect of Earth-Moon's gravity on TianQin's range acceleration noise. II. Impact of orbit selection
• Calibrating the cosmic distance ladder using gravitational-wave observations
• Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
• A Challenge to Identify an Optical Counterpart of the Gravitational Wave Event GW151226 with Hyper Suprime-Cam
• Silicon emissivity as a function of temperature
• Pre-merger localization of eccentric compact binary coalescences with second-generation gravitational-wave detector networks
• Primordial Gravitational Waves Assisted by Cosmological Scalar Perturbations
• Neutron Star instabilities in full General Relativity using a $\Gamma =2.75$ ideal fluid
• Dark Matter Induced Brownian Motion
• Time evolution of parametric instability in large-scale gravitational-wave interferometers
• Ranking Candidate Signals with Machine Learning in Low-Latency Search for Gravitational-Waves from Compact Binary Mergers
• Status of advanced ground-based laser interferometers for gravitational-wave detection
• Improved calculation of the gravitational wave spectrum from kinks on infinite cosmic strings
• Effect of squeezing on parameter estimation of gravitational waves emitted by compact binary systems
• Observing the dark sector
• Detectability of the cross-correlation between CMB lensing and stochastic GW background from compact object mergers
• Measurement of the Newtonian Constant of Gravitation $G$ by Precision Displacement Sensors
• Probing the Origin of Primordial Black Holes through Novel Gravitational Wave Spectrum
• Gravitational waves in neutrino plasma and NANOGrav signal
• Multi-messenger prospects for black hole - neutron star mergers in the O4 and O5 runs
• On Investigating EMD Parameters to Search for Gravitational Waves
• Recipes for computing radiation from a Kerr black hole using a generalized Sasaki-Nakamura formalism: Homogeneous solutions
• Gravitational Wave Memory from the Relativistic Jet of Gamma-Ray Bursts
• Achieving the fundamental quantum limit of linear waveform estimation
• Disformal transformations on the CMB
• Evolution of scalar fields surrounding black holes on compactified constant mean curvature hypersurfaces
• Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
• Reheating signature in the gravitational wave spectrum from self-ordering scalar fields
• Rapidly evaluating the compact binary likelihood function via interpolation
• The propagating speed of relic gravitational waves and their refractive index during inflation
• Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
• Survey of gravitational wave memory in intermediate mass ratio binaries
• Parameter estimation of neutron star-black hole binaries using an advanced gravitational-wave detector network: Effects of the full post-Newtonian waveform
• Neutron star mass in dark matter clumps
• A joint approach for reducing eccentricity and spurious gravitational radiation in binary black hole initial data construction
• Improved Coincident and Coherent Detection Statistics for Searches for Gravitational Wave Ringdown Signals
• Macroscopic quantum entanglement between an optomechanical cavity and a continuous field in presence of non-Markovian noise
• Relic gravitational waves in the frame of slow-roll inflation with a power-law potential and the detection
• Quantum functionalities via feedback amplification
• Subdominant Modes of Scalar Superradiant Instability and Gravitational Wave Beats
• An independent search of gravitational waves in the first observation run of advanced LIGO using cross-correlation
• An optimised gravitational wave follow-up strategy with the Australian Square Kilometre Array Pathfinder
• Possible confirmation of the existence of ergoregion by the Kerr quasinormal mode in gravitational waves from Pop III massive black hole binary
• A method for the experimental measurement of bulk and shear loss angles in amorphous thin films
• Gravitational lensing of gravitational waves: prospects for probing intermediate-mass black holes in galaxy lenses with global minima image
• Kerr-Enhanced Optical Spring
• The optical loss study of molecular layer for a cryogenic interferometric gravitational-wave detector
• Source localizations with the network of space-based gravitational wave detectors
• - Gravitational Waves - A Review on the Conceptual Foundations of Gravitational Radiation
• Low scatter and ultra-low reflectivity measured in a fused silica window
• Silk Damping in Scalar-Induced Gravitational Waves: A Novel Probe for New Physics
• Light Dark Matter Scattering in Gravitational Wave Detectors
• Horndeski fermion-boson stars
• Coherent coupling completes an unambiguous optomechanical classification framework
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity
• Quantum coherence of relic gravitons and Hanbury Brown-Twiss interferometry
• Detection of gravitational wave mixed polarization with single space-based detectors
• Numerically modeling Brownian thermal noise in amorphous and crystalline thin coatings
• The detection of quasinormal mode with $a/M\sim 0.95$ would prove a sphere $99\%$ soaking in the ergoregion of the Kerr space-time
• Estimation of the gravitational wave polarizations from a non template search
• Detectability of strongly lensed gravitational waves using model-independent image parameters
• Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia's Role
• A Rømer time-delay determination of the gravitational-wave propagation speed
• What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
• Stability of disformally coupled accretion disks
• Early warning of precessing neutron-star black-hole binary mergers with the near-future gravitational-wave detectors
• Global Optimization for Future Gravitational Wave Detectors' Sites
• Spline Based Search Method For Unmodeled Transient Gravitational Wave Chirps
• Note on Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals: Retrograde Orbits
• Length sensing and control of a Michelson interferometer with Power Recycling and Twin Signal Recycling cavities
• Maximal GW amplitude from bubble collisions in supercooled phase transitions
• Template-space metric for searches for gravitational waves from the inspiral, merger and ringdown of binary black holes
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• Exploring the distance-redshift relation with gravitational wave standard sirens and tomographic weak lensing
• Einstein-Klein-Gordon system via Cauchy-characteristic evolution: Computation of memory and ringdown tail
• Radiative Thermal Noise for Transmissive Optics in Gravitational-Wave Detectors
• Exploring dark photons via a subfrequency laser searchin gravitational wave detectors
• Two sides of the same coin: the F-statistic and the 5-vector method
• Analytic formula for the dynamics around inflation end and implications on primordial gravitational waves
• Gravitational Waves from Metastable Cosmic Strings in Supersymmetric New Inflation Model
• Prospects for reconstructing the gravitational-wave signals from core-collapse supernovae with Advanced LIGO-Virgo and the BayesWave algorithm
• How close can we approach the event horizon of the Kerr black hole from the detection of the gravitational quasinormal modes?
• Self-forced evolutions of an implicit rotating source: A natural framework to model comparable and intermediate mass-ratio systems from inspiral through ringdown
• Prospects for intermediate mass black hole binary searches with advanced gravitational-wave detectors
• Design study of the KAGRA output mode-cleaner
• The potential of advanced ground-based gravitational wave detectors to detect generic deviations from general relativity
• Point Absorber Limits to Future Gravitational-Wave Detectors
• Stable optical spring in aLIGO detector with unbalanced arms and in Michelson-Sagnac interferometer
• Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM
• High Speed Source Localization in Searches for Gravitational Waves from Compact Object Collisions
• Linear dynamics and classical tests of the gravitational quantum field theory
• Electromagnetic waves from neutron stars and black holes driven by polar gravitational perturbations
• The origin channels of hierarchical binary black hole mergers in the LIGO-Virgo-KAGRA O1, O2, and O3 runs
• Minimally modified gravity with auxiliary constraints formalism
• Measurement of Tidal Deformability in the Gravitational Wave Parameter Estimation for Nonspinning Binary Neutron Star Mergers
• Gravitational waves from cosmic strings for pedestrians
• Angular instability in high optical power suspended cavities
• First-step experiment in developing optical-spring quantum locking for DECIGO: sensitivity optimization for simulated quantum noise by completing the square
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Gas cooling of test masses for future gravitational-wave observatories
• Neutrino masses and ordering via multimessenger astronomy
• Corrections to the gravitational wave phasing
• Detection of GW200105 with a targeted eccentric search
• Recent LIGO-Virgo discoveries
• X- and Gamma-ray astrophysics in the era of Multi-messenger astronomy
• Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers
• Advanced technologies for future ground-based, laser-interferometric gravitational wave detectors
• New semicoherent targeted search for continuous gravitational waves from pulsars in binary systems
• Detection of short high-energy transients in the localuniverse with SVOM/ECLAIRs
• Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
• Comparison and application of different post-Newtonian models for inspiralling stellar-mass binary black holes with space-based GW detectors
• Primordial Black Holes and Gravitational Waves in the $U(1{)}_{B-L}$ Extended Inert Doublet Model: A First-Order Phase Transition Perspective
• The capability of the Australian Square Kilometre Array Pathfinder to detect prompt radio bursts from neutron star mergers
• Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground-based detectors
• Gravitational Wave Probe of Primordial Black Hole Origin via Superradiance
• Estimate of the radius responsible for quasinormal modes in the extreme Kerr limit and asymptotic behavior of the Sasaki-Nakamura transformation
• WINTER on S250206dm: A near-infrared search for an electromagnetic counterpart to a gravitational-wave event
• Uncovering faint lensed gravitational-wave signals and reprioritizing their follow-up analysis using galaxy lensing forecasts with detected counterparts
• Polarization Properties of the Electromagnetic Response to High-frequency Gravitational Wave
• Gravitational light deflection in Earth-based laser cavity experiments
• Constraining self-interactions of a massive scalar field using scalar gravitational waves from stellar core collapse
• Arm locking in conjunction with time-delay interferometry
• Exact solutions of primordial gravitational waves
• Tests of cryogenic Fabry-Perot cavity with mirrors on different substrates
• Review of Conformally Flat Approximation for Binary Neutron Star Initial Conditions
• Folding Gravitational-Wave Interferometers
• Stochastic backgrounds of gravitational waves from cosmological sources - The role of dark energy
• Gravitational Lensing of Core Collapse Supernova Gravitational Wave Signals
• First joint observation by the underground gravitational-wave detector, KAGRA, with GEO600
• Cryogenic optical shadow sensors for future gravitational wave detectors
• Atmospheric Newtonian noise modeling for third-generation gravitational wave detectors
• Development of advanced photon calibrator for Kamioka gravitational wave detector (KAGRA)
• Gravitational wave science with laser interferometers and pulsar timing
• Three mode interaction noise in laser interferometer gravitational wave detectors
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• Photothermal effect in macroscopic optomechanical systems with an intracavity nonlinear optical crystal
• Learning Transient Universe in Near-Ultraviolet By Wide-angle Cameras
• Conceptual design and science cases of a juggled interferometer for gravitational wave detection
• Synthetic streams in a Gravitational Wave inspiral search with a multi-detector network
• Quantum noise reduction techniques in KAGRA
• Confronting Inflation Models with the Coming Observations on Primordial Gravitational Waves
• Quasi-normal acoustic oscillations in the transonic Bondi flow
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Connecting Numerical Relativity and Data Analysis of Gravitational Wave Detectors
• Detecting Unmodeled, Source-dependent Signals in Gravitational Waves with SCoRe
• Compact object populations over cosmic time I. BOSSA: a Binary Object environment-Sensitive Sampling Algorithm
• Multi-Messenger Astrophysics with THESEUS in the 2030s
• A potential third-generation gravitational-wave detector based on autocorrelative weak-value amplification
• Particle Conversions Beyond the WKB Approximation and Solar-Induced Gravitational Waves from Dark Photon Dark Matter
• Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
• Diffraction losses of a Fabry-Perot cavity with nonidentical non-spherical mirrors
• Probing the equation of state of neutron stars with captured primordial black holes
• TOrsion-Bar Antenna: A Ground-Based Detector for Low-Frequency Gravity Gradient Measurement
• Detection of gravitational waves by light perturbation
• Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
• Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Investigating Binary Black Hole Mergers with Principal Component Analysis
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• Rotations of the polarization of a gravitational wave propagating in Universe
• Guided Lock of a Suspended Optical Cavity Enhanced by a Higher Order Extrapolation
• Optimal follow-up observations of gravitational wave events with small optical telescopes
• Dynamical friction from scalar dark matter in the relativistic regime
• Imprints of relic gravitational waves on pulsar timing
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Study of statistical properties of hybrid statistic in coherent multi-detector compact binary coalescences Search
• The Virgo Newtonian calibration system for the O4 observing run
• Investigation of Mechanical Properties of Cryogenically Treated Music Wire
• Target-based Optimization of Advanced Gravitational-Wave Detector Network Operations
• Performance comparison of multi-detector detection statistics in targeted compact binary coalescence GW search
• Impact of ultralight bosonic dark matter on the dynamical bar-mode instability of rotating neutron stars
• 3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
• Adaptive Modeling of Correlated Noise in Space-Based Gravitational Wave Detectors
• Cost-benefit analysis for commissioning decisions in GEO600
• A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Astrophysical and Cosmological Relevance of the High-Frequency Features in the Stochastic Gravitational-Wave Background
• Comprehensive analysis of dissipative effects in the induced gravitational waves
• Resonant behavior and stability of a linear three-mirror cavity
• Fighting Newtonian Noise with Gradient-Based Optimization at the Einstein Telescope
• Statistical biases in parametrized searches for gravitational-wave polarizations
• Neutron star evolution by combining discontinuous Galerkin and finite volume methods
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• Decline of the current quadrupole moment during the merger phase of binary black hole coalescence
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Discrimination of metric theories
• Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
• Tests of scalar polarizations with multi-messenger events
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Pulsar timing residuals due to individual non-evolving gravitational wave sources
• Quantum mechanical interaction of matter with the scalar mode of gravitational wave in modified gravity theories
• Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
• Upper Limit to the Transverse to Longitudinal Motion Coupling of a Waveguide Mirror
• Detectability of a spatial correlation between stellar-mass black hole mergers and Active Galactic Nuclei in the Local Universe
• Search for sub-solar primordial black holes in low mass ratio binaries with LIGO-Virgo O2 data and implications for the primordial black hole dark matter fraction
• Extracting the orbital axis from gravitational waves of precessing binary systems
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Demonstration of tilt sensing using a homodyne quadrature interferometric translational sensor