activity
20042024
most citedRelativistic tidal properties of neutron stars

851 citations · 9.6k across the 106 of their papers we have counts for

collaborators

108 papers

gr-qc2024

Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Angelica Albertini, Alessandro Nagar, Josh Mathews +1

We present the first comparison of waveforms evaluated using the effective-one-body (EOB) approach and gravitational self-force (GSF) theory for inspiralling black hole binaries wi…

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★ 32 cited

Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricity

Angelica Albertini, Rossella Gamba, Alessandro Nagar +1

We present a first complete implementation of an effective-one-body (EOB) model for extreme-mass-ratio inspirals (EMRIs) that incorporates aligned spins (on both the primary and th…

gr-qc2023★ 39 cited

Unveiling the merger structure of black hole binaries in generic planar orbits

Gregorio Carullo, Simone Albanesi, Alessandro Nagar +4

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 gravitatio…

gr-qc2023

Analytically improved and numerical-relativity informed effective-one-body model for coalescing binary neutron stars

Rossella Gamba, Matteo Breschi, Sebastiano Bernuzzi +9

Gravitational wave astronomy pipelines rely on template waveform models for searches and parameter estimation purposes. For coalescing binary neutron stars (BNS), such models need…

gr-qc2023★ 3 cited

Towards numerical-relativity informed effective-one-body waveforms for dynamical capture black hole binaries

Tomas Andrade, Juan Trenado, Simone Albanesi +10

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 det…