Exam 22: Cosmology

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What is the minimum combined energy of the photons that would produce an electron-positron pair? (Note: me is the rest mass of an electron.)

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If dark energy is causing the expansion rate of the universe to increase with time, does this mean that you should worry that the Sun, Earth, and your body itself are expanding? Why or why not?

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Describe two different experiments that offer evidence for a flat universe.

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The figure below shows five graphs of the scale factor of the universe as a function of time.Which of these graphs would occur for a universe with Ω\Omega m =1 and Ω\Omega ⋀\bigwedge = 0?  The figure below shows five graphs of the scale factor of the universe as a function of time.Which of these graphs would occur for a universe with   \Omega  <sub>m</sub> =1 and   \Omega  <sub> \bigwedge </sub>  = 0?

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Which of the following have both been predicted and conclusively confirmed experimentally?

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Which forces would a grand unified theory (GUT) unify?

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Explain what the anthropic principle implies for our visible universe, and give a specific example of a small change that would make life impossible.

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The mechanism of ________ can simultaneously solve both the flatness and horizon problems in cosmology.

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Explain why the Higgs boson is important in the context of the standard model.

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What would the universe be like if there were complete symmetry between matter and antimatter?

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In a closed (spherical) universe, the sum of the angles in a triangle is

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What was the temperature of the universe when photons were no longer able to spontaneously create proton-antiproton pairs? (Note that a photon's energy is equal to What was the temperature of the universe when photons were no longer able to spontaneously create proton-antiproton pairs? (Note that a photon's energy is equal to   , the cosmic background at any point in time has a blackbody spectrum that peaks at a wavelength   , and the mass of a single proton is 1.67*10<sup>-</sup><sup>27</sup> kg.) , the cosmic background at any point in time has a blackbody spectrum that peaks at a wavelength What was the temperature of the universe when photons were no longer able to spontaneously create proton-antiproton pairs? (Note that a photon's energy is equal to   , the cosmic background at any point in time has a blackbody spectrum that peaks at a wavelength   , and the mass of a single proton is 1.67*10<sup>-</sup><sup>27</sup> kg.) , and the mass of a single proton is 1.67*10-27 kg.)

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Summarize the possible shapes of the universe and indicate if the Euclidian geometry is applicable in each case.

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In the 1990s, astronomers studying distant Type Ia supernovae discovered that the

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If the Hubble constant had a value of 50 km/s/Mpc instead of 70 km/s/Mpc, the value of the critical density Ω\Omega 0 would be about

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The figure below shows a graph of the scale factor, RU, with time, for three different scenarios.The age of the universe is the difference between now and the time at which RU is zero.Which curve illustrates a universe that is expanding at a constant rate? The figure below shows a graph of the scale factor, R<sub>U</sub>, with time, for three different scenarios.The age of the universe is the difference between now and the time at which R<sub>U</sub> is zero.Which curve illustrates a universe that is expanding at a constant rate?

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At what temperature would the peak wavelength of blackbody radiation correspond to electron-positron pair production? This would have been the lowest temperature in the early universe at which this effect was common.(Note that a photon's energy is equal to At what temperature would the peak wavelength of blackbody radiation correspond to electron-positron pair production? This would have been the lowest temperature in the early universe at which this effect was common.(Note that a photon's energy is equal to   , the cosmic background at any point in time has a blackbody spectrum that peaks at a wavelength   , and the mass of a single electron or positron is 9.11 *10<sup>-31</sup> kg.) , the cosmic background at any point in time has a blackbody spectrum that peaks at a wavelength At what temperature would the peak wavelength of blackbody radiation correspond to electron-positron pair production? This would have been the lowest temperature in the early universe at which this effect was common.(Note that a photon's energy is equal to   , the cosmic background at any point in time has a blackbody spectrum that peaks at a wavelength   , and the mass of a single electron or positron is 9.11 *10<sup>-31</sup> kg.) , and the mass of a single electron or positron is 9.11 *10-31 kg.)

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Scientists think that, soon after the Big Bang, the four fundamental forces of nature were united into one "superforce," and ________ was the first to split off from the others.

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The figure below shows five graphs of the scale factor of the universe as a function of time.Which of these graphs would occur for a universe with Ω\Omega m = 1 and Ω\Omega ⋀\bigwedge = 0?  The figure below shows five graphs of the scale factor of the universe as a function of time.Which of these graphs would occur for a universe with   \Omega  <sub>m</sub> = 1 and   \Omega  <sub>  \bigwedge </sub>  = 0?

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Even with infinitely powerful telescopes, we can look back in time only until the time when

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