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20202026
most citedProspects for Fundamental Physics with LISA

401 citations · 983 across the 36 of their papers we have counts for

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21 papers · 1 filter

gr-qc2026

Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy

Caroline B. Owen, Alexandre Toubiana, Davide Gerosa

With increasingly large numbers of gravitational-wave events, population inference is now beginning to move beyond predictions of marginal distributions and to probe correlations b…

gr-qc2026

A framework for LISA population inference

Alexandre Toubiana, Jonathan Gair

The Laser Interferometer Space Antenna (LISA) is expected to have a source rich data stream containing signals from large numbers of many different types of source. This will inclu…

gr-qc2025★ 3 cited

Gravitational-Wave Background from Extragalactic Double White Dwarfs for LISA

Guillaume Boileau, Tristan Bruel, Alexandre Toubiana +2

Recent studies have revealed the contribution of extragalactic DWD to the astrophysical SGWB could be detectable in the mHz regime by LISA. Conversely, the presence of this SGWB co…

gr-qc2025★ 2 cited

Comparing astrophysical models to gravitational-wave data in the observable space

Alexandre Toubiana, Davide Gerosa, Matthew Mould +9

Comparing population-synthesis models to the results of hierarchical Bayesian inference in gravitational-wave astronomy requires a careful understanding of the domain of validity o…

gr-qc2025

Trust the process: mapping data-driven reconstructions to informed models using stochastic processes

Stefano Rinaldi, Alexandre Toubiana, Jonathan R. Gair

Gravitational-wave astronomy has entered a regime where it can extract information about the population properties of the observed binary black holes. The steep increase in the num…

gr-qc2025★ 3 cited

Black hole spectroscopy: from theory to experiment

Emanuele Berti, Vitor Cardoso, Gregorio Carullo +65

The "ringdown" radiation emitted by oscillating black holes has great scientific potential. By carefully predicting the frequencies and amplitudes of black hole quasinormal modes a…

gr-qc2025

A pipeline for searching and fitting instrumental glitches in LISA data

Martina Muratore, Jonathan Gair, Olaf Hartwig +2

Instrumental artefacts, such as glitches, can significantly compromise the scientific output of LISA. Our methodology employs advanced Bayesian techniques, including Reversible Jum…

gr-qc2024★ 32 cited

Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models

Arnab Dhani, Sebastian H. Völkel, Alessandra Buonanno +5

Gravitational-wave (GW) observations of binary black-hole (BBH) coalescences are expected to address outstanding questions in astrophysics, cosmology, and fundamental physics. Real…

gr-qc2024★ 2 cited

Indistinguishability criterion and estimating the presence of biases

Alexandre Toubiana, Jonathan R. Gair

In these notes, we comment on the standard indistinguishability criterion often used in the gravitational wave community to set accuracy requirements on waveforms. Revisiting the h…

gr-qc2023★ 29 cited

Gravitational wave populations and cosmology with neural posterior estimation

Konstantin Leyde, Stephen R. Green, Alexandre Toubiana +1

We apply neural posterior estimation for fast-and-accurate hierarchical Bayesian inference of gravitational wave populations. We use a normalizing flow to estimate directly the pop…

gr-qc2023★ 48 cited

Waveform Modelling for the Laser Interferometer Space Antenna

LISA Consortium Waveform Working Group, Niayesh Afshordi, Sarp Akçay +144

LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will exp…

gr-qc2023★ 1 cited

Measuring source properties and quasi-normal-mode frequencies of heavy massive black-hole binaries with LISA

Alexandre Toubiana, Lorenzo Pompili, Alessandra Buonanno +2

The laser-interferometer space antenna (LISA) will be launched in the mid 2030s. It promises to observe the coalescence of massive black-hole (BH) binaries with signal-to-noise rat…

gr-qc2023★ 26 cited

Is there an excess of black holes around ? Optimising the complexity of population models with the use of reversible jump MCMC

Alexandre Toubiana, Michael L. Katz, Jonathan R. Gair

Some analyses of the third gravitational wave catalogue released by the LIGO-Virgo-KAGRA collaboration (LVK) suggest an excess of black holes around . In order to…

gr-qc2022★ 17 cited

Detectability and parameter estimation of GWTC-3 events with LISA

Alexandre Toubiana, Stanislav Babak, Sylvain Marsat +1

Multiband observations of coalescing stellar-mass black holes binaries could deliver valuable information on the formation of those sources and potential deviations from General Re…

gr-qc2022

Observing GW190521-like binary black holes and their environment with LISA

Laura Sberna, Stanislav Babak, Sylvain Marsat +8

Binaries of relatively massive black holes like GW190521 have been proposed to form in dense gas environments, such as the disks of Active Galactic Nuclei (AGNs), and they might be…

gr-qc2021

Discriminating between different scenarios for the formation and evolution of massive black holes with LISA

Alexandre Toubiana, Kaze W. K. Wong, Stanislav Babak +5

Electromagnetic observations have provided strong evidence for the existence of massive black holes in the center of galaxies, but their origin is still poorly known. Different sce…

gr-qc2021★ 49 cited

Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA

Kallol Dey, Nikolaos Karnesis, Alexandre Toubiana +4

Massive black hole binaries are expected to provide the strongest gravitational wave signals for the Laser Interferometer Space Antenna (LISA), a space mission targeting mH…

gr-qc2020★ 25 cited

Modeling gravitational waves from exotic compact objects

Alexandre Toubiana, Stanislav Babak, Enrico Barausse +1

Exotic compact objects can be difficult to distinguish from black holes in the inspiral phase of the binaries observed by gravitational-wave detectors, but significant differences…

gr-qc2020★ 44 cited

Parameter estimation of stellar-mass black hole binaries with LISA

Alexandre Toubiana, Sylvain Marsat, Stanislav Babak +2

Stellar-mass black hole binaries (SBHBs), like those currently being detected with the ground-based gravitational-wave (GW) observatories LIGO and Virgo, are also an anticipated GW…

gr-qc2020★ 42 cited

Tests of general relativity with stellar-mass black hole binaries observed by LISA

Alexandre Toubiana, Sylvain Marsat, Enrico Barausse +2

We consider the observation of stellar-mass black holes binaries with the Laser Interferometer Space Antenna (LISA). Preliminary results based on Fisher information matrix analyses…

gr-qc2020★ 401 cited

Prospects for Fundamental Physics with LISA

Enrico Barausse, Emanuele Berti, Thomas Hertog +318

In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental…