Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 25, Problem 35Q

(a)

To determine

The reason due to which the radiation temperature was T0=T(1+z) at the redshift z. Let, T denotes today’s temperature of the cosmic microwave background. It is given that a proton of wavelength λ0 from the cosmic microwave background was emitted at redshift z. Today it’s wavelength is, λ=λ0(1+z).

(b)

To determine

The radiation temperature at z=1, if it is given that a proton of wavelength λ0 from the cosmic microwave background was emitted at redshift z. Today it’s wavelength is, λ=λ0(1+z).

(c)

To determine

The redshift at which the radiation temperature is equal to 293 K, if it is given that a proton of wavelength λ0 from the cosmic microwave background was emitted at redshift z. Today it’s wavelength is, λ=λ0(1+z).

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