activity
19952009
most citedOn the Nature of Core Collapse Supernova Explosions

686 citations · 1.6k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2009★ 26 cited

Self-Consistent Solution of Cosmological Radiation-Hydrodynamics and Chemical Ionization

Daniel R. Reynolds, John C. Hayes, Pascal Paschos +1

We consider a PDE system comprising compressible hydrodynamics, flux-limited diffusion radiation transport and chemical ionization kinetics in a cosmologically-expanding universe.…

astro-ph2007★ 12 cited

Resonance Related Spiral Substructure in a Galactic Gaseous Disk

Miguel A. Yáñez, Michael L. Norman, Marco A. Martos +1

We use high resolution 2D hydrodynamic simulations to study the formation of spiral substructure in the gaseous disk of a galaxy. The obtained gaseous response is driven by a self-…

astro-ph2007★ 57 cited

Modeling core collapse supernovae in 2 and 3 dimensions with spectral neutrino transport

S. W. Bruenn, C. J. Dirk, A. Mezzacappa +4

The overwhelming evidence that the core collapse supernova mechanism is inherently multidimensional, the complexity of the physical processes involved, and the increasing evidence…

astro-ph2005★ 318 cited

Simulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP

J. C. Hayes, M. L. Norman, R. A. Fiedler +5

This paper describes ZEUS-MP, a multi-physics, massively parallel, message- passing implementation of the ZEUS code. ZEUS-MP differs significantly from the ZEUS-2D code, the ZEUS-3…

astro-ph2002★ 113 cited

Beyond Flux-Limited Diffusion: Parallel Algorithms for Multidimensional Radiation Hydrodynamics

John C. Hayes, Michael L. Norman

This paper presents a new code for performing multidimensional radiation hydrodynamic (RHD) simulations on parallel computers involving anisotropic radiation fields and nonequilibr…

astro-ph1995★ 336 cited

Pulsar Recoil and Gravitational Radiation due to Asymmetrical Stellar Collapse and Explosion

Adam Burrows, John Hayes

New data imply that the average velocity of radio pulsars is large \cite{hla93}. Under the assumption that these data imply that a pulsar is born with an ``intrinsic'' kick, we inv…