The Gravitational-Wave Physics II: Progress

Abstract

It has been a half-decade since the first direct detection of gravitational waves, which signifies the coming of the era of the gravitational-wave astronomy and gravitational-wave cosmology. The increasing number of the detected gravitational-wave events has revealed the promising capability of constraining various aspects of cosmology, astronomy, and gravity. Due to the limited space in this review article, we will briefly summarize the recent progress over the past five years, but with a special focus on some of our own work for the Key Project ``Physics associated with the gravitational waves'' supported by the National Natural Science Foundation of China. In particular, (1) we have presented the mechanism of the gravitational-wave production during some physical processes of the early Universe, such as inflation, preheating and phase transition, and the cosmological implications of gravitational-wave measurements; (2) we have put constraints on the neutron star maximum mass according to GW170817 observations; (3) we have developed a numerical relativity algorithm based on the finite element method and a waveform model for the binary black hole coalescence along an eccentric orbit.

arXiv commentv1, 93 pages, 18 figures, prepared as a status review of project report for Sci. China Phys. Mech. Astron.; v2, 95 pages, minor revision, references added, accepted for publication in Sci. China Phys. Mech. Astron; v3, to match the published version

References in corpus (694)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Multi-messenger Observations of a Binary Neutron Star Merger
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• GW170817: Measurements of Neutron Star Radii and Equation of State
• Observational evidence for self-interacting cold dark matter
• TianQin: a space-borne gravitational wave detector
• In the Realm of the Hubble tension $-$ a Review of Solutions
• Towards the Theory of Reheating After Inflation
• Reheating after Inflation
• Tests of general relativity with GW150914
• Evolution of Binary Black Hole Spacetimes
• Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
• Laser Interferometer Space Antenna
• Effective one-body approach to general relativistic two-body dynamics
• A unified equation of state of dense matter and neutron star structure
• Gravitational wave extraction from an inspiraling configuration of merging black holes
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• A gravitational-wave standard siren measurement of the Hubble constant
• Did LIGO detect dark matter?
• Tensions between the Early and the Late Universe
• Non-Gaussianity from Inflation: Theory and Observations
• New cosmological constraints on primordial black holes
• Primordial Black Holes as Dark Matter
• Dark Matter Self-interactions and Small Scale Structure
• Acoustic Signatures in the Primary Microwave Background Bispectrum
• Magnetic Fields in the Early Universe
• Dark Energy after GW170817: dead ends and the road ahead
• A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
• Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds
• Composition and thermodynamics of nuclear matter with light clusters
• Primordial Black Hole Scenario for the Gravitational-Wave Event GW150914
• Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions
• Universe Reheating after Inflation
• Gravitational Radiation from First-Order Phase Transitions
• The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
• Strong constraints on cosmological gravity from GW170817 and GRB 170817A
• Primordial Black Holes - Perspectives in Gravitational Wave Astronomy -
• Dark Energy after GW170817 and GRB170817A
• Astrophysical Implications of the Binary Black-Hole Merger GW150914
• Cosmological Magnetic Fields: Their Generation, Evolution and Observation
• Primordial Black Holes as Dark Matter: Recent Developments
• Using gravitational-wave standard sirens
• The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave Background
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• Observation of gravitational waves from two neutron star-black hole coalescences
• Compact Object Modeling with the StarTrack Population Synthesis Code
• Density Perturbations and Black Hole Formation in Hybrid Inflation
• Gravitational-wave sensitivity curves
• Black holes, gravitational waves and fundamental physics: a roadmap
• Detecting gravitational waves from cosmological phase transitions with LISA: an update
• Beyond LISA: Exploring Future Gravitational Wave Missions
• The cosmological gravitational wave background from primordial density perturbations
• Primordial Black Holes as a dark matter candidate
• Tests of General Relativity with GW170817
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Energy Budget of Cosmological First-order Phase Transitions
• Gravitational Wave Production by Collisions: More Bubbles
• Binary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution
• Taiji Program: Gravitational-Wave Sources
• Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
• Gravitational waves from the sound of a first order phase transition
• Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations
• Sensitivity curves for searches for gravitational-wave backgrounds
• Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters
• Numerical simulations of acoustically generated gravitational waves at a first order phase transition
• European Pulsar Timing Array Limits On An Isotropic Stochastic Gravitational-Wave Background
• Microlensing constraints on primordial black holes with the Subaru/HSC Andromeda observation
• Primordial black holes from single field models of inflation
• A simple construction of initial data for multiple black holes
• Detector configuration of DECIGO/BBO and identification of cosmological neutron-star binaries
• Gravitational Radiation from Colliding Vacuum Bubbles: Envelope Approximation to Many-Bubble Collisions
• Relativistic Mean-Field Theory and the High-Density Nuclear Equation of State
• The stochastic gravitational wave background from turbulence and magnetic fields generated by a first-order phase transition
• Towards the Theory of Cosmological Phase Transitions
• The afterglow of GRB050709 and the nature of the short-hard gamma-ray bursts
• Gravitational waves from binary supermassive black holes missing in pulsar observations
• Science with the space-based interferometer eLISA. I: Supermassive black hole binaries
• High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array
• The origin, evolution and signatures of primordial magnetic fields
• Massive Primordial Black Holes from Hybrid Inflation as Dark Matter and the seeds of Galaxies
• Effective-one-body model for black-hole binaries with generic mass ratios and spins
• Low-frequency gravitational-wave science with eLISA/NGO
• Shape of the acoustic gravitational wave power spectrum from a first order phase transition
• Gravitational Waves Induced by non-Gaussian Scalar Perturbations
• Relativistic second-order perturbations of the Einstein-de Sitter Universe
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• Planck 2015 results. XVI. Isotropy and statistics of the CMB
• Double Compact Objects II: Cosmological Merger Rates
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background
• A massive binary black-hole system in OJ287 and a test of general relativity
• Constraints on Earth-mass primordial black holes from OGLE 5-year microlensing events
• Testing the no-hair theorem with GW150914
• Prospects for Fundamental Physics with LISA
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• Deformations of Accreting Neutron Star Crusts and Gravitational Wave Emission
• Features of heavy physics in the CMB power spectrum
• GW150914: Implications for the stochastic gravitational wave background from binary black holes
• The diversity of Type Ia Supernovae: evidence for systematics?
• The TianQin project: current progress on science and technology
• Relic gravitational waves produced after preheating
• Preheating in the Standard Model with the Higgs-Inflaton coupled to gravity
• Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources
• Analytic black hole perturbation approach to gravitational radiation
• Large-scale structure, the cosmic microwave background, and primordial non-gaussianity
• Gravitational radiation from compact binary systems: gravitational waveforms and energy loss to second post-Newtonian order
• The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
• On the Maximal Strength of a First-Order Electroweak Phase Transition and its Gravitational Wave Signal
• General Properties of the Gravitational Wave Spectrum from Phase Transitions
• Gravitational wave generation from bubble collisions in first-order phase transitions: an analytic approach
• No large population of unbound or wide-orbit Jupiter-mass planets
• The Association of Jet Production with Geometrically Thick Accretion Flows and Black Hole Rotation
• High-energy gravitational scattering and the general relativistic two-body problem
• A systematic search for close supermassive black hole binaries in the Catalina Real-Time Transient Survey
• Cosmic anti-friction and accelerated expansion
• Considerations for a Multi-beam Multi-purpose Survey with FAST
• Gravitational Radiation From Cosmological Turbulence
• GW190521: orbital eccentricity and signatures of dynamical formation in a binary black hole merger signal
• Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
• Spin-Isospin Structure and Pion Condensation in Nucleon Matter
• The International Pulsar Timing Array: Second data release
• Short GRB and binary black hole standard sirens as a probe of dark energy
• Gravitational wave energy budget in strongly supercooled phase transitions
• New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions
• The Astrophysics of Nanohertz Gravitational Waves
• High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
• First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
• Electroweak Bubble Wall Speed Limit
• Primordial black holes as a dark matter candidate are severely constrained by the Galactic Center 511 keV gamma-ray line
• Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
• General Relativistic Dynamics of Irrotational Dust: Cosmological Implications
• A Gravitational Wave Background from Reheating after Hybrid Inflation
• Cosmic String Interpretation of NANOGrav Pulsar Timing Data
• Single Field Double Inflation and Primordial Black Holes
• Primordial Black Holes as Generators of Cosmic Structures
• Gravitational waves from stochastic relativistic sources: primordial turbulence and magnetic fields
• Inference of the cosmological parameters from gravitational waves: application to second generation interferometers
• Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
• Scalaron from $R^2$-gravity as a Heavy Field
• Probing the gravitational wave background from cosmic strings with LISA
• Gravitational wave snapshots of generic extreme mass ratio inspirals
• The evolution of massive black holes and their spins in their galactic hosts
• Can electroweak bubble walls run away?
• How fast can the wall move? A study of the electroweak phase transition dynamics
• Has NANOGrav found first evidence for cosmic strings?
• Ultra-high precision cosmology from gravitational waves
• A Population of Short-Period Variable Quasars from PTF as Supermassive Black Hole Binary Candidates
• Gravitational Wave Production At The End Of Inflation
• Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism
• Cosmic microwave background bounds on primordial black holes including dark matter halo accretion
• Cosmic dynamics in the era of Extremely Large Telescopes
• Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
• Prototype effective-one-body model for nonprecessing spinning inspiral-merger-ringdown waveforms
• Scalar-tensor theories and modified gravity in the wake of GW170817
• Accurate evolutions of unequal-mass neutron-star binaries: properties of the torus and short GRB engines
• Femtolensing by Dark Matter Revisited
• The abundance of primordial black holes depends on the shape of the inflationary power spectrum
• A stochastic background of gravitational waves from hybrid preheating
• The cosmological Higgstory of the vacuum instability
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Second-order Perturbations of the Friedmann World Model
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Gravitational waves from bubble collisions: analytic derivation
• GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
• A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
• Dark Matter Triggers of Supernovae
• Inflationary Primordial Black Holes as All Dark Matter
• European Pulsar Timing Array Limits on Continuous Gravitational Waves from Individual Supermassive Black Hole Binaries
• Implications of the NANOGrav results for inflation
• Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
• Anisotropic stress as signature of non-standard propagation of gravitational waves
• Primordial Black Holes as All Dark Matter
• Cosmography with the Einstein Telescope
• Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
• Stochastic Gravitational Wave Production After Inflation
• Calculating the mass spectrum of primordial black holes
• Self-resonance after inflation: oscillons, transients and radiation domination
• Testing modified gravity at cosmological distances with LISA standard sirens
• Cosmic Conundra Explained by Thermal History and Primordial Black Holes
• Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice
• Could supermassive black holes be quintessential primordial black holes?
• The gravitational-wave memory effect
• The Growth of Bubbles in Cosmological Phase Transitions
• An improved effective-one-body Hamiltonian for spinning black-hole binaries
• The Threshold for Primordial Black Hole Formation: a Simple Analytic Prescription
• Revisiting constraints on asteroid-mass primordial black holes as dark matter candidates
• Gravitational waves at interferometer scales and primordial black holes in axion inflation
• Detecting gravitational-wave memory with LIGO: implications of GW150914
• Dark energy in Horndeski theories after GW170817: A review
• The Spectrum of Gravitational Radiation from Primordial Turbulence
• Cosmic phase transitions: their applications and experimental signatures
• Testing Primordial Black Holes as Dark Matter through LISA
• Electroweak Phase Transition in Two Higgs Doublet Models
• Primordial black holes with an accurate QCD equation of state
• Cosmology with the lights off: Standard sirens in the Einstein Telescope era
• Primordial Black Hole Formation in a Double Inflation Model in Supergravity
• Chaotic new inflation and formation of primordial black holes
• The gravitational-wave luminosity distance in modified gravity theories
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• Supersymmetric Electroweak Baryogenesis
• Theoretical uncertainties for cosmological first-order phase transitions
• Two populations of LIGO-Virgo black holes
• Dual Jets from Binary Black Holes
• Compact binary evolutions with the Z4c formulation
• Detecting a small perturbation through its non-Gaussianity
• A Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• Universal infrared scaling of gravitational wave background spectra
• Sound shell model for acoustic gravitational wave production at a first-order phase transition in the early Universe
• Primordial Black Holes from $\alpha$-attractors
• A new calculation of the mass fraction of primordial black holes
• Modified gravitational-wave propagation and standard sirens
• Neutrino and Positron Constraints on Spinning Primordial Black Hole Dark Matter
• Improved Results in Supersymmetric Electroweak Baryogenesis
• Constraint Likelihood analysis for a network of gravitational wave detectors
• Solar-Mass Primordial Black Holes Explain NANOGrav Hint of Gravitational Waves
• Pulsar searches and timing with the SKA
• Search for gravitational lensing signatures in LIGO-Virgo binary black hole events
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run
• Primordial black holes in non-Gaussian regimes
• Primordial black holes and second order gravitational waves from ultra-slow-roll inflation
• Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
• Generating PBHs and small-scale GWs in two-field models of inflation
• Primordial Black Holes from a tiny bump/dip in the Inflaton potential
• Post-Newtonian corrections to the gravitational-wave memory for quasicircular, inspiralling compact binaries
• A review of gravitational waves from cosmic domain walls
• The Equation of State and Duration to Radiation Domination After Inflation
• Primordial Black Holes Confront LIGO/Virgo data: Current situation
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Constraints on cosmic string tension imposed by the limit on the stochastic gravitational wave background from the European Pulsar Timing Array
• Hamiltonian of a spinning test-particle in curved spacetime
• The First Round Result from the TianQin-1 Satellite
• Primordial black hole formation from an axion-like curvaton model
• A waveform model for eccentric binary black hole based on effective-one-body-numerical-relativity (EOBNR) formalism
• Gravitational waves from a first order electroweak phase transition: a brief review
• Bubble Wall Velocity at the Electroweak Phase Transition
• Estimate of the primordial magnetic field helicity
• Seeding primordial black holes in multifield inflation
• Vorticity, kinetic energy, and suppressed gravitational wave production in strong first order phase transitions
• Constraining primordial black hole abundance with the Galactic 511 keV line
• Supersymmetric CP-violating Currents and Electroweak Baryogenesis
• The MSSM Electroweak Phase Transition on the Lattice
• The exponential tail of inflationary fluctuations: consequences for primordial black holes
• Gravitational waves from first order cosmological phase transitions in the Sound Shell Model
• The Ineludible non-Gaussianity of the Primordial Black Hole Abundance
• A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
• Primordial Black Holes from Sound Speed Resonance during Inflation
• Constraints on cosmic strings using data from the first Advanced LIGO observing run
• The Local Rate and the Progenitor Lifetimes of Short-Hard Gamma-Ray Bursts: Synthesis and Predictions for LIGO
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• Cosmology with Strong Lensing Systems
• Primordial black hole production during first-order phase transitions
• The Gravitational-Wave Physics
• Constraints on primordial black holes from Galactic gamma-ray background
• Constraints on binary neutron star merger product from short GRB observations
• An improved analysis of GW150914 using a fully spin-precessing waveform model
• Gravitational Waves Induced by Scalar Perturbations with a Lognormal Peak
• Induced gravitational waves in a general cosmological background
• Relic Backgrounds of Gravitational Waves from Cosmic Turbulence
• Dynamics of dwarf galaxies disfavor stellar-mass black hole dark matter
• PBHs and secondary GWs from ultra slow roll and punctuated inflation
• The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries
• A New Population of High Redshift Short-Duration Gamma-Ray Bursts
• Induced gravitational waves as a probe of thermal history of the universe
• Gravitational Waves from Abelian Gauge Fields and Cosmic Strings at Preheating
• Detection of Anisotropies in the Gravitational-Wave Stochastic Background
• A precise extragalactic test of General Relativity
• Massive black hole binaries: dynamical evolution and observational signatures
• The LISA-Taiji network
• Precision cosmology from future lensed gravitational wave and electromagnetic signals
• Phase Transitions in an Expanding Universe: Stochastic Gravitational Waves in Standard and Non-Standard Histories
• Second-order Gauge Invariant Cosmological Perturbation Theory: -- Einstein equations in terms of gauge invariant variables --
• Nuclear Equation of State from Observations of Short Gamma-Ray Burst Remnants
• Gravitational waves from vacuum first order phase transitions II: from thin to thick walls
• Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters
• Primordial Black Holes from Inflaton Fragmentation into Oscillons
• Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries
• Double inflation as a single origin of primordial black holes for all dark matter and LIGO observations
• Type Ia Supernovae, Evolution, and the Cosmological Constant
• Primordial seeds of supermassive black holes
• Numerical Simulations of Gravitational Waves from Early-Universe Turbulence
• Primordial black holes from supersymmetry in the early universe
• Descope of the ALIA mission
• Gravitational Waves and Dark Radiation from Dark Phase Transition: Connecting NANOGrav Pulsar Timing Data and Hubble Tension
• Primordial Black Holes from Inflation with Nonminimal Derivative Coupling
• Constraining the primordial black hole scenario with Bayesian inference and machine learning: the GWTC-2 gravitational wave catalog
• Analytic Description of Primordial Black Hole Formation from Scalar Field Fragmentation
• Nonlinear gravitational-wave memory from binary black hole mergers
• Science with the TianQin observatory: Preliminary results on massive black hole binaries
• Towards an all-orders calculation of the electroweak bubble wall velocity
• Gravitational Radiation, Inspiraling Binaries, and Cosmology
• How Gravitational-wave Observations Can Shape the Gamma-ray Burst Paradigm
• An all-sky search for continuous gravitational waves in the Parkes Pulsar Timing Array data set
• Constraints on cosmological models from strong gravitational lensing systems
• Exploring Primordial Black Holes from the Multiverse with Optical Telescopes
• Gravity Waves from Tachyonic Preheating after Hybrid Inflation
• Speed of Gravitational Waves from Strongly Lensed Gravitational Waves and Electromagnetic Signals
• Updated predictions for gravitational waves produced in a strongly supercooled phase transition
• Oscillations in the stochastic gravitational wave background from sharp features and particle production during inflation
• Flat-top oscillons in an expanding universe
• On the validity of perturbative studies of the electroweak phase transition in the Two Higgs Doublet model
• Gravitational waves from gauge preheating
• Complete waveform model for compact binaries on eccentric orbits
• Limits on primordial black holes from $\mu$ distortions in cosmic microwave background
• Model-independent energy budget of cosmological first-order phase transitions
• Lyman-$\alpha$ forest constraints on Primordial Black Holes as Dark Matter
• MSSM Electroweak Baryogenesis and Flavour Mixing in Transport Equations
• Gravitational waves from bubble dynamics: Beyond the Envelope
• Primordial black holes and secondary gravitational waves from k/G inflation
• Transient resonances in the inspirals of point particles into black holes
• Effective Theories of MSSM at High Temperature
• The Parkes Pulsar Timing Array Project: Second data release
• Gauge Independence of Induced Gravitational Waves
• Anisotropies and non-Gaussianity of the Cosmological Gravitational Wave Background
• Cosmography with strong lensing of LISA gravitational wave sources
• Primordial Black Holes for the LIGO Events in the Axion-like Curvaton Model
• Cosmic strings from preheating
• Scalar Induced Gravitational Waves in Different Gauges
• Bubble Expansion and the Viability of Singlet-Driven Electroweak Baryogenesis
• Bubble wall velocity: heavy physics effects
• Constraining axion inflation with gravitational waves from preheating
• Magnetic field production during preheating at the electroweak scale
• Gravitational radiation from a bulk flow model
• Extending the effective-one-body Hamiltonian of black-hole binaries to include next-to-next-to-leading spin-orbit couplings
• Primordial Black Holes from the inflating curvaton
• Anisotropies of Gravitational Wave Backgrounds: A Line Of Sight Approach
• The fate of large-scale structure in modified gravity after GW170817 and GRB170817A
• Evolution of hydromagnetic turbulence from the electroweak phase transition
• A milliparsec supermassive black hole binary candidate in the galaxy SDSS J120136.02+300305.5
• Primordial black holes and gravitational waves from parametric amplification of curvature perturbations
• The 2-loop MSSM finite temperature effective potential with stop condensation
• A Cosmological Signature of the Standard Model Higgs Vacuum Instability: Primordial Black Holes as Dark Matter
• Orbital Evolution of Extreme-Mass-Ratio Black-Hole Binaries with Numerical Relativity
• Bayesian Evidence for Both Astrophysical and Primordial Black Holes: Mapping the GWTC-2 Catalog to Third-Generation Detectors
• When Primordial Black Holes from Sound Speed Resonance Meet a Stochastic Background of Gravitational Waves
• Unified treatment of cosmological perturbations from super-horizon to small scales
• Detectability of Gravitational Waves from Phase Transitions
• Spectroscopic Indication for a Centi-parsec Supermassive Black Hole Binary in the Galactic Center of NGC 5548
• The NANOGrav 12.5-year Data Set: Wideband Timing of 47 Millisecond Pulsars
• Gravitational Waves from Oscillon Preheating
• Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
• Measuring the mass of solar system planets using pulsar timing
• Do Stops Slow Down Electroweak Bubble Walls?
• PBH in single field inflation: the effect of shape dispersion and non-Gaussianities
• On the Origin of GW190521-like events from repeated black hole mergers in star clusters
• Influence of heavy modes on perturbations in multiple field inflation
• The power spectrum on small scales: Robust constraints and comparing PBH methodologies
• Tests for primordial non-Gaussianity
• Turning in the landscape: a new mechanism for generating Primordial Black Holes
• Searching for gravitational wave memory bursts with the Parkes Pulsar Timing Array
• Standard sirens with a running Planck mass
• Primordial black hole production due to preheating
• Gravitational waves from oscillons after inflation
• Testing the speed of gravitational waves over cosmological distances with strong gravitational lensing
• Model-independent energy budget for LISA
• Primordial black holes from scalar field evolution in the early universe
• Gravitational Radiation from Primordial Helical Inverse Cascade MHD Turbulence
• Primordial black holes from sound speed resonance in the inflaton-curvaton mixed scenario
• Relic gravitational waves from colliding bubbles and cosmic turbulence
• Primordial Anisotropies in the Gravitational Wave Background from Cosmological Phase Transitions
• From Boltzmann equations to steady wall velocities
• High Temperature Dimensional Reduction of the MSSM and other Multi-Scalar Models
• Characterizing the Cosmological Gravitational Wave Background Anisotropies and non-Gaussianity
• General Relativistic Simulations of Magnetized Plasmas around Merging Supermassive Black Holes
• Resonant multiple peaks in the induced gravitational waves
• What if Planet 9 is a Primordial Black Hole?
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back)
• Thanks for the memory: measuring gravitational-wave memory in the first LIGO/Virgo gravitational-wave transient catalog
• Primordial Black Holes in Higgs-$R^2$ Inflation as a Whole Dark Matter
• Scalar induced gravitational waves in inflation with gravitationally enhanced friction
• Anisotropies in the stochastic gravitational-wave background: Formalism and the cosmic string case
• Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition
• Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
• A pulsar-based timescale from the International Pulsar Timing Array
• On the Gauge Invariance of Cosmological Gravitational Waves
• Cosmology and dark energy from joint gravitational wave-GRB observations
• Galaxy-Scale Strong Lensing Tests of Gravity and Geometric Cosmology: Constraints and Systematic Limitations
• Computation of Displacement and Spin Gravitational Memory in Numerical Relativity
• Pulsar Timing Array Constraints on the Induced Gravitational Waves
• Gravitational wave spectra from strongly supercooled phase transitions
• Please repeat: Strong lensing of gravitational waves as a probe of compact binary and galaxy populations
• Constraints on Stupendously Large Black Holes
• Primordial black holes dark matter from inflection point models of inflation and the effects of reheating
• Pre-Merger Localization of Gravitational-Wave Standard Sirens With LISA: Triggered Search for an Electromagnetic Counterpart
• Ultra-compact (X-ray) binaries
• The gravitational waves from the first-order phase transition with a dimension-six operator
• Baryogenesis, Electric Dipole Moments and Dark Matter in the MSSM
• Validating the Effective-One-Body Numerical-Relativity Waveform Models for Spin-aligned Binary Black Holes along Eccentric Orbits
• Nonperturbative Analysis of the Electroweak Phase Transition in the Two Higgs Doublet Model
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• Gauge dependence of gravitational waves generated from scalar perturbations
• MSSM Electroweak Baryogenesis and LHC Data
• Gravitational memory in binary black hole mergers
• Gravitational Waves produced by Compressible MHD Turbulence from Cosmological Phase Transitions
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• Whispers from the dark side: Confronting light new physics with NANOGrav data
• Detecting gravitational waves from mountains on neutron stars in the Advanced Detector Era
• Primordial black holes and associated gravitational waves in axion monodromy inflation
• Gravitational Waves from Oscillons with Cuspy Potentials
• Oscillons from String Moduli
• Phase transition dynamics and gravitational wave spectra of strong first-order phase transition in supercooled universe
• NANOGrav signal from MHD turbulence at QCD phase transition in the early universe
• Low-frequency Gravitational Waves from Double-inflection-point Inflation
• Gravitational waves from a supercooled electroweak phase transition and their detection with pulsar timing arrays
• Dark energy after GW170817, revisited
• Listening to the Universe with Gravitational-Wave Astronomy
• Primordial black hole tower: Dark matter, earth-mass, and LIGO black holes
• A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity
• Baryogenesis from a dark first-order phase transition
• Lattice formulation of axion inflation. Application to preheating
• Primordial black holes and secondary gravitational waves from inflationary model with a non-canonical kinetic term
• Constraining the primordial black hole abundance with 21cm cosmology
• Disentangling Coalescing Neutron Star-White Dwarf Binaries for LISA
• Field-theoretic derivation of bubble-wall force
• Testing the dark energy with gravitational lensing statistics
• Electroweak Bubble Wall Friction: Analytic Results
• A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity
• Probing cosmic anisotropy with gravitational waves as standard sirens
• Effect of eccentricity on binary neutron star searches in Advanced LIGO
• On bubble collisions in strongly supercooled phase transitions
• Evidence for periodicity in 43 year-long monitoring of NGC 5548
• Gravitational waves from the electroweak phase transition
• On the gravitational wave sources from the NANOGrav 12.5-yr data
• An analytical approximation of the scalar spectrum in the ultra-slow-roll inflationary models
• Forecasts for detecting the gravitational-wave memory effect with Advanced LIGO and Virgo
• Anisotropies in the Gravitational Wave Background from Preheating
• Bubble wall velocities in the Standard Model and beyond
• Constraint on the Post-Newtonian Parameter gamma on Galactic Size Scales
• Reconstructing the dark sector interaction with LISA
• Adding Gravitational Memory to Waveform Catalogs using BMS Balance Laws
• Velocity of electroweak bubble walls
• Constraining the Anisotropic Expansion of Universe
• Primordial Black Hole Production in Inflationary Models of Supergravity with a Single Chiral Superfield
• Gravitational waves from asymmetric oscillon dynamics?
• Revisiting the envelope approximation: gravitational waves from bubble collisions
• Electroweak phase transition in the $\Sigma$SM - I: Dimensional reduction
• Constraints on the primordial curvature power spectrum from primordial black holes
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Inflationary preheating and primordial black holes
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Search for Eccentric Binary Neutron Star Mergers in the first and second observing runs of Advanced LIGO
• Direct detection of gravitational waves can measure the time variation of the Planck mass
• Fluid equations for fast-moving electroweak bubble walls
• Direction Dependence of the Deceleration Parameter
• Lattice study of an electroweak phase transition at m_h ~ 126 GeV
• A fresh look at the gravitational-wave signal from cosmological phase transitions
• Approximate gauge independence of the induced gravitational wave spectrum
• On the gauge dependence of gravitational waves generated at second order from scalar perturbations
• The Galactic Gravitational wave foreground
• Spatially Resolved Interstellar Medium and Highly-Excited Dense Molecular Gas in the Most Luminous Quasar at z=6.327
• Jumping the gap: searching for LIGO's biggest black holes
• The electromagnetic chirp of a compact binary black hole: a phase template for the gravitational wave inspiral
• The gravitational-wave memory from eccentric binaries
• Pulsar Timing Array Based Search for Supermassive Black Hole Binaries in the Square Kilometer Array Era
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• A first survey of spinning eccentric black hole mergers: Numerical relativity simulations, hybrid waveforms, and parameter estimation
• A probable Milli-Parsec Supermassive Binary Black Hole in the Nearest Quasar Mrk 231
• Diagrammatic approach to non-Gaussianity from inflation
• Gravitational wave standard sirens and cosmological parameter measurement
• Multi-messenger Probes of Inflationary Fluctuations and Primordial Black Holes
• Dimensional reduction of the Standard Model coupled to a new singlet scalar field
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Measurement Accuracy of Inspiraling Eccentric Neutron Star and Black Hole Binaries Using Gravitational Waves
• Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run
• Importance of transient resonances in extreme-mass-ratio inspirals
• Bubble Wall Velocity at Strong Coupling
• A Systematic Search for Periodically Varying Quasars in Pan-STARRS1: An Extended Baseline Test in Medium Deep Survey Field MD09
• Bubble nucleation and growth in very strong cosmological phase transitions
• Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-Wave Detections
• The Imprint of Relativistic Particles on the Anisotropies of the Stochastic Gravitational-Wave Background
• Strongly lensed gravitational waves from intrinsically faint double compact binaries - prediction for the Einstein Telescope
• Gravitational-wave memory: waveforms and phenomenology
• Primordial black holes and oscillating gravitational waves in slow-roll and slow-climb inflation with an intermediate non-inflationary phase
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Generalized Non-Minimal Derivative Coupling: Application to Inflation and Primordial Black Hole Production
• Detectability of ultra-compact X-ray binaries as LISA sources
• Measuring the eccentricity of GW170817 and GW190425
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• On the Anisotropy of the Gravitational Wave Background from Massless Preheating
• Polarized Cosmological Gravitational Waves from Primordial Helical Turbulence
• Gravitational wave and collider implications of electroweak baryogenesis aided by non-standard cosmology
• Formation of primordial black holes in an axionlike curvaton model
• Measuring Parity Violation in the Stochastic Gravitational Wave Background with the LISA-Taiji network
• Can we observe the QCD phase transition-generated gravitational waves through pulsar timing arrays?
• Primordial black holes from modified supergravity
• Dirac-Born-Infeld realization of sound speed resonance mechanism for primordial black holes
• A hybrid simulation of gravitational wave production in first-order phase transitions
• Primordial black holes and secondary gravitational waves from natural inflation
• Primordial magnetic fields from preheating at the electroweak scale
• Beyond the Starobinsky model for inflation
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• Polarized Gravitational Waves from Cosmological Phase Transitions
• Massively Parallel Simulations of Binary Black Hole Intermediate-Mass-Ratio Inspirals
• The $N_{\ell }$ of gravitational wave background experiments
• Measurements of the Hubble constant and cosmic curvature with quasars: ultra-compact radio structure and strong gravitational lensing
• Rank deficiency and Tikhonov regularization in the inverse problem for gravitational-wave bursts
• Primordial black hole dark matter in dilaton-extended two-field Starobinsky inflation
• On the wave optics effect on primordial black hole constraints from optical microlensing search
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• A Pseudospectral Method for Gravitational Wave Collapse
• What constraints on the neutron star maximum mass can one pose from GW170817 observations?
• Generalized framework for testing gravity with gravitational-wave propagation. III. Future prospect
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Gravitational waves from first order phase transitions as a probe of an early matter domination era and its inverse problem
• Hydrodynamics of phase transition fronts and the speed of sound in the plasma
• Can the observed large scale magnetic fields be seeded by helical primordial fields?
• Gaussian processes reconstruction of modified gravitational wave propagation
• Exploring the small mass ratio binary black hole merger via Zeno's dichotomy approach
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Real-Time History of the Cosmological Electroweak Phase Transition
• Magnetic field and gravitational waves from the first-order Phase Transition
• Three-dimensional effective theories for the two Higgs doublet model at high temperature
• Gravitational waves from first-order phase transitions: Ultra-supercooled transitions and the fate of relativistic shocks
• Damping of gravitational waves by matter
• Test of parametrized post-Newtonian gravity with galaxy-scale strong lensing systems
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Search for nonlinear memory from subsolar mass compact binary mergers
• Constraints on a mixed model of dark matter particles and primordial black holes from the Galactic 511 keV line
• Studying the solar system with the International Pulsar Timing Array
• A Possible ~20 yr Periodicity in Long-term Optical Photometric and Spectral Variations of the Nearby Radio-Quiet Active Galactic Nucleus Ark 120
• Parameter estimation for inspiraling eccentric compact binaries including pericenter precession
• Gravitational waves generated by second order effects during inflation
• Impact of eccentricity on the gravitational wave searches for binary black holes: High mass case
• Testing the cosmic curvature at high redshifts: the combination of LSST strong lensing systems and quasars as new standard candles
• Production of high stellar-mass primordial black holes in trapped inflation
• Planning the scientific applications of the Five-hundred-meter Aperture Spherical radio Telescope
• Gravitational waves from a very strong electroweak phase transition
• What can we learn from the stochastic gravitational wave background produced by oscillons?
• Primordial black holes from metric preheating: mass fraction in the excursion-set approach
• Phase Transition Generated Cosmological Magnetic Field at Large Scales
• A Parametrized post-Einsteinian Framework for Gravitational Wave Bursts
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Large Scale Structure
• The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory
• Standard-siren cosmology using gravitational waves from binary black holes
• The LISA-Taiji network: precision localization of massive black hole binaries
• Large anisotropies of the stochastic gravitational wave background from cosmic domain walls
• Exploring the Spectral Shape of Gravitational Waves Induced by Primordial Scalar Perturbations and Connection with the Primordial Black Hole Scenarios
• Matter bounce cosmology with a generalized single field: non-Gaussianity and an extended no-go theorem
• Gravitational waves from first-order phase transitions: Towards model separation by bubble nucleation rate
• Observation of a new baryon state in the ${\Lambda }_b^0{\pi }^{+}{\pi }^{-}$ mass spectrum
• Strong lensing as a giant telescope to localize the host galaxy of gravitational wave event
• Late time cosmology with LISA: probing the cosmic expansion with massive black hole binary mergers as standard sirens
• The Benefits of Diligence: How Precise are Predicted Gravitational Wave Spectra in Models with Phase Transitions?
• Relativistic bubble collisions -- a closer look
• Variability of signal to noise ratio and the network analysis of gravitational wave burst signals
• Detonations and deflagrations in cosmological phase transitions
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Effective picture of bubble expansion
• Implications of the NANOGrav result on primordial gravitational waves in nonstandard cosmologies
• Searching for a dipole modulation in the large-scale structure of the Universe
• A Reinvestigation of Moving Punctured Black Holes with a New Code
• Ultra-compact X-ray binaries with He star companions
• Testing the Etherington's distance duality relation at higher redshifts: the combination of radio quasars and gravitational waves
• Changing-look active galactic nuclei: close binaries of supermassive black holes in action
• Eccentric Gravitational Wave Bursts in the Post-Newtonian Formalism
• Primordial black holes and secondary gravitational waves from chaotic inflation
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Gravitational-wave memory revisited: memory from the merger and recoil of binary black holes
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• The bubble wall velocity in the minimal supersymmetric light stop scenario
• Gravitational Radiation from Primordial Helical MHD Turbulence
• Circular Polarization of Gravitational Waves from Early-Universe Helical Turbulence
• Wall speed and shape in singlet-assisted strong electroweak phase transitions
• ET sensitivity to the anisotropic Stochastic Gravitational Wave Background
• Stochastic Gravitational Waves from Inflaton Decays
• Stability under radiation reaction of circular equatorial orbits around Kerr black holes
• Hubble parameter estimation via dark sirens with the LISA-Taiji network
• The search for anisotropy in the gravitational-wave background with pulsar-timing arrays
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Eccentric-orbit EMRI gravitational wave energy fluxes to 7PN order
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• The detectability of eccentric compact binary coalescences with advanced gravitational-wave detectors
• LISA Sensitivity to Gravitational Waves from Sound Waves
• The Eccentric Behavior of Inspiraling Compact Binaries
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• An efficient approach to electroweak bubble velocities
• Anomalies in Time Delays of Lensed Gravitational Waves and Dark Matter Substructures
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• On Primordial Black Holes from Rapid Turns in Two-field Models
• Gravitational wave production after inflation with cuspy potentials
• NANOGrav signal as mergers of Stupendously Large Primordial Black Holes
• First measurement of the Hubble parameter from bright binary black hole GW190521
• Formation threshold of rotating primordial black holes
• Testing clockwork axion with gravitational waves
• Energy budget and the gravitational wave spectra beyond the bag model
• Hereditary Effects in Eccentric Compact Binary Inspirals to Third Post-Newtonian Order
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Cosmic opacity: cosmological-model-independent tests from gravitational waves and Type Ia Supernova
• Oscillon collapse to black holes
• Constructing EOB dynamics with numerical energy flux for intermediate-mass-ratio inspirals
• Scalaron-Higgs inflation reloaded: Higgs-dependent scalaron mass and primordial black hole dark matter
• On the redundancy of operators and the bispectrum in the most general second-order scalar-tensor theory
• Identification of All Dark Matter as Black Holes
• The velocity dispersion function of early-type galaxies and its redshift evolution: the newest results from lens redshift test
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Compact binary coalescences: Constraints on waveforms
• Is there evidence for anomalous dipole anisotropy in the large-scale structure?
• Friction forces on phase transition fronts
• Gravitational wave as probe of superfluid dark matter
• Gauge transformation of scalar induced tensor perturbation during matter domination
• Implications from simulated strong gravitational lensing systems: constraining cosmological parameters using Gaussian Processes
• Bright "Merger-nova" Emission Powered by Magnetic wind from a New-Born Black Hole
• Fundamental frequencies and resonances from eccentric and precessing binary black hole inspirals
• Kinematic signatures of reverberation mapping of close binaries of supermassive black holes in active galactic nuclei
• A Critical Look at the Electroweak Phase Transition
• Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
• LISA Measurement of Gravitational Wave Background Anisotropy: Hexadecapole Moment via a Correlation Analysis
• Bubble wall velocity beyond leading-log approximation in electroweak phase transition
• Inflation model selection revisited after a 1.91% measurement of the Hubble constant
• Ultra-compact X-ray binaries as dual-line gravitational-wave sources
• Gravitational wave source localization for eccentric binary coalesce with a ground-based detector network
• Testing Primordial Black Holes as Dark Matter in Supergravity from Gravitational Waves
• Secondary graviton spectra and waterfall-like fields
• Orbital Evolution of Neutron-Star -- White-Dwarf Binaries by Roche-Lobe Overflow and Gravitational Wave Radiation
• Observational Constraints on Interacting Dark Matter Model Without Dark Energy
• A more stringent constraint on the mass ratio of binary neutron star merger GW170817
• Measuring the viscosity of dark matter with strongly lensed gravitational waves
• Forecast for weighing neutrinos in cosmology with SKA
• Inspiraling double compact object detection and lensing rate -- forecast for DECIGO and B-DECIGO
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Generation of Primordial Black Holes and Gravitational Waves from Dilaton-Gauge Field Dynamics
• Three-form inflation and non-Gaussianity
• Cosmological parameter measurement and neutral hydrogen 21 cm sky survey with the Square Kilometre Array
• Blindly Detecting Merging Supermassive Black Holes with Radio Surveys
• Studying the Solar system dynamics using pulsar timing arrays and the LINIMOSS dynamical model
• Echoes of Inflationary First-Order Phase Transitions in the CMB
• Convergence of Fourier-domain templates for inspiraling eccentric compact binaries
• Dynamics of Nambu monopole in two Higgs doublet models -- Cosmological Monopole Collider --
• A probabilistic model for learning in cortical microcircuit motifs with data-based divisive inhibition
• Ultracompact minihalos associated with stellar-mass primordial black holes
• Double peaks of gravitational wave spectrum induced from inflection point inflation
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• New probe of gravity: strongly lensed gravitational wave multi-messenger approach
• Kinematic signatures of reverberation mapping of close binaries of supermassive black holes in active galactic nuclei. II. Atlas of two-dimensional transfer functions
• Blindly detecting orbital modulations of jets from merging supermassive black holes
• Accurate calculation of gravitational wave memory
• Production of gravitational waves during preheating with nonminimal coupling
• Gauge Invariant Second Order Gravitational Waves
• Dynamical evidence of the sub-parsec counter-rotating disc for a close binary of supermassive black holes in the nucleus of NGC 1068
• Detecting circular polarisation in the stochastic gravitational-wave background from a first-order cosmological phase transition
• Analytic approach to the motion of cosmological phase transition fronts
• Analytic Waveforms for Eccentric Gravitational Wave Bursts
• Stochastic gravitational background from inflationary phase transitions
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• Testing gravity on kiloparsec scales with strong gravitational lenses
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Variation of Broad Emission Lines from QSOs with Optical/UV Periodicity to Test the Interpretation of Supermassive Binary Black Holes
• An analytical approach to the field amplification and particle production by parametric resonance during inflation and reheating
• Gravitational waves from first order phase transitions during inflation
• Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations
• Relativistic viscous effects on the primordial gravitational waves spectrum
• A single pulse study of PSR J1022+1001
• Testing the relativistic Doppler boost hypothesis for supermassive binary black holes candidates via broad emission line profiles
• Data Analysis Implications of Moderately Eccentric Gravitational Waves
• Mimicking alternatives to inflation with interacting spectator fields
• Energy budget of cosmological first-order phase transition in FLRW background
• Supermassive Binary Black Hole Evolution can be traced by a small SKA Pulsar Timing Array
• On the Gauge Invariance of Scalar Induced Gravitational Waves: Gauge Fixings Considered
• A novel method of measuring cosmological distances using broad-line regions of quasars
• Second-order cosmological perturbations. IV. Produced by scalar-tensor and tensor-tensor couplings during the radiation dominated stage
• Peak statistics for the primordial black hole abundance
• Power-law modulation of the scalar power spectrum from a heavy field with a monomial potential
• A dynamical approach in exploring the unknown mass in the Solar system using pulsar timing arrays
• Broad-line region configuration of the supermassive binary black hole candidate PG1302-102 in the relativistic Doppler boosting scenario
• Damping of gravitational waves in a viscous Universe and its implication for dark matter self-interactions
• Using Gravitational Wave Parallax to Measure the Hubble Parameter with Pulsar Timing Arrays
• Single-Source Gravitational Wave Limits from the J1713+0747 24-hr Global Campaign
• Continuous gravitational wave searches with pulsar timing arrays: Maximization versus marginalization over pulsar phase parameters
• Perturbational Treatment of the Gravitational Potential Effect on Binary Black Hole Evolution
• Differential Interferometric Signatures of Close Binaries of Supermassive Black Holes in Active Galactic Nuclei
• Spurious gauge-invariance of higher-order contributions to the spectral energy density of the relic gravitons
• Constraints on brane inflation after Planck 2015: Impacts of the latest local measurement of the Hubble constant
• Stochastic inflation and primordial black holes
• Production of gravitational waves during preheating in the Starobinsky inflationary model
• Analytic integral solutions for induced gravitational waves
• Bending the Bruhat-Tits Tree II: the p-adic BTZ Black hole and Local Diffeomorphism on the Bruhat-Tits Tree
• Constraints on individual supermassive binary black holes using observations of PSR J1909-3744
• Spherical harmonic analysis of anisotropies in polarized stochastic gravitational wave background with interferometry experiments
• Nature Abhors a Circle
• Sound speed induced production of primordial black holes
• Dependence of the amplitude of gravitational waves from preheating on the inflationary energy scale
• An Inflationary Probe of Cosmic Higgs Switching
• Holographic Charged Fluid with Chiral Electric Separation Effect
• Implications of NANOGrav results and UV freeze-in in a fast-expanding Universe
• Effective anisotropic stresses of the relic gravitons
• A unique gravitational wave signal from phase transition during inflation
• Binary black hole simulation with an adaptive finite element method III: Evolving a single black hole
• Linear Degeneracy of the First-Order Generalized-Harmonic Einstein System

Cited by in corpus (63)

• Primordial gravitational waves from NANOGrav: a broken power-law approach
• Primordial black hole production during first-order phase transitions
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• Probing QCD critical point and induced gravitational wave by black hole physics
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Implications of Nano-Hertz Gravitational Waves on Electroweak Phase Transition in the Singlet Dark Matter Model
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Gravitational Waves and Primordial Black Hole Productions from Gluodynamics by Holography
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Hydrodynamic sound shell model
• Cosmology with fast radio bursts in the era of SKA
• Effect of density fluctuations on gravitational wave production in first-order phase transitions
• Electroweak Phase Transition and Gravitational Waves in the Type-II Seesaw Model
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Hydrodynamic backreaction force of cosmological bubble expansion
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Sound from extra dimension: quasinormal modes of thick brane
• Primordial black holes and induced gravitational waves from double-pole inflation
• The energy budget of cosmological first-order phase transitions beyond the bag equation of state
• Primordial black holes and curvature perturbations from false vacuum islands
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Bubble expansion at strong coupling
• Null test for cosmic curvature using Gaussian process
• Axial gravitational quasinormal modes of a self-dual black hole in loop quantum gravity
• Constraints on ultra-slow-roll inflation from the third LIGO-Virgo observing run
• Stochastic gravitational wave background due to gravitational wave memory
• Constraints on new physics around the MeV scale with cosmological observations
• Constraint on the mass of graviton with gravitational waves
• Polarization modes of gravitational waves in generalized Proca theory
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• Characteristic modes of thick brane model: resonances and quasinormal modes
• White dwarf binary modulation can help stochastic gravitational wave background search
• Wave effect of gravitational waves intersected with a microlens field II: an adaptive hierarchical tree algorithm and population study
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• General bubble expansion at strong coupling
• Multiple peaks in gravitational waves induced from primordial curvature perturbations with non-Gaussianity
• Polarization modes of gravitational waves in general Einstein-vector theory
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• Gravitational Waves of GUT Phase Transition during Inflation
• Detecting the dark sector through scalar-induced gravitational waves
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• General backreaction force of cosmological bubble expansion
• A new way to test the WIMP dark matter models
• Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
• Measuring the modified gravitational waves propagation beyond general relativity from CMB observations
• Gravitational waves from vacuum bubbles: Ultraviolet dependence on wall thickness
• Constraints on ultra-slow-roll inflation with the NANOGrav 15-Year Dataset
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Scalar-induced gravitational waves including isocurvature perturbations with lattice simulations
• Bubbles kick off primordial black holes to form more binaries
• Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings
• Gravitational waves from patterns of electroweak symmetry breaking: an effective perspective
• Bayesian analysis of the complex singlet model with phase transition gravitational waves
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Detection of the Permanent Strain Offset Component of Gravitational-Wave Memory in Black Hole Mergers
• Gravitational waves from resonant amplification of curvature perturbations during inflation
• Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors
• Attenuated gravitational radiation