The Minimum Testable Abundance of Primordial Black Holes at Future Gravitational-Wave Detectors

Abstract

The next generation of gravitational-wave experiments, such as Einstein Telescope, Cosmic Explorer and LISA, will test the primordial black hole scenario. We provide a forecast for the minimum testable value of the abundance of primordial black holes as a function of their masses for both the unclustered and clustered spatial distributions at formation. In particular, we show that these instruments may test abundances, relative to the dark matter, as low as $10^{-10}$.

11 pages, 5 figures

References in corpus (37)

• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• Laser Interferometer Space Antenna
• The merger rate of primordial-black-hole binaries
• Double Compact Objects III: Gravitational Wave Detection Rates
• Constraints on Earth-mass primordial black holes from OGLE 5-year microlensing events
• Understanding caustic crossings in giant arcs: characteristic scales, event rates, and constraints on compact dark matter
• Lower bound on the primordial black hole merger rate
• Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run
• Updated Constraints on Asteroid-Mass Primordial Black Holes as Dark Matter
• Early Structure Formation in $\Lambda$PBH Cosmologies
• Bayesian analysis of LIGO-Virgo mergers: Primordial vs. astrophysical black hole populations
• The GW190521 Mass Gap Event and the Primordial Black Hole Scenario
• Constraining the primordial black hole scenario with Bayesian inference and machine learning: the GWTC-2 gravitational wave catalog
• The Clustering Evolution of Primordial Black Holes
• Evidence for primordial black hole dark matter from LIGO/Virgo merger rates
• PBH in single field inflation: the effect of shape dispersion and non-Gaussianities
• Primordial black holes as biased tracers
• Low Mass Black Holes from Dark Core Collapse
• Constraints on Primordial Black Holes: the Importance of Accretion
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• Gravitational waves from Population III binary black holes formed by dynamical capture
• Small-scale structure of primordial black hole dark matter and its implications for accretion
• Test for the Origin of Solar Mass Black Holes
• Search for gravitational waves from the coalescence of sub-solar mass binaries in the first half of Advanced LIGO and Virgo's third observing run
• The merger history of primordial-black-hole binaries
• Maximum redshift of gravitational wave merger events
• Unveiling early black hole growth with multi-frequency gravitational wave observations
• Cusp-to-core transition in low-mass dwarf galaxies induced by dynamical heating of cold dark matter by primordial black holes
• Primordial Black Holes as Silver Bullets for New Physics at the Weak Scale
• Interstellar Gas Heating by Primordial Black Holes
• The Astro-Primordial Black Hole Merger Rates: a Reappraisal
• A possible mass distribution of primordial black holes implied by LIGO-Virgo
• Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum
• Constraining the Initial Primordial Black Hole Clustering with CMB-distortion
• Prospects for detecting gravitational waves from eccentric subsolar mass compact binaries
• Dark Matter Simulations with Primordial Black Holes in the Early Universe
• Merger rates in primordial black hole clusters without initial binaries

Cited by in corpus (44)

• Science with the Einstein Telescope: a comparison of different designs
• New Horizons for Fundamental Physics with LISA
• The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities
• Primordial non-gaussianity up to all orders: theoretical aspects and implications for primordial black hole models
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• From inflation to black hole mergers and back again: Gravitational-wave data-driven constraints on inflationary scenarios with a first-principle model of primordial black holes across the QCD epoch
• Anatomy of single-field inflationary models for primordial black holes
• The Science of the Einstein Telescope
• Hunt for Light Primordial Black Hole Dark Matter with Ultra-High-Frequency Gravitational Waves
• Stochastic gravitational-wave background as a tool to investigate multi-channel astrophysical and primordial black-hole mergers
• How to assess the primordial origin of single gravitational-wave events with mass, spin, eccentricity, and deformability measurements
• Primordial black holes in the curvaton model: possible connections to pulsar timing arrays and dark matter
• Primordial black hole dark matter from inflation: the reverse engineering approach
• Search for a scalar induced stochastic gravitational wave background in the third LIGO-Virgo observing run
• Searching for mass-spin correlations in the population of gravitational-wave events: the GWTC-3 case study
• Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics
• On the single-event-based identification of primordial black hole mergers at cosmological distances
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics
• Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
• Signals of primordial black holes at gravitational wave interferometers
• Primordial black hole mergers from three-body interactions
• Dancing in the dark: detecting a population of distant primordial black holes
• Ultralight Black Holes as Sources of High-Energy Particles
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope
• Heavy primordial black holes from strongly clustered light black holes
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• Lensing constraints on ultradense dark matter halos
• Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations
• GW200105 and GW200115 are compatible with a scenario of primordial black hole binary coalescences
• Slaying Axion-Like Particles via Gravitational Waves and Primordial Black Holes from Supercooled Phase Transition
• Redshift evolution of primordial black hole merger rate
• Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation
• Strong clustering of primordial black holes from Affleck-Dine mechanism
• Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models
• Primordial Black Holes and Scalar-induced Gravitational Waves in Sneutrino Hybrid Inflation
• Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
• Search for sub-solar mass binaries with Einstein Telescope and Cosmic Explorer
• Projected gravitational wave constraints on primordial black hole abundance for extended mass distributions
• Primordial Black Holes and Second-order Gravitational Waves in Axion-like Hybrid Inflation
• The Quasar Candidates Catalogs of DESI Legacy Imaging Survey Data Release 9
• Primordial black holes with mass ratio-modulated initial clustering: merger suppression and projected constraints
• Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors