SpaceBear
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What's the bandwidth of CMB and what was the bandwidth of CMB when it was emitted (at the moment when the Universe was 379,000 years old)?
The Cosmic Microwave Background (CMB) radiation exhibits a spectrum closely resembling a black body with a temperature of approximately 2.73 K. The peak spectral density occurs at a frequency of 160.2 GHz, corresponding to a wavelength of 1.873 mm, while an alternative definition places the peak at 283 GHz (1.06 mm). The CMB does not have sharp upper and lower frequency limits, but its bandwidth can be approximated by analyzing the Planck function and determining the frequency range where the output is at 1/10 of the peak. This discussion emphasizes the CMB's near-perfect black body characteristics and its implications for understanding cosmic radiation.
PREREQUISITESAstronomers, physicists, and students interested in cosmology, particularly those studying the properties and implications of the Cosmic Microwave Background radiation.
Mordred said:Marcus I'm not sure I would call the CMB a perfect blackbody. A perfect blackbody had total absorbsion of all wavelengths from zero to infinity
Mordred said:Perhaps I am misunderstanding in how one defines a blackbody as opposed to a transparent, grey, colored etc body.
This is a subject covered in an article that I have been recently studying
http://books.google.ca/books?id=IIIVHRirRgEC&pg=PA386&redir_esc=y#v=onepage&q&f=false
I linked the section of the textbook at the descripive.
I would be interested in what is the mainstay definition of what defines a perfect blackbody in regards or opposition of the related link.
negativzero said:Could you make a lens with a diffraction grating and focus the microwave energy?
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Could you make a lens with a diffraction grating and focus the microwave energy?
Is there a practical way to soak up energy from the background?