scispace - formally typeset
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.

Papers
More filters
Journal ArticleDOI

Scientific objectives of Einstein Telescope

Bangalore Suryanarayana Sathyaprakash, +225 more
TL;DR: The advanced interferometer network will herald a new era in observational astronomy, and there is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz to 10 kHz, with sensitivity a factor 10 better in amplitude as discussed by the authors.
Journal ArticleDOI

Simulations of Magnetically Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation

TL;DR: In this article, the first 2D rotating, multigroup, radiation magnetohydrodynamics (RMHD) simulations of supernova core collapse, bounce, and explosion were presented.
Journal ArticleDOI

Neutrino signatures and the neutrino-driven wind in binary neutron star mergers

TL;DR: In this article, the authors presented VULCAN/2D multigroup flux-limited-diffusion radiation-hydrodynamics simulations of binary neutron star mergers, using the Shen equation of state, covering ≳ 100 ms, and starting from azimuthal-averaged two-dimensional slices obtained from three-dimensional smooth-particle-hydro-drone-based simulations of Rosswog & Price for 1.4M☉ (baryonic) neutron stars with no initial spins, co-rotating spins, or counter-
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.
Journal ArticleDOI

Two-Dimensional Multiangle, Multigroup Neutrino Radiation-Hydrodynamic Simulations of Postbounce Supernova Cores

TL;DR: In this article, a 2D discrete-ordinate (S_n) method was used to calculate the post-bounce phase of core-collapse supernovae using axisymmetric (2D) multiangle, multigroup neutrino radiation-hydrodynamic calculations.