User profiles for J. S. Oishi
Jeffrey S. OishiBates College Verified email at bates.edu Cited by 5714 |
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 …
yt: A multi-code analysis toolkit for astrophysical simulation data
… To circumvent this limitation, we will be providing a fully integrated GUI for yt written in HTML
and Javascript and served by a webserver running inside yt itself. Rather than a large, bulky …
and Javascript and served by a webserver running inside yt itself. Rather than a large, bulky …
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
Numerical solutions of partial differential equations enable a broad range of scientific research.
The Dedalus project is a flexible, open-source, parallelized computational framework for …
The Dedalus project is a flexible, open-source, parallelized computational framework for …
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 …
Weight loss prior to clinical AIDS as a predictor of survival
…, YD He, DA Hoover, JS Oishi… - JAIDS Journal of …, 1995 - journals.lww.com
In this analysis the aim was to determine the independent effect of moderate to severe weight
loss prior to an AIDS diagnosis on survival after AIDS. The study was conducted as part of …
loss prior to an AIDS diagnosis on survival after AIDS. The study was conducted as part of …