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空中平均スペクトルの78メガヘルツを中心とした吸収プロファイル
Judd D Bowman1, Alan E E Rogers2, Raul A Monsalve1,3,4
1School of Earth and Space Exploration, Arizona State University, Tempe, Arizona 85287, USA.
Nature
|March 2, 2018
まとめ
科学者は初期の恒星が 原始的な水素ガスと 相互作用するラジオ信号の 歪みを検出しました シグナル
科学分野:
- 宇宙学
- 天体物理学
- ラジオ天文学
背景:
- 初期の星は紫外線を放ち 原始的な水素ガスに影響を与えました
- この相互作用は観測可能な電波スペクトルの歪みを生み出すと予想されていた.
研究 の 目的:
- 初期の宇宙の星によって引き起こされたスペクトルの歪みを検出し分析する.
- 観測された信号と理論的な予測の間の不一致を調査する.
主な方法:
- 200メガヘルツ未満の周波数で天空平均のラジオスペクトルの観測.
- 78メガヘルツを中心に検出された吸収プロフィールの分析
主要な成果:
- 特定の周波数と振幅の特徴を持つ平らな吸収プロファイルの検出.
- 観測された振幅は,標準的な天体物理モデルによって予測されたより大幅に高かった.
結論:
- この差異は 原始的なガスが冷たいか 背景放射が熱いかのどちらかを示唆しています
- ダークマター-バリオン相互作用は観測された信号幅の潜在的な説明です.
- ビッグバンから1億8千万年後の初期恒星形成とライマンα光子の背景の証拠
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