C
Christian D. Ott
Researcher at California Institute of Technology
Publications - 54
Citations - 3622
Christian D. Ott is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Supernova & Neutron star. The author has an hindex of 25, co-authored 54 publications receiving 3322 citations. Previous affiliations of Christian D. Ott include Institute for the Physics and Mathematics of the Universe & University of Arizona.
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Proceedings ArticleDOI
Studies of Stellar Collapse and Black Hole Formation with the Open-Source Code GR1D
Christian D. Ott,Evan O'Connor +1 more
TL;DR: In this article, the authors discuss results from simulations of black hole formation in failing core-collapse supernovae performed with the code GR1D, a new open-source Eulerian spherically-symmetric general-relativistic hydrodynamics code.
Evolution of the magnetized, neutrino-cooled accretion disk in the aftermath of a black hole-neutron star binary merger
Fatemeh Hossein Nouri,Fatemeh Hossein Nouri,Matthew D. Duez,Francois Foucart,Francois Foucart,M. Brett Deaton,M. Brett Deaton,M. Brett Deaton,Roland Haas,Roland Haas,Roland Haas,Milad Haddadi,Lawrence E. Kidder,Christian D. Ott,Christian D. Ott,Harald P. Pfeiffer,Harald P. Pfeiffer,Harald P. Pfeiffer,Mark A. Scheel,Béla Szilágyi +19 more
TL;DR: In this paper, the Spectral Einstein Code (SpEC) was used to simulate the postmerger evolution of a magnetized black hole-neutron star binary system.
Journal ArticleDOI
Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star
TL;DR: This article carried out three-dimensional core-collapse supernova simulations with and without aspherical velocity perturbations to assess their potential impact on the supernova hydrodynamics in the stalled shock phase.
2d multi-angle, multi-group neutrino radiation-hydrodyn amic simulations of postbounce supernova cores
TL;DR: In this article, a 2D discrete-ordinate (Sn) method was used to perform axisymmetric (2D) multi-angle, multi-group neutrino radiation-hydrodynamic calculations of the postbounce phase of core-collapse supernovae.
Journal ArticleDOI
Magnetically-driven explosions of rapidly-rotating white dwarfs following Accretion-Induced Collapse
TL;DR: In this article, a 2D multi-group flux-limited diffusion magnetohydrodynamics (MHD) simulation of the AIC of a rapidly-rotating white dwarf is presented.