E V Vikhrov1, B B Zelener1, B V Zelener1

  • 1Joint Institute for High Temperatures, of the Russian Academy of Sciences, Izhorskaya Street 13, Building 2, Moscow 125412, Russia.

Physical review. E
|January 21, 2026
PubMed
まとめ

超冷キセノンプラズマのシミュレーションにより、雲の分裂とビーム形成という2つの電子損失経路が明らかになった。ディオコトロン不安定性の影響を受ける電子ビームは、一定速度でドリフトする。これらの発見は、電子顕微鏡への応用につながる可能性がある。

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