Document Type
Course
Journal/Book Title/Conference
Physics 3710 – Intermediate Modern Physics, Spring 2018
Publication Date
1-8-2018
First Page
1
Last Page
6
Abstract
The Cosmic Microwave Background (CMB)
As previously noted, the universe is filled with microwave radiation. The frequency spectrum of this ubiquitous radiation follows a blackbody curve, as shown to the right. (http://map.gsfc.nasa.gov/media/ContentMedia/990015b.jpg) Note that photon energy (proportional to 1/wavelength) increases to the right. You might think the curve shown is the plot of a theoretical equation, but what is shown is actual measured data taken during the flight of the COBE (Cosmic Microwave Explorer) satellite/microwave observatory in 1990. The uncertainties in the measurements are about the thickness of the curve plotted. When compared with a theoretical blackbody curve the disagreement is less than one part in 2000. The CMB isn’t LIKE a blackbody spectrum—it IS a blackbody spectrum! Note that the maximum in the CMB spectrum is at a wavelength of about 2 mm. The energy of a photon of that wavelength is E = hc λ 6.6x10–4 eV.
Recommended Citation
Peak, David, "General relativity, 8" (2018). General Relativity. Paper 8.
https://digitalcommons.usu.edu/intermediate_modernphysics_general/8