ALBANESI, SIMONE
ALBANESI, SIMONE
FISICA
Analytic systematics in next generation of effective-one-body gravitational waveform models for future observations
2023-01-01 Nagar, Alessandro; Rettegno, Piero; Gamba, Rossella; Albanesi, Simone; Albertini, Angelica; Bernuzzi, Sebastiano
Assessment of effective-one-body radiation reactions for generic planar orbits
2022-01-01 Simone Albanesi; Alessandro Nagar; Sebastiano Bernuzzi; Andrea Placidi; Marta Orselli
Effective one-body model for extreme-mass-ratio spinning binaries on eccentric equatorial orbits: Testing radiation reaction and waveform
2021-01-01 Simone Albanesi; Alessandro Nagar; Sebastiano Bernuzzi
Exploiting Newton-factorized, 2PN-accurate waveform multipoles in effective-one-body models for spin-aligned noncircularized binaries
2022-01-01 Andrea Placidi; Simone Albanesi; Alessandro Nagar; Marta Orselli; Sebastiano Bernuzzi; Gianluca Grignani
Faithful effective-one-body waveform of small-mass-ratio coalescing black hole binaries: the eccentric, nonspinning, case
2023-01-01 Simone Albanesi; Sebastiano Bernuzzi; Thibault Damour; Alessandro Nagar; Andrea Placidi
Fermion-axion stars: Static solutions and dynamical stability
2022-01-01 Fabrizio Di Giovanni; Davide Guerra; Simone Albanesi; Miquel Miravet-Tenés; Dimitra Tseneklidou
GW190521 as a dynamical capture of two nonspinning black holes
2023-01-01 Gamba R.; Breschi M.; Carullo G.; Albanesi S.; Rettegno P.; Bernuzzi S.; Nagar A.
New avenue for accurate analytical waveforms and fluxes for eccentric compact binaries
2022-01-01 Simone Albanesi; Andrea Placidi; Alessandro Nagar; Marta Orselli; Sebastiano Bernuzzi
Toward a gravitational self-force-informed effective-one-body waveform model for nonprecessing, eccentric, large-mass-ratio inspirals
2022-01-01 Alessandro Nagar; Simone Albanesi
Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
2022-01-01 Albertini A.; Nagar A.; Rettegno P.; Albanesi S.; Gamba R.