Gravitational Wave Astronomy With TianQin

Abstract

The opening of the gravitational wave window has significantly enhanced our capacity to explore the universe's most extreme and dynamic sector. In the mHz frequency range, a diverse range of compact objects, from the most massive black holes at the farthest reaches of the Universe to the lightest white dwarfs in our cosmic backyard, generate a complex and dynamic symphony of gravitational wave signals. Once recorded by gravitational wave detectors, these unique fingerprints have the potential to decipher the birth and growth of cosmic structures over a wide range of scales, from stellar binaries and stellar clusters to galaxies and large-scale structures. The TianQin space-borne gravitational wave mission is scheduled for launch in the 2030s, with an operational lifespan of five years. It will facilitate pivotal insights into the history of our universe. This document presents a concise overview of the detectable sources of TianQin, outlining their characteristics, the challenges they present, and the expected impact of the TianQin observatory on our understanding of them.

TianQin Gravitational Wave Whitepaper, 73 pages, 30 figures. Update to match published version

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• TianQin: a space-borne gravitational wave detector
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• The First Stars
• Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
• Observational constraints on growth of massive black holes
• The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
• Physics, Astrophysics and Cosmology with Gravitational Waves
• Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
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• Formation of the First Supermassive Black Holes
• Kerr black holes with scalar hair
• Using gravitational-wave standard sirens
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• An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
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• Pulsational Pair-Instability Supernovae
• Intermediate-Mass Black Holes
• The Black Hole Mass Distribution in the Galaxy
• The runaway growth of intermediate-mass black holes in dense star clusters
• The construction and use of LISA sensitivity curves
• Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
• The Assembly of the First Massive Black Holes
• Tests of General Relativity with GW170817
• A new route towards merging massive black holes
• Can environmental effects spoil precision gravitational-wave astrophysics?
• A relativistic jetted outburst from a massive black hole fed by a tidally disrupted star
• Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
• Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
• Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei
• Dwarf Galaxies with Optical Signatures of Active Massive Black Holes
• PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star
• One Hundred First Stars : Protostellar Evolution and the Final Masses
• Hydrodynamical Simulations to Determine the Feeding Rate of Black Holes by the Tidal Disruption of Stars: The Importance of the Impact Parameter and Stellar Structure
• Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
• The Mass Distribution of Stellar-Mass Black Holes
• Gravitational waves from scattering of stellar-mass black holes in galactic nuclei
• Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"
• The First Galaxies
• How Do Massive Black Holes Get Their Gas?
• Production of Intermediate-Mass Black Holes in Globular Clusters
• Science with the space-based interferometer eLISA. I: Supermassive black hole binaries
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• Formation of Primordial Stars in a LCDM Universe
• Simulations on a Moving Mesh: The Clustered Formation of Population III Protostars
• The gravitational wave signal from the Galactic disk population of binaries containing two compact objects
• The promise of multi-band gravitational wave astronomy
• Secular evolution of compact binaries near massive black holes: gravitational wave sources and other exotica
• Tidal Disruption Events
• Dynamical Friction and Galaxy Merging Timescales
• Accretion during the merger of supermassive black holes
• Stellar disk in the galactic center -- a remnant of a dense accretion disk?
• Population synthesis for double white dwarfs I.Close detached systems
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• Stellar Dynamics in the Galactic centre: Proper Motions and Anisotropy
• Formation of gas disks in merging galaxies
• Swift J2058.4+0516: Discovery of a Possible Second Relativistic Tidal Disruption Flare?
• Formation and Evolution of Compact Object Binaries in AGN Disks
• The Formation and Fragmentation of Disks around Primordial Protostars
• Protostellar Feedback Halts the Growth of the First Stars in the Universe
• Model Waveform Accuracy Standards for Gravitational Wave Data Analysis
• Fermi GBM Observations of LIGO Gravitational Wave event GW150914
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• Revised Rates of Stellar Disruption in Galactic Nuclei
• The Quest for B Modes from Inflationary Gravitational Waves
• The TianQin project: current progress on science and technology
• Protostar Formation in the Early Universe
• Progenitors of gravitational wave mergers: Binary evolution with the stellar grid-based code ComBinE
• Formation of the first three gravitational-wave observations through isolated binary evolution
• The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes
• A unified model for tidal disruption events
• The distribution and cosmic evolution of massive black hole spins
• Intermediate mass black holes in AGN disks: I. Production & Growth
• Dynamical Chern-Simons Modified Gravity I: Spinning Black Holes in the Slow-Rotation Approximation
• MOCCA-SURVEY Database I: Coalescing Binary Black Holes Originating From Globular Clusters
• Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole
• Formation of the First Stars
• Improving the open cluster census. II. An all-sky cluster catalogue with Gaia DR3
• Cosmological black hole spin evolution by mergers and accretion
• Concepts and status of Chinese space gravitational wave detection projects
• Binary black hole mergers from field triples: properties, rates and the impact of stellar evolution
• Primordial Star Formation under the Influence of Far Ultraviolet Radiation: 1540 Cosmological Halos and the Stellar Mass Distribution
• Radiative Models of Sgr A* from GRMHD Simulations
• The Mass Spectrum of the First Stars
• Evolution of Binary Compact Objects Which Merge
• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• Cosmology from the Chinese Space Station Optical Survey (CSS-OS)
• Long Term Evolution of Massive Black Hole Binaries
• The first stars: formation of binaries and small multiple systems
• Radiation Hydrodynamical Evolution of Primordial H II Regions
• Supermassive Black Hole Formation by Direct Collapse: Keeping Protogalactic Gas H_2--Free in Dark Matter Halos with Virial Temperatures T_vir >~ 10^4 K
• The effect of the metallicity-specific star formation history on double compact object mergers
• On stellar-mass black hole mergers in AGN disks detectable with LIGO
• Formation of Primordial Protostars
• Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus
• Formation of Primordial Supermassive Stars by Rapid Mass Accretion
• Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave
• Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars
• The Mass Function of Active Black Holes in the Local Universe
• Kerr black holes with Proca hair
• Primordial Star Formation under Far-ultraviolet radiation
• Rotating Black Holes in Dilatonic Einstein-Gauss-Bonnet Theory
• Hierarchical Black Hole Mergers in Active Galactic Nuclei
• Accretion onto the First Stellar Mass Black Holes
• The Assembly of Supermassive Black Holes at High Redshifts
• What is the Highest Plausible Redshift of Luminous Quasars?
• Short-period AM CVn systems as optical, X-ray and gravitational wave sources
• Merging black holes in young star clusters
• The origins of massive black holes
• Stellar-mass black holes in star clusters: implications for gravitational wave radiation
• Resonant Post-Newtonian Eccentricity Excitation in Hierarchical Three-body Systems
• The evolution of massive black holes and their spins in their galactic hosts
• Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries
• Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers
• The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View
• Fluctuations in the High-Redshift Lyman-Werner Background: Close Halo Pairs as the Origin of Supermassive Black Holes
• Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary-Binary Encounters
• Direct Formation of Supermassive Black Holes via Multi-Scale Gas Inflows in Galaxy Mergers
• Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
• Building up the Population III initial mass function from cosmological initial conditions
• The Formation of the First Stars II. Radiative Feedback Processes and Implications for the Initial Mass Function
• A tidal disruption event coincident with a high-energy neutrino
• Three Hypervelocity White Dwarfs in Gaia DR2: Evidence for Dynamically Driven Double-Degenerate Double-Detonation Type Ia Supernovae
• MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
• Runaway collisions in young star clusters. II. Numerical results
• Migration Traps in Disks Around Supermassive Black Holes
• Supermassive Stars in Quasar Disks
• The First Stars: Mass Growth Under Protostellar Feedback
• Hyper-Eddington accretion flows onto massive black holes
• Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections
• Mass Measurements of Stellar and Intermediate Mass Black-Holes
• Formation of massive black holes in rapidly growing pre-galactic gas clouds
• Relativistic Dynamics and Extreme Mass Ratio Inspirals
• Reconstructing the evolution of white dwarf binaries: further evidence for an alternative algorithm for the outcome of the common-envelope phase in close binaries
• The Submillimeter Bump in Sgr A* from Relativistic MHD Simulations
• A 20 Thousand Solar Mass Black Hole in the Stellar Cluster G1
• X-ray Quasi-Periodic Eruptions from two previously quiescent galaxies
• Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA
• JWST CEERS & JADES Active Galaxies at z = 4-7 Violate the Local $M_{\bullet }-M_{\star }$ Relation at $>3\sigma$: Implications for Low-Mass Black Holes and Seeding Models
• Fast prediction and evaluation of gravitational waveforms using surrogate models
• Consequences of Strong Compression in Tidal Disruption Events
• Three-dimensional simulations of super-critical black hole accretion disks --- luminosities, photon trapping and variability
• On the Life and Death of Satellite Haloes
• Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer
• Black hole triple dynamics: breakdown of the orbit average approximation and implications for gravitational wave detections
• Helium star donor channel for the progenitors of type Ia supernovae
• Growth and activity of black holes in galaxy mergers with varying mass ratios
• AGN as Potential Factories for Eccentric Black Hole Mergers
• Accretion-Driven Evolution of Black Holes: Eddington Ratios, Duty Cycles, and Active Galaxy Fractions
• Pulsational pair-instability supernovae in very close binaries
• A Sun-like star orbiting a black hole
• Active Galactic Nuclei in the Sloan Digital Sky Survey: II. Emission-Line Luminosity Function
• LISA verification binaries with updated distances from Gaia Data Release 2
• The cosmic merger rate of stellar black hole binaries from the Illustris simulation
• Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes
• X-ray quasi-periodic eruptions from the galactic nucleus of RX J1301.9+2747
• Physical parameters of the high-mass X-ray binary 4U1700-37
• The aftermath of the first stars: massive black holes
• Co-evolution of nuclear star clusters, massive black holes and their host galaxies
• Binary Black Hole Mergers from Planet-like Migrations
• Intermediate mass black holes in AGN disks II. Model predictions & observational constraints
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation
• Black Hole Mergers From Globular Clusters Observable by LISA I: Eccentric Sources Originating From Relativistic $N$-body Dynamics
• Evidence for Low Black Hole Spin and Physically Motivated Accretion Models from Millimeter VLBI Observations of Sagittarius A*
• The First Round Result from the TianQin-1 Satellite
• Multiband Gravitational-Wave Astronomy: Observing binary inspirals with a decihertz detector, B-DECIGO
• Massive binary black holes in galactic nuclei and their path to coalescence
• On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening
• eXTP -- enhanced X-ray Timing and Polarimetry Mission
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• Sagittarius A* Accretion Flow and Black Hole Parameters from General Relativistic Dynamical and Polarized Radiative Modeling
• The Observational Signatures of Supermassive Black Hole Seeds
• Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals
• A luminous, blue progenitor system for a type-Iax supernova
• Velocity Dispersions and X-Ray Temperatures of Galaxy Clusters
• AGN Disks Harden the Mass Distribution of Stellar-mass Binary Black Hole Mergers
• Feedback-regulated Super Massive Black Hole Seed Formation
• SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
• Stellar Dynamics and Stellar Phenomena Near A Massive Black Hole
• Gravitational Wave and X-ray Signals from Stellar Disruption by a Massive Black Hole
• Distinguishing Between Formation Channels for Binary Black Holes with LISA
• MOCCA Code for Star Cluster Simulations - II. Comparison with N-body Simulations
• Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up and ${}^{12}$C($\alpha$, $\gamma$)${}^{16}$O rate on the pair-instability black hole mass gap
• The Extremes of Thermonuclear Supernovae
• Gravitational Waves from the Remnants of the First Stars
• Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties
• The impact of mass-transfer physics on the observable properties of field binary black hole populations
• Evidence for hierarchical black hole mergers in the second LIGO--Virgo gravitational-wave catalog
• Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries
• A red giant orbiting a black hole
• Stellar-mass black holes in young massive and open stellar clusters and their role in gravitational-wave generation II
• Black Hole and Neutron Star Binary Mergers in Triple Systems: Merger Fraction and Spin-Orbit Misalignment
• Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
• Monte-Carlo simulations of black hole mergers in AGN disks: Low ${\chi }_{\mathrm{eff}}$ mergers and predictions for LIGO
• INTEGRAL upper limits on gamma-ray emission associated with the gravitational wave event GW150914
• On the number density of "direct collapse" black hole seeds
• The complete non-spinning effective-one-body metric at linear order in the mass ratio
• Growth of Intermediate-Mass Black Holes in Globular Clusters
• PeTar: a high-performance N-body code for modeling massive collisional stellar systems
• The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
• MOCCA code for star cluster simulations - I. Blue Stragglers, first results
• Supernova Explosions in the Early Universe: Evolution of Radiative Remnants and the Halo Destruction Efficiency
• Populating the upper black hole mass gap through stellar collisions in young star clusters
• Mass-gap Mergers in Active Galactic Nuclei
• Science with the TianQin observatory: Preliminary results on massive black hole binaries
• Binary black holes in the pair-instability mass gap
• Adiabatic waveforms for extreme mass-ratio inspirals via multivoice decomposition in time and frequency
• Hydrodynamics of galaxy mergers with supermassive black holes: is there a last parsec problem ?
• Measuring eccentricity in binary black hole inspirals with gravitational waves
• Eccentric Black Hole Mergers in Active Galactic Nuclei
• The late inspiral of supermassive black hole binaries with circumbinary gas discs in the LISA band
• Optical Spectroscopy and Velocity Dispersions of Galaxy Clusters from the SPT-SZ Survey
• On the Maximum Mass of Accreting Primordial Supermassive Stars
• Formation Rate of Extreme Mass Ratio Inspirals in Active Galactic Nuclei
• The erratic dynamical life of black hole seeds in high-redshift galaxies
• Binary Black Hole Accretion During Inspiral and Merger
• VLT Kinematics for omega Centauri: Further Support for a Central Black Hole
• Origin and properties of dual and offset active galactic nuclei in a cosmological simulation at z=2
• Rotation Speed of the First Stars
• The Birth of a Massive First-Star Binary
• Spin Evolution of Stellar-mass Black Hole Binaries in Active Galactic Nuclei
• Mass-accreting white dwarfs and type Ia supernovae
• Gravitational Wave Recoil and the Retention of Intermediate Mass Black Holes
• Early Results from GLASS-JWST. XIX: A High Density of Bright Galaxies at $z\approx 10$ in the Abell 2744 Region
• Failed Supernovae Explain the Compact Remnant Mass Function
• Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
• Transformations of asymptotic gravitational-wave data
• Formation of massive protostars in atomic cooling haloes
• Hierarchical Black-Hole Mergers in Multiple Systems: Constrain the Formation of GW190412, GW190814 and GW190521-like events
• Gravitational Waves and Intermediate-mass Black Hole Retention in Globular Clusters
• Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system
• Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes
• High-redshift formation and evolution of central massive objects II: The census of BH seeds
• Electromagnetic Counterparts to Massive Black Hole Mergers
• A Candidate of a Least-Massive Black Hole at the First 1.1 Billion Years of the Universe
• GSN 069 -- A Tidal Disruption Near-Miss
• Formation of Intermediate-Mass Black Holes through Runaway Collisions in the First Star Clusters
• The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy
• Binary Population Synthesis
• Maximum Black Hole mass across Cosmic Time
• Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
• Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
• Formation pathway of Population III coalescing binary black holes through stable mass transfer
• On the Origin of GW190521-like events from repeated black hole mergers in star clusters
• The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters
• X-ray Quasi-periodic Eruptions driven by Star-Disc Collisions : Application to GSN069 and Probing the Spin of Massive Black Holes
• Formation of an embryonic supermassive star in the first galaxy
• Super-Eddington Accretion and Feedback from the First Massive Seed Black Holes
• Intermediate Mass Black Hole Formation in compact Young Massive Star Clusters
• Massive black hole merger rates: the effect of kpc separation wandering and supernova feedback
• Evolution of Low-Mass Helium Stars in Semidetached Binaries
• A non-interacting Galactic black hole candidate in a binary system with a main-sequence star
• Electromagnetic Emission from Supermassive Binary Black Holes Approaching Merger
• Kinematic signature of an intermediate-mass black hole in the globular cluster NGC 6388
• Stellar Population in LLAGN.I: Ground-based observations
• Interacting Stellar EMRIs as Sources of Quasi-Periodic Eruptions in Galactic Nuclei
• Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band
• Repeating tidal disruptions in GSN 069: Long-term evolution and constraints on quasi-periodic eruptions' models
• Formation and survival of Population III stellar systems
• Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals
• Intermediate-mass Black Holes from High Massive-star Binary Fractions in Young Star Clusters
• Accretion disks around binary black holes of unequal mass: GRMHD simulations of postdecoupling and merger
• Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal
• Detecting triple systems with gravitational wave observations
• A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties
• Extreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole
• Science with the TianQin Observatory: Preliminary Results on Stochastic Gravitational-Wave Background
• Orbital evolution of binary black holes in active galactic nucleus disks: a disk channel for binary black hole mergers?
• Spectroscopic Evidence for a 5.4-Minute Orbital Period in HM Cancri
• Is GW190521 the merger of black holes from the first stellar generations?
• Modeling Seven Years of Event Horizon Telescope Observations with Radiatively Inefficient Accretion Flow Models
• On the GBM event seen 0.4 sec after GW 150914
• Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
• Direct formation of supermassive black holes in metal-enriched gas at the heart of high-redshift galaxy mergers
• Observationally driven Galactic double white dwarf population for LISA
• Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection
• Runaway collisions in young star clusters. I. Methods and tests
• Stellar transits across a magnetized accretion torus as a mechanism for plasmoid ejection
• The mass of first stars
• The Link between Warm Molecular Disks in Maser Nuclei and Star Formation near the Black Hole at the Galactic Center
• Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in nuclear star clusters
• The Fate of Binaries in the Galactic Center: The Mundane and the Exotic
• A light in the dark: searching for electromagnetic counterparts to black hole-black hole mergers in LIGO/Virgo O3 with the Zwicky Transient Facility
• A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes
• The route to massive black hole formation via merger-driven direct collapse: a review
• Black hole mergers: the first light
• Detectability of Intermediate-Mass Black Holes in Multiband Gravitational Wave Astronomy
• Ultra-compact (X-ray) binaries
• Probing vector hair of black holes with extreme mass ratio inspirals
• A new channel to form IMBHs throughout cosmic time
• Black Hole Mergers from Hierarchical Triples in Dense Star Clusters
• Collisions in Primordial Star Clusters: Formation Pathway for intermediate mass black holes
• On incorporating post-Newtonian effects in N-body dynamics
• The Formation of the First Massive Black Holes
• Detectable environmental effects in GW190521-like black-hole binaries with LISA
• The evolution of ultracompact X-ray binaries
• Testing general relativity with the reflection spectrum of the supermassive black hole in 1H0707$-$495
• Merge or survive: Number of Population III stars per minihalo
• Producing type Iax supernovae from a specific class of helium-ignited WD explosions?
• The Birth Mass Function of Pop III Stars
• Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects
• Population III Binary Black Holes: Effects of Convective Overshooting on Formation of GW190521
• Disentangling Coalescing Neutron Star-White Dwarf Binaries for LISA
• Extreme Dark Matter Tests with Extreme Mass Ratio Inspirals
• The importance of magnetic fields for the initial mass function of the first stars
• Relativistic Mergers of Supermassive Black Holes and their Electromagnetic Signatures
• The Effect of Massive Perturbers on Extreme Mass-Ratio Inspiral Waveforms
• The MEGaN project II. Gravitational waves from intermediate mass- and binary black holes around a supermassive black hole
• Host galaxy properties of quasi-periodically erupting X-ray sources
• Research Update on Extreme-Mass-Ratio Inspirals
• Enhancing the SEOBNRv5 effective-one-body waveform model with second-order gravitational self-force fluxes
• Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
• Black Hole Binary Formation in AGN Discs: From Isolation to Merger
• Gravitational-Wave Emission from Binary Black Holes Formed in Open Clusters
• Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc
• Formation of Binary Black Holes Similar to GW190521 with a Total Mass of $\sim 150M_{\odot }$ from Population III Binary Star Evolution
• Formation of GW190521 via gas accretion onto Population III stellar black hole remnants born in high-redshift minihalos
• A multi-messenger study of the Milky Way's stellar disc and bulge with LISA, Gaia and LSST
• First Stellar Binary Black Holes: Strongest Gravitational Wave Burst Sources
• Extreme mass-ratio inspirals into black holes surrounded by scalar clouds
• Shocks and angular momentum flips: a different path to feeding the nuclear regions of merging galaxies
• Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-Disks
• Tormund's return: Hints of quasi-periodic eruption features from a recent optical tidal disruption event
• Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
• An upper limit on the spin of SgrA${}^{\ast }$ based on stellar orbits in its vicinity
• Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries
• Detecting Intermediate-Mass Ratio Inspirals From The Ground And Space
• Hydrodynamical Evolution of Black-Hole Binaries Embedded in AGN Discs
• Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
• Intermediate-mass black holes in colliding clusters: Implications for lower-frequency gravitational-wave astronomy
• The electromagnetic chirp of a compact binary black hole: a phase template for the gravitational wave inspiral
• Populating the low-mass end of the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ relation
• eROSITA on SRG
• Quasi-periodic Eruptions from Helium Envelope of Hydrogen-deficient Stars Stripped by Supermassive Black Holes
• Populations of double white dwarfs in Milky Way satellites and their detectability with LISA
• A disk instability model for the quasi-periodic eruptions of GSN 069
• Effective one-body model for extreme-mass-ratio spinning binaries on eccentric equatorial orbits: testing radiation reaction and waveform
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
• Quasi-Periodicity of Supermassive Binary Black Hole Accretion Approaching Merger
• The complex time and energy evolution of quasi-periodic eruptions in eRO-QPE1
• The Population III origin of GW190521
• The Stellar Merger Scenario for Black Holes in the Pair-instability Gap
• Hydrodynamical Simulations of Black-Hole Binary Formation in AGN Disks
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• The eccentricity distribution of compact binaries
• Science with the TianQin Observatory: Preliminary Results on Testing the No-hair Theorem with EMRI
• Gravitational-Wave Localization Alone Probes AGN Origin of Stellar-Mass Black Hole Mergers
• Stellar Black Hole Binary Mergers in Open Clusters
• Perturbed disks get shocked. Binary black hole merger effects on accretion disks
• The last migration trap of compact objects in AGN accretion disc
• Nuclear coups: dynamics of black holes in galaxy mergers
• Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution
• A slow-down time-transformed symplectic integrator for solving the few-body problem
• Merger rate density of binary black holes formed in open clusters
• Revealing the formation of stellar-mass black hole binaries: The need for deci-Hertz gravitational wave observatories
• Gravitational waves from bodies orbiting the Galactic Center black hole and their detectability by LISA
• Binary radial velocity measurements with space-based gravitational-wave detectors
• Supermassive black hole pairs in clumpy galaxies at high redshift: delayed binary formation and concurrent mass growth
• Binary Mergers near a Supermassive Black Hole: Relativistic Effects in Triples
• Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries and gravitational wave sources
• Detectability of ultra-compact X-ray binaries as LISA sources
• Alive and kicking: A new QPE phase in GSN 069 revealing a quiescent luminosity threshold for QPEs
• The formation of neutron star systems through accretion-induced collapse in white-dwarf binaries
• Forming massive seed black holes in high-redshift quasar host progenitors
• Astronomical tests for quantum black hole structure
• Chirp Mass and Spin of Binary Black Holes from First Star Remnants
• The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay between Radiative Cooling, Star Formation, and Feedback Processes
• Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger
• Circularization vs. Eccentrification in Intermediate Mass Ratio Inspirals inside Dark Matter Spikes
• Gas dynamical friction as a binary formation mechanism in AGN discs
• Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
• Periodic orbits and their gravitational wave radiations in a polymer black hole in loop quantum gravity
• Bayesian parameter estimation of stellar-mass black-hole binaries with LISA
• The birth of a supermassive black hole binary
• Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
• A model for the possible connection between tidal disruption event and quasi-periodic eruption in GSN 069
• Effects of Intermediate Mass Black Holes on Nuclear Star Clusters
• The M_BH - sigma relation for intermediate-mass black holes in globular clusters
• Hot Circumsingle Disks Drive Binary Black Hole Mergers in Active Galactic Nucleus Disks
• Hydrodynamical Response of a Circumbinary Gas Disk to Black Hole Recoil and Mass Loss
• White dwarf binaries suggest a common envelope efficiency $\alpha \sim 1/3$
• Repeated Gravitational Lensing of Gravitational Waves in Hierarchical Black Hole Triples
• Observable signature of merging stellar-mass black holes in active galactic nuclei
• The double-degenerate model for the progenitors of type Ia supernovae
• Testing General Relativity with NuSTAR data of Galactic Black Holes
• MOCCA-SURVEY Database I: Assessing GW kick retention fractions for BH-BH mergers in globular clusters
• Tidal Interactions in Merging White Dwarf Binaries
• Extreme mass ratio inspirals on the equatorial plane in the adiabatic order
• Quasi-circular inspirals and plunges from non-spinning effective-one-body Hamiltonians with gravitational self-force information
• Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA
• Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA and the next generation of gravitational wave detectors
• In-situ extreme mass ratio inspirals via sub-parsec formation and migration of stars in thin, gravitationally unstable AGN discs
• Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries II: the large-mass-ratio case
• Expanding the LISA Horizon from the Ground
• Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks
• Long-term Evolution of Tightly-Packed Stellar Black Holes in AGN Disks: Formation of Merging Black-Hole Binaries via Close Encounters
• Can stellar-mass black hole growth disrupt disks of active galactic nuclei? The role of mechanical feedback
• The Origin of inequality: isolated formation of a 30+10Msun binary black-hole merger
• Impact of gas hardening on the population properties of hierarchical black hole mergers in AGN disks
• Binary formation through gas-assisted capture and the implications for stellar, planetary and compact-object evolution
• Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
• The Physics of Accretion Discs, Winds And Jets in Tidal Disruption Events
• Comments on Graviton Propagation in Light of GW150914
• Investigating the retention of intermediate-mass black holes in star clusters using N-body simulations
• The Burst Mode of Accretion in Primordial Protostars
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• Gaseous Dynamical Friction in Presence of Black Hole Radiative Feedback
• Accretion Phase of Star Formation in Clouds with Different Metallicities
• On the interpretation of the Fermi GBM transient observed in coincidence with LIGO Gravitational Wave Event GW150914
• Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties
• Eccentric binary black hole mergers in globular clusters hosting intermediate-mass black holes
• Feedback-Dominated Accretion Flows
• The Common Envelope Evolution Outcome -- A Case Study on Hot Subdwarf B Stars
• Ultra-compact X-ray binaries with He star companions
• Dark matter minispike: a significant enhancement of eccentricity for intermediate-mass-ratio-inspirals
• The Process of Stellar Tidal Disruption by Supermassive Black Holes. The first pericenter passage
• Phase shift of gravitational waves induced by aberration
• Novel modelling of ultra-compact X-ray binary evolution - stable mass transfer from white dwarfs to neutron stars
• Application of the disk instability model to all Quasi-Periodic Eruptions
• Simulations predict intermediate-mass black hole formation in globular clusters
• Contracting and Expanding Binary Black Holes in 3D Low-Mass AGN Disks: The Importance of Separation
• Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances
• Pulsational instability of supergiant protostars: Do they grow supermassive by accretion?
• Gravitational waves from eccentric intermediate-mass black hole binaries
• Binaries of massive black holes in rotating clusters: Dynamics, gravitational waves, detection and the role of eccentricity
• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
• Gravitational wave of intermediate-mass black holes in Population III star clusters
• SIRIUS Project. III. Star-by-star simulations of star cluster formation using a direct N-body integrator with stellar feedback
• Gravitational Waves from Hierarchical Triple Systems with Kozai-Lidov Oscillation
• Milli-Hertz Gravitational Wave Background Produced by Quasi-Periodic Eruptions
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• The Decoupling of Binaries from Their Circumbinary Disks
• Prospects of eLISA for Detecting Galactic Binary Black Holes Similar to GW150914
• Detecting the Beaming Effect of Gravitational Waves
• Simulation of a Compact Object with Outflows Moving Through a Gaseous Background
• Gravitational waves from eccentric extreme mass-ratio inspirals as probes of scalar fields
• The violent white dwarf merger scenario for the progenitors of type Ia supernovae
• Modeling transient resonances in extreme-mass-ratio inspirals
• Populating the Black Hole Mass Gaps In Stellar Clusters: General Relations and Upper Limits
• Intermediate Mass-Ratio Inspirals with Dark Matter Minispikes
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
• Capture of stars into gaseous discs around massive black holes: Alignment, circularization and growth
• Hydrodynamical Evolution of Black-Hole Binaries Embedded in AGN Discs: II. Dependence on Equation of State, Binary Mass, and Separation Scales
• A Systematic Search for Short-period Close White Dwarf Binary Candidates Based on Gaia EDR3 Catalog and Zwicky Transient Facility Data
• Compact Binary Waveform Center-of-Mass Corrections
• Nonlinear dynamical tides in white dwarf binaries
• Stellar-mass black holes in young massive and open stellar clusters V: comparisons with LIGO-Virgo merger rate densities
• Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricity
• Tidal Novae in Compact Binary White Dwarfs
• Tidal Stripping of a White Dwarf by an Intermediate-Mass Black Hole
• Detectability of Gravitational Waves from the Coalescence of Massive Primordial Black Holes with Initial Clustering
• Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN
• Spin Evolution of Stellar-mass Black Holes Embedded in AGN disks: Orbital Eccentricity Produces Retrograde Circumstellar Flows
• The Role of Outflow Feedback on Accretion of Compact Objects in Accretion Disk of Active Galactic Nuclei
• Multi-band gravitational wave astronomy: science with joint space- and ground-based observations of black hole binaries
• Direct determination of supermassive black hole properties with gravitational-wave radiation from surrounding stellar-mass black hole binaries
• Super-critical accretion of medium-weight seed black holes in gaseous proto-galactic nuclei
• Final compact remnants in core-collapse supernovae from 20 to 40 $M_{\odot }$: the lower mass gap
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• Massive binary black holes from Population II and III stars
• Extreme-mass-ratio burst detection with TianQin
• On the population III binary black hole mergers beyond the pair-instability mass gap
• Growth of stellar mass black holes in dense molecular clouds and GW190521
• The formation of single neutron-stars from double white-dwarf mergers via accretion-induced collapse
• The most luminous AGN do not produce the majority of the detected stellar-mass black hole binary mergers in the local Universe
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Massive Black Hole Binaries and Where to Find Them with Dual Detector Networks
• Optical Emission Model for Binary Black Hole Merger Remnants Travelling through Discs of Active Galactic Nuclei
• Fully General Relativistic Magnetohydrodynamic Simulations of Accretion Flows onto Spinning Massive Black Hole Binary Mergers
• Orbital Evolution of Neutron-Star -- White-Dwarf Binaries by Roche-Lobe Overflow and Gravitational Wave Radiation
• Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than $\sim 20M_{\odot }$
• Direct collapse of exceptionally heavy black holes in the merger-driven scenario
• Measuring Individual Masses of Binary White Dwarfs with Space-based Gravitational-wave Interferometers
• Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA
• High Frequency Gravitational Waves from Supermassive Black Holes: Prospects for LIGO-Virgo Detections
• Maximising the detection probability of kilonovae associated with gravitational wave observations
• Gravitational wave emission under general parametrized metric from extreme mass ratio inspirals
• Chaotic Gas Accretion by Black Holes Embedded in AGN Discs as Cause of Low-spin Signatures in Gravitational Wave Events
• The Milky Way's bar structural properties from gravitational waves
• Testing general relativity with TianQin: the prospect of using the inspiral signals of black hole binaries
• Eccentric Binary Black Holes with Spin via the Direct Integration of the Post-Newtonian Equations of Motion
• Evolution of high-redshift quasar hosts and promotion of massive black hole seed formation
• The Population of Eccentric Binary Black Holes: Implications for mHz Gravitational Wave Experiments
• Observable gravitational waves from tidal disruption events and their electromagnetic counterpart
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
• Exciting modes due to the aberration of gravitational waves: Measurability for extreme-mass-ratio inspirals
• Hunting for wandering massive black holes
• On the Mass Ratio Distribution of Black Hole Mergers in Triple Systems
• Detecting the stochastic gravitational wave background with the TianQin detector
• Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA
• Near Real-Time Gravitational Wave Data Analysis of the Massive Black Hole Binary with TianQin
• Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO
• Self-forced inspirals with spin-orbit precession
• Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion
• The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
• The role of bars on the dynamical-friction driven inspiral of massive perturbers
• On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
• Influence of a mass transfer stability criterion on double white dwarf populations
• Weighing Milky Way Satellites with LISA
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Binary black holes mergers from hierarchical triples in open clusters
• Measuring eccentricity and gas-induced perturbation from gravitational waves of LISA massive black hole binaries
• Localization of Binary Black-Hole Mergers with Known Inclination
• Angular correlation as a novel probe of supermassive primordial black holes
• LISA sources from young massive and open stellar clusters
• The gravitational capture of compact objects by massive black holes
• Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals
• Advancing Space-Based Gravitational Wave Astronomy: Rapid Parameter Estimation via Normalizing Flows
• The minimum measurable eccentricity from gravitational waves of LISA massive black hole binaries
• Gravitational waves from tidal disruption events: an open and comprehensive catalogue
• A correlation between Ha trough depth and inclination in quiescent X-ray transients: evidence for a low-mass black hole in GRO J0422+32
• Repeating Nuclear Transients as Candidate Electromagnetic Counterparts of LISA Extreme Mass Ratio Inspirals
• Prograde and Retrograde Gas Flow around Disk-embedded Companions: Dependence on Eccentricity, Mass and Disk Properties
• Evolution of AM CVn binaries with WD donors
• The Large Magellanic Cloud Revealed in Gravitational Waves with LISA
• RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
• Constraining white dwarf viscosity through tidal heating in detached binary systems
• Measuring the Galactic Binary Fluxes with LISA: Metamorphoses and Disappearances of White Dwarf Binaries
• An implementation of Galactic white dwarf binary data analysis for MLDC-3.1
• A seven-Earth-radius helium-burning star inside a 20.5-min detached binary
• Black Hole Mass Function of Coalescing Binary Black Hole Systems: Is There a Pulsational Pair Instability Mass Cutoff?
• Exploring the nature of black hole and gravity with an imminent merging binary of supermassive black holes
• Moving gravitational wave sources at cosmological distances: Impact on the measurement of the Hubble constant
• Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation
• Synchronizing the EMRIs and IMRIs in AGN accretion disks
• Repeated mergers of black hole binaries: implications for GW190521
• Very extreme mass-ratio bursts in the Galaxy and neighbouring galaxies in relation to space-borne detectors
• Influence of mass-ratio corrections in extreme-mass-ratio inspirals for testing general relativity
• Geometrized effective-one-body formalism for extreme-mass-ratio limits: Generic orbits
• 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
• Premerger detection of massive black hole binaries using deep learning
• Observing white dwarf tidal stripping with TianQin gravitational wave observatory
• Accurate modeling of intermediate-mass-ratio inspirals: Exploring the form of the self-force in the intermediate-mass-ratio regime
• Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
• QPE or QPO? -- Quasiperiodic Activity in Low-Mass Galaxy Nuclei
• How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Decihertz gravitational waves from double white dwarf merger remnants
• Calculating the Gravitational Waves Emitted from High-speed Sources
• Source localizations with the network of space-based gravitational wave detectors
• Searching for gravitational-wave bursts with space-borne detectors
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Gravitational Radiation from Eccentric Binary Black Hole System in Dynamical Chern-Simons Gravity
• Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
• SgrA${}^{\ast }$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral
• Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Gravitational Wave Signal Extraction Against Non-Stationary Instrumental Noises with Deep Neural Network
• Intermediate-mass ratio inspirals in merging elliptical galaxies
• Unveiling the solution to the final-parsec problem by combining milli-Hertz gravitational-wave observation and AGN survey
• Sky location of Galactic white dwarf binaries in space-based gravitational wave detection
• Parameter inference for coalescing massive black hole binaries using deep learning
• Measuring mass transfer of AM CVn binaries with a space-based gravitational wave detector
• Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
• Lensing of gravitational waves from tidal disruption events
• On the resonant detonation of sub-Chandrasekhar mass white dwarfs during binary inspiral
• Testing dispersion of gravitational waves from eccentric extreme-mass-ratio inspirals
• Black hole-galaxy co-evolution and the role of feedback
• Identifying Disappearance of a White Dwarf Binary with LISA
• Potential Tertiary Effects on the LISA Verification Binary HM Cancri
• Tracking the Long-Term GW Phase Evolution for HM Cancri-like Binaries with LISA
• Intermediate-mass black holes in globular clusters: observations and simulations
• Perturbative Frequency Expansion for Nearly Monochromatic Binary Black Holes Detectable with LISA

Cited by in corpus (21)

• Post-adiabatic waveform-generation framework for asymmetric precessing binaries
• Fundamental Physics and Cosmology with TianQin
• Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
• Toward Second-Order Self-Force for Eccentric Extreme-Mass Ratio Inspirals in Schwarzschild Spacetime
• Impact of mass transfer on the orbital evolution of a white dwarf close to an intermediate-mass black hole
• Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Signal-to-noise Ratio Analytic Formulae of the Inspiral Binary Black Holes in TianQin
• SgrA* spin and mass estimates through the detection of multiple extremely large mass-ratio inspirals
• Effect of kick velocity on gravitational wave detection of binary black holes with space- and ground-based detectors
• Dynamical backreaction of a mass-acquiring scalar field on first-order phase transitions
• Secular evolution of orbital parameters for general bound orbits in Kerr spacetime
• Ultra-compact X-ray Binaries: A Review
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Distinguishing gravity theories with networks of space-based gravitational-wave detectors
• Gravitational-Wave Signatures of Massive Black Hole Formation
• Gravitational Wave Signatures of Quasi-Periodic Eruptions: LISA Detection Prospects for RX J1301.9+2747
• Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss
• Gravitational-wave standard sirens and application in cosmology