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General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30...

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General Relativity Jeopardy Equivalence Principle Spacetime Diagrams Black Holes Curved Space 10 10 10 10 20 20 20 20 30 30 30 30 40 40 40 40
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Page 1: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

General Relativity Jeopardy

Equivalence Principle

Spacetime Diagrams Black Holes Curved Space

10 10 10 10

20 20 20 20

30 30 30 30

40 40 40 40

Page 2: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

The effects of gravity are exactly equivalent to the effects of acceleration.

Page 3: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

Rocket ship on the left is floating free in space; one on the right is accelerating at 1 g. The person on the right feels this.

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Page 4: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

The reason the person on the left feels weightless.

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Page 5: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

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Page 6: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.
Page 7: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.
Page 8: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.
Page 9: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.
Page 10: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

According to general relativity, a black hole is this.

Page 11: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

We would see a strong gravitational redshift of light near a black hole because of this running more slowly.

Page 12: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.
Page 13: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

This happens to you well before you even reach the event horizon.

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Page 14: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

One way we can get more bending in spacetime.

Page 15: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

The explanation for the Einstein cross.

Page 16: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

The speed at which gravitywaves travel.

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Page 17: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

One of the goals of GravityProbe B was to measure this.

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Page 18: General Relativity Jeopardy Equivalence Principle Spacetime DiagramsBlack HolesCurved Space 10 20 30 40.

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