General Relativistic MHD Simulations of the Gravitational Collapse of a Rotating Star with Magnetic Field as a Model of Gamma-Ray Bursts
書誌事項
- タイトル別名
-
- General Relativistic MHD Simulations of the Gravitational Collapse of a Rotating Star with Magnetic Field as a Model of Gamma-Ray Bursts(Poster) :
この論文をさがす
抄録
We have performed 2.5-dimensional general relativistic magnetohydrodynamic (MHD) simulations of collapsars as a model of gamma ray bursts (GRBs). This simulation showed the formation of a disk-like structure and the generation of a mildly relativistic jet (~0.3c). We have found the jet is accelerated by the magnetic pressure and the centrifugal force and is collimated by the pinching force of the toroidal magnetic field amplified by the rotation.
収録刊行物
-
- Progress of Theoretical Physics Supplement
-
Progress of Theoretical Physics Supplement 155 387-388, 2004
Oxford University Press (OUP)
- Tweet
詳細情報 詳細情報について
-
- CRID
- 1360003446877762048
-
- NII論文ID
- 110001216429
- 210000127868
-
- NII書誌ID
- AA00791466
-
- ISSN
- 03759687
-
- データソース種別
-
- Crossref
- NDL-Digital
- CiNii Articles