The Geometry of Special Relativity (Tevian Dray)_slides

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  • THE GEOMETRY OFSPECIAL RELATIVITY

    Tevian Dray

    Oregon State University

    I: Circle Geometry

    II: Hyperbola Geometry

    III: Special Relativity

    IV: What Next?

  • CIRCLE GEOMETRY

    .1 (cos , sin )

    r = arclength

    4

    53

    cos =4

    5= tan =

    3

    4

  • WHICH GEOMETRY?

    Euclidean

    ds2 = dx2 + dy2

    y

    B

    A

    y

    x

    x

    4

    53

    tan = 34

    B = (cos , sin )

    A = ( sin , cos )

    Trigonometry!

  • Return

    MEASUREMENTS

    Width:

    1

    1

    1

    cos

    1

    cos

    Apparent width > 1

    Slope:y

    x

    y

    x

    y

    x

    m 6= m1 + m2

  • HYPERBOLA GEOMETRY

    .1

    (cosh , sinh )

    x2 y2 = 1

    r = arclength

    ds2 = |dx2 dy2|

    cosh =1

    2

    (

    e + e)

    sinh =1

    2

    (

    e e)

  • HYPERBOLIC TRIANGLE TRIG

    d cosh

    d sinhd

    4

    5

    3

    tanh = 3/5

    5

    4

    3

    tanh = 4/5

  • RIGHT TRIANGLES

    B

    y y

    A

    x

    x

    right angles are not angles!

  • WHICH GEOMETRY?

    signature

    (+ + ...+) Euclidean( + ...+) Minkowskian

    ds2 = c2 dt2 + dx2ct

    A

    B

    ct

    x

    x

    4

    5

    3

    tanh = 35

    B = (cosh , sinh )

    Special Relativity!

  • Compare

    SPECIAL RELATIVITY

    ct

    A

    B

    ct

    x

    x

    v

    c= tanh

    tanh( + ) =tanh + tanh

    1 + tanh tanh=

    uc +

    vc

    1 + uvc2

    Einstein addition formula!

  • Compare

    LENGTH CONTRACTION

    x

    ctct

    x

    = cosh

    x

    ctct

    x

    =

    cosh

  • TIME DILATION

    x

    ctct

    x

  • COSMIC RAYS

    (Taylor & Wheeler, 1st edition, Ex. 42, p. 89.)

    Consider -mesons produced by the collision of cosmic rays with gas nuclei inthe atmosphere 60 kilometers above the surface of the earth, which then movevertically downward at nearly the speed of light. The half-life before -mesonsdecay into other particles is 1.5 microseconds (1.5 106 s). Assuming it doesnt decay, how long would it take a -meson to reach the

    surface of the earth?60 km

    3 108 ms= 200 s

    Assuming there were no time dilation, about what fraction of the mesonsreaches the earth?

    200 s3

    2s per half-life

    =400

    3half-lives

    In actual fact, roughly 18

    of the mesons would reach the earth! How fast arethey going?

  • COSMIC RAYS

    400

    3half-lives

    3 half-lives=

    400

    9

    9400

    v

    c= tanh =

    4002 92

    400 .99974684

  • COSMIC RAYS

    (60 km)(1000 mkm

    )

    (4.5 106 s)(3 108 ms )=

    400

    9

    400

    9

    v

    c= tanh =

    4004002 + 92

    .99974697

  • TWIN PARADOX

    One twin travels 24 light-years to star X at speed 2425c; her twin brother stays

    home. When the traveling twin gets to star X, she immediately turns around,

    and returns at the same speed. How long does each twin think the trip took?

    24

    25 7

    cosh =25

    7

    7

    q

    q =7

    cosh =

    49

    2549/25

    7

    24

    25

    Straight path takes longest!

  • SUMMARY

    Lorentz transformations are hyperbolic rotations Beautifully treated in Taylor & Wheeler, 1st ed Removed from Taylor & Wheeler, 2nd edition Not currently covered in existing texts

    http://www.math.oregonstate.edu/~tevian/geometry

  • WHICH GEOMETRY?

    signature flat curved

    (+ + ...+) Euclidean Riemannian( + ...+) Minkowskian

    ds2 = r2(d2 + sin2 d2)

    Tidal forces!

  • WHICH GEOMETRY?

    signature flat curved

    (+ + ...+) Euclidean Riemannian( + ...+) Minkowskian Lorentzian

    General Relativity!

    ds2 = dt2 + a(t) dx2Cosmology!

    (c = 1)ds2 =

    (

    1 2mr)

    dt2 +dr2

    (

    1 2mr)

    + r2(

    d2 + sin2 d2)

  • Start Close Exit

    THE GEOMETRY OFSPECIAL RELATIVITY

    Tevian Dray

    Oregon State University

    http://www.math.oregonstate.edu/~tevian/geometry