Joshua C. Dolence, Ph.D.
Affiliations: | 2011 | Astronomy | University of Illinois, Urbana-Champaign, Urbana-Champaign, IL |
Area:
Astrophysics Physics, Astronomy and Astrophysics, Theory PhysicsGoogle:
"Joshua Dolence"Parents
Sign in to add mentorCharles F. Gammie | grad student | 2011 | UIUC | |
(Self-consistent dynamical and radiative models of low-luminosity active galactic nuclei.) |
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Publications
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Ryan BR, Dolence JC. (2020) MOCMC: Method of Characteristics Moment Closure, a Numerical Method for Covariant Radiation Magnetohydrodynamics The Astrophysical Journal. 891: 118 |
Miller JM, Ryan BR, Dolence JC. (2019) ν bhlight: Radiation GRMHD for Neutrino-driven Accretion Flows Astrophysical Journal Supplement Series. 241: 30 |
Skinner MA, Dolence JC, Burrows A, et al. (2019) Fornax: A Flexible Code for Multiphysics Astrophysical Simulations The Astrophysical Journal Supplement Series. 241: 7 |
Mabanta QA, Murphy JW, Dolence JC. (2019) Convection-aided Explosions in One-dimensional Core-collapse Supernova Simulations. I. Technique and Validation The Astrophysical Journal. 887: 43 |
Miller JM, Ryan BR, Dolence JC, et al. (2019) Full transport model of GW170817-like disk produces a blue kilonova Physical Review D. 100: 23008 |
Burrows A, Radice D, Vartanyan D, et al. (2019) The overarching framework of core-collapse supernova explosions as revealed by 3D fornax simulations Monthly Notices of the Royal Astronomical Society. 491: 2715-2735 |
Murphy JW, Mabanta Q, Dolence JC. (2019) A comparison of explosion energies for simulated and observed core-collapse supernovae Monthly Notices of the Royal Astronomical Society. 489: 641-652 |
Grinstein F, Saenz JA, Dolence JC, et al. (2019) Effects of operator splitting and low Mach-number correction in turbulent mixing transition simulations Computers & Mathematics With Applications. 78: 437-458 |
Ryan BR, Ressler SM, Dolence JC, et al. (2018) Two-temperature GRRMHD Simulations of M87 The Astrophysical Journal. 864: 126 |
Vartanyan D, Burrows A, Radice D, et al. (2018) Revival of the fittest: exploding core-collapse supernovae from 12 to 25 M⊙ Monthly Notices of the Royal Astronomical Society. 477: 3091-3108 |