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Updated: May 11, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses

Published on: July 2, 2012

最も明るく輝く超新星についての説明として,脈動性ペアの不安定性

S E Woosley1, S Blinnikov, Alexander Heger

  • 1Department of Astronomy and Astrophysics, UCSC, Santa Cruz, California 95064, USA. woosley@ucolick.org

Nature
|November 16, 2007
PubMed
まとめ

明るい超新星は,ペアの不安定性を経験している巨大な恒星からの噴出物殻の衝突の結果である. このプロセスは,SN 2006gyのような非常に明るい出来事を説明し,コア崩壊モデルに挑戦します.

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