Papers

Papers published after the start of GWSky in 2025. Links go to arXiv and INSPIRE-HEP.

25 papers

  • 2026-09 · Submitted

    Nonlinear evolution in Galileon EFTs: Regularization and screening

    F. Thaalba, A. Held, R. Cayuso, T. P. Sotiriou

    In a scalar effective field theory with Galileon symmetry, we distinguish the strong-field expansion from the derivative expansion and study spherically symmetric classical nonlinear dynamics, including screening.

  • 2026-09 · Submitted

    Introducing SINFONIA: Symplectic, slimplectic and Magnusian (Neural) Flows for Orbital Numerical Integration and Acceleration

    L. J. Gomes Da Silva

    Introduces three structure-preserving neural-flow architectures for long-duration gravitational-wave inspirals, showing that encoding secular energy–angular-momentum balance keeps chained phase errors small at orbital-period timesteps.

  • 2026-07 · Submitted

    Environmental effects vs. modified gravity in the LISA massive black hole binary population

    L. Copparoni, E. Barausse

    Gravitational-wave signals from massive black hole binaries observed by LISA can carry imprints of both the astrophysical environment of the source and possible deviations from general relativity. We investigate whether environmental effects leave a detectable imprint on the LISA binary population, and whether they can mimic modified-gravity effects with the same frequency dependence.

  • 2026-05 · Submitted

    When the Ringing Stops: Purely Imaginary Modes in the Ringdown Spectrum of Dynamical Black Holes

    L. Capuano, T. Lovo, G. Prieto-Varela, S. Sarkar, A. Kuntz, E. Barausse, D. Kothawala

    We extend the frequency-domain analysis of quasinormal modes in a dynamical, spherically symmetric black hole spacetime undergoing constant-rate mass evolution, and report purely imaginary eigenvalues in addition to the usual light-ring modes.

  • 2026-05 · Submitted

    Impact of sky localization uncertainty on ringdown inference

    K. Dey, E. Barausse, M. Crisostomi, R. Trotta

    Assesses how uncertainty in gravitational-wave sky localization propagates into black-hole ringdown parameter inference, with implications for tests of gravity with next-generation detectors.

  • 2026-05 · Phys. Rev. D 114, 063026 (2026)

    Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum

    R. Chen, R. S. Chandramouli, F. Pozzoli, R. Buscicchio, E. Barausse

    Astrophysical formation channels of stellar-mass binary black holes can induce significant orbital eccentricities in their early inspiral. We analyze the implications for the LISA stochastic gravitational-wave background from unresolved sBBHs.

  • 2026-05 · Submitted

    Constraints on Einstein-aether gravity from the precision timing of PSR J1738+0333

    M. Vaglio, A. Carleo, A. Susobhanan, E. Barausse, B. B. Salem, A. Corongiu, P. C. Freire, D. Perrodin

    Uses the precision timing of the binary pulsar PSR J1738+0333 to constrain Einstein-aether gravity.

  • 2026-05 · Phys. Rev. D 114, 024073 (2026)

    Scalar emission from binary neutron stars in scalar-tensor theories with kinetic screening

    R. Cayuso, A. Kuntz, T. Assumpcao, M. Bezares, E. Barausse

    Numerical-relativity study of scalar emission from binary neutron stars in scalar-tensor theories with kinetic screening, relevant for tests of gravity with next-generation detectors.

  • 2026-04 · Submitted

    The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

    D. Izquierdo-Villalba, M. Habouzit, M. Bonetti et al. (incl. E. Barausse)

    Comparison of simulated massive black hole binary catalogues for LISA astrophysics, produced by the LISA Astrophysics Working Group.

  • 2026-03 · Submitted

    Reducing cosmological degeneracies by combining multiple classes of LISA gravitational-wave standard sirens

    D. Laghi, N. Tamanini, A. Sesana, J. Gair, E. Barausse, C. Caprini, W. Del Pozzo, A. Mangiagli, S. Marsat

    Shows how combining multiple classes of LISA standard sirens reduces cosmological parameter degeneracies for next-generation gravitational-wave cosmology.

  • 2026-03 · Submitted

    Looking for non-gaussianity in Pulsar Timing Arrays through the four point correlator

    A. Kuntz, C. Smarra, M. Vaglio

    Searches for non-Gaussian signatures in pulsar-timing-array stochastic backgrounds using the four-point correlator.

  • 2026-03 · Submitted

    Extreme mass ratio head-on collisions of black holes in Einstein-scalar-Gauss-Bonnet theory

    A. M. Frassino, D. C. Lopes, J. V. Rocha

    Ray-tracing study of event-horizon evolution in infinite-mass-ratio head-on collisions of hairy black holes in Einstein-scalar-Gauss-Bonnet gravity, compared with general relativity.

  • 2026-02 · Phys. Rev. D 114, 024017 (2026)

    Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries

    S. Yi, F. Iacovelli, E. Berti, R. S. Chandramouli, S. Marsat, D. Wadekar, N. Yunes

    Assesses systematic parameter-estimation biases for LISA massive black hole binaries when higher harmonics are dropped from spin-aligned, high-mass waveform models.

  • 2026-02 · Phys. Rev. D 113, 124038 (2026)

    Dynamical hair growth in black hole binaries in Einstein-scalar-Gauss-Bonnet gravity

    L. Capuano, L. Aresté Saló, D. D. Doneva, S. S. Yazadjiev, E. Barausse

    Numerical-relativity study of dynamical scalar hair growth in black hole binaries in Einstein-scalar-Gauss-Bonnet gravity.

  • 2026-01 · Phys. Rev. D 113, 104034 (2026)

    Detectability of gravitational-wave memory with LISA: A Bayesian approach

    A. Cogez, S. Gasparotto, J. Zosso, H. Inchauspé, C. Pitte, L. Magaña Zertuche, A. Petiteau, M. Besancon

    Bayesian study of whether LISA can detect and reconstruct the displacement memory effect from individual massive black hole binary mergers.

  • 2025-12 · Astrophys. J. Lett. 996, L9 (2026)

    Search for Gravitational-wave Memory in PPTA and EPTA Data: A Complete Signal Model

    S. M. Tomson, B. Goncharov, R. van Haasteren et al. (incl. R. Srinivasan, E. Barausse)

    A complete signal model for gravitational-wave memory searches in PPTA and EPTA pulsar-timing data.

  • 2025-10 · Phys. Rev. D 113, 064001 (2026)

    Hierarchical modeling of gravitational-wave populations for disentangling environmental and modified-gravity effects

    S. Kejriwal, E. Barausse, A. J. Chua

    Hierarchical population modelling designed to separate astrophysical environmental effects from genuine deviations from general relativity in gravitational-wave catalogues.

  • 2025-10 · Phys. Rev. Lett. 137, 021405 (2026)

    When Vacuum Breaks: A Self-Consistency Test for Astrophysical Environments in Extreme Mass Ratio Inspirals

    L. Copparoni, R. S. Chandramouli, E. Barausse

    Proposes a self-consistency test to decide when vacuum gravitational-wave models fail for extreme mass-ratio inspirals embedded in astrophysical environments.

  • 2025-07 · Phys. Rev. D 113, 124003 (2026)

    Searching for gravitational waves with Gaia and its cross-correlation with PTA: Absolute vs differential astrometry

    M. Vaglio, M. Falxa, G. Mentasti, A. I. Renzini, A. Kuntz, E. Barausse, C. R. Contaldi, A. Sesana

    Compares absolute and differential astrometry for gravitational-wave searches with Gaia and their cross-correlation with pulsar timing arrays.

  • 2025-07 · Phys. Lett. B 869, 139877 (2025)

    Weak cosmic censorship with spinning particles in Kerr-(A)dS spacetimes

    A. M. Frassino, J. V. Rocha, A. P. Sanna

    Tests whether spinning particles dropped into extremal Kerr-(A)dS black holes can overspin them, extending the Wald–Needham analysis to a nonzero cosmological constant.

  • 2025-07 · Phys. Rev. D 112, 084053 (2025)

    Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries

    R. Chen, R. S. Chandramouli, F. Pozzoli, R. Buscicchio, E. Barausse

    Quantifies how astrophysical environments modify the LISA stochastic gravitational-wave signal produced by stellar-mass black hole binaries.

  • 2025-06 · Phys. Rev. D 112, 103043 (2025)

    Simulation-based population inference of LISA’s Galactic binaries: Bypassing the global fit

    R. Srinivasan, E. Barausse, N. Korsakova, R. Trotta

    A simulation-based inference pipeline for the Galactic-binary population in LISA that can bypass a computationally expensive global fit.

  • 2025-06 · Phys. Rev. D 112, 104031 (2025)

    Systematic bias in LISA ringdown analysis due to waveform inaccuracy

    L. Capuano, M. Vaglio, R. S. Chandramouli, C. L. Pitte, A. Kuntz, E. Barausse

    Assesses systematic biases in LISA ringdown analyses of massive black hole binaries caused by incomplete waveform models.

  • 2025-05 · Int. J. Mod. Phys. D 34, 2544024 (2025)

    Quantum censors: Backreaction builds horizons

    A. M. Frassino, R. A. Hennigar, J. F. Pedraza, A. Svesko

    Gravity Research Foundation essay arguing that semi-classical backreaction generates horizons that enforce cosmic censorship, using holographic solutions of semi-classical gravity.

  • 2025-02 · Phys. Rev. D 111, 104079 (2025)

    Implications of stochastic gas torques for asymmetric binaries in the LISA band

    L. Copparoni, E. Barausse, L. Speri, L. Sberna, A. Derdzinski

    Studies how stochastic gas torques in accretion disks affect asymmetric black-hole binaries in the LISA band.