Background Radiation Quotes (3 quotes)
A possible explanation for the observed excess noise is the one given by Dicke, Peebles, Roll, and Wilkinson (1965) in a companion letter in this issue.
[The low-key announcement of the detection of the cosmic microwave background radiation which is the afterglow of the Big Bang. Co-author with Robert Wilson. They received the 1978 Nobel Prize for their discovery.]
[The low-key announcement of the detection of the cosmic microwave background radiation which is the afterglow of the Big Bang. Co-author with Robert Wilson. They received the 1978 Nobel Prize for their discovery.]
Cosmology is a science which has only a few observable facts to work with. The discovery of the cosmic microwave background radiation added one—the present radiation temperature of the universe. This, however, was a significant increase in our knowledge since it requires a cosmology with a source for the radiation at an early epoch and is a new probe of that epoch. More sensitive measurements of the background radiation in the future will allow us to discover additional facts about the universe.
The most important thing accomplished by the ultimate discovery of the 3° K radiation background (Penzias and Wilson, 1965) was to force all of us to take seriously the idea that there was an early universe.