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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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超新星残骸の殻における高エネルギー粒子加速

F A Aharonian1, A G Akhperjanian, K-M Aye

  • 1Max-Planck-Institut für Kernphysik, PO Box 103980, D 69029 Heidelberg, Germany.

Nature
|November 5, 2004
PubMed
まとめ

超新星残骸 (SNR) は高エネルギー宇宙線の源として確認されています. SNR RX J1713.7-3946の観測は,粒子加速が100TeVを超えることを示し,宇宙線起源の理論を支持しています.

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