Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes
arXiv:1903.09220
Abstract
Next-generation observations will revolutionize our understanding of binary black holes and will detect new sources, such as intermediate-mass black holes. Primary science goals include: Discover binary black holes throughout the observable Universe; Reveal the fundamental properties of black holes; Uncover the seeds of supermassive black holes.
14 pages, 3 figures, White Paper Submitted to Astro2020 (2020 Astronomy and Astrophysics Decadal Survey) by GWIC 3G Science Case Team (GWIC: Gravitational Wave International Committee)
References in corpus (76)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- 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
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- Tests of general relativity with GW150914
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Massive Black Holes as Population III Remnants
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- An ultra-luminous quasar with a twelve-billion-solar-mass black hole at redshift 6.30
- Pulsational Pair-Instability Supernovae
- Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
- Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226
- Pulsational pair instability as an explanation for the most luminous supernovae
- Tests of General Relativity with GW170817
- A new route towards merging massive black holes
- Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
- The Mass Distribution of Stellar-Mass Black Holes
- Science with the space-based interferometer eLISA. I: Supermassive black hole binaries
- The promise of multi-band gravitational wave astronomy
- Double Compact Objects II: Cosmological Merger Rates
- Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies
- Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code
- Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (II) Ringdown
- The Formation and Evolution of Massive Black Holes
- Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor
- How Mergers May Affect The Mass Scaling Relations Between Black Holes, Galaxies, and Other Gravitationally Bound Systems
- Massive black hole binaries from runaway collisions: the impact of metallicity
- Does the Black Hole Merger Rate Evolve with Redshift?
- Dynamical Formation of the GW150914 Binary Black Hole
- MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters
- Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state
- Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope
- The spin of the second-born black hole in coalescing binary black holes
- Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
- The cosmic merger rate of neutron stars and black holes
- Journey to the M_BH -sigma relation: the fate of low mass black holes in the Universe
- Compact Binary Coalescences in the Band of Ground-based Gravitational-Wave Detectors
- Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
- The cosmic merger rate of stellar black hole binaries from the Illustris simulation
- Bayesian model selection for testing the no-hair theorem with black hole ringdowns
- Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes
- Determining the population properties of spinning black holes
- Black hole mergers from an evolving population of globular clusters
- Formation of supermassive black hole seeds
- Gravitational Waves from the Remnants of the First Stars
- Scientific Discovery with the James Webb Space Telescope
- Measuring eccentricity in binary black hole inspirals with gravitational waves
- From the first stars to the first black holes
- Accuracy of inference on the physics of binary evolution from gravitational-wave observations
- Measuring the star formation rate with gravitational waves from binary black holes
- Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
- The influence of the distribution of cosmic star formation at different metallicities on the properties of merging double compact objects
- The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region
- Probing Cosmic Dawn with Emission Lines: Predicting Infrared and Nebular Line Emission for ALMA and JWST
- Parameter estimation for binary black holes with networks of third generation gravitational-wave detectors
- Seeing the First Supernovae at the Edge of the Universe with JWST
- Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
- GWLSS: Chasing the Progenitors of Merging Binary Black Holes
- Signatures of primordial black holes as seeds of supermassive black holes
- Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes
- The structure and evolution of quasi-stars
- The most massive black holes on the Fundamental Plane of Black Hole Accretion
- Intermediate-mass black holes from Population III remnants in the first galactic nuclei
- Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation
- Spectroscopic analysis of stellar mass black-hole mergers in our local universe with ground-based gravitational wave detectors
- Intermediate-mass-ratio-inspirals in the Einstein Telescope. II. Parameter estimation errors
- Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies
- Observing Supermassive Black Holes across cosmic time: from phenomenology to physics
- Characterization of binary black holes by heterogeneous gravitational-wave networks
- Athena+: The first Deep Universe X-ray Observatory