Simone Albanesi
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View article: GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-spin Black Hole Coalescences
GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-spin Black Hole Coalescences Open
We report the observation of gravitational waves from two binary black hole coalescences during the fourth observing run of the LIGO–Virgo–KAGRA detector network, GW241011 and GW241110. The sources of these two signals are characterized by…
View article: GW231123: A Binary Black Hole Merger with Total Mass 190–265 <i>M</i> <sub>⊙</sub>
GW231123: A Binary Black Hole Merger with Total Mass 190–265 <i>M</i> <sub>⊙</sub> Open
On 2023 November 23, the two LIGO observatories both detected GW231123, a gravitational-wave signal consistent with the merger of two black holes with masses and (90% credible intervals), at a luminosity dis…
View article: Late-Time Tails in Nonlinear Evolutions of Merging Black Holes
Late-Time Tails in Nonlinear Evolutions of Merging Black Holes Open
We uncover late-time gravitational-wave tails in fully nonlinear 3+1 dimensional numerical relativity simulations of merging black holes, using the highly accurate p code. We achieve this result by exploiting the strong magnification of la…
View article: Perturbative hyperboloidal extraction of gravitational waves in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>3</mml:mn><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:math> numerical relativity
Perturbative hyperboloidal extraction of gravitational waves in numerical relativity Open
We present a framework to propagate to null infinity gravitational waves computed at timelike world tubes in the interior of 3+1 (Cauchy) numerical relativity simulations. In our method, numerical relativity data are used as the inner infl…
View article: Binary black hole merger in the extreme mass ratio limit: a multipolar analysis of the inclined orbit case
Binary black hole merger in the extreme mass ratio limit: a multipolar analysis of the inclined orbit case Open
We compute the gravitational waveform emitted during the transition from quasi-spherical inspiral to plunge, merger and ringdown for a system of two black holes in the extreme mass ratio limit, where the primary is spinning and the seconda…
View article: GW250114: Testing Hawking’s Area Law and the Kerr Nature of Black Holes
GW250114: Testing Hawking’s Area Law and the Kerr Nature of Black Holes Open
The gravitational-wave signal GW250114 was observed by the two LIGO detectors with a network matched-filter signal-to-noise ratio of 80. The signal was emitted by the coalescence of two black holes with near-equal masses m1=33.6−0.8+1.2M⊙ …
View article: Perturbative Hyperboloidal Extraction of Gravitational Waves in 3+1 Numerical Relativity
Perturbative Hyperboloidal Extraction of Gravitational Waves in 3+1 Numerical Relativity Open
We present a framework to propagate to null infinity gravitational waves computed at timelike worldtubes in the interior of a 3+1 (Cauchy) numerical relativity simulations. In our method, numerical relativity data are used as the inner inf…
View article: Gravitational scattering of two neutron stars
Gravitational scattering of two neutron stars Open
We present the first numerical relativity simulations of the gravitational scattering of two neutron stars. Constraint-satisfying initial data for two equal-mass nonspinning sequences are constructed at fixed energy and various initial ang…
View article: Real modes and null memory contributions in effective-one-body models
Real modes and null memory contributions in effective-one-body models Open
We introduce a novel approach to describe real-valued m=0 modes from inspiral to merger and ringdown in effective-one-body models, including both oscillatory and null memory contributions. A crucial aspect of the modelization of the oscill…
View article: Black hole spectroscopy: from theory to experiment
Black hole spectroscopy: from theory to experiment Open
The "ringdown" radiation emitted by oscillating black holes has great scientific potential. By carefully predicting the frequencies and amplitudes of black hole quasinormal modes and comparing them with gravitational-wave data from compact…
View article: Search for Gravitational Waves Emitted from SN 2023ixf
Search for Gravitational Waves Emitted from SN 2023ixf Open
We present the results of a search for gravitational-wave transients associated with core-collapse supernova SN 2023ixf, which was observed in the galaxy Messier 101 via optical emission on 2023 May 19, during the LIGO–Virgo–KAGRA 15th Eng…
View article: Effective-one-body modeling for generic compact binaries with arbitrary orbits
Effective-one-body modeling for generic compact binaries with arbitrary orbits Open
We present the first unified model for the general relativistic dynamics and gravitational radiation of generic compact binaries. TEOBResumS-Dalí is a model based on the effective-one-body framework incorporating tidal interactions, generi…
View article: The Science of the Einstein Telescope
The Science of the Einstein Telescope Open
Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science objectives, providing state-of-the-art predictions for the ca…
View article: Swift-BAT GUANO Follow-up of Gravitational-wave Triggers in the Third LIGO–Virgo–KAGRA Observing Run
Swift-BAT GUANO Follow-up of Gravitational-wave Triggers in the Third LIGO–Virgo–KAGRA Observing Run Open
We present results from a search for X-ray/gamma-ray counterparts of gravitational-wave (GW) candidates from the third observing run (O3) of the LIGO–Virgo–KAGRA network using the Swift Burst Alert Telescope (Swift-BAT). The search include…
View article: GR-Athena++: General-relativistic Magnetohydrodynamics Simulations of Neutron Star Spacetimes
GR-Athena++: General-relativistic Magnetohydrodynamics Simulations of Neutron Star Spacetimes Open
We present the extension of GR-Athena++ to general-relativistic magnetohydrodynamics (GRMHD) for applications to neutron star spacetimes. The new solver couples the constrained transport implementation of Athena++ to the Z4c formulation of…
View article: Scattering and dynamical capture of two black holes: Synergies between numerical and analytical methods
Scattering and dynamical capture of two black holes: Synergies between numerical and analytical methods Open
International audience
View article: Late-time tails in nonlinear evolutions of merging black holes
Late-time tails in nonlinear evolutions of merging black holes Open
We uncover late-time gravitational-wave tails in fully nonlinear 3+1 dimensional numerical relativity simulations of merging black holes, using the highly accurate SpEC code. We achieve this result by exploiting the strong magnification of…
View article: A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154
A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154 Open
The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935+2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomic…
View article: Direct current memory effects in effective-one-body waveform models
Direct current memory effects in effective-one-body waveform models Open
The direct current (DC) memory is a non-oscillatory, hereditary component of the gravitational wave (GW) signal that represents one of the most peculiar manifestations of the nonlinear nature of GW emission and propagation. In this work, b…
View article: Inspiral-inherited ringdown tails
Inspiral-inherited ringdown tails Open
We study the late-time relaxation of a perturbed Schwarzschild black hole, driven by a source term representing an infalling particle in generic orbits. We consider quasi-circular and eccentric binaries, dynamical captures and radial infal…
View article: A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run
A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run Open
We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advance…
View article: Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations Open
Because of the electromagnetic (EM) radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow up on the gravitational-wave (GW) signal with EM telesc…
View article: GR-Athena++: General-relativistic magnetohydrodynamics simulations of neutron star spacetimes
GR-Athena++: General-relativistic magnetohydrodynamics simulations of neutron star spacetimes Open
We present the extension of GR-Athena++ to general-relativistic magnetohydrodynamics (GRMHD) for applications to neutron star spacetimes. The new solver couples the constrained transport implementation of Athena++ to the Z4c formulation of…
View article: Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations Open
Because of the electromagnetic radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow up on the gravitational-wave signal with electromagnetic tel…
View article: Unveiling the merger structure of black hole binaries in generic planar orbits
Unveiling the merger structure of black hole binaries in generic planar orbits Open
The precise modeling of binary black hole coalescences in generic planar orbits is a crucial step to disentangle dynamical and isolated binary formation channels through gravitational-wave observations. The merger regime of such coalescenc…
View article: Towards numerical-relativity informed effective-one-body waveforms for dynamical capture black hole binaries
Towards numerical-relativity informed effective-one-body waveforms for dynamical capture black hole binaries Open
Dynamical captures of black holes may take place in dense stellar media due to the emission of gravitational radiation during a close passage. Detection of such events requires detailed modelling, since their phenomenology qualitatively di…
View article: Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case
Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case Open
We present a new effective-one-body (EOB) waveform for eccentric, nonspinning, binaries in the extreme mass ratio limit, with initial eccentricities up to $0.95$. The EOB analytical waveform, that includes noncircular corrections up to sec…
View article: GW190521 as a dynamical capture of two nonspinning black holes
GW190521 as a dynamical capture of two nonspinning black holes Open
Data release associated to "GW190521 as a dynamical capture of two nonspinning black holes" [1]. The posterior samples have been obtained with bajes [2], a pipeline for gravitational wave (GW) and multimessenger astronomy, publicly availab…
View article: GW190521 as a dynamical capture of two nonspinning black holes
GW190521 as a dynamical capture of two nonspinning black holes Open
Data release associated to "GW190521 as a dynamical capture of two nonspinning black holes" [1]. The posterior samples have been obtained with bajes [2], a pipeline for gravitational wave (GW) and multimessenger astronomy, publicly availab…
View article: Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
Towards a gravitational self force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals Open
Building upon several recent advances in the development of effective-one-body models for spin-aligned eccentric binaries with individual masses $(m_1,m_2)$ we introduce a new EOB waveform model that aims at describing inspiralling binarie…