Published March 21, 2006
| Version v1
Journal article
Numerical simulations of core-collapse supernovae imposing steady shock approximation
- 1. Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555 (Japan)
- 2. Department of Astronomy, Faculty of Science, Kyoto University, Oiwaki-cho, Sakyou-ku, Kyoto 606-8502 (Japan)
- 3. Faculty of Science and Technology, Tokyo University of Science, Yamazaki 2641, Noda, Chiba 278-8510 (Japan)
- 4. Advanced Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555 (Japan)
Description
We carried out one-dimensional long-term numerical simulations of core-collapse supernovae imposing steady shock approximation. As a result of a computation, we found core does not explode and shock wave stalls within several hundreds milliseconds from bounce. However, we execute long-term numerical simulation until 3.5 seconds from bounce with short CPU time using Personal Computer
Availability note (English)
Available online at http://stacks.iop.org/1742-6596/31/155/jpconf6_31_030.pdf or at the Web site for the Journal of Physics. Conference Series (Online) (ISSN 1742-6596) http://www.iop.org/Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 31
- Journal Issue
- 1
- Journal Page Range
- p. 155-156
- ISSN
- 1742-6596
Conference
- Title
- 3. 21COE symposium on astrophysics as interdisciplinary science
- Dates
- 1-3 Sep 2005
- Place
- Tokyo (Japan)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37058982
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- APPROXIMATIONS; COSMOLOGY; SHOCK WAVES; SIMULATION; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; CALCULATION METHODS; ERUPTIVE VARIABLE STARS; STARS; VARIABLE STARS