microwave background radiation

基本解釋

The glow of cosmic microwave background radiation, which is found throughout the universe, is thought to be a tangible remnant of leftover light from the big bang.
在整個宇宙中都能觀測到的宇宙微波背景輻射的余暉被認為是大爆炸產生的光芒的可感知的余燼。
The theory of the big bang gained widespread support in the scientific community after Arno Penzias and Robert Wilson discovered cosmic microwave background radiation in 1965.
阿爾諾·彭齊亞斯和羅伯特·威爾遜在1965年發(fā)現了宇宙微波背景輻射，這使得大爆炸理論在科學界獲得了廣泛支持。
It was awarded for the discovery of the blackbody spectrum and anisotropy of the cosmic microwave background radiation which strongly supports the big bang theory of cosmology.
這個獎授予宇宙微波背景輻射的黑體譜形和各向異性的發(fā)現，強有力地支持了大爆炸宇宙學。

In 1966 Kenneth Greisen, Vadim Kuzmin and Georgiy Zatsepin showed that high-energy charged particles (cosmic rays are mostly atomic nuclei, and thus positively charged) should be slowed by collisions with the photons of the cosmic microwave background (radiation left over from the Big Bang that permeates all space).
ECONOMIST: Cosmic rays: They came from outer space The