The "Flash" problem is centered on simulating the accretion of matter onto a compact star, and the subsequent stellar evolution, including nuclear burning either on the surface of the compact star, or in its interior.
- Flash Science Overview
- Science Summary
- Flash Research Groups
- Astrophysics Group
- Basic Physics Group
- Computational Physics and Validation Group
- Computer Science Group
- Flash Code Group
- Visualization Group
- Current Research
- Computational Results Gallery
- FLASH Publications
- FLASH Proceedings and Talks
- FLASH V&V archive
- Popular Science Resources
- Popular science resources
ASC / Alliances Center
