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Strong-field scattering of two spinning black holes: Numerical Relativity versus post-Minkowskian gravity

New paper comparing effective-one-body and Numerical-Relativity scattering angle for spinning black holes. Check it out at https://arxiv.org/abs/2307.06999

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Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case

New paper on the construction and validation of EOB waveform through merger and ringdown for eccentric binaries in the small mass ratio limit, i.e. a particle inspiralling and plunging on a Schwarzschild black hole. Check it out at https://arxiv.org/abs/2305.19336

TEOBResumS: Analytic systematics in next-generation of effective-one-body gravitational waveform models for future observations

Most recent version of the TEOBResumS quasi-circular with improved accuracy and EOB/NR unfaithfulness at most of order 0.001. Detailed study of analytic systematics.Check it out at https://arxiv.org/abs/2304.09662 .  

Recontres de Physique de la Vallée d’Aoste, La Thuile 5-11 March 2023

Alessandro speaks on GW190521 as dynamical capture of two nonspinning black holes, presenting our Nature Astronomy paper. Here we use our  TEOBResumS waveform model to  analyze GW190521 under te assumption the signal was generated by a dynamical encounter of two black holes instead of two objects on a bound, quasi-circular, orbit.

Jobs

Upcoming position on detector noise characterisation with GANs

Within the European Project InterTwin  we are about to open a position  (Assegno di Ricerca) for 1+1 years on the topic: Characterisation of detector noise for Gravitational Wave experiments using Generative Adversarial Networks.  The sensitivity of GW interferometers is limited by noise. We will use Generative Adversarial Networks (GANs) to produce a Digital Twin (DT)…

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