FIRE-2 simulations: physics versus numerics in galaxy formation
PF Hopkins, A Wetzel, D Kereš… - Monthly Notices of …, 2018 - academic.oup.com
ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …
A new class of accurate, mesh-free hydrodynamic simulation methods
PF Hopkins - Monthly Notices of the Royal Astronomical Society, 2015 - academic.oup.com
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
How to model supernovae in simulations of star and galaxy formation
PF Hopkins, A Wetzel, D Kereš… - Monthly Notices of …, 2018 - academic.oup.com
We study the implementation of mechanical feedback from supernovae (SNe) and stellar
mass loss in galaxy simulations, within the Feedback In Realistic Environments (FIRE) …
mass loss in galaxy simulations, within the Feedback In Realistic Environments (FIRE) …
Numerical relativity in spherical coordinates: A new dynamical spacetime and general relativistic MHD evolution framework for the Einstein Toolkit
We present SphericalNR, a new framework for the publicly available Einstein Toolkit that
numerically solves the Einstein field equations coupled to the equations of general …
numerically solves the Einstein field equations coupled to the equations of general …
White dwarf mergers on adaptive meshes. i. methodology and code verification
ABSTRACT The Type Ia supernova (SN Ia) progenitor problem is one of the most perplexing
and exciting problems in astrophysics, requiring detailed numerical modeling to complement …
and exciting problems in astrophysics, requiring detailed numerical modeling to complement …
Harnessing billions of tasks for a scalable portable hydrodynamic simulation of the merger of two stars
T Heller, BA Lelbach, KA Huck… - … Journal of High …, 2019 - journals.sagepub.com
We present a highly scalable demonstration of a portable asynchronous many-task
programming model and runtime system applied to a grid-based adaptive mesh refinement …
programming model and runtime system applied to a grid-based adaptive mesh refinement …
Handing off the outcome of binary neutron star mergers for accurate and long-term postmerger simulations
We perform binary neutron star (BNS) merger simulations in full dynamical general relativity
with illinoisgrmhd, on a Cartesian grid with adaptive-mesh refinement. After the remnant …
with illinoisgrmhd, on a Cartesian grid with adaptive-mesh refinement. After the remnant …
[PDF][PDF] Introducing Octo-tiger/HPX: Simulating interacting binaries with adaptive mesh refinement and the fast multipole method
Here we present Octo-tiger/HPX, a computer code for simulating self-gravitating
astrophysical fluids. Octo-tiger/HPX is designed to address issues particular to the self …
astrophysical fluids. Octo-tiger/HPX is designed to address issues particular to the self …
[图书][B] White Dwarf Mergers on Adaptive Meshes
MP Katz - 2016 - search.proquest.com
The mergers of binary white dwarf systems are potential progenitors of astrophysical
explosions such as Type Ia supernovae. These white dwarfs can merge either by orbital …
explosions such as Type Ia supernovae. These white dwarfs can merge either by orbital …