Laser Interferometer Space Antenna

Abstract

Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missions for L3. The observatory will be based on three arms with six active laser links, between three identical spacecraft in a triangular formation separated by 2.5 million km. LISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using Gravitational Waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the infant Universe at TeV energy scales, has known sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales near the horizons of black holes, all the way to cosmological scales. The LISA mission will scan the entire sky as it follows behind the Earth in its orbit, obtaining both polarisations of the Gravitational Waves simultaneously, and will measure source parameters with astrophysically relevant sensitivity in a band from below $10^{-4}$Hz to above $10^{-1}$Hz.

Submitted to ESA on January 13th in response to the call for missions for the L3 slot in the Cosmic Vision Programme

Cited by in corpus (830)

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• Black Holes on FIRE: Stellar Feedback Limits Early Feeding of Galactic Nuclei
• The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
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• Modified gravitational-wave propagation and standard sirens
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• Gravitational waves induced from primordial black hole fluctuations: The effect of an extended mass function
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• Astrophysical Black Holes: A Compact Pedagogical Review
• A systematic search of Zwicky Transient Facility data for ultracompact binary LISA-detectable gravitational-wave sources
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• When Primordial Black Holes from Sound Speed Resonance Meet a Stochastic Background of Gravitational Waves
• Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA
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• The Gravitational-Wave Physics II: Progress
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• Prospects for observing extreme-mass-ratio inspirals with LISA
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• Primordial Anisotropies in the Gravitational Wave Background from Cosmological Phase Transitions
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• Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band
• Characterizing the Cosmological Gravitational Wave Background Anisotropies and non-Gaussianity
• Detection of Early-Universe Gravitational Wave Signatures and Fundamental Physics
• Constraining axion inflation with gravitational waves across 29 decades in frequency
• Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition
• Post-Newtonian Gravitational and Scalar Waves in Scalar-Gauss-Bonnet Gravity
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• Orbital Evolution of Binaries in Circumbinary Disks
• Cosmological Phase Transitions in Warped Space: Gravitational Waves and Collider Signatures
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• Probing Massive Black Hole Binary Populations with LISA
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• Gravitational wave background from extreme mass ratio inspirals
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• Gravitational-wave glitches in chaotic extreme-mass-ratio inspirals
• Intermediate mass black holes from stellar mergers in young star clusters
• Parametrized ringdown spin expansion coefficients: a data-analysis framework for black-hole spectroscopy with multiple events
• Decoding the phases of early and late time reheating through imprints on primordial gravitational waves
• Origins and Demographics of Wandering Black Holes
• Gravitational radiation from inspiralling compact objects: Spin effects to fourth Post-Newtonian order
• Extreme mass ratio inspirals with spinning secondary: a detailed study of equatorial circular motion
• Probing Primordial-Black-Hole Dark Matter with Gravitational Waves
• On the origin of GW190425
• Dynamical Friction in Gravitational Atoms
• Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach
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• Modeling and searching for a stochastic gravitational-wave background from ultralight vector bosons
• Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers
• Primordial Black Holes from Multifield Inflation with Nonminimal Couplings
• Detecting Double Neutron Stars with LISA
• Time-Delay Interferometry and Clock-Noise Calibration
• Multi-messenger tests of gravity with weakly lensed gravitational waves
• 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
• Star Formation in Accretion Disks and SMBH Growth
• Implications for the Supermassive Black Hole Binaries from the NANOGrav 15-year Data Set
• High Eccentricities and High Masses Characterize Gravitational-wave Captures in Galactic Nuclei as Seen by Earth-based Detectors
• Approximate gauge independence of the induced gravitational wave spectrum
• Evolution of small-mass-ratio binaries with a spinning secondary
• Jumping the gap: searching for LIGO's biggest black holes
• Scalar induced gravitational waves in light of Pulsar Timing Array data
• Quasi-periodic Eruptions from Helium Envelope of Hydrogen-deficient Stars Stripped by Supermassive Black Holes
• Fingerprinting models of first-order phase transitions by the synergy between collider and gravitational-wave experiments
• Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation
• Amplification of Primordial Perturbations from the Rise or Fall of the Inflaton
• Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
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• Scalar induced gravitational waves from primordial black hole Poisson fluctuations in $f(R)$ gravity
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• The complex time and energy evolution of quasi-periodic eruptions in eRO-QPE1
• Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
• Quasi-Periodicity of Supermassive Binary Black Hole Accretion Approaching Merger
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• Time-dependence of the astrophysical stochastic gravitational wave background
• Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
• Cosmology and modified gravitational wave propagation from binary black hole population models
• Probing the nature of central objects in extreme-mass-ratio inspirals with gravitational waves
• Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
• The Minimum Testable Abundance of Primordial Black Holes at Future Gravitational-Wave Detectors
• Gravitational Waves and Dark Photon Dark Matter from Axion Rotations
• Generation of gravitational waves from freely decaying turbulence
• Multi-mode black hole spectroscopy
• Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals
• Self-Force Calculations with a Spinning Secondary
• Bridging the $\mu$Hz gap in the gravitational-wave landscape with binary resonance
• Constraints on primordial curvature power spectrum with pulsar timing arrays
• A catalogue of cataclysmic variables from 20 years of the Sloan Digital Sky Survey with new classifications, periods, trends and oddities
• Asteroids for $\mu$Hz gravitational-wave detection
• Cosmological bubble friction in local equilibrium
• Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
• Extracting the Gravitational Recoil from Black Hole Merger Signals
• Precision Charge Control for Isolated Free-Falling Test Masses: LISA Pathfinder Results
• GWFish: A simulation software to evaluate parameter-estimation capabilities of gravitational-wave detector networks
• The last migration trap of compact objects in AGN accretion disc
• Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
• Multiparameter tests of general relativity using multiband gravitational-wave observations
• Stellar binary black holes in the LISA band: a new class of standard sirens
• Exciting black hole modes via misaligned coalescences: II. The mode content of late-time coalescence waveforms
• Gravitational wave and collider signals in complex two-Higgs doublet model with dynamical CP-violation at finite temperature
• Ultra-relativistic bubbles from the simplest Higgs portal and their cosmological consequences
• The mass-radius relation for neutron stars in $f(R)=R+\alpha R^2$ gravity: a comparison between purely metric and torsion formulations
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• Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries and gravitational wave sources
• Assessing the detectability of the secondary spin in extreme mass-ratio inspirals with fully-relativistic numerical waveforms
• Hamilton-Jacobi equation for spinning particles near black holes
• Hereditary Terms at Next-To-Leading Order in Two-Body Gravitational Dynamics
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Effect of filters on the time-delay interferometry residual laser noise for LISA
• LISA parameter estimation and source localization with higher harmonics of the ringdown
• Learning about black hole binaries from their ringdown spectra
• Prompt Electromagnetic Transients from Binary Black Hole Mergers
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• Primordial black holes and secondary gravitational waves from natural inflation
• CLASS_GWB: robust modeling of the astrophysical gravitational wave background anisotropies
• A hybrid simulation of gravitational wave production in first-order phase transitions
• StarTrack predictions of the stochastic gravitational-wave background from compact binary mergers
• Supercool subtleties of cosmological phase transitions
• Gravitational wave research using pulsar timing arrays
• Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger
• Mini-disk accretion onto spinning black hole binaries: quasi-periodicities and outflows
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Transmuted Gravity Wave Signals from Primordial Black Holes
• Bayesian parameter estimation of stellar-mass black-hole binaries with LISA
• Testing the Quasar Hubble Diagram with LISA Standard Sirens
• Possible Causes of False General Relativity Violations in Gravitational Wave Observations
• Sr atom interferometry with the optical clock transition as a gravimeter and a gravity gradiometer
• Gravitational Waves from Fundamental Axion Dynamics
• Stochastic Gravitational Waves from Particle Origin
• Where are the double-degenerate progenitors of type Ia supernovae?
• Multi-messenger Time-domain Signatures Of Supermassive Black Hole Binaries
• Dynamics of Quadruple Systems Composed of Two Binaries: Stars, White Dwarfs, and Implications for Ia Supernovae
• Gravitational Wave from Graviton Bremsstrahlung during Reheating
• Assessing the impact of transient orbital resonances
• Primordial black holes and scalar induced gravitational waves from the $E$ model with a Gauss-Bonnet term
• Primordial gravitational waves and the H0-tension problem
• Repeated Gravitational Lensing of Gravitational Waves in Hierarchical Black Hole Triples
• Primordial black holes and secondary gravitational waves from the Higgs field
• Induced gravitational waves from the cosmic coincidence
• A Unique Multi-Messenger Signal of QCD Axion Dark Matter
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Cosmological perturbation effects on gravitational-wave luminosity distance estimates
• Higgsless simulations of cosmological phase transitions and gravitational waves
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone
• Eigenvalue repulsions in the quasinormal spectra of the Kerr-Newman black hole
• Gravitational Waves from Density Perturbations in an Early Matter Domination Era
• Measuring the propagation speed of gravitational waves with LISA
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Probing Dark Matter Spikes via Gravitational Waves of Extreme Mass Ratio Inspirals
• Dissipation in extreme-mass ratio binaries with a spinning secondary
• Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
• Impact of infrasound atmospheric noise on gravity detectors used for astrophysical and geophysical applications
• Expanding the LISA Horizon from the Ground
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions
• Cosmological constraints on dark energy in light of gravitational wave bounds
• Generation of squeezed vacuum state in the millihertz frequency band
• Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity
• Observational constraints of a new unified dark fluid and the $H_0$ tension
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Primordial black holes in nonminimal derivative coupling inflation with quartic potential and reheating consideration
• Multimessenger Cosmology: correlating CMB and SGWB measurements
• Propagating Speed of Primordial Gravitational Waves
• Discovery and characterization of five new eclipsing AM CVn systems
• Maximum redshift of gravitational wave merger events
• Detecting Gravitational Wave Bursts with LISA in the presence of Instrumental Glitches
• Primordial black holes and gravitational waves induced by exponential-tailed perturbations
• On the detectability of ultralight scalar field dark matter with gravitational-wave detectors
• Fast and Fourier: Extreme Mass Ratio Inspiral Waveforms in the Frequency Domain
• Time Delay Interferometry combinations as instrument noise monitors for LISA
• Gravitational shine of dark domain walls
• Listening to the gravitational wave sound of circumbinary exoplanets
• Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA
• Identifying LISA verification binaries among the Galactic population of double white dwarfs
• Large anisotropies of the stochastic gravitational wave background from cosmic domain walls
• Detecting stochastic gravitational waves with binary resonance
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• Primordial black holes and scalar-induced gravitational waves from the generalized Brans-Dicke theory
• Adding eccentricity to quasicircular binary-black-hole waveform models
• Scalar QED as a toy model for higher-order effects in classical gravitational scattering
• Gravitational waves and the polarizations in Hořava gravity after GW170817
• TDI-infinity: time-delay interferometry without delays
• Model-independent reconstruction of the primordial curvature power spectrum from PTA data
• Second-order gravitational self-force in a highly regular gauge
• Disks Around Merging Binary Black Holes: From GW150914 to Supermassive Black Holes
• Precision cosmology and the stiff-amplified gravitational-wave background from inflation: NANOGrav, Advanced LIGO-Virgo and the Hubble tension
• Gravitational waves from phase transition in split NMSSM
• The Combined Effects of Two-Body Relaxation Processes and the Eccentric Kozai-Lidov Mechanism on the EMRI Rate
• Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens
• Black Hole Growth and Feedback in Isolated Romulus25 Dwarf Galaxies
• Alternative LISA-TAIJI networks
• Turn up the volume: Listening to phase transitions in hot dark sectors
• Ultra-compact X-ray binaries with He star companions
• Primordial Monopoles and Strings, Inflation, and Gravity Waves
• Repeated Imaging of Massive Black Hole Binary Orbits with Millimeter Interferometry: measuring black hole masses and the Hubble constant
• Gravitational waveforms from periodic orbits around a quantum-corrected black hole
• Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources
• Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins
• Accelerating the evaluation of inspiral-merger-ringdown waveforms with adapted grids
• The stochastic gravitational wave background from close hyperbolic encounters of primordial black holes in dense clusters
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Multiband gravitational-wave searches for ultralight bosons
• Unveiling early black hole growth with multi-frequency gravitational wave observations
• Glimmering in the dark: modeling the low-mass end of the $M_{\bullet }-\sigma$ relation and of the quasar luminosity function
• Tests of general relativity with stellar-mass black hole binaries observed by LISA
• Unveiling the Population of Wandering Black Holes via Electromagnetic Signatures
• Improved sensitivity of interferometric gravitational wave detectors to ultralight vector dark matter from the finite light-traveling time
• Beyond freeze-in: Dark Matter via inverse phase transition and gravitational wave signal
• Non-geometric tilt-to-length coupling in precision interferometry: mechanisms and analytical descriptions
• Calibrating the system dynamics of LISA Pathfinder
• Enhancement of primordial curvature perturbations in $R^3$-corrected Starobinsky-Higgs inflation
• Bayesian Metric Reconstruction with Gravitational Wave Observations
• Signatures of the Many Supermassive Black Hole Mergers in a Cosmologically Forming Massive Early-Type Galaxy
• Improved limits on a stochastic gravitational-wave background and its anisotropies from Advanced LIGO O1 and O2 runs
• Electroweak baryogenesis in aligned two Higgs doublet models
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• The ELM Survey. IX. A Complete Sample of Low Mass White Dwarf Binaries in the SDSS Footprint
• Constraining modified gravity with ringdown signals: an explicit example
• Hubble parameter estimation via dark sirens with the LISA-Taiji network
• Circumbinary Disk Accretion into Spinning Black Hole Binaries
• Stochastic Gravitational Waves from Inflaton Decays
• Mesoscopic Interference for Metric and Curvature (MIMAC) & Gravitational Wave Detection
• Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves
• Cusp-to-core transition in low-mass dwarf galaxies induced by dynamical heating of cold dark matter by primordial black holes
• Filtered pseudo-scalar dark matter and gravitational waves from first order phase transition
• Escape from supercooling with or without bubbles: gravitational wave signatures
• Limits on the cosmic neutrino background
• Hot subdwarf stars identified in Gaia DR2 with spectra of LAMOST DR6 and DR7 I. Single-lined spectra
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• Milli-Hertz Gravitational Wave Background Produced by Quasi-Periodic Eruptions
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone
• Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters
• Black hole spectroscopy horizons for current and future gravitational wave detectors
• Discovery of a Candidate Binary Supermassive Black Hole in a Periodic Quasar from Circumbinary Accretion Variability
• Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• Gravitational waves from eccentric extreme mass-ratio inspirals as probes of scalar fields
• Detecting the Beaming Effect of Gravitational Waves
• A Higher Probability of Detecting Lensed Supermassive Black Hole Binaries by LISA
• The Interplay between the Dark Matter Axion and Primordial Black Holes
• NANOGrav signal and LIGO-Virgo Primordial Black Holes from the Higgs field
• Prospects for LISA to detect a gravitational-wave background from first order phase transitions
• Testing primordial black hole and measuring the Hubble constant with multiband gravitational-wave observations
• Correlating Gravitational Waves with $W$-boson Mass, FIMP Dark Matter, and Majorana Seesaw Mechanism
• Thermonuclear Explosions and Accretion-induced Collapses of White Dwarfs in Active Galactic Nucleus Accretion Disks
• Dark matter, electroweak phase transition and gravitational wave in the type-II two-Higgs-doublet model with a singlet scalar field
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Effect of density fluctuations on gravitational wave production in first-order phase transitions
• Enhancing gravitational wave anisotropies with peaked scalar sources
• Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy
• From regular black holes to horizonless objects: quasi-normal modes, instabilities and spectroscopy
• Signals of primordial black holes at gravitational wave interferometers
• Label Switching Problem in Bayesian Analysis for Gravitational Wave Astronomy
• New Graviton Mass Bound from Binary Pulsars
• Friction on ALP domain walls and gravitational waves
• Testing clockwork axion with gravitational waves
• Relativistic Tidal Disruption and Nuclear Ignition of White Dwarf Stars by Intermediate Mass Black Holes
• Primordial black hole dark matter from catastrogenesis with unstable pseudo-Goldstone bosons
• Complementarity of the future $e^{+}{e}^{-}$ colliders and gravitational waves in the probe of complex singlet extension to the Standard Model
• Gravitational Wave Detection with Photometric Surveys
• Sensitivity functions for space-borne gravitational wave detectors
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• Primordial black holes in non-canonical scalar field inflation driven by quartic potential in the presence of bump
• Reconstructing physical parameters from template gravitational wave spectra at LISA: first order phase transitions
• Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
• Constraining the Stochastic Gravitational Wave Background with Photometric Surveys
• Transient acceleration events in LISA Pathfinder data: properties and possible physical origin
• Effect of Earth-Moon's gravity on TianQin's range acceleration noise
• Energy budget and the gravitational wave spectra beyond the bag model
• The influence of Massive Black Hole Binaries on the Morphology of Merger Remnants
• Impact of $H_0$ priors on $f(T)$ late time cosmology
• Joint cosmological inference of standard sirens and gravitational wave weak lensing
• On the eccentricity evolution of massive black hole binaries in stellar backgrounds
• Algorithm for TDI numerical simulation and sensitivity investigation
• Constraining early dark energy with gravitational waves before recombination
• Where intermediate-mass black holes could hide in the Galactic Centre: A full parameter study with the S2 orbit
• Gravitational waves from plunges into Gargantua
• Multi-messenger-Athena Synergy White Paper
• Numerical-relativity simulations of the quasi-circular inspiral and merger of non-spinning, charged black holes: methods and comparison with approximate approaches
• Apparent Superluminality of Lensed Gravitational Waves
• Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
• The Bright Reverse Shock Emission in the Optical Afterglows of Gamma-ray Bursts in a Stratified Medium
• Gravitational Wave Probes of Massive Gauge Bosons at the Cosmological Collider
• A Systematic Search for Short-period Close White Dwarf Binary Candidates Based on Gaia EDR3 Catalog and Zwicky Transient Facility Data
• A Single Progenitor Model for GW150914 and GW170104
• Tidal heating of Quantum Black Holes and their imprints on gravitational waves
• Microlensing of gravitational waves by dark matter structures
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
• Massive Black Hole Mergers with Orbital Information: Predictions from the ASTRID Simulation
• Dancing in the dark: detecting a population of distant primordial black holes
• Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
• Gravitational footprints of massive neutrinos and lepton number breaking
• Inflation, superheavy metastable strings and gravitational waves in non-supersymmetric flipped SU(5)
• Machine learning forecasts of the cosmic distance duality relation with strongly lensed gravitational wave events
• Time delay interferometry without clock synchronisation
• Electroweak Phase Transition and Gravitational Waves in the Type-II Seesaw Model
• Refined clock-jitter reduction in the Sagnac-type time-delay interferometry combinations
• Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters
• Gravitational Wave Background Search by Correlating Multiple Triangular Detectors in the mHz Band
• Testing gravitational wave propagation with multiband detections
• Polarization of gravitational waves from helical MHD turbulent sources
• Dynamical Friction From Ultralight Dark Matter
• High Quality QCD Axion at Gravitational Wave Observatories
• The lifetime of binary black holes in Sérsic galaxy models
• A paradigm of warm quintessential inflation and production of relic gravity waves
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• $\mu$-hybrid Inflation, Gravitino Dark Matter and Stochastic Gravitational Wave Background from Cosmic Strings
• Investigating the relation between gravitational wave tests of general relativity
• Testing the violation of the equivalence principle in the electromagnetic sector and its consequences in $f(T)$ gravity
• On networks of space-based gravitational-wave detectors
• Gravitational waves from in-spirals of compact objects in binary common-envelope evolution
• Model independent tests of the Kerr bound with extreme mass ratio inspirals
• Towards a framework for testing general relativity with extreme-mass-ratio-inspiral observations
• Spherically symmetric static black holes in Einstein-aether theory
• Oscillations in the EMRI gravitational wave phase correction as a probe of reflective boundary of the central black hole
• Sowing black hole seeds: Direct collapse black hole formation with realistic Lyman-Werner radiation in cosmological simulations
• Detecting primordial features with LISA
• The Active Fraction of Massive Black Holes in Dwarf Galaxies
• Direct determination of supermassive black hole properties with gravitational-wave radiation from surrounding stellar-mass black hole binaries
• Evaluating Black Hole Detectability with LISA
• Kinematic signatures of reverberation mapping of close binaries of supermassive black holes in active galactic nuclei
• Full analytical formulas for frequency response of space-based gravitational wave detectors
• Resonant self-force effects in extreme-mass-ratio binaries: A scalar model
• Circumbinary disc self-gravity governing supermassive black hole binary mergers
• The ZTF Source Classification Project: II. Periodicity and variability processing metrics
• Gravitational Imprints from Heavy Kaluza-Klein Resonances
• Inward Bound: The incredible journey of massive black holes as they pair and merge; I. The effect of mass ratio in flattened rotating galactic nuclei
• Toward the primordial black hole formation threshold in a time-dependent equation-of-state background
• Primordial black holes and induced gravitational waves from double-pole inflation
• Primordial black holes and induced gravitational waves from logarithmic non-Gaussianity
• Spritz: a new fully general-relativistic magnetohydrodynamic code
• Mass Transfer and Stellar Evolution of the White Dwarfs in AM CVn Binaries
• On the population III binary black hole mergers beyond the pair-instability mass gap
• Gravitational Waves from Current-Carrying Cosmic Strings
• An optimized PyCBC search for gravitational waves from intermediate-mass black hole mergers
• Monopoles, Strings and Gravitational Waves in Non-minimal Inflation
• Criterion for ultra-fast bubble walls: the impact of hydrodynamic obstruction
• Observing gravitational wave polarizations with LISA-TAIJI network
• Gravity Gradient Noise from Asteroids
• Hunting the stochastic gravitational wave background in pulsar timing array cross correlations through theoretical uncertainty
• Large fluctuations and Primordial Black Holes
• The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential
• Integrability of eccentric, spinning black hole binaries up to second post-Newtonian order
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Testing Primordial Black Holes as Dark Matter in Supergravity from Gravitational Waves
• Intermediate-mass black holes and the fundamental plane of black hole accretion
• Charging of free-falling test masses in orbit due to cosmic rays: results from LISA Pathfinder
• Excitation of gravitational wave modes by a center-of-mass velocity of the source
• Upper Bound on Thermal Gravitational Wave Backgrounds from Hidden Sectors
• Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna
• Gravitational wave and electroweak baryogenesis with two Higgs doublet models
• Post-Merger Jets from Supermassive Black Hole Coalescences as Electromagnetic Counterparts of Gravitational Wave Emission
• Modified gravitational wave propagation with higher modes and its degeneracies with lensing
• Numerical Modeling and Experimental Demonstration of Pulsed Charge Control for the Space Inertial Sensor used in LISA
• Sky localization of space-based gravitational wave detectors
• Massive Black Hole Binaries and Where to Find Them with Dual Detector Networks
• Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
• Self-force framework for transition-to-plunge waveforms
• Shallow relic gravitational wave spectrum with acoustic peak
• Multi-step phase transitions and gravitational waves in the inert doublet model
• Sharp turns in axion monodromy: primordial black holes and gravitational waves
• Geometric approach for the modified second generation time delay interferometry
• Gravitational Wave Signals from Multiple Hidden Sectors
• Sterile neutrino dark matter catalyzed by a very light dark photon
• Spin-orbit effects for compact binaries in scalar-tensor gravity
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• Probing Stochastic Gravitational Wave Background from $SU(5)\times U(1{)}_{\chi }$ Strings in Light of NANOGrav 15-Year Data
• Gravitational Wave Echo of Relaxion Trapping
• Chasing Super-Massive Black Hole merging events with $Athena$ and LISA
• Constraining extra dimensions on cosmological scales with LISA future gravitational wave siren data
• How to detect the shortest-period binary pulsars in the era of LISA
• LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode
• Black hole science with the Laser Interferometer Space Antenna
• The energy budget of cosmological first-order phase transitions beyond the bag equation of state
• Modeling gravitational waves from exotic compact objects
• Higher-Curvature Corrections and Tensor Modes
• Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
• Model-Independent Radiative Symmetry Breaking and Gravitational Waves
• Multiband gravitational wave cosmology with stellar origin black hole binaries
• Dissecting the Stochastic Gravitational Wave Background with Astrometry
• Pinning down the primordial black hole formation mechanism with gamma-rays and gravitational waves
• The Population of Eccentric Binary Black Holes: Implications for mHz Gravitational Wave Experiments
• Star cluster disruption by a massive black hole binary
• Revisiting evolution of domain walls and their gravitational radiation with CosmoLattice
• Primordial black holes and inflation from double-well potentials
• The new discontinuous Galerkin methods based numerical relativity program Nmesh
• The role of low-energy electrons in the charging process of LISA test masses
• Polarization Modes of Gravitational Waves in Palatini Horndeski theory
• A statistical inference approach to time-delay interferometry for gravitational-wave detection
• Baryogenesis in the paradigm of quintessential inflation
• Primordial black holes and gravitational waves from dissipation during inflation
• Double peaks of gravitational wave spectrum induced from inflection point inflation
• Evolution of black hole shadows from superradiance
• A thorough investigation of the prospects of eLISA in addressing the Hubble tension: Fisher Forecast, MCMC and Machine Learning
• How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
• Heavier $W$ boson, dark matter and gravitational waves from strings in an $SO(10)$ axion model
• Probes of Gravitational Waves with Atom Interferometers
• Strong electroweak phase transition in $t$-channel simplified dark matter models
• Periodic orbits and their gravitational wave radiations around the Schwarzschild-MOG black hole
• The role of bars on the dynamical-friction driven inspiral of massive perturbers
• Improved Constraints on Modified Gravity with Eccentric Gravitational Waves
• Orbital effects on time delay interferometry for TianQin
• BCS in the Sky: Signatures of Inflationary Fermion Condensation
• Lepton Flavour Asymmetries and the Mass Spectrum of Primordial Black Holes
• Formation of supermassive black holes in galactic nuclei II: retention and growth of seed intermediate-mass black holes
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Eccentric-orbit extreme-mass-ratio-inspiral radiation II: 1PN correction to leading-logarithm and subleading-logarithm flux sequences and the entire perturbative 4PN flux
• The Eccentric and Accelerating Stellar Binary Black Hole Mergers in Galactic Nuclei: Observing in Ground and Space Gravitational Wave Observatories
• Inherently stable effective field theory for dark energy and modified gravity
• Merger-Ringdown Consistency: A New Test of Strong Gravity using Deep Learning
• Hunting WIMPs with LISA: Correlating dark matter and gravitational wave signals
• Self-force correction to geodetic spin precession in Kerr spacetime
• Tilt-to-length coupling in LISA Pathfinder: a data analysis
• The Bardeen-Petterson effect in accreting supermassive black-hole binaries: disc breaking and critical obliquity
• Limits on Runaway Growth of Intermediate Mass Black Holes from Advanced LIGO
• A Predictive $SO(10)$ Model
• A consistency-test for determining whether ultra-compact dwarf galaxies could be the remnant nuclei of threshed galaxies
• Dynamics of Intermediate-Mass Black Holes Wandering in the Milky Way Galaxy Using the Illustris TNG50 Simulation
• ALP dark matter with non-periodic potentials: parametric resonance, halo formation and gravitational signatures
• Gravitational waves from fast-spinning white dwarfs
• Low-frequency Gravitational Wave Detection via Double Optical Clocks in Space
• Angular correlation as a novel probe of supermassive primordial black holes
• Cosmology of Supercooled Universe
• Formation and Destiny of White Dwarf and Be Star Binaries
• Searching for lepton portal dark matter with colliders and gravitational waves
• Circularly polarized scalar induced gravitational waves from the Chern-Simons modified gravity
• Effect of orbital eccentricity on the dynamics of precessing compact binaries
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• The effect of multiple features on the power spectrum in two-field inflation
• Modified gravitational wave propagation and the binary neutron star mass function
• The gravitational capture of compact objects by massive black holes
• Prospects for Taiji to detect a gravitational-wave background from cosmic strings
• Primordial black holes and scalar-induced gravitational waves from the perturbations on the inflaton potential in peak theory
• The optical geometry definition of the total deflection angle of a light ray in curved spacetime
• Merging Hierarchical Triple Black Hole Systems with Intermediate-mass Black Holes in Population III Star Clusters
• Sound velocity effects on the phase transition gravitational wave spectrum in the sound shell model
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Gravitational waves from tidal disruption events: an open and comprehensive catalogue
• Quasinormal Modes for Dynamical Black Holes
• Model systematics in time domain tests of binary black hole evolution
• Highly reflective low-noise etalon-based meta-mirror
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Testing the nature of dark compact objects with gravitational waves
• Detection and estimation of the cosmic dipole with the Einstein Telescope and Cosmic Explorer
• Precision cosmology with primordial GW backgrounds in presence of astrophysical foregrounds
• Accretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
• STOLAS: STOchastic LAttice Simulation of cosmic inflation
• The observed number counts in luminosity distance space
• Waves from the Centre: Probing PBH and other Macroscopic Dark Matter with LISA
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Unified mapmaking for an anisotropic stochastic gravitational wave background
• Fundamental physics using the temporal gravitational wave background
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Motion deviation of test body induced by spin and cosmological constant in extreme mass ratio inspiral binary system
• Detecting Gravitational Self Lensing from Stellar-Mass Binaries Composed of Black Holes or Neutron Stars
• The Bardeen-Petterson effect in accreting supermassive black-hole binaries: a systematic approach
• Induced Gravitational Waves from Multi-Sound Speed Resonances during Cosmological Inflation
• Testing the Kerr nature of intermediate-mass and supermassive black hole binaries using spin-induced multipole moment measurements
• The Large Magellanic Cloud Revealed in Gravitational Waves with LISA
• Census of R Coronae Borealis stars I: Infrared light curves from Palomar Gattini IR
• Endpoint of the up-down instability in precessing binary black holes
• A taxonomy of black-hole binary spin precession and nutation
• Gravitational waves from bubble collisions in FLRW spacetime
• Sudden braking and turning with a two-field potential bump: primordial black hole formation
• Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies
• Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*
• Constraining Horndeski theory with gravitational waves from coalescing binaries
• RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
• Bayesian Characterisation of Circumbinary Exoplanets with LISA
• Search for Neutron Star Binaries in the Local Group Galaxies Using LISA
• Scope out multiband gravitational-wave observations of GW190521-like binary black holes with space gravitational wave antenna B-DECIGO
• Degeneracy between mass and peculiar acceleration for the double white dwarfs in the LISA band
• Probing the Merger Rates of Supermassive Black Holes and Galaxies with Gravitational Waves
• Freeze-in Dark Matter Through Forbidden Channel in $U(1{)}_{B-L}$
• Mergers of Maximally Charged Primordial Black Holes
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs
• The Search for Binary Supermassive Black Holes Amongst Quasars with Offset Broad Lines Using the Very Long Baseline Array
• The (Black Hole Mass)-(Spheroid Stellar Density) Relations: $M_{\mathrm{BH}}$--$\mu$ (and $M_{\mathrm{BH}}$--$\Sigma$) and $M_{\mathrm{BH}}$--$\rho$
• Ultra-deep tidal disruption events: prompt self-intersections and observables
• Scalar induced gravitational waves from Chern-Simons gravity during inflation era
• Stellar-mass black-hole binaries in LISA: characteristics and complementarity with current-generation interferometers
• Accelerated motion and the self-force in Schwarzschild spacetime
• Analytic thin wall false vacuum decay rate
• Pulsar Timing Array Experiments
• A rapid channel for the collisional formation and gravitational wave driven mergers of supermassive black hole seeds at high redshift
• Boosting GWs in Supersolid Inflation
• Multi-Messenger Constraints on Magnetic Fields in Merging Black Hole-Neutron Star Binaries
• Heavy dark matter and Gravitational waves
• Systematics in tests of general relativity using LISA massive black hole binaries
• Background for gravitational wave signal at LISA from refractive index of solar wind plasma
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Testing gravity with gravitational wave friction and gravitational slip
• Non-linear effects in EMRI dynamics and their imprints on gravitational waves
• Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals
• Cataclysmic variables are a key population of gravitational wave sources for LISA
• Observable Primordial Gravitational Waves from Non-minimally Coupled $R^2$ Palatini Modified Gravity
• GRMHD study of accreting massive black hole binaries in astrophysical environment: a review
• Primordial Stochastic Gravitational Wave Background Anisotropies: in-in Formalization and Applications
• Gravitational Self-Force Regularization in the Regge-Wheeler and Easy Gauges
• Baryogenesis via Leptogenesis: Spontaneous B and L Violation
• Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
• Model-dependent analysis method for energy budget of the cosmological first-order phase transition
• Conditions for direct black hole seed collapse near a radio-loud quasar 1 Gyr after the Big Bang
• Anatomy of parameter-estimation biases in overlapping gravitational-wave signals
• Tomography of flavoured leptogenesis with primordial blue gravitational waves
• Testing aligned CP-violating Higgs sector at future lepton colliders
• Learning orbital dynamics of binary black hole systems from gravitational wave measurements
• Discovering new forces with gravitational waves from supermassive black holes
• Evolution of supermassive black hole binaries and tidal disruption rates in nonspherical galactic nuclei
• Constraining the Gravitational-Wave Spectrum from Cosmological First-Order Phase Transitions Using Data from LIGO-Virgo First Three Observing Runs
• Probing the Origin of Primordial Black Holes through Novel Gravitational Wave Spectrum
• Detection of Low Tension Cosmic Superstrings
• Searching for gravitational waves via Doppler tracking by future missions to Uranus and Neptune
• Adaptive mesh refinement in binary black holes simulations
• Gravitational waves detectable in laser interferometers from axion-SU(2) inflation
• Measuring the primordial gravitational wave background in the presence of other stochastic signals
• Polarized gravitational waves in the parity violating scalar-nonmetricity theory
• Probing the primordial Universe with 21-cm line from cosmic dawn/epoch of reionization
• Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
• On Detecting Stellar Binary Black Holes via the LISA-Taiji Network
• Supercooling of the A phase of ${}^3$He
• Enhance Primordial Black Hole Abundance through the Non-linear Processes around Bounce Point
• Using Gravitational Wave Parallax to Measure the Hubble Parameter with Pulsar Timing Arrays
• Waterfall stiff period can generate observable primordial gravitational waves
• Geodesic Congruences and a Collapsing Stellar Distribution in f (T ) Theories
• The Electro-Weak Phase Transition at Colliders: Discovery Post-Mortem
• Sensitivity limits of space-based interferometric gravitational wave observatories from the solar wind
• Neutron star mass in dark matter clumps
• Accuracy of estimation of parameters with space-borne gravitational wave observatory
• Gravitational Wave Sources as Timing References for LISA Data
• No slip gravity in light of LISA standard sirens
• Path-Dependent Supercooling of the ${}^3$He Superfluid A-B transition
• On the gauge dependence of scalar induced secondary gravitational waves during radiation and matter domination eras
• Dynamical Formation Scenarios for GW190521 and Prospects for Decihertz Gravitational-Wave Astronomy with GW190521-Like Binaries
• Gravitational waves in neutrino plasma and NANOGrav signal
• Inspirals into a charged black hole
• Detecting the Orbital Motion of Nearby Supermassive Black Hole Binaries with Gaia
• Time-crystal ground state and production of gravitational waves from QCD phase transition
• Detection of Gravitational Waves using Parametric Resonance in Bose-Einstein Condensates
• Model-independent features of gravitational waves from bubble collisions
• Cosmological Tests of Gravity: A Future Perspective
• 2MASX J00423991+3017515: An offset active galactic nucleus in an interacting system
• Future merger of the Milky Way with the Andromeda galaxy and the fate of their supermassive black holes
• How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
• Impact of dipolar magnetic fields on gravitational wave strain by galactic binaries
• Boltzmann equations for astrophysical Stochastic Gravitational Wave Backgrounds scattering off of massive objects
• Detection of gravitational waves in circular particle accelerators
• The Pairing Probability of Massive Black Holes in Merger Galaxies in the Presence of Radiative Feedback
• LISA Constraints on an Intermediate-Mass Black Hole in the Galactic Centre
• Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants
• Proving the short-wavelength approximation in Pulsar Timing Array gravitational-wave background searches
• Stochastic gravitational wave background: birth from string-wall death
• Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
• Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Divergences in gravitational-wave emission and absorption from extreme mass ratio binaries
• The effect of screening mechanisms on black hole binary inspiral waveforms
• Eclipses of continuous gravitational waves as a probe of stellar structure
• Iterative time-domain method for resolving multiple gravitational wave sources in Pulsar Timing Array data
• Post-Newtonian Kozai-Lidov Mechanism and its Effect on Cumulative Shift of Periastron Time of Binary Pulsar
• Tidally excited oscillations in hot white dwarfs
• Gravitational wave cosmology I: high frequency approximation
• Imprint of Early Dark Energy in Stochastic Gravitational Wave Background
• Probing the Delay Time of Supermassive Black Hole Binary Mergers With Gravitational Waves
• Motion of localized sources in general relativity: gravitational self-force from quasilocal conservation laws
• Prospecting bipartite Dark Matter through Gravitational Waves
• Leptogenesis, Dark Matter and Gravitational Waves from Discrete Symmetry Breaking
• Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319
• On the detectability of ultra-compact binary pulsar systems
• Spherical harmonic analysis of anisotropies in polarized stochastic gravitational wave background with interferometry experiments
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Continuous gravitational waves from trapped magnetar ejecta and the connection to glitches and antiglitches
• Symbolic Knowledge Extraction from Opaque Predictors Applied to Cosmic-Ray Data Gathered with LISA Pathfinder
• Were recently reported MHz events planet mass primordial black hole mergers?
• Whispers from the quantum core: the ringdown of semiclassical stars
• Gravitational spin-orbit dynamics at the fifth-and-a-half post-Newtonian order
• Gravitational effects on fluid dynamics in cosmological first-order phase transitions
• Predictions for LISA and PTA based on SHARK galaxy simulations
• Detection of gravitational wave mixed polarization with single space-based detectors
• Asymptotic behavior of null geodesics near future null infinity: Significance of gravitational waves
• Lifshitz scaling, ringing black holes, and superradiance
• Characteristic formulation of the Regge-Wheeler and Zerilli Green functions
• Distortion of Gravitational-wave Signals by Astrophysical Environments
• Transition from inspiral to plunge for braneworld EMRI
• Gravitational wave spectral synthesis
• Sparsity Based Recovery of Galactic Binaries Gravitational Waves
• Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
• A model-independent tripartite test of cosmic distance relations
• Gravitational waves for eccentric extreme mass ratio inspirals of self-dual spacetime
• Multiple peaks in gravitational waves induced from primordial curvature perturbations with non-Gaussianity
• A novel stacked hybrid autoencoder for imputing LISA data gaps
• Detectability of Gravitational Wave from a population of Inspiralling Black Holes in Milky Way Mass Galaxies
• Orbit Tomography of Binary Supermassive Black Holes with Very Long Baseline Interferometry
• Tracing Astrophysical Black Hole Seeds and Primordial Black Holes with LISA-Taiji Network
• Assessing the Impact of Unequal Noises and Foreground Modeling on SGWB Reconstruction with LISA
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Stochastic gravitational waves from spin-3/2 fields -- Hunting SUSY in the sky
• Anisotropies of cosmological gravitational wave backgrounds in non-flat spacetime
• Searching for clues of past binary supermassive black hole mergers in nuclear star clusters
• GPU-Accelerated Periodic Source Identification in Large-Scale Surveys: Measuring $P$ and $\dot{P}$
• Intermediate-mass ratio inspirals in merging elliptical galaxies
• Effects of the Hubble Parameter on the Cosmic Growth of the First Quasars
• Extracting parity-violating gravitational waves from projected tidal force tensor in three dimensions
• Reissner-Nordström perturbation framework with gravitational wave applications
• Core Noise Requirements, and GW Sensitivities of AMIGO
• The Merger Rate of Black Holes in a Primordial Black Hole Cluster
• Ultra-low noise laser and optical frequency comb-based timing system for the Black Hole Explorer (BHEX) mission
• What do gravitational wave detectors say about polymer quantum effects?
• Gamma rays from dark matter spikes in EAGLE simulations
• Discovering neutron stars with LISA via measurements of orbital eccentricity in Galactic binaries
• Can we use next-generation gravitational wave detectors for terrestrial precision measurements of Shapiro delay?
• Cosmic superstrings in large volume compactifications: PTAs, LISA and time-varying tension
• Black holes in General Relativity and beyond
• Accretion of clumpy cold gas onto massive black holes binaries: the challenging formation of extended circumbinary structures
• Circumbinary discs from tidal disruption events
• Testing gravitational waveform models using angular momentum
• On exotic objects made of dark energy and dark matter: Mass-to-radius profiles and tidal Love numbers
• Compact object populations over cosmic time II. Compact object merger rates and masses over redshift from varying initial conditions
• Gravitational Wave luminosity distance in viscous cosmological models
• Will Gravitational Waves Discover the First Extra-Galactic Planetary System?
• Effect of solar free oscillations on TianQin's range acceleration noise
• Multipolar Particles in Helically Symmetric Spacetimes
• Probing PeV scale SUSY-breaking with Satellite Galaxies and Primordial Gravitational Waves
• Exploring Dark Forces with Multimessenger Studies of Extreme Mass Ratio Inspirals
• Primordial black holes in SB SUSY Gauss-Bonnet inflation
• Gravitational Wave Probe of Primordial Black Hole Origin via Superradiance
• Astrophysical Parameter Inference on Accreting White Dwarf Binaries using Gravitational Waves
• Next step in gravity and cosmology: fundamental theory or data-driven models?
• Probing the formation of the seeds of supermassive black holes with gravitational waves
• Properties of loss cone stars in a cosmological galaxy merger remnant
• Co-Interacting Dark Matter
• Periodicities in the K2 lightcurve of HP Librae
• On the Formation of GW190521-like Binary Black Hole Merger Systems
• Science Potential for Stellar-mass Black Holes as Neighbors of Sgr A*
• Gravitational wave background from primordial black holes in globular clusters
• Black-Hole Perturbation Plus Post-Newtonian Theory: Hybrid Waveform for Neutron Star Binaries
• Gravitational radiation in Infinite Derivative Gravity and connections to Effective Quantum Gravity
• Gravitational Wave Signatures of Primordial Black Hole Reheating in Upcoming Interferometry Missions
• Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
• Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
• Primordial black holes and magnetic fields in conformal neutrino mass models
• Disturbances from Single Event Upsets in the GRACE Follow-On Laser Ranging Interferometer
• Can asteroid-mass PBHDM be compatible with catalyzed phase transition interpretation of PTA?
• A protocol of potential advantage in the low frequency range to gravitational wave detection with space based optical atomic clocks
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• On the anisotropies of the cosmological gravitational-wave background from pulsar timing array observations
• Angular Momentum Loss for a Binary System in Einstein-Æther Theory
• Trumpet Initial Data for Boosted Black Holes
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Sky localization of space-based detectors with time-delay interferometry
• Lensing convergence and anisotropic dark energy in galaxy redshift surveys
• Magnetic Field Simulation and Correlated Low-Frequency Noise Subtraction for an In-Orbit Demonstrator of Magnetic Measurements
• Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
• A prototype differential atom interferometer for fundamental physics
• A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
• Geometry-Information Duality: Quantum Entanglement Contributions to Gravitational Dynamics
• Projected gravitational wave constraints on primordial black hole abundance for extended mass distributions
• Probing the horizon of black holes with gravitational waves
• Testing Lorentz symmetry with space-based gravitational-wave detectors
• Scalar Self-force for High Spin Black Holes
• 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
• Binary Black Hole Information Loss Paradox & Future Prospects
• An estimate of the gravitational-wave background from the observed cosmological distribution of quasars
• Conformal Unification in a Quiver Theory and Gravitational Waves
• On the effect of pulsar evaporation on the cooling of white dwarfs
• Detecting the heterodyning of gravitational waves
• Prospects for gravitational wave astronomy with next generation large-scale pulsar timing arrays
• Formation of counter-rotating and highly eccentric massive black hole binaries in galaxy mergers
• Merging Black Holes in Dwarf Galaxies: Calculating Binary Black Hole Coalescence Timescales from Simulations for LISA Detection
• Testing hilltop supernatural inflation with gravitational waves
• Regularization of a scalar charged particle for generic orbits in Kerr spacetime
• Constraints on Population I/II neutron star-black hole binary formation by gravitational wave and radio observations
• Co-interacting dark matter and conformally coupled light scalars
• Spin dynamics of moving bodies in rotating black hole spacetimes
• Rotations of the polarization of a gravitational wave propagating in Universe
• Circularly Polarized Gravitational Wave Background Search with a Network of Space-borne Triangular Detectors
• Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
• Gravitational waves from patterns of electroweak symmetry breaking: an effective perspective
• PCB Transducer Coil Design for a Low-Noise Magnetic Measurement System in Space Missions
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• Population Synthesis of Gravitational Wave Sources
• Constraints on the Scale Parameter of Regular Black Hole in Asymptotically Safe Gravity from Extreme Mass Ratio Inspirals
• Thermal X-ray signatures in late-stage unequal-mass massive black hole binary mergers
• Quantum gravity phenomenology from the perspective of quantum general relativity and quadratic gravity
• Gravitational waves from primordial black hole dominance: The effect of inflaton decay rate
• Connecting low-redshift LISA massive black hole mergers to the nHz stochastic gravitational wave background
• Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum
• Gravitational Wave Emission by Accretion of Matter and Magnetic Deformation in Fast Rotating White Dwarfs
• Dipolar magnetic fields in binaries and gravitational waves
• Gravitational wave energy spectral density properties from BPASS Galactic binary population in the Milky Way galaxy
• Signatures of Exploding Supermassive PopIII Stars at High Redshift in JWST, EUCLID and Roman Space Telescope
• Gravitational waves from a first-order phase transition of the inflaton
• Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions
• Spontaneous baryogenesis and generation of gravitational waves in a new model of quintessential $\alpha$-attractor
• An introduction to gravitational waves through electrodynamics: a quadrupole comparison
• Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts
• The Stochastic Gravitational Wave Background from Primordial Gravitational Atoms
• GWAI: Artificial Intelligence Platform for Enhanced Gravitational Wave Data Analysis
• Spatial Dependence of the Growth Factor in Scalar-Tensor Cosmology
• Parsec-scale jet precession and a putative supermassive binary black hole system in the blazar AO 0235+164
• Extracting the orbital axis from gravitational waves of precessing binary systems
• Rapid multi-band space-based optical timing: revolutionizing accretion physics
• Cosmology of the companion-axion model: dark matter, gravitational waves, and primordial black holes
• Chirping compact stars: gravitational radiation and detection degeneracy with binary systems A conceptual pathfinder for space-based gravitational-wave observatories
• Demonstration of tilt sensing using a homodyne quadrature interferometric translational sensor
• Description and Application of the Surfing Effect
• Radiation Tolerance of Low-Noise Photoreceivers for the LISA Space Mission
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Optimal design of interpolation methods for time-delay interferometry
• Spectroscopic confirmation of dual and offset quasars from the Subaru HSC-SSP program
• Computing Challenges for the Einstein Telescope project
• Preliminary census of galaxies in the LISA localisation volume: I. Searching for LISA candidate massive black hole binary merger hosts using Sloan Digital Sky Survey photometry