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Updated: May 6, 2026

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中性子星の合併GW170817/SSS17aの光の曲線: rプロセス核合成への影響

M R Drout1, A L Piro2, B J Shappee2,3

  • 1The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA. mdrout@carnegiescience.edu.

Science (New York, N.Y.)
|October 18, 2017
PubMed
まとめ

GW170817のような 二重中性子星の融合により 重元素が生成されます GW170817からの観測された光は,これらの宇宙現象が急速な中性子捕獲 (rプロセス) 核合成に不可欠であることを示しています.

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