恒星 の 元素 の 豊富 度 は,ウラン より 重い 原子 核 の 分裂 を 示し て い ます
Ian U Roederer1, Nicole Vassh2, Erika M Holmbeck3
1Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA.
まとめ
急速な中性子捕獲プロセス (rプロセス) で重元素が生成される. この研究では,トランスウラン原子核からの分裂断片が元素の豊富さに寄与し,質量数260を超える中性子に富んだ原子核がrプロセスで生成されることを示唆している.
科学分野:
- 核天体物理学
- 宇宙化学
背景:
- 最も重い元素は,中性子星の融合のようなエネルギーに満ちた宇宙現象で,急速な中性子捕獲プロセス (rプロセス) によって形成される.
- 実験的な限界のために,ウランより重い元素 (トランスウラン核) の r-プロセス生成を理解することは困難であり,理論的な核合成モデルに頼る必要がある.
研究 の 目的:
- 超ウラン核の分裂断片が,恒星におけるrプロセス元素の観測値に与える影響を調査する.
- 分裂断片の貢献の証拠として役立つ特定の元素の豊富さの相関を特定する.
主な方法:
- rプロセス元素で濃縮された恒星における元素の豊富さの分析.
- 特定の質量と原子番号の範囲に焦点を当てた元素の豊富さの統計的相関分析.
主要な成果:
- ルテニウム,ロジウム,パラジウム,銀 (Z=44-47) とより重い元素 (Z=63-78) の豊富さとの間に有意な相関が発見された.
- 隣接する元素 (Z=34−42,Z=48−62) の場合,そのような相関は観察されなかった.
- これらの相関は,トランスウラン核からの分裂断片がrプロセス核合成において役割を果たすという仮説を支持する.
結論:
- 観測された豊富なパターンは,トランスウラン原子核からの分裂断片のrプロセス元素の在庫への貢献の証拠を提供します.
- この発見は,260を超える質量を持つ中性子に富んだ原子核が,rプロセスで合成されていることを示している.
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