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Scattering And Absorption of Light in Planetary Regoliths
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散らばった γ 線 の 背景 は,恒星 を 形成 し て いる 銀河 に 支配 さ れ て いる
Matt A Roth1, Mark R Krumholz2,3, Roland M Crocker2
1Research School of Astronomy and Astrophysics, The Australian National University, Canberra, Australian Capital Territory, Australia. matt.roth@anu.edu.au.
Nature
|September 16, 2021
まとめ
恒星形成銀河だけが 拡散したガンマ線背景を説明します 銀河の宇宙線相互作用によるガンマ線放出を正確に予測する新しい物理モデルが,フェルミ望遠鏡の観測と一致しています.
科学分野:
- 天体物理学
- 宇宙線物理学
- 銀河天文学
背景:
- フェルミ・ガンマ線宇宙望遠鏡は 拡散したガンマ線背景を検出しました
- 過去のモデルでは 活発な銀河核や 恒星を形成する銀河からの貢献を 制限するのに苦労しました
研究 の 目的:
- 恒星形成銀河からのガンマ線放射の物理モデルを開発する.
- 恒星形成の銀河が 同位体ガンマ線背景を 完全に説明できるかどうかを判断する.
主な方法:
- 恒星間介質との宇宙線相互作用によるガンマ線放射の物理モデルを開発した.
- 地元の銀河の観測で モデルを検証した
- 宇宙の星形成銀河群に モデルを適用した
主要な成果:
- 物理モデルは,観測されたガンマ線背景の強度とスペクトルの傾きと正確に一致します.
- 恒星形成の銀河だけで 完全拡散の同位体ガンマ線背景が説明できます
- このモデルは,経験的なスケーリングに依存していません.
結論:
- 星を形成する銀河は,拡散した銀河外ガンマ線背景の主要な寄与者です.
- この研究は,観測されたガンマ線背景について 堅固な物理的な説明を提供します.
- この発見は高エネルギー天体物理学における 長年の疑問を解決しました
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