宇宙微波背景
參考資料

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Kragh, H. . 1999. ISBN 0-691-00546-X. 「在1946年，羅伯特·迪克和他的同事在麻省理工學院測試設備，可以測到強度對應在微波波段20K左右的宇宙微波背景。然而，他們並未提出如此的背景，只說「輻射來自宇宙物質」。此外，這項工作與宇宙學無關，只因1950年被建議而提及，背景輻射的偵測可能技術上可行，也因為迪克的後期發現主導」。參見Dicke, R. H.; et al.. . Physical Review. 1946, 70 (5–6): 340–348. Bibcode:1946PhRv...70..340D. doi:10.1103/PhysRev.70.340.  引文使用过时参数coauthors (帮助)
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↑  Kragh，H. (1999:132).「當他們在1948年報告的值為5 K時，阿爾菲和赫爾曼首先計算了目前脫耦的原始輻射溫度。雖然當時或往後的出版物並未提及該輻射在微波波段，但立即沿用了該溫度...阿爾菲和赫爾曼明確表示，他們已經將早年提及與太陽光完全不同的黑體輻射溫度背景輻射稱為『在宇宙中的溫度』」。
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↑  . Release Number 2014-05. Harvard-Smithsonian Center for Astrophysics. March 17, 2014  [2014-03-18]. （原始内容存档于2014-03-21）. In the first fleeting fraction of a second, the universe expanded exponentially, stretching far beyond the view of our best telescopes. All this, of course, was just theory. Researchers from the BICEP2 collaboration today announced the first direct evidence for this cosmic inflation. Their data also represent the first images of gravitational waves, or ripples in space-time. These waves have been described as the 'first tremors of the Big Bang.' Finally, the data confirm a deep connection between quantum mechanics and general relativity.
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