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Updated: May 6, 2026

1,3,5-Triphenylbenzene and Corannulene as Electron Receptors for Lithium Solvated Electron Solutions
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低金属性の小マゲラン雲の星間リチウムの観測

J Christopher Howk1, Nicolas Lehner, Brian D Fields

  • 1Department of Physics, Center for Astrophysics, University of Notre Dame, Notre Dame, Indiana 46556, USA. jhowk@nd.edu

Nature
|September 8, 2012
PubMed
まとめ

ビッグバン核合成 (BBN) 理論は,恒星で観測されるよりも高いリチウム-7の豊富さを予測しています. 小さなマゲラン雲の測定結果は,BBNの予測と一致しており,恒星の過程がリチウムレベルを変化させる可能性があることを示唆しています.

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