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Imagine being an ant… living in 2D You would understand: left, right, forward, backward, but NOT up/down… How do you know your world is curved? Curvature in 2D…

Curvature in 2D…

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Curvature in 2D…. Imagine being an ant… living in 2D You would understand: left, right, forward, backward, but NOT up/down… How do you know your world is curved?. Curvature in 2D…. Curvature in 2D…. Geodesics. To do geometry, we need a way to measure distances - PowerPoint PPT Presentation

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Page 1: Curvature in 2D…

• Imagine being an ant… living in 2D

• You would understand:

left, right, forward, backward,

but NOT up/down…

• How do you know your world is curved?

Curvature in 2D…

Page 2: Curvature in 2D…

Curvature in 2D…

Page 3: Curvature in 2D…

Curvature in 2D…

Page 4: Curvature in 2D…

Geodesics

• To do geometry, we need a way to measure distances

• In flat space, the shortest distance between P1 and P2 is

a straight line

• In curved space, the ant follows a

• Geodesic: shortest line between P1 and P2

(the fewest possible ant steps)

P1 P2

ant

To the ant, the geodesic is a straight line,

i.e., the ant never has to turn

Page 5: Curvature in 2D…

Curvature and Clocks (time)

I

If both ants walk at constant velocity and leave P1 at the same time, then the ants arrive at point P2 at different times – the top ant gets their “first”. If both ants record the time when they first reach P2 – their clocks are no longer synchronized

Page 6: Curvature in 2D…

E = mc2

• Photons have an energy related mass and are affected by gravity.

• The geometric surface shape of the Universe is determined by the mass distribution

• Photons are therefore constrained to always travel on the surface of the Universe

• Space is flat where there is no mass and curved where there is mass.

Page 7: Curvature in 2D…

Experimental Evidence for GR

• If mass is small / at large distances, curvature is weak

=> Newton’s laws are good approximation

• But: Detailed observations confirm GR

1) Orbital deviations for Mercury (perihelion precession)

Newton: Einstein:

Page 9: Curvature in 2D…

2) Deflection of light

Experimental Evidence for GR

Page 10: Curvature in 2D…

Experimental Evidence for GR

Page 11: Curvature in 2D…

• What happens as the star shrinks / its mass increases? How much can spacetime be distorted by a very massive object?

• Remember: in a Newtonian black hole, the escape speed simply exceeds the speed of light

=> Can gravity warp spacetime to the point where even light cannot escape it’s grip?

That, then, would be a black hole.

Black Holes

Page 12: Curvature in 2D…

Black Holes

Page 13: Curvature in 2D…

• To a stationary oberserver far away, time flow at the critical surface (at RS) is slowed down infinitely.

• Light emitted close to the critical surface is severely red-shifted (the frequency is lower) and at the critical surface, the redshift is infinite.

From inside this region

no informationcan escape red-shifted

red-shifted intooblivion

Black Holes