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Relativity

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To understand special relativity, you have to accept two basic ideas ... a clock; when the clock receives light from the bulb it starts ticking. ... – PowerPoint PPT presentation

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Title: Relativity


1
Relativity
  • Relativity by M.C. Escher

2
Types
  • Special Relativity Deals with the behavior of
    objects at high speeds (close to the speed of
    light)
  • General Relativity Deals with how mass and
    energy affect space and time

3
Buying In
  • To understand special relativity, you have to
    accept two basic ideas
  • 1 The laws of Physics work the same in all
    inertial reference frames
  • 2 The speed of light has the same value in all
    inertial reference frames

4
Inertial Reference Frames?
  • This is just a fancy way of describing a place
    that isnt pushed around
  • Example A car moving at 60 mph in a straight
    line, but not a car changing speeds

5
Pushing the Issue
  • Why does pushing and pulling matter?
  • Imagine that youre riding in your car and you
    throw a ball into the air
  • If the car is moving at constant speed, the ball
    drops back in your lap
  • If you hit the brakes, the ball goes flying into
    the windshield

6
Weird Stuff in Special Relativity
  • Time-Dilation (the Twin Paradox)
  • Length Contraction
  • Relativistic Quantities (the ever so famous Emc2)

7
Time Dilation
8
Twin Paradox
  • Suppose you have two twins, one of which is
    placed in a ship and rockets away towards a
    nearby start, the other remains on Earth.
  • What will happen when the traveling twin returns?

9
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10
  • The clock in Twin 1s ship physically moves
    slower than Twin 2s clock on Earth
  • This means time is moving slower in the ship than
    on Earth (if Twin 2 could look inside the ship,
    she would see everything happening slower)
  • But Twin 1 still experiences a normal flow of
    time (for her, 1 second might represent a couple
    minutes back on Earth)

11
Time as a Substance?
  • So now were left with a situation in which time
    is no longer just a measurement, completely
    independent from space
  • Time in inevitably linked with space
  • To cope with this, Einstein came up with a
    mathematical construct called space-time, a 4
    dimensional representation of the universe in
    which time and space are combined

12
Length Contraction
  • Proof runs the same as that of time dilation
  • The faster you move, the shorter an object
    appears

13
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14
Applications of This
  • Could you fit a 10ft car in an 8 ft garage?
  • Possibly for a minute, but when the car slows
    down it stretches to its original length and
    either breaks the garage or gets compressed
  • In a relativistic situation, the acceleration is
    where the magic happens (time slows down,
    length contracts)

15
Consequences of This Ideology
  • We are now left with a theory in which two
    people, witnessing two entirely different things,
    can be correct
  • This almost compromises the idea of absolute
    right and wrong what you see and experience
    depends on your reference frame
  • Analogs w/ moral relativity?

16
Mix of Cause and Effect
  • Imagine a situation where you have a light bulb
    triggering a clock when the clock receives light
    from the bulb it starts ticking. Say the clock
    turns on at time (t) 0

17
The clock and bulb are separated by distance x.
B/c light has a finite speed, and observer at
rest will see the clock triggered a time t (x/c)
after the bulb turns on.
18
A Moving Observer
  • Suppose you are an observer flying by at speed v.
    What would you see in this situation?

19
Lorrentz Transforms
  • You can translate between quantities (time,
    distance) in a reference at rest and a moving
    reference frame by using a few equations called
    Lorrentz Transforms

20
  • In the light bulb situation, wed use the
    following equation
  • t g(t (v/c2)x)
  • t is the time measured by the moving observer t
    is at rest observers time
  • x is the distance between the bulb and clock v
    is the moving observers speed
  • g is a factor that increases the faster you go
  • g 1/(1-(v/c)2)1/2

21
  • You can see from this equation that if v and x
    are big enough, t will be negative
  • What does this mean?
  • If you set your light bulb/clock configuration up
    right, you will see the clock turn on before the
    light bulb turns on!

22
  • In this sense, you lose the relationship between
    cause and effect

23
Relativistic Quantities
  • -Einstein Discovered that mass and energy are
    interchangeable, related by the famous
    equation
  • Emc2
  • -Besides simply tweaking our notions of what mass
    and energy really are, there are some other
    consequences of this

24
  • When you speed something up, you have to put
    energy into it
  • But relativity says that nothing can be
    accelerated faster the speed of light
  • So if you have a particle moving very near c,
    what if you keep putting energy into it?

25
  • Quite simply, as an object gets closer to the
    speed of light it gets heavier (gains momentum)

26
Applications of This
  • Nuclear Reactions
  • Particle-Antiparticle Interactions

27
Pair-Antiparticle Pairs
  • Every known particle has an antiparticle
  • It is possible for a photon to give up its energy
    to the formation of a particle-antiparticle pair
  • In a sense, mass and energy are interchangeable
    mass is just concentrated energy

28
Nuclear Reactions
  • When you split or fuse atoms (fission and fusion,
    respectively), you get a mass change in the
    nucleus
  • This is why so much powers involved (according
    to Einsteins equation, even a tiny amount of
    mass can generate a lot of energy b/c c2 is
    such a big number)

29
  • The mass of a nucleus is always less than the sum
    of particle masses
  • This mass loss comes from a difference in
    arrangement of particles in the nucleus (nuclear
    binding energy)
  • In a nuclear reaction, this binding energy is
    released

30
Relativistic Doppler Shifts
  • As an object moves towards you, it has a higher
    frequency/pitch (blue-shifted)
  • As it moves away from you, the frequency is lower
    (red-shifted)

31
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32
Basics of General Relativity
  • A person in a closed box cannot distinguish
    whether or not the box is in a gravitational
    field or is accelerating
  • Einstein proposed that space-time was curved

33
Einsteins Equivalence Principle
  • An observer cannot tell the difference between an
    accelerated reference frame and one in a
    gravitational field

34
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35
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36
  • To an observer at rest to the frame, light
    appears to follow a curved path
  • However, we know light always travels the
    shortest possible path
  • Therefore, the space through which the light is
    moving must be bent
  • I.e, gravitational fields bend space-time

37
Curving of Space-Time
  • Mass and Energy warp space-time
  • Objects move in straight lines through
    space-time, but their paths bent because of the
    curvature of space itself
  • Certain objects are massive enough to infinitely
    curve space (black holes, quasars)

38
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39
  • Massive objects bend the path of light traveling
    by, creating an effect known as gravitational
    lensing

40
Black Holes
41
  • Light is trapped in a black hole (hence the name)
    because of the infinite curvature of space time

42
So Youve Decided to Fall into a Black Hole.
  • Assuming you could survive the many death traps a
    black hole has to offer (jets of intense
    radiation, strong tidal forces that could tear
    you apart, etc), you might witness some pretty
    neat stuff.

43
The Photon Sphere
  • At a certain distance out from a black hole,
    gravity is strong enough to force light emitted
    by your body into a circular orbit
  • In other words, if you looked in front of
    yourself, you would see the back of your head

44
Redshifts/Final Image
45
Event Horizon
46
Once Inside.
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