TianQin: a space-borne gravitational wave detector

Abstract

TianQin is a proposal for a space-borne detector of gravitational waves in the millihertz frequencies. The experiment relies on a constellation of three drag-free spacecraft orbiting the Earth. Inter-spacecraft laser interferometry is used to monitor the distances between the test masses. The experiment is designed to be capable of detecting a signal with high confidence from a single source of gravitational waves within a few months of observing time. We describe the preliminary mission concept for TianQin, including the candidate source and experimental designs. We present estimates for the major constituents of the experiment's error budget and discuss the project's overall feasibility. Given the current level of technology readiness, we expect TianQin to be flown in the second half of the next decade.

32 pages, 4 figures, to be published in Class. Quantum Grav

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• Circularly polarized scalar induced gravitational waves from the Chern-Simons modified gravity
• Periodic orbits and their gravitational wave radiations in black hole with dark matter halo
• Low Latency Detection of Massive Black Hole Binaries
• Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation
• Angular correlation as a novel probe of supermassive primordial black holes
• Sound velocity effects on the phase transition gravitational wave spectrum in the sound shell model
• Advancing Space-Based Gravitational Wave Astronomy: Rapid Parameter Estimation via Normalizing Flows
• Gravitational waves from tidal disruption events: an open and comprehensive catalogue
• Fully Relativistic Treatment of Extreme Mass-Ratio Inspirals in Collisionless Environments
• STOLAS: STOchastic LAttice Simulation of cosmic inflation
• Constraining the Extra Polarization Modes of Gravitational Waves with Double White Dwarfs
• Quasinormal Modes for Dynamical Black Holes
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals
• Slaying Axion-Like Particles via Gravitational Waves and Primordial Black Holes from Supercooled Phase Transition
• Detecting Strong Gravitational Lensing of Gravitational Waves with TianQin
• Bound Orbits and Gravitational Wave Radiation Around the Hairy Black Hole
• Effect of Noise Estimation in Time-Domain Ringdown Analysis: A Case Study with GW150914
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1
• Analytic Solution for the Motion of Spinning Particles in Kerr Space-Time
• Scalar-Induced Gravitational Waves from Ghost Inflation and Parity Violation
• Eppur si muove: Evidence of disc precession or a sub-milliparsec SMBH binary in the QPE-emitting galaxy GSN 069
• Motion deviation of test body induced by spin and cosmological constant in extreme mass ratio inspiral binary system
• Catastrogenesis with unstable ALPs as the origin of the NANOGrav 15 yr gravitational wave signal
• The Large Magellanic Cloud Revealed in Gravitational Waves with LISA
• Evolution of AM CVn binaries with WD donors
• Sensitivity to Dark Sector Scales from Gravitational Wave Signatures
• Constrains on the electric charges of the binary black holes with GWTC-1 events
• Velocity Distribution of Dark Matter Spike around Schwarzschild Black Holes and Effects on Gravitational Waves from EMRIs
• Analytical effective-one-body formalism for extreme-mass-ratio inspirals: eccentric orbits
• A combinatorial algebraic approach for the modified second-generation time-delay interferometry
• Detecting Ultralight Dark Matter Gravitationally with Laser Interferometers in Space
• Mapping the Outcomes of Stellar Evolution in the Disks of Active Galactic Nuclei
• Implication of Pulsar Timing Array Experiments on Cosmological Gravitational Wave Detection
• Matrix method for perturbed black hole metric with discontinuity
• PeV-Scale SUSY and Cosmic Strings from F-term Hybrid Inflation
• Invoking the virial theorem to understand the impact of (dry) mergers on the $M_{\mathrm{bh}}$-$\sigma$ relation
• Gravitational waves from bubble collisions in FLRW spacetime
• Accretion-modified stellar-mass black hole distribution and milli-Hz gravitational wave backgrounds from galaxy centre
• Quantum loop corrections in the modified gravity model of Starobinsky inflation with primordial black hole production
• Electroweak phase transition in the nearly aligned Higgs effective field theory
• Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Testing the Speed of Gravity with Black Hole Ringdown
• Ripples in Spacetime from Broken Supersymmetry
• Stochastic gravitational wave background due to gravitational wave memory
• High-order matrix method with delimited expansion domain
• GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins
• Constraints on compact dark matter from lensing of gravitational waves for the third-generation gravitational wave detector
• Gravitational atoms in the braneworld scenario
• Accelerated binary black holes in globular clusters: forecasts and detectability in the era of space-based gravitational-wave detectors
• Collapsing domain walls beyond $Z_2$
• RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
• Equatorial periodic orbits and gravitational waveforms in a black hole free of Cauchy horizon
• An implementation of Galactic white dwarf binary data analysis for MLDC-3.1
• Probing the Merger Rates of Supermassive Black Holes and Galaxies with Gravitational Waves
• Gauged Q-ball dark matter through a cosmological first-order phase transition
• Mergers of Maximally Charged Primordial Black Holes
• Continuous Gravitational Waves: A New Window to Look for Heavy Non-annihilating Dark Matter
• The (Black Hole Mass)-(Spheroid Stellar Density) Relations: $M_{\mathrm{BH}}$--$\mu$ (and $M_{\mathrm{BH}}$--$\Sigma$) and $M_{\mathrm{BH}}$--$\rho$
• A seven-Earth-radius helium-burning star inside a 20.5-min detached binary
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Multi-brane cosmology
• Scalar induced gravitational waves from Chern-Simons gravity during inflation era
• Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs
• Space-borne atom interferometric gravitational wave detections. Part III. Eccentricity on dark sirens
• Dynamics of extended bodies with spin-induced quadrupole in Kerr spacetime: generic orbits
• Measuring the Galactic Binary Fluxes with LISA: Metamorphoses and Disappearances of White Dwarf Binaries
• Astrometric Gravitational-Wave Detection via Stellar Interferometry
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• Accuracy of source localization for eccentric inspiraling binary mergers using a ground-based detector network
• Analytic properties of electromagnetic field of binary compact stars and electromagnetic precursors to gravitational waves
• Multi-Messenger Constraints on Magnetic Fields in Merging Black Hole-Neutron Star Binaries
• Gravitational memory effects in Brans-Dicke theory
• The three body first post-Newtonian effects on the secular dynamics of a compact binary near a spinning supermassive black hole
• Dilated convolutional neural network for detecting extreme-mass-ratio inspirals
• A rapid channel for the collisional formation and gravitational wave driven mergers of supermassive black hole seeds at high redshift
• Heavy dark matter and Gravitational waves
• Phenomenological relationship between eccentric and quasi-circular orbital binary black hole waveform
• Evaluating residual acceleration noise for TianQin gravitational waves observatory with an empirical magnetic field model
• Searching for Dark Clumps with Gravitational-Wave Detectors
• Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
• Strongly first-order electroweak phase transition by relatively heavy additional Higgs bosons
• Vector dark matter in supercooled Higgs portal models
• High bandwidth laser-frequency-locking for wideband noise suppression
• PhaseTracer2: from the effective potential to gravitational waves
• Motion of Spinning Particles around Electrically Charged Black Hole in Eddington-inspired Born-Infeld Gravity
• Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
• Examining the effects of dark matter spikes on eccentric intermediate mass ratio inspirals using N-body simulations
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Scalar induced gravitational waves in metric teleparallel gravity with the Nieh-Yan term
• Are single-field models of inflation and PBHs production ruled out by ACT observations?
• Effect of Earth-Moon's gravity on TianQin's range acceleration noise. II. Impact of orbit selection
• Plasma noise in TianQin time delay interferometry
• Effects of the space plasma density oscillation on the inter-spacecraft laser ranging for TianQin gravitational wave observatory
• Constraint on the mass of graviton with gravitational waves
• Cataclysmic variables are a key population of gravitational wave sources for LISA
• Exploring the nature of black hole and gravity with an imminent merging binary of supermassive black holes
• Model-dependent analysis method for energy budget of the cosmological first-order phase transition
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Testing gravity with Extreme-Mass-Ratio Inspirals
• Fast resolving Galactic binaries in LISA data and its ability to study the Milky Way
• Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
• A Catalogue of Ultracompact Mass-Transferring White Dwarf Binaries
• Uncovering a hidden black hole binary from secular eccentricity variations of a tertiary star
• Probing the Spins of Supermassive Black Holes with Gravitational Waves from Surrounding Compact Binaries
• Distinguishing black holes with and without spontaneous scalarization in Einstein-scalar-Gauss-Bonnet theories via optical features
• A long-period pre-ELM system discovered from LAMOST medium-resolution survey
• Angular bispectrum and trispectrum of scalar-induced gravitational waves: all contributions from primordial non-Gaussianity $f_{\mathrm{NL}}$ and $g_{\mathrm{NL}}$
• Inflation, space-borne interferometers and the expansion history of the Universe
• Very extreme mass-ratio bursts in the Galaxy and neighbouring galaxies in relation to space-borne detectors
• Gravitational waves from low-scale cosmic strings
• Massive White Dwarfs in the Galactic Center: A Chandra X-ray Spectroscopy of Cataclysmic Variables
• Constraining the evolution of Newton's constant with slow inspirals observed from spaceborne gravitational-wave detectors
• FIMP dark matter mediated by massive gauge boson around the phase transition period and the gravitational waves production
• Constraining changes in the merger history of (P)BH binaries with the stochastic gravitational wave background
• Towards a Consistent Calculation of the Lunar Response to Gravitational Waves
• Poisson-Arago spot for gravitational waves
• Polarization modes of gravitational waves in generalized Proca theory
• New Physics Search at the CEPC: a General Perspective
• Geometrized effective-one-body formalism for extreme-mass-ratio limits: Generic orbits
• How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way?
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• Influence of mass-ratio corrections in extreme-mass-ratio inspirals for testing general relativity
• Fast Multipole Methods for $N$-body Simulations of Collisional Star Systems
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Premerger detection of massive black hole binaries using deep learning
• Splitting the lentils: Clues to galaxy/black hole coevolution from the discovery of offset relations for non-dusty versus dusty (wet-merger-built) lenticular galaxies in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ diagram
• Polarized gravitational waves in the parity violating scalar-nonmetricity theory
• Full analytic expression of overlap reduction function for gravitational wave background with pulsar timing arrays
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• On the gauge dependence of scalar induced secondary gravitational waves during radiation and matter domination eras
• Gravitational waves from $\mathrm{SU}($$N$$)/Sp($$N$$)$ composite Higgs models
• Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
• Dark Matter Mounds: towards a realistic description of dark matter overdensities around black holes
• Post-Newtonian expansions of extreme mass ratio inspirals of spinning bodies into Schwarzschild black holes
• Gravitational Waves from Incomplete Inflationary Phase Transitions
• Electrostatic effect due to patch potentials between closely spaced surfaces
• Impact of combinations of time-delay interferometry channels on stochastic gravitational wave background detection
• Sensitivity of third-generation interferometers to extra polarizations in the Stochastic Gravitational Wave Background
• Resonant amplification of curvature perturbations in inflation model with periodical derivative coupling
• Cosmological phase transitions, gravitational waves and self-interacting dark matter in the singlet extension of MSSM
• Rotating white dwarf models with finite-temperature envelope
• Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term
• Overlap reduction functions for a polarized stochastic gravitational-wave background in the Einstein Telescope-Cosmic Explorer and the LISA-Taiji networks
• Doppler effect in TianQin time-delay interferometry
• Primordial non-Guassianity in inflation with gravitationally enhanced friction
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• No slip gravity in light of LISA standard sirens
• Post-adiabatic waveform-generation framework for asymmetric precessing binaries
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• Probing Stochastic Ultralight Dark Matter with Space-based Gravitational-Wave Interferometers
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Observing white dwarf tidal stripping with TianQin gravitational wave observatory
• Hydrodynamic effects on the filtered dark matter produced by a first-order phase transition
• Indication for a compact object next to a LIGO-Virgo binary black hole merger
• Dynamical Instability of Self-Gravitating Membranes
• Polarization modes of gravitational waves in general modified gravity: General metric theory and general scalar-tensor theory
• Probing new physics with multi-vacua quantum tunnelings beyond standard model through gravitational waves
• Stochastic gravitational wave background: birth from string-wall death
• On the decoherence effect of a stochastic gravitational perturbation on scalar matter and the possibility of its interferometric detection
• How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
• Numerical convergence of model Cauchy-characteristic extraction and matching
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• Formalism for power spectral density estimation for non-identical and correlated noise using the null channel in Einstein Telescope
• Time-crystal ground state and production of gravitational waves from QCD phase transition
• Constraining the EdGB Theory with Extreme Mass-Ratio Inspirals
• Subdominant Modes of Scalar Superradiant Instability and Gravitational Wave Beats
• On point-ahead angle control strategies for TianQin
• Arm locking using laser frequency comb
• Determining the nature of white dwarfs from low-frequency gravitational waves
• Stringent Tests of Gravity with Highly Relativistic Binary Pulsars in the Era of LISA and SKA
• Imprints of ultralight axions on the gravitational wave and pulsar timing measurement
• Bubble wall velocity and gravitational wave in the minimal left-right symmetric model
• Expected insights on type Ia supernovae from LISA's gravitational wave observations
• Actions of spinning compact binaries: Spinning particle in Kerr matched to dynamics at 1.5 post-Newtonian order
• GWSpace: a multi-mission science data simulator for space-based gravitational wave detection
• Source localizations with the network of space-based gravitational wave detectors
• Silk Damping in Scalar-Induced Gravitational Waves: A Novel Probe for New Physics
• Probing the Delay Time of Supermassive Black Hole Binary Mergers With Gravitational Waves
• Gravitational wave cosmology I: high frequency approximation
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Post-Newtonian effects in compact binaries with a dark matter spike: A Lagrangian approach
• Iterative time-domain method for resolving multiple gravitational wave sources in Pulsar Timing Array data
• $2\cdot 10^{-13}$ fractional laser frequency stability with a 7-cm unequal-arm Mach-Zehnder interferometer
• An Eclipsing 47 minute Double White Dwarf Binary at 400 pc
• Searching for gravitational-wave bursts with space-borne detectors
• Gravitational waves and primordial black holes from chirality imbalanced QCD first-order phase transition with $\mathcal{P}$ and $\mathcal{C}\mathcal{P}$ violation
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Decihertz gravitational waves from double white dwarf merger remnants
• The geometry and environment of repeating FRBs
• On second-order combinatorial algebraic time-delay interferometry
• Primordial Clocks within Stochastic Gravitational Wave Anisotropies
• Testing alternative theories of gravity with space-based gravitational wave detectors
• Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation
• White dwarf binary modulation can help stochastic gravitational wave background search
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Tidally excited oscillations in hot white dwarfs
• Gravitational waves from axions annihilation through quantum field theory
• Probing new fundamental fields with Extreme Mass Ratio Inspirals
• Gravitational waves and electromagnetic radiation from charged black hole binaries
• Bubble nucleation and gravitational wave from holography
• Secondary spins of extreme mass ratio inspirals: A probe to the formation channels
• Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Measuring the maximally allowed polarization states of the isotropic stochastic gravitational wave background with the ground-based detectors
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Shortcut in codimension-2 brane cosmology in light of GW170817
• SgrA${}^{\ast }$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral
• Effects of lunisolar perturbations on TianQin constellation: An analytical model
• Detection of gravitational wave mixed polarization with single space-based detectors
• Searching for wormholes with gravitational wave scattering
• Orbit design and thruster requirement for various constant-arm space mission concepts for gravitational-wave observation
• Possibility of a coordinated signaling scheme in the Galaxy and SETI experiments
• Continuous gravitational waves from trapped magnetar ejecta and the connection to glitches and antiglitches
• Induced gravitational waves from statistically anisotropic scalar perturbations
• One-loop corrections to the E-type $\alpha$-attractor models of inflation and primordial black hole production
• Spherical harmonic analysis of anisotropies in polarized stochastic gravitational wave background with interferometry experiments
• 3 m$\times$3 m heterolithic passive resonant gyroscope with cavity length stabilization
• Evolution of Massive Black Hole Binaries in Collisionally Relaxed Nuclear Star Clusters -- Impact of Mass Segregation
• Reanalyzing the ringdown signal of GW150914 using the F-statistic method
• Duality between Seiberg-Witten Theory and Black Hole Superradiance
• Gravitational Radiation from Eccentric Binary Black Hole System in Dynamical Chern-Simons Gravity
• Qusinormal oscillations and late-time tail of massless scalar perturbations of a magnetized black hole in Rastall gravity
• Light propagation in the field of the N-body system and the application in the TianQin mission
• Scalar induced gravitational waves review
• Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
• Multi-messenger observations of double neutron stars in Galactic disk with gravitational and radio waves
• Fundamental Physics and Cosmology with TianQin
• Distinguish the environmental effects and modified theory of gravity with multiple massive black-hole binaries
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Prospects for Axion Dark Matter Searches at LISA-like Interferometers
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• Multiple peaks in gravitational waves induced from primordial curvature perturbations with non-Gaussianity
• Polarization modes of gravitational waves in general Einstein-vector theory
• Constraining the stochastic gravitational wave background using the future lunar seismometers
• Scalar induced gravitational waves in chiral scalar-tensor theory of gravity
• Gravitational Wave Signal Extraction Against Non-Stationary Instrumental Noises with Deep Neural Network
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• Gravitational waves from cosmic superstrings and gauge strings
• Gravitational wave spectral synthesis
• The Effect of Non-minimally Coupled Scalar Field on Gravitational Waves from First-order Vacuum Phase Transitions
• Modern Cosmology, an Amuse-Gueule
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Anisotropies of cosmological gravitational wave backgrounds in non-flat spacetime
• Intermediate-mass ratio inspirals in merging elliptical galaxies
• Gravitational waves and monopoles dark matter from first-order phase transition
• Searching for continuous gravitational waves from slowly spinning neutron stars with DECIGO, Big Bang Observer, Einstein Telescope and Cosmic Explorer
• Extracting parity-violating gravitational waves from projected tidal force tensor in three dimensions
• Searching for gravitational waves from stellar-mass binary black holes early inspiral
• A back-linked Fabry-Perot interferometer for space-borne gravitational wave observations
• Progress in Nuclear Astrophysics of East and Southeast Asia
• Gravitational Waves of GUT Phase Transition during Inflation
• The FAST Galactic Plane Pulsar Snapshot Survey: VII. Six millisecond pulsars in compact orbits with massive white dwarf companions
• On-axis Optical Bench for Laser Ranging Instruments in future gravity missions
• Ultra-compact binary pulsars as continuous dual-line gravitational wave sources
• Two Approaches for the Passive Charge Management of Contactless Test Masses
• Tracking Down the Route to the SM with Inflation and Gravitational Waves
• Unveiling the solution to the final-parsec problem by combining milli-Hertz gravitational-wave observation and AGN survey
• Gravitational wave fluxes on generic orbits in near-extreme Kerr spacetime: higher spin and large eccentricity
• Phase Transitions and Gravitational Waves in a Model of ${\mathbb{Z}}_3$ Scalar Dark Matter
• Probing the axion-photon coupling with space-based gravitational waves detectors
• Breaking black-hole uniqueness at supermassive scales
• Space-based optical lattice clocks as gravitational wave detectors in search for new physics
• Calibration of the in-orbit center-of-mass of TaiJi-1
• Assessing the systematic errors of extreme-mass-ratio inspirals waveforms for testing general relativity
• The orbital evolution of the tidally stripped star and disk-driven stable mass transfer for QPEs in GSN 069
• Orbit Design for Space Atom-Interferometer AIGSO
• Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
• Testing gravitational waveform models using angular momentum
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• Detecting the dark sector through scalar-induced gravitational waves
• Measuring mass transfer of AM CVn binaries with a space-based gravitational wave detector
• Population Synthesis of Black Hole Binaries with Compact Star Companions
• Measuring the anisotropies in astrophysical and cosmological gravitational-wave backgrounds with Taiji and LISA networks
• Improving the scalability of Gaussian-process error marginalization in gravitational-wave inference
• Dealing with data gaps for TianQin with massive black hole binary signal
• Parameter inference for coalescing massive black hole binaries using deep learning
• Linear dynamics and classical tests of the gravitational quantum field theory
• Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
• Cosmic superstrings in large volume compactifications: PTAs, LISA and time-varying tension
• Gravitational Wave Signatures from Periodic Orbits around a non-commutative inspired black hole surrounded by quintessence
• Observable-based reformulation of time-delay interferometry
• G4.8+6.2, a possible kilonova remnant?
• Astrophysics with the Laser Interferometer Space Antenna
• Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications
• Universal Density and Velocity Distributions of Dark Matter around Massive Black Holes
• Self-interaction effects on the Kerr black hole superradiance and their observational implications
• Demonstration of a dual-pass differential Fabry-Perot interferometer for future interferometric space gravitational wave antennas
• Imprints of extra dimensions in eccentric extreme-mass-ratio inspirals gravitational waveforms
• Hot, cold, and multi-component accretion flows around supermassive black hole binaries
• Toward Second-Order Self-Force for Eccentric Extreme-Mass Ratio Inspirals in Schwarzschild Spacetime
• Probing intermediate-mass black hole binaries with the Lunar Gravitational-wave Antenna
• Post-adiabatic waveforms from extreme mass ratio inspirals in the presence of dark matter
• Quantum Corrected Geodesic Motion in Polymer Kerr-like Spacetime
• Systematic bias in LISA ringdown analysis due to waveform inaccuracy
• Dark I-Love-Q
• Probing WIMPs in space-based gravitational wave experiments
• Non-Gaussianities and Primordial Black Holes
• Dynamics of bubble walls at the electroweak phase transition
• Meso-inflationary Peccei-Quinn symmetry breaking with non-minimal coupling
• Stochastic Gravitational Wave Background from PBH-ABH Mergers
• Gravitational Wave From Axion-like Particle Inflation
• Prospects of constraining on the polarizations of gravitational waves from binary black holes using space- and ground-based detectors
• Crescendo Beyond the Horizon: More Gravitational Waves from Domain Walls Bounded by Inflated Cosmic Strings
• Probing PeV scale SUSY-breaking with Satellite Galaxies and Primordial Gravitational Waves
• Effect of solar free oscillations on TianQin's range acceleration noise
• Clock synchronization and light-travel-time estimation for space-based gravitational-wave detectors
• Electroweak Phase Transition in Two Scalar Singlet Model with pNGB Dark Matter
• The first law of binary black hole scattering
• Intermediate mass ratio inspirals in dark matter halos
• Effect of Earth-Moon's gravity on TianQin's range acceleration noise. III. An analytical model
• Testing dispersion of gravitational waves from eccentric extreme-mass-ratio inspirals
• Gravitational-wave memory effects in the Damour-Esposito-Farèse extension of Brans-Dicke theory
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• Escape, bound and capture geodesics in local static coordinates in Schwarzschild spacetime
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• Probing a Lorentz-violating parameter from orbital precession of the S2 star around the galactic centre supermassive black hole
• A Systematic Approach for Inertial Sensor Calibration of Gravity Recovery Satellites and Its Application to Taiji-1 Mission
• On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations
• Gravitational waves from first-order phase transitions in Majoron models of neutrino mass
• CP-violating effects on gravitational waves in a complex singlet extension of the Standard Model with degenerate scalars
• Spherical inspirals of spinning bodies into Kerr black holes
• Primordial black holes save $R^2$ inflation
• Evolution and detection of vector superradiant instabilities
• Gravitational waves from vacuum bubbles: Ultraviolet dependence on wall thickness
• Probing Kalb-Ramond field with extreme mass ratio inspirals
• Observable effect of quantized cylindrical gravitational waves
• Arm locking in conjunction with time-delay interferometry
• The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
• Prospects for the Observation of Continuous Gravitational Waves from Deformed Fast-spinning White Dwarfs
• Propagation and lensing of gravitational waves in Palatini $f(\hat{R})$ gravity
• Probing Spin-2 Ultralight Dark Matter with Space-based Gravitational Wave Detectors in the mHz Regime
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• Experiment demonstration of tilt-to-length coupling suppression by beam-alignment-mechanism
• Intermediate-mass-ratio inspirals with general dynamical friction in dark matter minispikes
• Identifying Disappearance of a White Dwarf Binary with LISA
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• The Dawn of Black Holes
• Extreme resonant eccentricity excitation of stars around merging black-hole binary
• Can asteroid-mass PBHDM be compatible with catalyzed phase transition interpretation of PTA?
• Different effects of the Lorentz and Gaussian bump functions on the formation of primordial black holes and secondary gravitational waves
• A protocol of potential advantage in the low frequency range to gravitational wave detection with space based optical atomic clocks
• Probing Supermassive Black Hole Binaries with Orbital Resonances of Laser-Ranged Satellite
• Compact Binary Coalescence Gravitational Wave Signals Counting and Separation
• Gravitational wave lensing: probing Fuzzy Dark Matter with LISA
• A full waveform model for arbitrarily axis-symmetric black hole mergers
• Gravitational Wave Duet by Resonating Binary Black Holes within Ultralight Dark Matter
• Testing Lorentz symmetry with space-based gravitational-wave detectors
• NICER observations reveal doubled timescales in Ansky's quasi-periodic eruptions (QPEs)
• Tracking the Long-Term GW Phase Evolution for HM Cancri-like Binaries with LISA
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• The first OGLE-discovered ultracompact X-ray binary is an intermediate polar
• Sky localization of space-based detectors with time-delay interferometry
• Primordial black holes and scalar-induced gravitational waves from the polynomial attractor model
• On the effect of pulsar evaporation on the cooling of white dwarfs
• Potential Tertiary Effects on the LISA Verification Binary HM Cancri
• Massive vector field perturbations in the Schwarzschild spacetime from supersymmetric gauge theory
• Distinguishing Monochromatic Signals in LISA and Taiji: Ultralight Dark Matter versus Gravitational Waves
• Electroweak Phase Transition, Gravitational Waves and Collider Probes in Multi-Scalar Dark Matter Scenarios
• Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
• Distinguishing dark matter halos with Extreme mass ratio inspirals
• Adaptive extended Kalman filter and point ahead angle prediction in the detection of gravitational waves in space
• Enhancement of small-scale induced gravitational waves from the soliton/oscillon domination
• Cold Atoms in Space: Community Workshop Summary and Proposed Road-Map
• Dependence of Electrostatic Patch Force Evaluation on the Lateral Resolution of Kelvin Probe Force Microscopy
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
• Extreme mass-ratio inspirals and extra dimensions: Insights from modified Teukolsky framework
• DeepSSM: an emulator of gravitational wave spectra from sound waves during cosmological first-order phase transitions
• Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
• Conceptual design and science cases of a juggled interferometer for gravitational wave detection
• A hydrodynamical description of gravitational waves
• Inflation, Proton Decay and Gravitational Waves from Metastable Strings in $SU(4{)}_C\times SU(2{)}_L\times U(1{)}_R$ Model
• Probing the Dark Solar System: Detecting Binary Asteroids with a Space-Based Interferometric Asteroid Explorer
• Dark matter production accompanied by gravitational wave signals during cosmological phase transitions
• On the noise effect of test mass surface roughness in spaceborne gravitational wave detectors
• Probing the equation of state of neutron stars with captured primordial black holes
• The Role of r-Modes in Pulsar Spin-down, Pulsar Timing, and Gravitational Waves
• Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
• Improved model of large-field inflation with primordial black hole production in Starobinsky-like supergravity
• Exploring Time Delay Interferometry Ranging as a Practical Ranging Approach in the Bayesian Framework
• Cross-Correlated Force Measurement for Thermal Noise Reduction in Torsion Pendulum
• Extracting overlapping gravitational-wave signals of galactic compact binaries: a mini review
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
• Particle Conversions Beyond the WKB Approximation and Solar-Induced Gravitational Waves from Dark Photon Dark Matter
• Dynamical friction from scalar dark matter in the relativistic regime
• Effects of orbital eccentricity on continuous gravitational waveforms from triaxially deformed precessing neutron stars in tight binaries
• Circularly Polarized Gravitational Wave Background Search with a Network of Space-borne Triangular Detectors
• Signal-to-noise Ratio Analytic Formulae of the Inspiral Binary Black Holes in TianQin
• Adiabatic Duality: Duality of cosmological models with varying slow-roll parameter and sound speed
• SgrA* spin and mass estimates through the detection of multiple extremely large mass-ratio inspirals
• Gravitational wave and dark matter from Axion-Higgs string
• Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
• Fundamental quantum limits for detecting ultrahigh frequency gravitational waves
• Gravitational decoherence: a non relativistic spin 1/2 fermionic model
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Time delay interferometry with minimal null frequencies and shortened time span
• A practical Bayesian method for gravitational-wave ringdown analysis with multiple modes
• Constraints on the Scale Parameter of Regular Black Hole in Asymptotically Safe Gravity from Extreme Mass Ratio Inspirals
• Constraining the Deviation of Kerr Metric via Bumpy Parameterization and Particle Swarm Optimization in Extreme Mass-Ratio Inspirals
• Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals
• Black holes as telescopes: Discovering supermassive binaries through quasi-periodic lensed starlight
• A note on the Kerr-Newman metric in five dimensions
• Search for Higher Harmonic Signals from Close White Dwarf Binaries in the mHz Band
• A Multimessenger Strategy for Downselecting the Orientations of Galactic Close White Dwarf Binaries
• Freeze-in gravitational waves and dark matter in warm inflation
• A New Source of Phase Transition Gravitational Waves: Heavy Particle Braking Across Bubble Walls
• Scalar-induced gravitational waves in spatially covariant gravity
• Bayesian Analysis of Wave-Optics Gravitationally Lensed Massive Black Hole Binaries with Space-Based Gravitational Wave Detector
• QNM families: classification and competition
• Co-evolution of Nuclear Star Clusters and Massive Black Holes: Extreme Mass-Ratio Inspirals
• Scalar-induced gravitational waves including isocurvature perturbations with lattice simulations
• Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings
• Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• Holographic Principle and the Second Law in Stephani Cosmology Revisited
• Searching for supermassive black holes binaries within SRG/eROSITA-De I: Properties of the X-ray selected candidates
• Quantum theory of cross-correlation heterodyne detection
• Geometric tilt-to-length coupling in precision interferometry: mechanisms and analytical descriptions
• Space-based Gravitational Wave Observatories
• Toward an inner connection of SNe Ic, SLSNe Ic, XRF connected SNe, SNe Ic-BL, and GRB connected SNe
• Pseudospectrum of Reissner-Nordström black holes: quasinormal mode instability and universality
• Imprints of an early matter-dominated era arising from dark matter dilution mechanism on cosmic string dynamics and gravitational wave signatures
• Geometric properties of slowly rotating black holes embedded in matter environments
• Observing Double White Dwarfs with the Lunar GW Antenna
• Rigorous analytic solution to the gravitational-wave overlapping event rates
• Gravitational waves from equatorially eccentric extreme mass ratio inspirals around swirling Kerr black holes
• Adaptive Modeling of Correlated Noise in Space-Based Gravitational Wave Detectors
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Parameter Estimation Precision with Geocentric Gravitational Wave Interferometers: Monochromatic Signals
• Ultra-compact X-ray Binaries: A Review
• Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
• Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
• Gauge-independent Gravitational Waves from Cogenesis in a $B-L$ Conserving Universe
• Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions
• Bayesian analysis of the complex singlet model with phase transition gravitational waves
• Periodic orbits and gravitational waveforms of black holes in bumblebee gravity
• Classification of radial Kerr geodesic motion
• Neutron star evolution by combining discontinuous Galerkin and finite volume methods
• Perturbative Frequency Expansion for Nearly Monochromatic Binary Black Holes Detectable with LISA
• Measurement of the central Galactic black hole by extremely large mass-ratio inspirals
• Temperature-insensitive fused-tapered fiber couplers based on negative thermal expansion material coating
• Shadow constraints of charged black hole with scalar hair and gravitational waves from extreme mass ratio inspirals
• Lensing by primordial black holes: constraints from gravitational wave observations
• Observing Orbital Decay in the Ultracompact Hot Subdwarf Binary System ZTFJ213056.71+442046.5
• Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories
• Gravitational waveforms from periodic orbits around a novel regular black hole
• Search for Continuous Gravitational Wave Signals in Pulsar Timing Residuals: A New Scalable Approach with Diffusive Nested Sampling
• Gravitational radiations from periodic orbits around a black hole in the effective field theory extension of general relativity
• Overlap reduction function for gravitational wave detectors in an expanding Universe
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• Preliminary forecasting constraint on scalar charge with LISA in non-vacuum environments
• Mass and spin coevolution of black holes inspiralling through dark matter
• Comprehensive analysis of dissipative effects in the induced gravitational waves
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Revisiting Singlet Fermion Dark Matter with a Scalar Portal: Connecting Higgs Phenomenology and Strong Electroweak Phase Transition
• Primordial black holes and induced gravitational waves from localized features in DBI inflation
• Compact binary system dynamics at the second post-Newtonian order: analytical formula of the coordinate time for eccentric and circular orbits
• GWAI: Artificial Intelligence Platform for Enhanced Gravitational Wave Data Analysis
• Confronting SO(10) GUTs with proton decay and gravitational waves
• Numerical computation of electromagnetically sourced nonlinear tails
• The evolutionary history of ultra-compact accreting binaries. I. Chemical abundances and formation channel of the eclipsing AM CVn system ZTF J225237.05-051917.4 from HST spectroscopy
• General Fourier expansion of post-Newtonian binary dynamics based on a quasi-Keplerian framework
• Bispectrum of induced gravitational waves in the poltergeist mechanism
• Detectability of compact intermediate-mass black hole binaries as low-frequency gravitational wave sources: the influence of dynamical friction of dark matter
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Rising Tides: Analytic Modeling of Tidal Effects in Binary Neutron Star Mergers
• Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
• A Catalog of First-Order Electroweak Phase Transitions in the Standard Model Effective Field Theory
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Demonstration of tilt sensing using a homodyne quadrature interferometric translational sensor
• Testing the Kerr nature with binary black hole inspirals
• Quantum Physics in Space
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• Exploring the parameter space of modified supergravity for double inflation and primordial black hole formation
• Probing Dark Matter's Gravitational Effects Locally with TianQin
• Evaluating statistical significance for massive black hole binary mergers with space-based gravitational wave detectors
• Extending the micro-Hertz detection horizons via orbital resonance effect for geocentric gravitational wave antennas
• Development of generic no-scale inflation
• Correlation of Gravitational Wave Background Noises and Statistical Loss for Angular Averaged Sensitivity Curves
• Tidal heating in detached double white dwarf binaries
• Generic effective sources for first-order in mass-ratio gravitational self-force calculations in Schwarzschild spacetime
• Gravitational-wave constraints on noncommutative spacetime from GW190814
• Precision requirements and innovative manufacturing for ultrahigh precision laser interferometry of gravitational-wave astronomy
• Quantum Search for Gravitational Wave of Massive Black Hole Binaries
• superB/NRPy: Scalable, Task-Based Numerical Relativity for 3G Gravitational Wave Science
• Testing Nambu-Goto approximation of cosmic string by lattice field simulations
• Gravitational wave complementarity and impact of NANOGrav data on gravitational leptogenesis: cosmic strings
• Merging of unequal mass binary black holes in non-axisymmetric galactic nuclei
• Capability for detection of GW190521-like binary black holes with TianQin
• Ringdown mode amplitudes of charged binary black holes
• Primordial black holes and scalar induced gravitational waves from sound speed resonance in non-minimal derivative coupling inflation model
• Distinguishing between dark-matter interactions with gravitational-wave detectors
• Investigating the Accretion Nature of Binary Supermassive Black Hole Candidate SDSS J025214.67-002813.7
• Primordial Black Hole Formation and Multimessenger Signals in a Complex Singlet Extension of the Standard Model
• Particles with precessing spin in Kerr spacetime: analytic solutions for eccentric orbits and homoclinic motion near the equatorial plane
• Initial acquisition requirements for optical cavities in the space gravitational wave antennae DECIGO and B-DECIGO
• Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources
• Modeling coupled constellation dynamics for TianQin under self-gravity
• Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model
• Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors
• Experimental Demonstration of an On-Axis Laser Ranging Interferometer for Future Gravity Missions
• Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands
• Analytical solutions of bound timelike geodesic orbits in effective-one-body frame
• The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
• Searching systematically for coupling of laser and phase-modulation noise in heterodyne interferometry
• Nonlinear tails of massive scalar fields around a black hole
• Gravitational wave background from mergers of large primordial black holes
• Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations
• Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals
• Chirping compact stars: gravitational radiation and detection degeneracy with binary systems A conceptual pathfinder for space-based gravitational-wave observatories
• Circularly polarized gravitational waves from parity-violating scalar-tensor theory
• Merger rates of intermediate-mass black hole binaries in nuclear star clusters
• Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes
• Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors
• Correlation analysis for isotropic stochastic gravitational wave backgrounds with maximally allowed polarization degrees
• A Falsifiable Timing Test for the Double-White-Dwarf Model of Long-Period Transients
• Complementary probe of dark matter blind spots by lepton colliders and gravitational waves
• Direct N-body simulations of rotating and extremely massive Population III star clusters
• Primordial Black Holes: A Review of Formation and Evolution
• Extreme Mass Ratio Inspirals in Light of Quasi-periodic Eruptions: Milli-Hertz Gravitational Wave Background
• Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes
• Efficient Evaluation of Gravitational Lensing Amplification Factors: A Deep Learning Framework
• Gravitational-wave standard sirens and application in cosmology
• Detecting Lorentz-violation induced by a tensor field with S-star's motion around Sgr A*
• Wigner multiplets in QFT: dark sector and CPT-violating scenarios
• Impact of particle production during inflation on the CMB detection
• Detectability of continuous gravitational waves from planetary-mass companions orbiting compact stars
• Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant