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General Relativity: Part II

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Title: General Relativity: Part II


1
General Relativity Part II
  • Gravity is Curved Space

2
  • 1) You walk 10 km south, 10 km west and then 10
    km north and you are back where you started.
  • What colour is the bear?
  • a) brown b) black c) white

Hint There is only one place in the world where
this would happen.
3
  • We live in a 4-dimensional curved space which we
    cannot see or experience directly.
  • We can get a sense of how it works by using an
    analogy with fewer dimensions.

4
  • Imagine that you are a smart blind ant moving
    about on the surface of a balloon. Draw the path
    of the polar explorer from the the riddle on your
    balloon.
  •  

5
  • 2) Suppose that there is a light at the North
    Pole. The light radiates in all directions and
    follows the straightest lines in this space. What
    will an ant at the South Pole notice?
  • a)      Nothing.
  • b)      A bright spot.
  • c)      A bright ring.
  •  

6
The curved arcs that you see in this photograph
are coming from a distant light. Between it and
the Earth there is a large mass that warps the
space, so that light appears to come from many
directions.
7
  • We can detect how mass distorts the three
    dimensions of space but we cant picture it.

4) How would an ant explain this motion?
8
  • When Einstein first calculated the curvature of
    light he got it wrong by a factor of two. Half
    the curvature is from the equivalence principle
    and the second half is from the curvature of
    space.

9
  • Mass curves spacetime into gravitational lenses.

10
  • Gravitational lenses are used by astronomers to
    measure the mass of regular matter and dark
    matter.

11
  • Draw a 15-cm line on your balloon. At right
    angles to that, draw another 15-cm line. Draw two
    more of them. What do you get?

12
  • Planetary orbits dont form simple ellipses
    either. They form patterns like Daisy petals -
    this is called the precession of the equinoxes.
    This was a known problem with Newtonian
    Gravitation that General Relativity was able to
    solve.

13
  • 5) The planet with the greatest precession will
    be
  • a)      Jupiter because it is biggest
  • b)      Mercury because it is smallest
  • c)      Mercury because it is closest to the
    sun
  • d)      Neptune because it is farthest

14
  • Suppose, the balloon was expanding.
  • What would the ant notice?

15
The galaxies are all moving away from us and the
more distant ones are moving faster.
16
  • There is a simple relationship between velocity
    and distance. This suggests that everything in
    the universe was once gathered in one point that
    exploded around 14 billion years ago the Big
    Bang.


17
  • 6) Gravity should cause this expansion to
  • a) slow down b) speed up c) remain constant.


Best-fit
Constant velocity
18
  • 7)As a stars life ends, it collapses and gets
    much denser. What would you see if you got close
    to dense star whose escape velocity was almost c?
  • a) Light rising and falling
  • b) Faint radio waves
  • c) Faint gamma rays

19
  • 8) What happens if the escape velocity is
    greater than c?
  • a) only gamma rays escape
  • b) only radio waves escape
  • c) nothing escapes
  • d) nothing escapes so it cant be detected

20
  • You can detect one by the way it warps light.

21
  • You can detect black holes that have matter
    spiraling into them. This matter will form hot
    disks that give off x-rays.

22
  • Black Holes often produce jets spewing matter
    out at speeds close to c. Many of these have been
    found.

23
Black holes can also be detected by measuring
the speeds of orbiting bodies. This data can be
used to calculate the mass and density of the
central body.
M v2 r /G
24
  • What is it like inside a Black Hole? All light
    and matter will be driven by the extremely curved
    spacetime into a singularity of infinite density.

25
  • Rapidly orbiting massive objects should generate
    gravitational waves, ripples in the fabric of
    space.
  • These waves take energy away, so the objects
    should spiral into the center.

26
  • Taylor and Hulse have measured a binary pulsar
    doing exactly that.

27
  • Large detectors are being built around the world
    to detect gravitational waves directly.
  • This is LIGO.

28
  • An even larger gravity detector called LISA, is
    being built. It is made of three satellites in a
    huge triangle. It may be able to measure the
    curvature near a Black Hole.
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