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中性子星の合体GW170817における光学超光の運動測定
Kunal P Mooley1,2, Jay Anderson3, Wenbin Lu4,5,6,7
1Caltech, Pasadena, CA, USA. kunal@astro.caltech.edu.
Nature
|October 12, 2022
まとめ
二重中性子星の融合は 短時間のガンマ線爆発に 関連した相対論的ジェットを作り出します GW170817の新たな分析により ジェット速度の上昇が明らかになり 宇宙現象の理解が深まりました
科学分野:
- 天体物理学
- 高エネルギー天体物理学
- 重力波天文学
背景:
- 二重中性子星の合併GW170817は,構造的相対論ジェットと短いガンマ線爆発とのリンクを証明しました.
- 以前の研究では 放射性VLBIと後照光の曲線を用いて 視角と開口角を制限し ジェットコアの初期ローレンツ因子を測定した.
研究 の 目的:
- ハッブル宇宙望遠鏡の精密天文測定を用いて GW170817の新しい超光速運動測定を報告する.
- ジェット機の翼のローレンツ因子を測定する.
- ジェットコアの初期ローレンツ因子を改善します.
主な方法:
- ハッブル宇宙望遠鏡の精密天文学を用いて
- GW170817に関する以前のVLBIデータと組み合わせたものです.
- 光速の7倍で測定した 超光速の動きを分析する
主要な成果:
- 構造ジェットの翼のローレンツ因子の測定.
- 視角 (19〜25度) の制限を大幅に改善しました.
- ジェットコアの初期ローレンツ因数 (40以上) の制限を大幅に改善した.
結論:
- この研究は,GW170817からの相対論ジェットの構造と性質のより正確な理解を提供します.
- 強化された制約は ニュートロン星の融合における ジェット発射と拡散の物理を 明らかにします
- この研究は 二重中性子星の融合,相対論的ジェット,そして短いガンマ線爆発の間の関連を 洗練している.
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