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Evan O'Connor

Researcher at Stockholm University

Publications -  128
Citations -  6072

Evan O'Connor is an academic researcher from Stockholm University. The author has contributed to research in topics: Neutrino & Supernova. The author has an hindex of 40, co-authored 117 publications receiving 5198 citations. Previous affiliations of Evan O'Connor include National Research Council & California Institute of Technology.

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Black hole formation in failing core-collapse supernovae

Evan O'Connor, +1 more
- 01 Apr 2011 - 
TL;DR: In this article, the authors present results of a systematic study of failing core-collapse supernovae and the formation of stellar-mass black holes (BHs) using GR1D equipped with a three-species neutrino leakage/heating scheme.
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A new open-source code for spherically symmetric stellar collapse to neutron stars and black holes

Evan O'Connor, +3 more
- 07 Jun 2010 - 
TL;DR: GR1D as mentioned in this paper is a spherically symmetric general-relativistic (GR) hydrodynamics code for the simulation of stellar collapse to neutron stars and black holes and will also serve as a testbed for modeling technology to be incorporated in multi-D GR codes.
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General-relativistic simulations of three-dimensional core-collapse supernovae

Christian D. Ott, +14 more
- 10 May 2013 - 
TL;DR: In this article, the authors studied the 3D hydrodynamics of the post-core-bounce phase of the collapse of a 27 M_☉ star and paid special attention to the development of the standing accretion shock instability (SASI) and neutrino-driven convection.
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Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae

Evan O'Connor, +1 more
- 25 Sep 2018 - 
TL;DR: The physical mechanism that drives core-collapse supernovae (CCSNe) remains uncertain this article, while there is an emerging consensus on the qualitative outcome of detailed CCSN mechanism simulations.
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Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling

Carlos Palenzuela, +6 more
- 07 May 2015 - 
TL;DR: In this article, the influence of the equation of state on the gravitational wave signature and its role in determining the properties of the hypermassive neutron star resulting from the merger, the production of neutrinos, and the characteristics of ejecta from the system.