Chapter 26: Problem 24
What was the era of recombination? What significant events occurred in the universe during this era? Was the universe matter-dominated or radiation- dominated during this era?
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Chapter 26: Problem 24
What was the era of recombination? What significant events occurred in the universe during this era? Was the universe matter-dominated or radiation- dominated during this era?
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If a photon from the cosmic microwave background had wavelength \(\lambda_{0}\) when it was emitted at redshift \(z\), its wavelength today is \(\lambda=\lambda_{0} /(1+z)\). (a) Let \(T\) be the symbol for the temperature of the cosmic microwave background today. Explain why the radiation temperature was \(T_{0}=T(1+z)\) at redshift \(z\). (b) What was the radiation temperature at \(z=1\) ? (c) At what redshift was the radiation temperature equal to \(293 \mathrm{~K}\) (a typical room temperature)?
How can astronomers measure the average mass density of the universe?
The host galaxy of the supernova HST04Sas (see the image that opens this chapter) has a redshift \(z=1.390\). The light from this galaxy includes the Lyman-alpha \(\left(\mathrm{L}_{\alpha}\right)\) spectral line of hydrogen, with an unshifted wavelength of \(121.6 \mathrm{~nm}\). Calculate the wavelength at which we detect the Lyman-alpha photons from this galaxy. In what part of the electromagnetic spectrum does this wavelength lie?
Can you see the cosmic background radiation with the naked eye? With a visible-light telescope? Explain why or why not.
Imagine an astronomer living in a galaxy a billion light-years away. Is the observable universe for that astronomer the same as for an astronomer on Earth? Why or why not?
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