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The Mathematics of Star Trek

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Title: The Mathematics of Star Trek


1
The Mathematics of Star Trek
  • Lecture 5 General Relativity

2
Topics
  • Captain Picard and Einsteins Elevator
  • Principal of Equivalence
  • Bending of Light
  • General Relativity and Curved Spacetime
  • Einsteins Equations of General Relativity
  • Mercurys Orbit
  • Faster than Light (FTL) Travel
  • Impulse Drive, Tractor Beams, Deflector Shields,
    and Cloaking Devices

3
Captain Picard and Einsteins Elevator
Romulan Frame
  • Suppose that just as a phaser (light) beam is
    shot by a Romulan Warbird at Captain Picards
    yacht Calypso, the Calypso accelerates forward,
    perpendicular to the phaser shot.
  • In the Romulans frame of reference, the phaser
    beam travels in a straight line.
  • Thinking of light as a particle, it can be shown
    with vectors and the equations of motion that
    Picard will see the light beam travel along a
    curved path!
  • Mathematica example!

Picard Frame
4
Captain Picard and Einsteins Elevator (cont.)
  • If Picards acceleration is the same as that due
    to gravity at the Earths surface, then Picard
    will feel the same force pushing him back in his
    seat as he would due to the downward force of
    gravity at the Earths surface!
  • Einstein argued that Picard (or someone in an
    elevator being accelerated upwards with the same
    acceleration) will never be able to perform any
    experiment to tell the difference between the
    reaction force due to accelerated motion and that
    due to the pull of gravity from some nearby heavy
    object outside the ship.
  • Einstein concluded that whatever phenomena an
    accelerating object experiences would be the same
    as the phenomena an observer in a gravitational
    field experiences!

5
The Principle of Equivalence
  • Einsteins idea, known as the Principle of
    Equivalence, says that inertial mass and
    gravitational mass are the same and is the
    starting point for the theory of General
    Relativity!
  • Here is one implication of the Principle of
    Equivalence
  • Since Picard observes the light ray bending when
    he is accelerating away from it, it follows from
    Principle of Equivalence that the light ray would
    also bend in a gravitational field!
  • Matter produces a gravitational field, so matter
    must bend the path of a light beam.

6
Bending of Light
  • In 1911, using the idea that light will be bent
    in a gravitational field, along with Newtons
    Laws, Einstein predicted that light passing by
    the outer edge of the Sun should be bent by an
    angle of approximately 0.85 seconds.
  • In 1919, Sir Arthur Eddington led one of two
    expeditions (his went to Sobral Brazil) to
    observe the apparent position of stars on the sky
    near the Sun during a solar eclipse.
  • During the eclipse, rays of light from stars
    passing close to the sun would be bent.
  • The amount by which the light is bent could be
    deduced by comparing the stars relative
    positions to those at some other time of the
    year.
  • Eddington found that the light bends exactly
    twice as much as that predicted by Einstein!

7
Bending of Light (cont.)
  • The phenomenon observed by Eddington is the same
    as that of gravitational lensing, where a cluster
    of galaxies can produce multiple magnified images
    of a galaxy twice as far away, which has been
    seen using the Hubble Space Telescope.
  • A gravitational lens is a massive object that
    magnifies or distorts the light of objects lying
    behind it.
  • For example, the powerful gravitational field of
    a massive cluster of galaxies can bend the light
    rays from more distant galaxies, just as a camera
    lens bends light to form a picture.

8
General Relativity and Curved Spacetime
  • In 1916, Einstein published a paper that
    introduced the world to his theory of General
    Relativity.
  • Unable to incorporate gravity directly into the
    theory of Special Relativity, he was led to the
    idea that gravity is not a force, but a
    manifestation of the curvature of spacetime.
  • Masses in space such as the Sun cause spacetime
    to be curved and the curved paths that we see
    objects (or light) following near these masses
    are simply the straightest possible paths in the
    curved spacetime!
  • Adding in the idea that spacetime is curved, he
    was able to show that the predicted bending of
    light by the Sun during the 1919 eclipse was
    right!

9
Einsteins Equations of General Relativity
  • Mathematically, General Relativity is built upon
    a set of ten coupled hyperbolic-elliptic
    nonlinear partial differential equations, which
    can be represented symbolically as shown at the
    right. (Click on the image for a link to the
    equations!)
  • The equations boil down to this CURVATURE (LHS)
    MATTER AND ENERGY (RHS).
  • This theory is hard to work with, because
  • The curvature of space is determined by the
    distribution of matter and energy in the
    universe.
  • The distribution of matter and energy in the
    universe is determined by the curvature of space.

10
Mercurys Orbit
  • Another way that the theory of General Relativity
    was shown to be correct was by answering a
    question about Mercurys orbit!
  • According to Newtons Laws, the planet Mercury
    moves around the Sun in an elliptical orbit with
    the Sun at one focus of the ellipse.
  • After one revolution around the Sun, the Mercury
    should come back to its starting point, which
    isnt what happens.
  • It turns out that the perihelion (closest point
    to the Sun) of the orbit of the planet Mercury
    advances approximately 0.012 degree per century
    (image is from Hyper Physics website).
  • One way to account for this advance is due to the
    force of gravity from other planets in the solar
    system, but this only takes care of 80 seconds of
    arc.

11
Mercurys Orbit (cont.)
  • Astronomers guessed that the last 40 seconds of
    arc might be due to another (unknown) planet in
    our solar system, which they named Vulcan.
  • This is how the planet Neptune was discovered!
  • Neptune was the first planet located through
    mathematical predictions rather than through
    systematic observations of the sky!
  • After the discovery of Uranus in 1781,
    astronomers noted that Uranus was not faithfully
    following its predicted path.
  • Uranus seemed to accelerate in its orbit before
    1822 and to slow after that.

12
Mercurys Orbit (cont.)
  • One possible explanation was that the gravity of
    an undiscovered planet was affecting the orbit of
    Uranus.
  • Starting in 1841, British astronomer John Couch
    Adams and the following summer, French astronomer
    Urbain Jean Joseph Le Verrier without knowledge
    of each other independently calculated where the
    new planet should be.
  • At first, neither was taken seriously, but by
    1846, based on their work, Neptune was discovered!

13
Experimental Verification Mercurys Orbit
(cont.)
  • Einstein suggested that the extra advance of
    Mercurys perihelion could be due to the
    curvature of spacetime near the Sun.
  • He predicted that the amount by which the
    Mercurys perihelion should advance is given by
  • where a is the length of the semi-major axis of
    Mercurys elliptical orbit, e is the eccentricity
    of the ellipse, c is the speed of light, and T is
    the period of revolution.
  • HW See if this formula works!

14
Faster Than Light (FTL) Travel
  • One of the implications of curved spacetime is
    the idea that what we perceive as a straight line
    need not be the shortest path between two points!
  • Krauss gives an explanation of how this might
    occur in two-dimensions!
  • Consider a piece of elastic material, as shown on
    p. 36 of our textbook.
  • If the material is laid flat and a circle drawn
    on the sheet, the shortest path between two
    opposite points on the circle, A and B, would be
    a straight line through the center.

15
FTL Travel (cont.)
  • If the center is pushed down and the material
    stretched, then the shortest path may be along
    the circle.
  • The sheet has been curved (in 3-space), but to a
    bug walking on the line from A to B, it thinks
    it is moving in a straight line.
  • This is the idea we want to extend to spacetime -
    we are the bug and cannot perceive the curve of
    spacetime in 3-space!
  • It may be possible to traverse what appears to be
    a huge distance (line-of-sight wise) by finding a
    shorter route through spacetime!
  • If spacetime itself can be manipulated, then
    objects can travel locally at low velocities, yet
    an accompanying expansion or contraction of space
    could allow huge distances to be traversed in
    short time intervals!

16
FTL Travel (cont.)
  • An example of this idea has been developed by
    physicist Miguel Alcubierre, who has shown that
    mathematically warp drive could be possible in
    the theory of general relativity.
  • According to Alcubierre, a spacetime
    configuration can be created in which a
    spacecraft could traverse a distance between two
    points in an arbitrarily short period of time.
  • Throughout this journey, the spacecraft would
    move with respect to its local surroundings at
    speeds much less than the speed of light!
  • Therefore clocks on the ship would stay
    synchronized with the outside world.

17
FTL Travel (cont.)
  • The idea works like this warp spacetime so it
    expands behind the ship and contracts in front of
    it, thus propelling the ship along with the space
    surrounding the ship (like a surfboard and surfer
    on a wave).
  • The spaceship will never travel faster than the
    speed of light, as the light near the ship will
    be carried along with the ship!
  • In this theory, it would be possible to arrange
    for the huge gravitational fields needed to be
    somewhere far from the spaceship or star bases or
    planets the ship may travel to as a destination,
    thus avoiding problems with slow clocks.

18
Impulse Drive, Tractor Beams, Deflector Shields,
and Cloaking Devices
  • The same idea that works for warp drive, namely
    warping spacetime, would allow for travel at
    impulse speeds!
  • The crew wouldnt be subjected to large
    accelerations, so inertial dampers would no
    longer be needed!
  • Warping spacetime could also be used to move a
    planet contract space behind the asteroid and
    expand space in front of it!
  • This could be how the tractor beam really works
    if so, then Newtons Third Law doesnt apply any
    more!
  • Two other applications of warping spacetime might
    be deflector shields and cloaking devices!
  • Deflector shields are force fields that prevent
    phaser beams (light rays) from hitting a
    starship.
  • Cloaking devices make a ship invisible.
  • In each case, space would be warped to either
    deflect (bend) the light rays away from the ship
    or cause the light rays to bend around the ship
    (cloak it).

19
References
  • Relativity The Special and General Theory by
    Albert Einstein
  • The Geometry of Spacetime by James Callahan
  • The Physics of Star Trek by Laurence Krauss
  • http//hyperphysics.phy-astr.gsu.edu/hbase/hph.htm
    l
  • http//www-groups.dcs.st-and.ac.uk/history/index.
    html
  • http//hubblesite.org/newscenter/newsdesk/archive/
    releases/2004/08/text/
  • http//archive.ncsa.uiuc.edu/Cyberia/NumRel/Einste
    inEquations.htmlintro
  • http//pds.jpl.nasa.gov/planets/captions/neptune/f
    ullnep.htm
  • http//members.aol.com/nogravityguy/book02.htm
  • http//marge.uvm.edu/Sdempse/images/TV_Movies/Star
    _Trek/borgtrac.gif
  • http//www.thasos.ukgateway.net/images/Ent_Warp_Sm
    all.jpg
  • http//www.exn.ca/mini/startrek/warpdrive.cfm
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