Exam 22: Modern Cosmology

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A grand unified theory unites which forces?

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The observations that show that the expansion of the universe is speeding up tell us the universe must contain:

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Why is the fact that the cosmic microwave background radiation (CMB)is very smooth considered a problem?

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According to superstring theory,how are different varieties of elementary particles similar? How do they differ?

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Which was a triumph of quantum electrodynamics (QED)?

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Which of the following is a FALSE statement about inflation?

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The concept of inflation helps solve both the problems of the flatness of the universe and smoothness of the cosmic background radiation.

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

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If gravity were slowing down the expansion of the universe,how would very distant galaxies differ from nearby galaxies?

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If there were enough mass to slow down the expansion rate of the universe,how would the Hubble constant measured using very distant galaxies be different from what is observed in galaxies that are closer to us? Explain your answer.Is this what we observe in our universe?

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The ratio of the average density in all forms of matter (luminous and dark)in our universe to the critical density is approximately 0.3.

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According to the theory of inflation.when the universe was approximately 1 second old,its size grew by a factor of 1030.

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Why does a unified force split to become two separate forces?

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If Ωmass = 0.5 today and there were no dark energy,the universe would:

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Which of these are possible types of multiple universes that could exist?

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The fact that the currently observed Ωmass + ΩΛ is very close to 1 means that its value has always been very close to 1.

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Why does the critical mass density of the universe depend on the value of Hubble's constant,H0?

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Grand unified theories are very attractive because they can explain:

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Why does the sum of Ωmass and ΩΛ determine the shape of our universe?

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Explain why astronomers cannot accurately model the exact history of the universe in the first few fractions of a second after the Big Bang.

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