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[HTML][HTML] DYAMOND: the DYnamics of the Atmospheric general circulation Modeled On Non-hydrostatic Domains
A review of the experimental protocol and motivation for DYAMOND, the first
intercomparison project of global storm-resolving models, is presented. Nine models …
intercomparison project of global storm-resolving models, is presented. Nine models …
Vlasov methods in space physics and astrophysics
M Palmroth, U Ganse, Y Pfau-Kempf… - Living reviews in …, 2018 - Springer
This paper reviews Vlasov-based numerical methods used to model plasma in space
physics and astrophysics. Plasma consists of collectively behaving charged particles that …
physics and astrophysics. Plasma consists of collectively behaving charged particles that …
Binary neutron star mergers: mass ejection, electromagnetic counterparts, and nucleosynthesis
D Radice, A Perego, K Hotokezaka… - The Astrophysical …, 2018 - iopscience.iop.org
We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …
Self-consistent 3D supernova models from− 7 minutes to+ 7 s: A 1-bethe explosion of A∼ 19 M⊙ progenitor
R Bollig, N Yadav, D Kresse, HT Janka… - The Astrophysical …, 2021 - iopscience.iop.org
To date, modern three-dimensional (3D) supernova (SN) simulations have not demonstrated
that explosion energies of 10 51 erg (= 1 bethe= 1 B) or more are possible for neutrino …
that explosion energies of 10 51 erg (= 1 bethe= 1 B) or more are possible for neutrino …
Exploring fundamentally three-dimensional phenomena in high-fidelity simulations of core-collapse supernovae
EP O'Connor, SM Couch - The Astrophysical Journal, 2018 - iopscience.iop.org
The details of the physical mechanism that drives core-collapse supernovae (CCSNe)
remain uncertain. While there is an emerging consensus on the qualitative outcome of …
remain uncertain. While there is an emerging consensus on the qualitative outcome of …
A magnetar engine for short GRBs and kilonovae
We investigate the influence of magnetic fields on the evolution of binary neutron star (BNS)
merger remnants via three-dimensional (3D) dynamical-spacetime general-relativistic …
merger remnants via three-dimensional (3D) dynamical-spacetime general-relativistic …
Three-dimensional models of core-collapse supernovae from low-mass progenitors with implications for Crab
G Stockinger, HT Janka, D Kresse… - Monthly Notices of …, 2020 - academic.oup.com
We present 3D full-sphere supernova simulations of non-rotating low-mass (∼ 9 M⊙)
progenitors, covering the entire evolution from core collapse through bounce and shock …
progenitors, covering the entire evolution from core collapse through bounce and shock …
VisIt: An end-user tool for visualizing and analyzing very large data
VisIt is a popular open source tool for visualizing and analyzing data. It owes its success to
its foci of increasing data understanding, large data support, and providing a robust and …
its foci of increasing data understanding, large data support, and providing a robust and …
Numerical simulations of multiphase winds and fountains from star-forming galactic disks. I. Solar neighborhood TIGRESS model
CG Kim, EC Ostriker - The Astrophysical Journal, 2018 - iopscience.iop.org
Gas blown away from galactic disks by supernova (SN) feedback plays a key role in galaxy
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
In Situ Methods, Infrastructures, and Applications on High Performance Computing Platforms
The considerable interest in the high performance computing (HPC) community regarding
analyzing and visualization data without first writing to disk, ie, in situ processing, is due to …
analyzing and visualization data without first writing to disk, ie, in situ processing, is due to …