Astrophysics with the Laser Interferometer Space Antenna

Abstract

The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA's first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultracompact stellar-mass binaries, massive black hole binaries, and extreme or intermediate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe.

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• Binary black holes' effects on electromagnetic fields
• Black hole-neutron star mergers from triples
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• Relativistic Suppression of Black Hole Recoils
• An alternative method to study star cluster disruption
• Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
• Resonant Tidal Excitation of Oscillation Modes in Merging Binary Neutron Stars: Inertial-Gravity Modes
• Atypical Thermonuclear Supernovae from Tidally Crushed White Dwarfs
• A numerical study of vector resonant relaxation
• Episodic mass ejections from common-envelope objects
• Spin-Orbit Misalignment of Merging Black-Hole Binaries with Tertiary Companions
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• Supermassive black holes from primordial black hole seeds
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• Supermassive black holes formed by direct collapse of inflationary perturbations
• The origin and fate of short-period low-mass black-hole binaries
• Accreting Double white dwarf binaries: Implications for LISA
• Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole to the 11th Post-Newtonian Order
• Black Hole Formation in the Lower Mass Gap through Mergers and Accretion in AGN Disks
• Radiation hydrodynamics simulations of the formation of direct-collapse supermassive stellar systems
• Final spins from the merger of precessing binary black holes
• Evolution of Close White Dwarf Binaries
• Hunting Black Holes with Gaia
• Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes
• Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-Disks
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• Detecting Double Neutron Stars with LISA
• A practical, covariant puncture for second-order self-force calculations
• The population of AM CVn stars from the Sloan Digital Sky Survey
• Conditions for Optimal Growth of Black Hole Seeds
• The Spitzer mid-infrared AGN survey. II-the demographics and cosmic evolution of the AGN population
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• Star Formation in Accretion Disks and SMBH Growth
• Disk Evolution and Bar Triggering Driven by Interactions with Dark Matter Substructure
• The numerical relativity breakthrough for binary black holes
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• Secular dynamics in hierarchical three-body systems with mass loss and mass transfer
• The HU Aqr planetary system hypothesis revisited
• Kinematics of the ultra-compact helium accretor AM Canum Venaticorum
• White dwarf pollution by planets in stellar binaries
• Off-nuclear AGN as a signature of recoiling massive black holes
• Importance of transient resonances in extreme-mass-ratio inspirals
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• The Stability of Double White Dwarf Binaries Undergoing Direct Impact Accretion
• Luminous Red Novae: population models and future prospects
• HST/WFPC2 imaging of the circumnuclear structure of LLAGNs. I Data and nuclear morphology
• Growth of resonances and chaos for a spinning test particle in the Schwarzschild background
• Detecting Supermassive Black Hole-Induced Binary Eccentricity Oscillations with LISA
• Distances to Galactic X-ray Binaries with Gaia DR2
• Report on the second Mock LISA Data Challenge
• Mass without radiation: heavily obscured AGN, the X-ray Background and the Black Hole Mass Density
• X-MRIs: Extremely Large Mass-Ratio Inspirals
• Black hole kicks as new gravitational wave observables
• Gravitational waves from bodies orbiting the Galactic Center black hole and their detectability by LISA
• Measuring the eccentricity of GW170817 and GW190425
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Modelling the formation of double white dwarfs
• Slowly, slowly in the wind: 3D hydrodynamical simulations of wind mass transfer and angular-momentum loss in AGB binary systems
• Seeding Black Holes in Cosmological Simulations
• Monte Carlo simulations of post-common-envelope white dwarf + main sequence binaries: The effects of including recombination energy
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• Prompt Electromagnetic Transients from Binary Black Hole Mergers
• Black Hole Binaries in Galactic Nuclei and Gravitational Wave Sources
• Massive perturbers and the efficient merger of binary massive black holes
• Gravitational wave bursts from the Galactic massive black hole
• Very Broad [O III]4959,5007 Emission from the NGC 4472 Globular Cluster RZ2109 and Implications for the Mass of Its Black Hole X-ray Source
• Accreting black hole binaries in globular clusters
• The Pairing of Accreting Massive Black Holes in Multiphase Circumnuclear Disks: the Interplay between Radiative Cooling, Star Formation, and Feedback Processes
• Recoiling Supermassive Black Holes: a search in the Nearby Universe
• Eccentric double white dwarfs as LISA sources in globular clusters
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• An algorithm for detection of extreme mass ratio inspirals in LISA data
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• The birth of a supermassive black hole binary
• Exploring SMBH Assembly with Semi-analytic Modelling
• The tidal remnant of an unusually metal-poor globular cluster
• Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen Poor Low Mass White Dwarf
• Multiband Observation of LIGO/Virgo Binary Black Hole Mergers in the Gravitational-wave Transient Catalog GWTC-1
• Retaining Black Holes with Very Large Recoil Velocities
• Effects of Intermediate Mass Black Holes on Nuclear Star Clusters
• Observing white dwarfs orbiting massive black holes in the gravitational wave and electro-magnetic window
• Magnetorotational collapse of very massive stars to black holes in full general relativity
• Investigating spinning test particles: spin supplementary conditions and the Hamiltonian formalism
• Detection and characterization of instrumental transients in LISA Pathfinder and their projection to LISA
• Searching for Binary Supermassive Black Holes via Variable Broad Emission Line Shifts: Low Binary Fraction
• Opacity Driven Convection and Variability in Accretion Disks around Supermassive Black Holes
• Resolving massive black hole binaries evolution via adaptive particle-splitting
• The effects of host galaxy properties on merging compact binaries detectable by LIGO
• Stability criteria for hierarchical triple systems
• Effects of post-Newtonian Spin Alignment on the Distribution of Black-Hole Recoils
• Millimetre-wave Emission from an Intermediate-Mass Black Hole Candidate in the Milky Way
• Gravitational-wave glitches: resonant islands and frequency jumps in non-integrable extreme-mass-ratio inspirals
• Common Envelope Evolution on a Moving Mesh
• A New Gravitational Wave Verification Source
• Separating Accretion and Mergers in the Cosmic Growth of Black Holes with X-ray and Gravitational Wave Observations
• The thermal equilibrium mass loss model and its applications in binary evolution
• A new class of Roche lobe-filling hot subdwarf binaries
• Observing the Galaxy's massive black hole with gravitational wave bursts
• Calculation of radiation reaction effect on orbital parameters in Kerr spacetime
• Pruning The ELM Survey: Characterizing Candidate Low-Mass White Dwarfs Through Photometric Variability
• Second-order perturbation theory: the problem of infinite mode coupling
• The sustainable growth of the first black holes
• Formation and merging of Mass Gap Black Holes in Gravitational Wave Merger Events from Wide Hierarchical Quadruple Systems
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• Colloquium: Comparison of Astrophysical and Terrestrial Frequency Standards
• Indication of Another Intermediate-mass Black Hole in the Galactic Center
• Unveiling early black hole growth with multi-frequency gravitational wave observations
• $N-$body dynamics of Intermediate mass-ratio inspirals in globular clusters
• Compact massive objects in Virgo galaxies: the black hole population
• Making massive stars in the Galactic Centre via accretion onto low-mass stars within an accretion disc
• Double Neutron Star Formation: Merger Times, Systemic Velocities, and Travel Distances
• Novel modelling of ultra-compact X-ray binary evolution - stable mass transfer from white dwarfs to neutron stars
• Construction of the second-order gravitational perturbations produced by a compact object
• Radio-quiet and radio-loud pulsars: similar in Gamma-rays but different in X-rays
• Heavy double neutron stars: birth, mid-life and death
• Origin of supermassive black holes in massive metal-poor protoclusters
• Comment on "A non-interacting low-mass black hole -- giant star binary system"
• Galaxy Rotation and Supermassive Black Hole Binary Evolution
• Galaxy formation with radiative and chemical feedback
• A Constrained Metropolis-Hastings Search for EMRIs in the Mock LISA Data Challenge 1B
• Detecting Kozai-Lidov imprints on the gravitational waves of intermediate-mass black holes in galactic nuclei
• AGN-starburst evolutionary connection : a physical interpretation based on radiative feedback
• The competing effect of gas and stars in massive black hole binaries evolution
• Relativistic dynamics of stars near a supermassive black hole
• MOCCA SURVEY Database I: Binary Black Hole Mergers from Globular Clusters with Intermediate Mass Black Holes
• The mass assembly of high-redshift black holes
• A conservative effect of the second-order gravitational self-force on quasicircular orbits in Schwarzschild spacetime
• Was GW190412 born from a hierarchical 3+1 quadruple configuration?
• A synthetic model of the gravitational wave background from evolving binary compact objects
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- I. cataclysmic variables -- present-day population
• Improved time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data
• Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars
• On the stability and collisions in triple stellar systems
• On the orbital periods of the AM CVn stars HP Librae and V803 Centauri
• Population Estimates for Electromagnetically-Distinguishable Supermassive Binary Black Holes
• Black Hole Hunting with LISA
• A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph
• Transient acceleration events in LISA Pathfinder data: properties and possible physical origin
• The High Time Resolution Universe Pulsar Survey -- XVI. Discovery and timing of 40 pulsars from the southern Galactic plane
• Lack of nuclear clusters in dwarf spheroidal galaxies: implications for massive black holes formation and the cusp/core problem
• General relativistic smoothed particle hydrodynamics
• On the eccentricity evolution of massive black hole binaries in stellar backgrounds
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• Nonlinear dynamical tides in white dwarf binaries
• Automated bar detection in local disc galaxies from the SDSS - The colors of bars
• The statistical mechanics of relativistic orbits around a massive black hole
• Binary formation and mass function variations in fragmenting discs with short cooling times
• Can supernova kicks trigger EMRIs in the Galactic Centre?
• Galaxy fields of LISA massive black hole mergers in a simulated Universe
• Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters
• The lifetime of binary black holes in Sérsic galaxy models
• XMM-Newton observations of AM CVn binaries: V396 Hya & SDSS J1240-01
• Numerical Simulations of Equatorially-Asymmetric Magnetized Supernovae: Formation of Magnetars and Their Kicks
• Spatial dispersion of light rays propagating through a plasma in Kerr spacetime
• Extreme recoils: impact on the detection of gravitational waves from massive black hole binaries
• The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center
• The OmegaWhite survey for short-period variable stars - V. Discovery of an ultracompact hot subdwarf binary with a compact companion in a 44 minute orbit
• 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
• Circumbinary disc self-gravity governing supermassive black hole binary mergers
• Expected intermediate-mass black holes in the Virgo cluster. I. Early-type galaxies
• SDSS J1056+5516: A Triple AGN or an SMBH Recoil Candidate?
• Estimating the outcomes of common envelope evolution in triple stellar systems
• Ultra-compact X-ray binaries as dual-line gravitational-wave sources
• Measuring tides and binary parameters from gravitational wave data and eclipsing timings of detached white dwarf binaries
• Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna
• Accuracy of the post-Newtonian approximation. II. Optimal asymptotic expansion of the energy flux for quasicircular, extreme mass-ratio inspirals into a Kerr black hole
• Constraining parameters of white-dwarf binaries using gravitational-wave and electromagnetic observations
• Detecting extreme mass ratio inspiral events in LISA data using the Hierarchical Algorithm for Clusters and Ridges (HACR)
• Orbital Evolution of Neutron-Star -- White-Dwarf Binaries by Roche-Lobe Overflow and Gravitational Wave Radiation
• Demographics of triple systems in dense star clusters
• On the formation of hot and warm Jupiters via secular high-eccentricity migration in stellar triples
• How to detect the shortest-period binary pulsars in the era of LISA
• New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations
• Star cluster disruption by a massive black hole binary
• Bondi-Hoyle-Lyttleton accretion by binary stars
• The gravitational wave background signal from tidal disruption events
• Fast Spinning Pulsars as Probes of Massive Black Holes' Gravity
• Cosmic archaeology with massive stellar black hole binaries
• The Carnegie Supernova Project II. Observations of the luminous red nova AT 2014ej
• How bright are the gaps in circumbinary disk systems?
• Spin dynamics of a millisecond pulsar orbiting closely around a massive black hole
• Discovery of a high state AM CVn binary in the Galactic Bulge Survey
• Double Neutron Stars: Evidence For Two Different Neutron-Star Formation Mechanisms
• Time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data
• Galaxies with monstrous black holes in galaxy cluster environments
• Evolution of dwarf galaxies hosting GW150914-like events
• Mergers of supermassive and intermediate-mass black holes in galactic nuclei from disruptions of star clusters
• On the maximum stellar rotation to form a black hole without an accompanying luminous transient
• Evolution of Low-Mass X-ray Binaries: the Effect of Donor Evaporation
• Bayesian inference on EMRI signals using low frequency approximations
• On the maximum accretion rate of supermassive stars
• Formation constraints indicate a black-hole accretor in 47 Tuc X9
• The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments
• Binaries Wandering Around Supermassive Black Holes Due To Gravito-electromagnetism
• Cosmological Physics with Black Holes (and Possibly White Dwarfs)
• Automatic Bayesian inference for LISA data analysis strategies
• The evolution of a binary in a retrograde circular orbit embedded in an accretion disk
• Common Envelope Wind Tunnel: Range of Applicability and Self-Similarity in Realistic Stellar Envelopes
• An ancient double degenerate merger in the Milky Way halo
• A Gemini Snapshot Survey for Double Degenerates
• Composition of an Emission Line System in Black Hole Host Globular Cluster RZ2109
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• Estimating the fossil disc mass during supermassive black hole mergers: the importance of torque implementation
• Orbital period variation of KIC 10544976: Applegate mechanism versus light travel time effect
• Massive Star Formation in Metal-Enriched Haloes at High Redshift
• Complex orbital dynamics of a double neutron star system revolving around a massive black hole
• Search for a stochastic gravitational-wave signal in the second round of the Mock LISA Data Challenges
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• Orbital spin dynamics of a millisecond pulsar around a massive black hole with an general mass quadrupole
• Binary white dwarfs in the halo of the Milky Way
• How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way?
• The Evolution of Kicked Stellar-Mass Black Holes in Star Cluster Environments
• Verifying black hole orbits with gravitational spectroscopy
• Connecting traces of galaxy evolution: the missing core mass -- morphological fine structure relation
• A Markov Chain Monte Carlo approach for measurement of jet precession in radio-loud active galactic nuclei
• Tidal disruption rates in non-spherical galactic nuclei formed by galaxy mergers
• MOCCA-Survey Database: Extra Galactic Globular Clusters. II. Milky Way and Andromeda
• Real galaxy mergers from galaxy pair catalogs
• Gravitational Burst Radiation from Pulsars in the Galactic centre and stellar clusters
• The X-ray variable sky as seen by MAXI: the future of dust echo tomography with bright Galactic X-ray bursts
• Analytic Approximations in GR and Gravitational Waves
• The most massive galaxies with large depleted cores: structural parameter relations and black hole masses

Cited by in corpus (2)

• The NewAthena mission concept in the context of the next decade of X-ray astronomy
• Probing the Low-mass End of the Black Hole Mass Function via a Study of Faint Local Spiral Galaxies