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Special Relativity

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Special Relativity David Berman Queen Mary College ... Einstein In 1905, while working as a patent office clerk in Bern, published his work on special relativity. – PowerPoint PPT presentation

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Title: Special Relativity


1
Special Relativity
  • David Berman
  • Queen Mary College
  • University of London

2
Symmetries in physics
  • The key to understanding the laws of nature is
    to determine what things can depend on.
  • For example, the force of attraction between
    opposite charges will depend on how far apart
    they are. Yet to describe how far apart they are
    I need to use some coordinates to describe where
    the charges are. The coordinate system I use
    CANNOT matter.

3
Symmetries in physics
  • Lets use Cartesian coordinates.
  • Object 1 is distance x1 along the x-axis and
    distance y1 along the y-axis
  • Object 2 is distance x2 along the x-axis and
    distance y2 along the y-axis
  • The distance squared between the two objects will
    be given by

4
Symmetries in physics
  • The force is inversely proportional to the
    distance squared.
  • What transformations can we do that will
    leave the distance unchanged?
  • Translation

5
Symmetries in physics
  • Rotations

6
Symmetries in physics
  • We can carry out the transformations described of
    translations and rotations and yet the physical
    quantity which is the distance between the two
    charges remains the same.
  • That is a symmetry. We carry out a transformation
    and yet the object upon which the transformation
    takes place remains the same or is left
    invariant.

7
Symmetries in physics
  • The important quantities in physics are those
    that are invariants. That is the things that
    dont transform.
  • Other things will change under transformations
    and so will depend typically on our choice of
    description, for example which way we are facing.

8
Space and Time
  • We live in both space and time. There are the
    usual three dimensions of space we are used to
    and also one more of time. We perceive time as
    being very different to space though.
  • How different is it really?
  • To arrange a meeting I need to specify a time
    and a place. I can describe the place by using
    some coordinates and the time by specifying the
    hour of the day (thats just a time coordinate).

9
Space and Time
  • Distances in space can given as we have shown.
  • Distances in time would also be given by the
    difference of the two times that is

10
Space and Time
  • How do we add up distances in different
    directions?
  • Weve already seen that it is NOT just the sum of
    the distances in the different directions rather
    the total distance is given by

11
Space and Time
  • How do we find the distance in space-time. That
    is given the distance in space and the distance
    in time how can we combine them to give the total
    distance in space-time?
  • Wrong guess

12
Space and Time
  • Einstein had a better idea.
  • He combined space and time found the right way to
    describe distances in spacetime.

13
Einstein
  • In 1905, while working as a patent office clerk
    in Bern, published his work on special
    relativity. His insights in that paper were
    essentially that space and time should be
    combined in one thing, spacetime. He also
    realised the right way to construct invariant
    distances in spacetime.
  • The same year he also published two other key
    papers in other areas of physics. It really was
    an enormous break through year for Einstein.

14
Spacetime
  • The distance in spacetime is given by

15
Spacetime
  • When we measure distances we use the same units
    for x and y. If we didnt then we could convert
    between units in the distance formula like so
  • With w the ratio of the two different units.
  • Instead we pick w1 and use the same units
    for our x and y distances.

16
Spacetime
  • For spacetime, what is the choice of units of
    time that will set w1 and give us the equivalent
    unit for time as for space?
  • If we measure space in meters then we should
    measure time in light meters. (More about this
    later).

17
Spacetime
  • Given that the distance in spacetime is given by
  • What are the transformations that leave this
    distance invariant? What is the symmetry? That is
    how can we transform space and time so that the
    distance in spacetime remains the same.

18
Spacetime
  • Lorentz realised that there was a symmetry in
    nature where you could transform space and time
    distances in the following way.

19
Lorentz Transformations
20
Lorentz Transformations
  • Spatial distances can shorten
  • Time distances can also shorten
  • The spacetime distance is the same that is it is
    invariant under these transformations.
  • v is a velocity
  • Units are chosen such that time is measured in
    light meters.

21
Lorentz Transformations
  • Distances in space will depend on the velocity of
    the observer.
  • Distances in time will depend on the velocity of
    the observer.
  • This is just like saying that spatial distance in
    one direction depends on which way you are
    facing.
  • The equivalent to the angle you are facing is
    velocity you are moving at.

22
Experiments
  • Thousands of experiments have been done checking
    the Lorentz transformations and the altering of
    time and space depending on velocity.

23
Experiments
  • Lifetime of elementary particles
  • Orbiting atomic clocks
  • Collider physics
  • Michaelson Morley experiment Speed of light is
    constant no matter what your velocity

24
Experiments
  • In the experiment carried out by Michaelson
    and Morley an attempt was made to measure speed
    of light parallel to the motion of the earth and
    at right angles to the motion of the earth.
  • According to our usual notions of how
    velocities add there should have been a
    difference.
  • They found the speed of light was the same
    whether it was directed alongs the earths motion
    or not. This agrees with relativity, the speed of
    light is the same no matter how fast you are
    going!

25
Consequences
  • How big is a light meter?
  • Speed of light is about 300000000m/s
  • One light meter is about 0.0000000033333 s
  • To convert to velocities measured in m/s we need
    to divide by c- the speed of light a big number.
  • Most velocities in every day are much much less
    than the speed of light which is why we dont
    notice the Lorentz transformations in ordinary
    life.

26
Consequences
  • Notice that v/c cant be 1 or the Lorentz
    transformation become infinite and time and space
    become infinitely transformed.
  • We cant travel faster than the speed of light.

27
Consequences
  • Just as space and time rotate into each other so
    do other physical quantities. What matter is the
    invariant quantity.
  • Energy and Momentum also transform into each
    other under Lorentz transformations. The
    invariant quantity is

28
Consequences
  • Putting back in c, the speed of light so that
    energy and momentum would be measured in SI units
    this equation becomes
  • If p is zero we get the celebrated equation

29
Conclusions
  • Space and time should be combined to spacetime a
    single entity.
  • The invariant measure of distance on spacetime is
  • With the unit the light meter.
  • Lorentz transformations leave this distance
    invariant.

30
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