Exam 22: Cosmology

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Explain why inflation could lead to an infinite number of multiverses inside our own universe.Are they likely to be similar to or different from our own universe?

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The universe can be infinite in size for which large-scale geometries?

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What is basis for the idea of multiverses, and what evidence is there for the existence of multiverses?

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Why is the smoothness of the cosmic microwave background radiation (CMB) considered a problem?

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Compared to an electron, the antiparticle of an electron has

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In the very early universe, which of the following types of particles and antiparticles first stopped being spontaneously formed out of photons and why?

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In a universe dominated by an accelerated expansion rate, the actual age of the universe is ________ the Hubble time.

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Imagine that you lived in a universe where there is enough mass to slow the expansion rate of the universe.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.

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The flatness problem arises because only a universe with a value of ________ can have that value forever and also contain matter.

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In some particle physics theories, the universe must have more than three spatial dimensions, but we experience only three.Why would we not see the other spatial dimensions?

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String theory is

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In a universe with no dark energy, what will happen to the expansion of the universe in the future if (a) Ω\Omega m >\gt 1, (b) Ω\Omega m =1, and (c) Ω\Omega m <\lt 1?

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Which of the fundamental forces in nature have an infinite range of action?

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In the string theory that could successfully unite gravity and quantum mechanics, the universe must have

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Why does inflation not violate the fundamental rule that nothing can travel through space faster than the speed of light?

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What would be the eventual state of the universe if the mass density Ω\Omega = Ω\Omega 0, and dark energy did not exist?

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Which of the curves in the figure shown below would best describe the scenario of a Big Rip for the universe? Which of the curves in the figure shown below would best describe the scenario of a Big Rip for the universe?

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What is the "flatness problem" in cosmology?

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How does the critical density, ρ\rho c, depend on the observed value of the Hubble constant, H0?

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Which list correctly orders objects from the first one to form after the Big Bang to the last one to form?

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