Exam 18: Modern Cosmology

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The cosmological redshifts of galaxies are Doppler shifts.

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Olber's paradox is explained by the fact that the Universe is neither static nor infinite in age.

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The cosmic microwave background radiation comes from the time when neutral hydrogen atoms formed in the process of _______________.

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  Figure 18-12 (for the following questions) One year after the big bang, the temperature of the Universe was approximately____ degrees Kelvin. Figure 18-12 (for the following questions) One year after the big bang, the temperature of the Universe was approximately____ degrees Kelvin.

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Scientists who study the Universe as a whole are called _______________.

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How did dark matter behave differently from normal matter during the early stages of the big bang, and how is this important for the formation of stars and galaxies?

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The observed distribution of matter in the Universe is best understood as being caused by ____.

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  Figure 18-12 (for the following questions) The re-ionization of the Universe occurredclosest to ____ degrees Kelvin. Figure 18-12 (for the following questions) The re-ionization of the Universe occurredclosest to ____ degrees Kelvin.

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After nuclear reactions in the big bang had ended, about 25% of the mass of the Universe was in the form of helium nuclei.

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In the early universe, the electromagnetic and strong nuclear forces were joined together to make the electrostrong force.

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The big bang happened everywhere in the Universe at the same time.

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The "big bang" was an explosion of material that created galaxies flying away from the center of the explosion.

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The density of the Universe comes from baryonic matter, non-baryonic dark matter, and dark energy. What percentage of the density of the Universe do each of the three represent?

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The cosmological principle states that any observer in any galaxy sees the same general properties for the Universe.

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The big bang only created hydrogen and helium (with miniscule amounts of lithium) because____.

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  Figure 18-12 (for the following questions) The change from a radiation-dominated to a matter-dominated Universe occurred at a temperature closest to ____ of degrees Kelvin. Figure 18-12 (for the following questions) The change from a radiation-dominated to a matter-dominated Universe occurred at a temperature closest to ____ of degrees Kelvin.

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Modern observations have shown that the geometry of the Universe is ____.

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  Figure 18-12 (for the following questions) The Universe had a temperature of a few hundred million degrees K at approximately ____ after the big bang. Figure 18-12 (for the following questions) The Universe had a temperature of a few hundred million degrees K at approximately ____ after the big bang.

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The Universe is isotropic, but not homogenous.

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During one phase of the big bang, gamma ray photons were creating electrons and positrons (anti-electrons). At this time, the Universe also contained ____.

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