Exam 21: Modern Cosmology

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

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D

To determine how the expansion rate of the universe has changed over time,astronomers must measure __________ for a sample of Type I supernovae in distant galaxies.

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Grand unified theories are very attractive because they can explain

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

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If the sum of the mass and energy density in the universe yields If the sum of the mass and energy density in the universe yields   then the universe will recollapse in a Big Crunch. then the universe will recollapse in a Big Crunch.

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Is Einstein's "biggest blunder" still considered a mistake?

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Inflation happened

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What is the name of the particle that mediates the electromagnetic force in quantum electrodynamics (QED)and the strong force in quantum chromodynamics (QCD)?

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

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As the universe cooled shortly after the Big Bang,which was the first fundamental force to separate itself out from the others?

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Astronomers have confirmed the grand unified theory by observing that protons decay in laboratory experiments.

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If you found a globular cluster that had an age of 20 billion years,what cosmological observations would conflict with this observation?

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

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What are two observations that when combined tell us that the universe has What are two observations that when combined tell us that the universe has   and is flat? and is flat?

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

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The standard model of particle physics is incomplete because it leaves which question(s)unanswered?

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What was the temperature of the universe when a typical CBR photon was no longer able to spontaneously create an electron and positron pair? Note that a photon has an energy equal to What was the temperature of the universe when a typical CBR photon was no longer able to spontaneously create an electron and positron pair? Note that a photon has an energy equal to   the CBR at any point in time has a blackbody spectrum that peaks at   ,and the mass of a single electron is   . the CBR at any point in time has a blackbody spectrum that peaks at What was the temperature of the universe when a typical CBR photon was no longer able to spontaneously create an electron and positron pair? Note that a photon has an energy equal to   the CBR at any point in time has a blackbody spectrum that peaks at   ,and the mass of a single electron is   . ,and the mass of a single electron is What was the temperature of the universe when a typical CBR photon was no longer able to spontaneously create an electron and positron pair? Note that a photon has an energy equal to   the CBR at any point in time has a blackbody spectrum that peaks at   ,and the mass of a single electron is   . .

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

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

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