LEARNING GOALS -- At the conclusion of this part of the unit, I will be able to:
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explain our 'critical' time periods after the Big Bang in appropriate scientific phrasing:
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Planck Time (10-43 sec): When time/space began-- infinitely hot, infinitely dense, infinitely small
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Inflation (10-37 - 10-32 sec): The Universe abruptly expands MUCH more rapidly than in the periods before and after
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CMBR Created (380,000 years) Atomic nuclei capture electrons to form atoms. Light is free to roam!
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First Stars/Galaxies (~1 Billion years)
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relate the idea of 'heat death' and The Big Freeze and why that is the leading current theory for the fate of the Universe
- Open
- Shape: Saddle (hyperbolic)
- Expands forever, gets very dark, very cold, very empty
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relate the idea of "The Modified Big Freeze" and why that is so similar to the Big Freeze theory for the fate of the Universe
- Flat/disk shaped
- perfect amount of mass to stop expansion
- cools off, just like the Big Freeze but without expanding
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relate the idea of "The Big Crunch" and why that is a mostly discredited theory for the fate of the Universe
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relate the idea of "The Big Rip" and why that is controversial theory for the fate of the Universe
- put into context the unimaginable time scales involved in the fate of the Universe.
Radiation Era
Star Era
Degenerate Era*
Black Hole Era*
Dark Era*
* Infinite Time
7. Comment on ideas developed in our readings "The Last Question", "How the Universe Will End" and the "End of the Universe" video
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