User profiles for Jeffrey S. Oishi
Jeffrey S. OishiBates College Verified email at bates.edu Cited by 5706 |
yt: A multi-code analysis toolkit for astrophysical simulation data
The analysis of complex multiphysics astrophysical simulations presents a unique and rapidly
growing set of challenges: reproducibility, parallelization, and vast increases in data size …
growing set of challenges: reproducibility, parallelization, and vast increases in data size …
Rapid planetesimal formation in turbulent circumstellar disks
During the initial stages of planet formation in circumstellar gas disks, dust grains collide and
build up larger and larger bodies 1 . How this process continues from metre-sized boulders …
build up larger and larger bodies 1 . How this process continues from metre-sized boulders …
Enzo: An adaptive mesh refinement code for astrophysics
This paper describes the open-source code Enzo, which uses block-structured adaptive mesh
refinement to provide high spatial and temporal resolution for modeling astrophysical fluid …
refinement to provide high spatial and temporal resolution for modeling astrophysical fluid …
Dedalus: A flexible framework for numerical simulations with spectral methods
… Further distribution of this work must maintain attribution to the author(s) and the published
article’s title, journal citation, and DOI. … We outline these ideas in detail in Oishi et al. [96]. …
article’s title, journal citation, and DOI. … We outline these ideas in detail in Oishi et al. [96]. …
Simulating the common envelope phase of a red giant using smoothed-particle hydrodynamics and uniform-grid codes
We use three-dimensional hydrodynamical simulations to study the rapid infall phase of the
common envelope (CE) interaction of a red giant branch star of mass equal to 0.88 M☉ and …
common envelope (CE) interaction of a red giant branch star of mass equal to 0.88 M☉ and …
Magnetic fields in population III star formation
We study the buildup of magnetic fields during the formation of Population III star-forming
regions by conducting cosmological simulations from realistic initial conditions and varying the …
regions by conducting cosmological simulations from realistic initial conditions and varying the …
The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintained
The Pencil Code is a highly modular physics-oriented simulation code that can be adapted
to a wide range of applications. It is primarily designed to solve partial differential equations (…
to a wide range of applications. It is primarily designed to solve partial differential equations (…
A validated non-linear Kelvin–Helmholtz benchmark for numerical hydrodynamics
The non-linear evolution of the Kelvin–Helmholtz instability is a popular test for code verification.
To date, most Kelvin–Helmholtz problems discussed in the literature are ill-posed: they …
To date, most Kelvin–Helmholtz problems discussed in the literature are ill-posed: they …
ENZO: An adaptive mesh refinement code for astrophysics (version 2.6)
Enzo (Enzo Developers, 2019a) is a block-structured adaptive mesh refinement code that is
widely used to simulate astrophysical fluid flows (primarily, but not exclusively, cosmological …
widely used to simulate astrophysical fluid flows (primarily, but not exclusively, cosmological …
Numerical simulations of internal wave generation by convection in water
Water's density maximum at 4∘ C makes it well suited to study internal gravity wave excitation
by convection: an increasing temperature profile is unstable to convection below 4∘ C, but …
by convection: an increasing temperature profile is unstable to convection below 4∘ C, but …