activity
19952013
most citedEnzo: An Adaptive Mesh Refinement Code for Astrophysics

869 citations · 1.2k across the 9 of their papers we have counts for

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6 papers · 1 filter

astro-ph2007★ 12 cited

Late Reheating of the IGM by Quasars: A Radiation Hydrodynamical Simulation of Helium II Reionization

Pascal Paschos, Michael L. Norman, James O. Bordner +1

We study the ionization and thermal evolution of the intergalactic medium during the epoch of \heii reionization by means of radiation hydrodynamical cosmological simulations. We p…

astro-ph2007

Simulating Cosmological Evolution with Enzo

Michael L. Norman, Greg L. Bryan, Robert Harkness +4

In this paper we describe our massively parallel version of Enzo, a multiphysics, parallel, AMR application for simulating cosmological structure formation developed at UCSD and Co…

astro-ph2007★ 71 cited

The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys

Eric J. Hallman, Brian W. O'Shea, Jack O. Burns +3

We present the first results from a new generation of simulated large sky coverage (~100 square degrees) Sunyaev-Zeldovich effect (SZE) cluster surveys using the cosmological adapt…

astro-ph2004★ 36 cited

Introducing Enzo, an AMR Cosmology Application

Brian W. O'Shea, Greg Bryan, James Bordner +4

In this paper we introduce Enzo, a 3D MPI-parallel Eulerian block-structured adaptive mesh refinement cosmology code. Enzo is designed to simulate cosmological structure formation,…

astro-ph1997

Explosion Diagnostics of Type Ia Supernovae from Early Infrared Spectra

C. J. Wheeler, P. Hoeflich, R. Harkness +1

Models of infrared spectra of Type Ia supernovae around maximum light are presented. The underlying dynamic models are delayed detonation explosions in Chandrasekhar mass carbon/ox…

astro-ph1995★ 128 cited

Gamma-Ray Transfer and Energy Deposition in Supernovae

Douglas A. Swartz, Peter G. Sutherland, Robert P. Harkness

Solutions to the energy-independent (gray) radiative transfer equations are compared to results of Monte Carlo simulations of the \Ni and \Co radioactive decay \GR energy depositio…