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20192026
most citedMachine Learning Gravitational Waves from Binary Black Hole Mergers

59 citations · 126 across the 19 of their papers we have counts for

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8 papers · 1 filter

gr-qc2024

Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations

Alireza Rashti, Rossella Gamba, Koustav Chandra +4

The detection and subsequent inference of binary black hole signals rely heavily on the accuracy of the waveform model employed. In the highly non-linear, dynamic, and strong-field…

gr-qc2024

Spin the black circle: horizon absorption on non-circular, planar binary black hole dynamics

Danilo Chiaramello, Rossella Gamba

Binary systems of black holes emit gravitational waves as they move through their orbits. While most of the emitted radiation escapes to future null infinity, a small fraction is a…

gr-qc2024

Effective-one-body waveform model for noncircularized, planar, coalescing black hole binaries II:high accuracy by improving logarithmic terms in resummations

Alessandro Nagar, Danilo Chiaramello, Rossella Gamba +5

Effective-one-body (EOB) models are based on analytical building blocks that, mathematically, are truncated Taylor series with logarithms. These functions are usually resummed usin…

astro-ph.HE20242 cited

Everything everywhere all at once: A detailed study of GW230529

Koustav Chandra, Ish Gupta, Rossella Gamba +5

This study investigates the origins of GW230529, delving into its formation from massive stars within isolated binary systems. Utilizing population synthesis models, we present com…

gr-qc2024

Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods

Simone Albanesi, Alireza Rashti, Francesco Zappa +6

We study initially unbound systems of two black holes using numerical relativity (NR) simulations performed with GR-Athena++. We focus on regions of the parameter space close to th…

gr-qc2024

Towards efficient Effective One Body models for generic, non-planar orbits

Rossella Gamba, Danilo Chiaramello, Sayan Neogi

Complete waveform models able to account for arbitrary non-planar orbits represent a holy grail in current gravitational-wave astronomy. Here, we take a step towards this direction…