P
Pedro Marronetti
Researcher at National Science Foundation
Publications - 79
Citations - 5198
Pedro Marronetti is an academic researcher from National Science Foundation. The author has contributed to research in topics: Gravitational wave & Type II supernova. The author has an hindex of 34, co-authored 77 publications receiving 4855 citations. Previous affiliations of Pedro Marronetti include University of Notre Dame & University of Illinois at Urbana–Champaign.
Papers
More filters
Journal ArticleDOI
Accurate Evolutions of Orbiting Black-Hole Binaries without Excision
TL;DR: A new algorithm for evolving orbiting black-hole binaries that does not require excision or a corotating shift is presented and fourth-order convergence of waveforms is shown and the radiated gravitational energy and angular momentum from the plunge is computed.
Journal ArticleDOI
Three-dimensional Core-collapse Supernova Simulated Using a 15 M⊙ Progenitor
Eric J. Lentz,Eric J. Lentz,Stephen W. Bruenn,W. Raphael Hix,W. Raphael Hix,Anthony Mezzacappa,Anthony Mezzacappa,O. E. Bronson Messer,O. E. Bronson Messer,O. E. Bronson Messer,Eirik Endeve,Eirik Endeve,John M. Blondin,J. Austin Harris,Pedro Marronetti,Konstantin N. Yakunin,Konstantin N. Yakunin +16 more
TL;DR: In this paper, the authors performed ab initio neutrino radiation hydrodynamics simulations in three and two spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 M⊙ progenitor through 440 ms after core bounce.
Journal ArticleDOI
Three-dimensional core-collapse supernova simulated using a 15 $M_\odot$ progenitor
Eric J. Lentz,Stephen W. Bruenn,W. Raphael Hix,Anthony Mezzacappa,O. E. Bronson Messer,Eirik Endeve,John M. Blondin,J. Austin Harris,Pedro Marronetti,Konstantin Yakunin +9 more
TL;DR: In this article, the authors performed ab initio neutrino radiation hydrodynamics simulations in three and two spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 $M_\odot$ progenitor through 440 ms after core bounce.
Journal ArticleDOI
The development of explosions in axisymmetric ab initio core-collapse supernova simulations of 12–25 M⊙ stars
Stephen W. Bruenn,Eric J. Lentz,Eric J. Lentz,W. Raphael Hix,W. Raphael Hix,Anthony Mezzacappa,Anthony Mezzacappa,J. Austin Harris,O. E. Bronson Messer,O. E. Bronson Messer,O. E. Bronson Messer,Eirik Endeve,Eirik Endeve,John M. Blondin,Merek A. Chertkow,Eric J. Lingerfelt,Pedro Marronetti,Konstantin N. Yakunin,Konstantin N. Yakunin +18 more
TL;DR: In this article, four axisymmetric core-collapse supernova simulations were presented from 12, 15, 20, and 25 M−1 main sequence progenitors.
Journal ArticleDOI
Relativistic numerical model for close neutron-star binaries.
TL;DR: The evidence that general relativistic effects may cause the stars to individually collapse into black holes prior to merging and the strong fields cause the last stable orbit to occur at a larger separation distance and lower frequency than previously estimated is discussed.