抜粋
We develop a new numerical code of the multi-energy and multi-angle neutrino-radiation transfer in three dimensions (3D) for core-collapse supernovae. Our 3D code to solve the Boltzmann equations is based on the discretized-ordinate (S N) method with a fully implicit differencing for time advance. A basic set of neutrino reactions is implemented in the collision terms together with a realistic equation of state. By following the time evolution of neutrino distributions in six dimensions (3 spatial and 3 momentum-space) by the 3D Boltzmann solver, we study the 3D feature of neutrino transfer for given background models of supernova cores in order to understand the explosion mechanism through neutrino heating in multi dimensions.
| 元の言語 | English |
|---|---|
| ホスト出版物のタイトル | Death of Massive Stars |
| ホスト出版物のサブタイトル | Supernovae and Gamma-Ray Bursts |
| 編集者 | Peter W. A. San Antonio, Nobuyuki Kawai, Elena Pian |
| ページ | 395-396 |
| ページ数 | 2 |
| エディション | S279 |
| DOI | |
| 出版物ステータス | Published - 2011 4 1 |
出版物シリーズ
| 名前 | Proceedings of the International Astronomical Union |
|---|---|
| 番号 | S279 |
| 巻 | 7 |
| ISSN（印刷物） | 1743-9213 |
| ISSN（電子版） | 1743-9221 |
ASJC Scopus subject areas
- Medicine (miscellaneous)
- Astronomy and Astrophysics
- Nutrition and Dietetics
- Public Health, Environmental and Occupational Health
- Space and Planetary Science
フィンガープリント Numerical code of the neutrino-transfer in three dimensions for core-collapse supernovae' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。
これを引用
Sumiyoshi, K., & Yamada, S. (2011). Numerical code of the neutrino-transfer in three dimensions for core-collapse supernovae. ： P. W. A. San Antonio, N. Kawai, & E. Pian (版), Death of Massive Stars: Supernovae and Gamma-Ray Bursts (S279 版, pp. 395-396). (Proceedings of the International Astronomical Union; 巻数 7, 番号 S279). https://doi.org/10.1017/S1743921312013518