Exam 22: Modern Cosmology

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

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What are two observations that, when combined, tell us that the universe has Ω\Omega mass + Ω\Omega ∧\wedge = 1 and is flat?

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How does the existence of dark energy affect the expansion of the universe?

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The Big Rip could occur in a universe where the effect of __________ increases with time.

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Which of the following are NOT considered carrier particles used to mediate forces between other particles?

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What is the "flatness problem" in cosmology?

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In the 1990s, astronomers found that distant Type I supernova were __________ than they expected, leading them to conclude that __________.

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Which of these is a restatement of the anthropic principle?

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At what stage in the universe's history do we think the asymmetry between matter and antimatter was created?

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Why does the overall mass and energy density of the universe decide its ultimate fate?

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The universe can be infinite in size for which shapes of the universe?

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What are the names of the two particles that mediate the electromagnetic force in quantum electrodynamics (QED) and the strong force in quantum chromodynamics (QCD)?

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In the superstring theory that successfully unites gravity and quantum mechanics, the universe must have:

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The four fundamental forces of nature are gravity, electromagnetism, the weak force, and the strong force.

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If Ω\Omega mass = 0.5 today and there were no dark energy, the universe would:

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The critical mass density of the universe today is 9.5 *10-27 kg/m3. Using the current observed value of Ω\Omega luminous, what is the average density of protons in the universe? If they were spread evenly throughout the universe, what would be their typical separation? Note that the typical separation between protons would be roughly equal to the cube root of the average volume occupied by one proton, and the mass of a proton is 1.7 * 10-27 kg.

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The weak force mediates the beta decay of neutrons into protons, electrons, and antineutrinos.

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

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The figure below illustrates pair production in the early universe, with one particle labeled with a question mark. The figure below illustrates pair production in the early universe, with one particle labeled with a question mark.   What type of particle must this be? What type of particle must this be?

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