The Lunar Gravitational-wave Antenna: Mission Studies and Science Case

Abstract

The Lunar Gravitational-wave Antenna (LGWA) is a proposed array of next-generation inertial sensors to monitor the response of the Moon to gravitational waves (GWs). Given the size of the Moon and the expected noise produced by the lunar seismic background, the LGWA would be able to observe GWs from about 1 mHz to 1 Hz. This would make the LGWA the missing link between space-borne detectors like LISA with peak sensitivities around a few millihertz and proposed future terrestrial detectors like Einstein Telescope or Cosmic Explorer. In this article, we provide a first comprehensive analysis of the LGWA science case including its multi-messenger aspects and lunar science with LGWA data. We also describe the scientific analyses of the Moon required to plan the LGWA mission.

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• Repeating tidal disruptions in GSN 069: Long-term evolution and constraints on quasi-periodic eruptions' models
• Multi-band gravitational-wave astronomy: parameter estimation and tests of general relativity with space and ground-based detectors
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• Constraining the Orbit of Supermassive Black Hole Binary 0402+379
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• On choosing the start time of binary black hole ringdown
• A new channel to form IMBHs throughout cosmic time
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• Ultralight dark matter detection with mechanical quantum sensors
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• The nature of massive black hole binary candidates: I. Spectral properties and evolution
• In-depth analysis of the clustering of dark matter particles around primordial black holes I: density profiles
• Where are the double-degenerate progenitors of type Ia supernovae?
• Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
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• A model for the possible connection between tidal disruption event and quasi-periodic eruption in GSN 069
• Order in the chaos: eccentric black hole binary mergers in triples formed via strong binary-binary scatterings
• A Unique Multi-Messenger Signal of QCD Axion Dark Matter
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• A Catalogue of Potential Post Common Envelope Binaries
• Evidence of a tidal disruption event in GSN 069 from the abnormal carbon and nitrogen abundance ratio
• Resolving massive black hole binaries evolution via adaptive particle-splitting
• Reverberation in tidal disruption events: dust echoes, coronal emission lines, multi-wavelength cross-correlations, and QPOs
• Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA "Verification Binaries"
• Dark matter: an efficient catalyst for intermediate-mass-ratio-inspiral events
• Searching for Binary Supermassive Black Holes via Variable Broad Emission Line Shifts: Low Binary Fraction
• Tidal Interactions in Merging White Dwarf Binaries
• The Lynx Mission Concept Study Interim Report
• Tidal Disruptions of White Dwarfs: Theoretical Models and Observational Prospects
• Breaching the limit: formation of GW190521-like and IMBH mergers in young massive clusters
• In-situ extreme mass ratio inspirals via sub-parsec formation and migration of stars in thin, gravitationally unstable AGN discs
• The Intermediate Mass Black Hole Candidate in the Center of NGC 404: New Evidence from Radio Continuum Observations
• Type Ia Supernova Sub-classes and Progenitor Origin
• Expanding the LISA Horizon from the Ground
• Measuring dark matter spikes around primordial black holes with Einstein Telescope and Cosmic Explorer
• Physics of Binary Star Evolution -- from Stars to X-ray Binaries and Gravitational Wave Sources
• The formation of ultra-massive carbon-oxygen core white dwarfs and their evolutionary and pulsational properties
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Multi-band gravitational wave tests of general relativity
• Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant
• Detectability of double white dwarfs in the Local Group with LISA
• The role of supernova convection for the lower mass gap in the isolated binary formation of gravitational wave sources
• Accretion disc cooling and narrow absorption lines in the tidal disruption event AT 2019dsg
• The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
• Interpretation of the observed neutrino emission from three Tidal Disruption Events
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolution
• Calcium-Rich Gap Transients: Tidal Detonations of White Dwarfs?
• Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational-wave astronomy
• Identifying LISA verification binaries among the Galactic population of double white dwarfs
• Mass, Spin, and Ultralight Boson Constraints from the Intermediate Mass Black Hole in the Tidal Disruption Event 3XMM J215022.4-055108
• Emission of gravitational radiation from ultra-relativistic sources
• Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe
• Modelling neutron star mountains in relativity
• Cosmology with Standard Sirens at Cosmic Noon
• LISA Definition Study Report
• Progenitor constraints on the Type-Ia supernova SN2011fe from pre-explosion Hubble Space Telescope HeII narrow-band observations
• Search of sub-parsec massive binary black holes through line diagnosis
• A Rosetta Stone for eccentric gravitational waveform models
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• Seismic Search for Strange Quark Nuggets
• Binary black hole spectroscopy: a no-hair test of GW190814 and GW190412
• The nucleation fraction of Local Volume galaxies
• A compact, large-range interferometer for precision measurement and inertial sensing
• Dark matter minispike: a significant enhancement of eccentricity for intermediate-mass-ratio-inspirals
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Tidal deformations of neutron stars with elastic crusts
• A helical jet model for OJ287
• Faint rapid red transients from Neutron star -- CO white-dwarf mergers
• Very low mass white dwarfs with a C-O core
• Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach
• Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
• Constraining the gravitational wave energy density of the Universe using Earth's ring
• Pre-merger localization of compact-binary mergers with third generation observatories
• Application of the disk instability model to all Quasi-Periodic Eruptions
• On the radio properties of the intermediate-mass black hole candidate ESO 243-49 HLX-1
• Gravitational Wave mergers as tracers of Large Scale Structures
• Extreme mass ratio inspirals and tidal disruption events in nuclear clusters. I. Time dependent rates
• Cosmological inference from standard sirens without redshift measurements
• Milky Way Satellites Shining Bright in Gravitational Waves
• The ELM Survey. IX. A Complete Sample of Low Mass White Dwarf Binaries in the SDSS Footprint
• Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors
• Boosted Tidal Disruption by Massive Black Hole Binaries During Galaxy Mergers FROM The View of N-Body Simulation
• The competing effect of gas and stars in massive black hole binaries evolution
• The core helium flash revisited III. From Pop I to Pop III stars
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• Was the Sun a Slow Rotator? -- Sodium and Potassium Constraints from the Lunar Regolith
• Machine learning for gravitational-wave detection: surrogate Wiener filtering for the prediction and optimized cancellation of Newtonian noise at Virgo
• On the rates of type Ia supernovae originating from white dwarf collisions in quadruple star systems
• Gravitational radiation from precessing accretion disks in gamma-ray bursts
• The extended radio jet of an off-nuclear low-mass AGN in NGC 5252
• Unveiling sub-parsec supermassive black hole binary candidates in active galactic nuclei
• Neutron Star Crust Can Support A Large Ellipticity
• Optimizing LIGO with LISA forewarnings to improve black-hole spectroscopy
• The nuclear transient AT 2017gge: a tidal disruption event in a dusty and gas-rich environment and the awakening of a dormant SMBH
• A Multi-wavelength Study of the Turbulent Central Engine of the Low-mass AGN hosted by NGC404
• Toward the unambiguous identification of supermassive binary black holes through Bayesian inference
• Optical follow-up of the tidal disruption event iPTF16fnl: new insights from X-shooter observations
• Neutrino Emissions from Tidal Disruption Remnants
• Multiband Gravitational Wave Parameter Estimation: A Study of Future Detectors
• Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
• The Rapid X-ray and UV Evolution of ASASSN-14ko
• Isolated and dynamical black hole mergers with \texttt{B-POP}: the role of star formation and dynamics, star cluster evolution, natal kicks, mass and spins, and hierarchical mergers
• General relativistic smoothed particle hydrodynamics
• Tidal disruptions of main sequence stars -- IV. Relativistic effects and dependence on black hole mass
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• A Systematic Search for Short-period Close White Dwarf Binary Candidates Based on Gaia EDR3 Catalog and Zwicky Transient Facility Data
• Swift data hint at a binary Super Massive Black Hole candidate at sub-parsec separation
• Hundreds of Low-Mass Active Galaxies in the Galaxy And Mass Assembly (GAMA) Survey
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• Tossing Black Hole Spin Axes
• Testing gravitational wave propagation with multiband detections
• Polarization of gravitational waves from helical MHD turbulent sources
• Continuous gravitational waves from Galactic neutron stars: demography, detectability and prospects
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• A Linear and Quadratic Time-Frequency Analysis of Gravitational Waves from Core-Collapse Supernovae
• Spin Evolution of Stellar-mass Black Holes Embedded in AGN disks: Orbital Eccentricity Produces Retrograde Circumstellar Flows
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• Gravitational Waves from Core-Collapse Supernovae
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• Spectropolarimetry of the Type Ib Supernova iPTF 13bvn: Revealing the complex explosion geometry of a stripped-envelope core-collapse supernova
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• NELIOTA: Methods, statistics and results for meteoroids impacting the Moon
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• SCATTER: A New Common Envelope Formalism
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• The last three years: multiband gravitational-wave observations of stellar-mass binary black holes
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• An Electromagnetic Signature of Galactic Black Hole Binaries That Enter Their Gravitational-Wave Induced Inspiral
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• The gravitational wave background signal from tidal disruption events
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• Toward Realistic Models of Core Collapse Supernovae: A Brief Review
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• Normal type Ia supernovae from disruptions of hybrid He-CO white-dwarfs by CO white-dwarfs
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• Double-Peaked Emission Lines due to A Radio Outflow in KISSR1219
• The MPIfR-MeerKAT Galactic Plane Survey II. The eccentric double neutron star system PSR J1208-5936 and a neutron star merger rate update
• Neutrinos from tidal disruption events
• Mergers of supermassive and intermediate-mass black holes in galactic nuclei from disruptions of star clusters
• Photometric and Structural Parameters of Newly Discovered Nuclear Star Clusters in Local Volume Galaxies
• Secondary accretion of dark matter in intermediate mass-ratio inspirals: Dark-matter dynamics and gravitational-wave phase
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• The Carnegie Supernova Project-I. Spectroscopic analysis of stripped-envelope supernovae
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• An elusive dark central mass in the globular cluster M4
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• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• Spectropolarimetry of Type II supernovae (II) Intrinsic supernova polarization and its relations with the photometric/spectroscopic properties
• Detectability and parameter estimation of GWTC-3 events with LISA
• Tycho's supernova: the view from {\it Gaia}
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• The Detectability of Kiloparsec Scale Dual AGNs: The Impact of Galactic Structure and Black Hole Orbital Properties
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• Dynamical He Flashes in Double White Dwarf Binaries
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• Jetted and Turbulent Stellar Deaths: New LVK-Detectable Gravitational Wave Sources
• Detecting subparsec super-massive binary black holes: Long termmonitoring perspective
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• Gravitational-Wave Radiation from Magnetized Accretion Disks
• Towards a Consistent Calculation of the Lunar Response to Gravitational Waves
• LION :Laser Interferometer On the mooN
• Gravitational Wave Sources as Timing References for LISA Data
• Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
• Brief Follow-up on Recent Studies of Theia's Accretion
• Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries
• Suspension-thermal noise in spring-antispring systems for future gravitational-wave detectors
• Expected insights on type Ia supernovae from LISA's gravitational wave observations
• How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
• Validating Prior-informed Fisher-matrix Analyses against GWTC Data
• Gravitational wave emission from dynamical stellar interactions
• Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
• An Eclipsing 47 minute Double White Dwarf Binary at 400 pc
• Correlation of the rate of Type Ia supernovae with the parent galaxy properties: Light and shadows
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• On the detectability of ultra-compact binary pulsar systems
• Formation and Evolution of Compact Stellar X-ray Sources
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• Update on gravitational wave signals from post-inflationary phase transitions
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• Relevance of Precession for Tests of the Black Hole No Hair Theorems
• Lensing of gravitational waves from tidal disruption events
• The Next-Generation Very Large Array: Supermassive Black Hole Pairs and Binaries
• Black hole-galaxy co-evolution and the role of feedback
• Hydrodynamic simulations of shell convection in stellar cores
• Spectropolarimetry of Core-Collapse Supernovae
• Detecting massive black hole binaries and unveiling their cosmic history with gravitational wave observations
• The Dragon-II simulations -- I. Evolution of single and binary compact objects in star clusters with up to 1 million stars
• RX J1420.4+5334 - another tidal disruption event?
• Identifying Disappearance of a White Dwarf Binary with LISA
• Constraining Supernova Physics through Gravitational-Wave Observations
• Optical Observations of Core-Collapse Supernovae
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Progress on the SOXS transients chaser for the ESO-NTT
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• The Science of the Einstein Telescope
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• Modeling lunar response to gravitational waves using normal-mode approach and tidal forcing
• Search for continuous gravitational wave signals from luminous dark photon superradiance clouds with LVK O3 observations
• Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• Probing intermediate-mass black hole binaries with the Lunar Gravitational-wave Antenna
• A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments
• Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
• Toward Black Hole Stars: supermassive black hole growth in nuclear clusters via stellar-object and gas accretion
• Observing Double White Dwarfs with the Lunar GW Antenna
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions
• Enhanced activity in close dual-AGN systems in the local Universe
• Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
• GEMINI: The First Underground Testbed for Seismic Isolation and Interplatform Control in Next-Generation Gravitational-Wave Detectors
• Detecting White Dwarf Binary Mergers with Gravitational Waves
• Gravitational wave distance estimation using intrinsic signal properties: dark sirens as distance indicators