The redshifted radiation from the Big Bang which is observed to be nearly isotropic.It was first unambiguously detected by Penzias(1979) and Robert Wilson(1979) in the microwave at a brightness temperatureof
K.However, evidence for a 3 K background had been seen in the optical and submillimeter by noting excitation of CN rotation states at 3874 Å and 1.32 mm.The temperature require to produce the observed excitation was
K. The COBE satellite measured the temperature to be 2.735 K ± 12
K, with variations of ± 30
K.
The temperature of the CBR as time progresses can be computed starting from the equation of free-streaming photons,







Therefore, if the spectrum starts out as a blackbody spectrum, it will remain a blackbody spectrum, but will have temperature with

entropy is also conserved. Let a be the Stefan-Boltzmann constant.



If the pressure is small,
, so











The temperature of the CBR as time progresses can be computed starting from the equation of free-streaming photons,

(1)

(2)

(3)

(4)

(5)

(6)

(7)
Therefore, if the spectrum starts out as a blackbody spectrum, it will remain a blackbody spectrum, but will have temperature with

(8)
entropy is also conserved. Let a be the Stefan-Boltzmann constant.

(9)

(10)

(11)
If the pressure is small,


(12)

(13)

(14)

(15)

(16)

(17)

(18)
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