On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences

Abstract

The observation of massive black hole binary systems is one of the main science objectives of the Laser Interferometer Space Antenna (LISA). The instrument's design requirements have recently been revised: they set a requirement at $0.1\mathrm{mHz}$, with no additional explicit requirements at lower frequencies. This has implications for observations of the short-lived signals produced by the coalescence of massive and high-redshift binaries. Here we consider the most pessimistic scenario: the (unlikely) case in which LISA has no sensitivity below $0.1\mathrm{mHz}$. We show that the presence of higher multipoles (beyond the dominant $\ell =|m|=2$ mode) in the gravitational radiation from these systems, which will be detectable with a total signal-to-noise ratio $\sim 10^3$, allows LISA to retain the capability to accurately measure the physical parameters, the redshift, and to constrain the sky location. To illustrate this point, we consider a few select binaries in a total (redshifted) mass range of $4\times 10^6-4\times 10^7{M}_{\odot }$ whose ($\ell =|m|=2$) gravitational-wave signals last between $\approx 12$ hours and $\approx 20$ days in band. We model the emitted gravitational radiation using the highly accurate (spin-aligned) waveform approximant IMRPhenomXHM and carry out a fully coherent Bayesian analysis on the LISA noise-orthogonal time-delay-interferometry channels.

arXiv comment13 pages, 6 figures, comments welcome!

References in corpus (60)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• LSST: from Science Drivers to Reference Design and Anticipated Data Products
• dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
• The James Webb Space Telescope
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Massive Black Holes as Population III Remnants
• Formation of Supermassive Black Holes by Direct Collapse in Pregalactic Halos
• Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe
• Formation of Supermassive Black Holes
• Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Coalescence of Two Spinning Black Holes: An Effective One-Body Approach
• Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
• The Atacama Large Millimeter/submillimeter Array
• Science with the space-based interferometer eLISA. I: Supermassive black hole binaries
• Simulations on a Moving Mesh: The Clustered Formation of Population III Protostars
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• Rapid Bayesian position reconstruction for gravitational-wave transients
• The evolution of massive black hole seeds
• Networks of gravitational wave detectors and three figures of merit
• IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
• Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
• Alignment of the spins of supermassive black holes prior to coalescence
• Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
• The LISA Optimal Sensitivity
• The evolution of massive black holes and their spins in their galactic hosts
• Towards models of gravitational waveforms from generic binaries: A simple approximate mapping between precessing and non-precessing inspiral signals
• Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
• Dual Jets from Binary Black Holes
• LISA observations of rapidly spinning massive black hole binary systems
• Measuring coalescing massive binary black holes with gravitational waves: The impact of spin-induced precession
• Measuring the spin of black holes in binary systems using gravitational waves
• Forward Modeling of Space-borne Gravitational Wave Detectors
• Exploring the Bayesian parameter estimation of binary black holes with LISA
• Gravitational-wave observations of binary black holes: Effect of non-quadrupole modes
• Massive Black Hole Binary Inspirals: Results from the LISA Parameter Estimation Taskforce
• On the properties of the massive binary black hole merger GW170729
• Can we measure individual black-hole spins from gravitational-wave observations?
• Parameter estimation for heavy binary-black holes with networks of second-generation gravitational-wave detectors
• Black hole mergers: the first light
• Constraining the Inclination of Binary Mergers from Gravitational-wave Observations
• Effects of nonquadrupole modes in the detection and parameter estimation of black hole binaries with nonprecessing spins
• Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• LISA parameter estimation and source localization with higher harmonics of the ringdown
• Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
• GPU-accelerated massive black hole binary parameter estimation with LISA
• Bayesian parameter estimation of stellar-mass black-hole binaries with LISA
• Black hole mass estimation for Active Galactic Nuclei from a new angle
• Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies
• Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems
• Measuring precession in asymmetric compact binaries
• Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
• Identifying LISA verification binaries among the Galactic population of double white dwarfs
• Milky Way Satellites Shining Bright in Gravitational Waves
• Viewing angle of binary neutron star mergers
• Identifying and Addressing Nonstationary LISA Noise
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Black hole science with the Laser Interferometer Space Antenna
• The Bardeen-Petterson effect, disk breaking, and the spin orientations of supermassive black-hole binaries

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• Advancing Space-Based Gravitational Wave Astronomy: Rapid Parameter Estimation via Normalizing Flows
• Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
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• Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
• Accurate and efficient simulation-based inference for massive black-hole binaries with LISA