no code implementations • 28 Jul 2020 • Roxana Rosca-Mead, Christopher J. Moore, Ulrich Sperhake, Michalis Agathos, Davide Gerosa
We compute families of spherically symmetric neutron-star models in two-derivative scalar-tensor theories of gravity with a massive scalar field.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
1 code implementation • 13 Jul 2020 • Davide Gerosa, Geraint Pratten, Alberto Vecchio
We present a novel machine-learning approach to estimate selection effects in gravitational-wave observations.
no code implementations • 4 Mar 2020 • Matthew Mould, Davide Gerosa
We finally apply these findings to a simple astrophysical population of binary black holes where a formation mechanism aligns the spins without preference for co- or counter-alignment, as might be the case for stellar-mass black holes embedded in the accretion disk of a supermassive black hole.
General Relativity and Quantum Cosmology Astrophysics of Galaxies High Energy Astrophysical Phenomena
no code implementations • 13 Sep 2019 • Kaze W. K. Wong, Davide Gerosa
We report on advances to interpret current and future gravitational-wave events in light of astrophysical simulations.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
1 code implementation • 12 Jun 2019 • Davide Gerosa, Emanuele Berti
Pair instabilities in supernovae might prevent the formation of black holes with masses between $\sim 50 M_\odot$ and $\sim 130 M_\odot$.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
2 code implementations • 22 May 2019 • Vijay Varma, Scott E. Field, Mark A. Scheel, Jonathan Blackman, Davide Gerosa, Leo C. Stein, Lawrence E. Kidder, Harald P. Pfeiffer
The final black hole model, \RemnantModel, models the mass, spin, and recoil kick velocity of the remnant black hole.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
1 code implementation • 31 Jan 2019 • Davide Gerosa, Sizheng Ma, Kaze W. K. Wong, Emanuele Berti, Richard O'Shaughnessy, Yanbei Chen, Krzysztof Belczynski
We use population synthesis simulations of isolated binary stars to explore some of the stellar physics that could be constrained with multiband events, and we show that specific formation pathways might be overrepresented in multiband events compared to ground-only detections.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
no code implementations • 14 Nov 2018 • Davide Gerosa, Alicia Lima, Emanuele Berti, Ulrich Sperhake, Michael Kesden, Richard O'Shaughnessy
Within the framework of 2PN black-hole binary spin precession, we explore configurations where one of the two spins oscillates from being completely aligned with the orbital angular momentum to being completely anti-aligned with it during a single precession cycle.
General Relativity and Quantum Cosmology Astrophysics of Galaxies High Energy Astrophysical Phenomena
1 code implementation • 24 Sep 2018 • Vijay Varma, Davide Gerosa, François Hébert, Leo C. Stein, Hao Zhang
We present accurate fits for the remnant properties of generically precessing binary black holes, trained on large banks of numerical-relativity simulations.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
2 code implementations • 7 Aug 2018 • Davide Gerosa, Emanuele Berti, Richard O'Shaughnessy, Krzysztof Belczynski, Michael Kesden, Daniel Wysocki, Wojciech Gladysz
We study the expected spin misalignments of merging binary black holes (BHs) formed in isolation by combining state-of-the-art population synthesis models with efficient post-Newtonian evolutions, thus tracking sources from stellar formation to gravitational-wave detection.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
no code implementations • 29 Jun 2018 • Rhondale Tso, Davide Gerosa, Yanbei Chen
The early inspiral of massive stellar-mass black-hole binaries merging in LIGO's sensitivity band will be detectable at low frequencies by the upcoming space mission LISA.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
2 code implementations • 21 Jun 2018 • Stephen R. Taylor, Davide Gerosa
Catalogs of stellar-mass compact binary systems detected by ground-based gravitational-wave instruments (such as LIGO and Virgo) will offer insights into the demographics of progenitor systems and the physics guiding stellar evolution.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology Data Analysis, Statistics and Probability
2 code implementations • 12 Feb 2018 • Davide Gerosa, François Hébert, Leo C. Stein
Our procedure uses a numerical-relativity surrogate model to obtain the gravitational waveform given a set of binary parameters, then from this waveform we directly integrate the gravitational-wave linear momentum flux.
General Relativity and Quantum Cosmology Astrophysics of Galaxies High Energy Astrophysical Phenomena
no code implementations • 27 Nov 2017 • Davide Gerosa
Measurements of black-hole spins are of crucial importance to fulfill the promise of gravitational-wave astronomy.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
no code implementations • 14 Jul 2017 • Salvatore Vitale, Davide Gerosa, Carl-Johan Haster, Katerina Chatziioannou, Aaron Zimmerman
In a regime where data are only mildly informative, prior choices can play a significant role in Bayesian statistical inference, potentially affecting the inferred physics.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 5 May 2017 • Xinyu Zhao, Michael Kesden, Davide Gerosa
We use analytic solutions for generic spin precession at 2PN order to derive Fourier series for the total and orbital angular momenta in which each term is a sinusoid with frequency $\Omega - n\omega$ for integer $n$.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 18 Mar 2017 • Davide Gerosa, Emanuele Berti
Advanced LIGO detectors at Hanford and Livingston made two confirmed and one marginal detection of binary black holes during their first observing run.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 15 Dec 2016 • Davide Gerosa, Ulrich Sperhake, Jakub Vošmera
We analyze the inspiral dynamics of equal-mass precessing black-hole binaries using multi-timescale techniques.
General Relativity and Quantum Cosmology Astrophysics of Galaxies High Energy Astrophysical Phenomena
no code implementations • 14 Jun 2016 • Davide Gerosa, Christopher J. Moore
Generic black hole binaries radiate gravitational waves anisotropically, imparting a recoil, or kick, velocity to the merger remnant.
General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
1 code implementation • 3 May 2016 • Davide Gerosa, Michael Kesden
We present the numerical code PRECESSION: a new open-source python module to study the dynamics of precessing black-hole binaries in the post-Newtonian regime.
High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies General Relativity and Quantum Cosmology
no code implementations • 20 Jul 2015 • Daniele Trifirò, Richard O'Shaughnessy, Davide Gerosa, Emanuele Berti, Michael Kesden, Tyson Littenberg, Ulrich Sperhake
Gravitational waves from coalescing binary black holes encode the evolution of their spins prior to merger.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 30 Jun 2015 • Davide Gerosa, Michael Kesden, Richard O'Shaughnessy, Antoine Klein, Emanuele Berti, Ulrich Sperhake, Daniele Trifirò
In this work, we show that these solutions can be unstable when the spin of the higher-mass black hole is aligned with the orbital angular momentum and the spin of the lower-mass black hole is anti-aligned.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 10 Jun 2015 • Davide Gerosa, Michael Kesden, Ulrich Sperhake, Emanuele Berti, Richard O'Shaughnessy
The dynamics of precessing binary black holes (BBHs) in the post-Newtonian regime has a strong timescale hierarchy: the orbital timescale is very short compared to the spin-precession timescale which, in turn, is much shorter than the radiation-reaction timescale on which the orbit is shrinking due to gravitational-wave emission.
General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
no code implementations • 23 Mar 2015 • Davide Gerosa, Benedetta Veronesi, Giuseppe Lodato, Giovanni Rosotti
While binary migration is due to angular-momentum transfer within the circumbinary disc, the spin-alignment process is driven by the mass accreting on to each black hole.
Astrophysics of Galaxies High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
no code implementations • 3 Nov 2014 • Michael Kesden, Davide Gerosa, Richard O'Shaughnessy, Emanuele Berti, Ulrich Sperhake
We derive an effective potential for binary black-hole (BBH) spin precession at second post-Newtonian order.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 8 May 2014 • Davide Gerosa, Alberto Sesana
We investigate the consequences of superkicks on the population of supermassive black holes (SMBHs) in the Universe residing in brightest cluster galaxies (BCGs).
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
no code implementations • 18 Feb 2013 • Davide Gerosa, Michael Kesden, Emanuele Berti, Richard O'Shaughnessy, Ulrich Sperhake
Under the plausible assumption that tidal interactions are efficient at aligning the spins of few-solar mass black-hole progenitors with the orbital angular momentum, we find that black-hole spins should be expected to preferentially lie in a plane when they become detectable by gravitational-wave interferometers.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena