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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
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GRB03032929の熱計から推論された宇宙爆発の共通の起源
E Berger1, S R Kulkarni, G Pooley
1Caltech Optical Observatories 105-24, California Institute of Technology, Pasadena, California 91125, USA. ejb@astro.caltech.edu
Nature
|November 14, 2003
まとめ
この研究は,ガンマ線爆発 (GRBs) が二つの爆発成分を持っていることを明らかにしています. 狭いジェットがガンマ線を生成し,より広いアウトフローが総エネルギーを支配し,変数GRBエネルギーを説明します.
科学分野:
- 天体物理学 天体物理学
- 宇宙の爆発,宇宙の爆発.
- ガンマ線爆発の研究
背景:
- 長期ガンマ線爆発 (GRB) は,標準的なエネルギー出力を有すると考えられていた.
- GRB980425のようなサブエネルギー GRBは,この標準モデルに挑戦します.
- GRB980425は超新星SN1998bw.と関連していた.
研究 の 目的:
- ラジオ観測を用いてGRB030329爆発の熱測定を行う.
- GRB爆発におけるエネルギー分布を調査するために.
- GRBと超新星との関係を理解するために.
主な方法:
- GRB030329.9のラジオ観測について
- 爆発エネルギーを測定する熱計.
- 射出成分とその相対論的性質の分析.
主要な成果:
- GRB030329は2つの構成要素の爆発を示した.
- 狭い,超相対論的成分は,ガンマ線と初期の後光を生成した.
- 幅広く,わずかに相対論的なコンポーネントは,後の無線と光学的後光を生成しました.
結論:
- GRBで放出されるエネルギーの総量は,他の宇宙爆発と比較できます.
- ガンマ線放射は,爆発の総エネルギーと比較してエネルギー的に小さい.
- 宇宙爆発には共通の起源があるが,高速噴出物のエネルギーには大きな違いがある.
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