L
Luciano Rezzolla
Researcher at Frankfurt Institute for Advanced Studies
Publications - 35
Citations - 1024
Luciano Rezzolla is an academic researcher from Frankfurt Institute for Advanced Studies. The author has contributed to research in topics: Neutron star & Binary black hole. The author has an hindex of 18, co-authored 35 publications receiving 885 citations. Previous affiliations of Luciano Rezzolla include International School for Advanced Studies & University of Trieste.
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Error-analysis and comparison to analytical models of numerical waveforms produced by the NRAR Collaboration
Ian Hinder,Alessandra Buonanno,Michael Boyle,Zachariah B. Etienne,James Healy,Nathan K. Johnson-McDaniel,Alessandro Nagar,Hiroyuki Nakano,Hiroyuki Nakano,Yi Pan,Harald P. Pfeiffer,Harald P. Pfeiffer,M. Pürrer,Christian Reisswig,Mark A. Scheel,Erik Schnetter,Erik Schnetter,Erik Schnetter,Ulrich Sperhake,Béla Szilágyi,Wolfgang Tichy,Barry Wardell,Barry Wardell,Anil Zenginoglu,Daniela Alic,Sebastiano Bernuzzi,Tanja Bode,Bernd Brügmann,Luisa T. Buchman,Manuela Campanelli,Tony Chu,Tony Chu,Thibault Damour,Jason D. Grigsby,Mark Hannam,Roland Haas,Roland Haas,Daniel A. Hemberger,Daniel A. Hemberger,Sascha Husa,Lawrence E. Kidder,Pablo Laguna,Lionel London,Geoffrey Lovelace,Geoffrey Lovelace,Geoffrey Lovelace,Carlos O. Lousto,Pedro Marronetti,Pedro Marronetti,Richard A. Matzner,Philipp Mösta,Philipp Mösta,Abdul Mroue,Doreen Müller,Bruno C. Mundim,Bruno C. Mundim,Andrea Nerozzi,Vasileios Paschalidis,Denis Pollney,George Reifenberger,Luciano Rezzolla,Stuart L. Shapiro,Deirdre Shoemaker,Andrea Taracchini,Nicholas Taylor,Saul A. Teukolsky,Marcus Thierfelder,Helvi Witek,Helvi Witek,Yosef Zlochower +69 more
TL;DR: The first stage of the NRAR project focused on producing an initial set of numerical waveforms from binary black holes with moderate mass ratios and spins, as well as one non-spinning binary configuration which has a mass ratio of 10 as mentioned in this paper.
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Equilibrium models of relativistic stars with a toroidal magnetic field
Joachim Frieben,Luciano Rezzolla +1 more
TL;DR: In this article, a model of rotating relativistic stars with a toroidal magnetic field and rotation has been proposed to compute the surface deformation and the quadrupole distortion up to significant levels of rotation and magnetisation.
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Accurate Simulations of Binary Black Hole Mergers in Force-free Electrodynamics
TL;DR: In this paper, the authors provide additional information on the electromagnetic emission produced during the inspiral and merger of supermassive black holes when these are immersed in a force-free plasma threaded by a uniform magnetic field.
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When Did the Remnant of GW170817 Collapse to a Black Hole
TL;DR: In this paper, the survival time of GW170817 was determined by combining two different constraints, namely, the time needed to produce the requisite blue-ejecta mass and that necessary for the relativistic jet to bore its way out of the expanding ejecta.
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Instability-driven evolution of poloidal magnetic fields in relativistic stars
TL;DR: In this article, the authors consider the nonlinear evolution of a nonrotating neutron star with a purely poloidal magnetic field in general relativity and find that an instability develops in the region of the closed magnetic field lines and over an Alfven timescale, as predicted by perturbation theory.