Published June 1, 2007
| Version v1
Miscellaneous
MHD Models of Stellar Core Collapse with GenASiS
Creators
- 1. Oak Ridge National Lab., Oak Ridge, TN (United States)
- 2. University of Tennessee (United States)
Description
We present magnetohydrodynamic (MHD) models of stellar core collapse computed with our astrophysical MHD code GenASiS. Microphysics in the models include a realistic equation of state and a simple parameterization of deleptonization during collapse. We give a brief description of some numerical results, and discuss requirements for capturing the physics of the magnetorotational instability in the context of core collapse supernovae
Availability note (English)
Available from Oak Ridge National Laboratory (US)Additional details
Publishing Information
- Imprint Pagination
- vp.
Conference
- Title
- Scientific Discovery through Advanced Computing
- Acronym
- SciDAC 2007
- Dates
- 25-28 Jun 2007
- Place
- Boston, MA (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 40013758
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Resource subtype / Literary indicator
- Conference, Non-conventional Literature
- Descriptors DEI
- COMPUTERIZED SIMULATION; INSTABILITY; MAGNETOHYDRODYNAMICS; PHYSICS; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; ERUPTIVE VARIABLE STARS; FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; SIMULATION; STARS; VARIABLE STARS
Optional Information
- Contract/Grant/Project number
- KB0301020; ERKBP05; AC05-00OR22725
- Notes
- article 012016
- Funding organization
- SC USDOE - Office of Science (Seychelles) (US)
- Secondary number(s)
- ORNL/PTS--7025