Chapter 26: Problem 19
How did the abundance of helium in the universe suggest the existence of the cosmic background radiation?
Chapter 26: Problem 19
How did the abundance of helium in the universe suggest the existence of the cosmic background radiation?
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Get started for freeIf 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)?
What is meant by "the observable universe"?
Before the discovery of the cosmic microwave background, it seemed possible that we might be living in a "steady-state universe" with overall properties that do not change with time. The steady-state model, like the Big Bang model, assumes an expanding universe, but does not assume a "creation event." Instead, matter is assumed to be created continuously everywhere in space to ensure that the average density of the universe remains constant. Search the World Wide Web for information about the steady-state theory. Explain why the existence of the cosmic microwave background was a fatal blow to the steady- state theory.
(a) Explain why the radius of the observable universe is continually increasing. (b) Although the universe is \(13.7\) billion years old, the observable universe includes objects that are more than \(13.7\) billion light- years away from Earth. Explain why.
What is a cosmological constant? Why did Einstein introduce it into cosmology?
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