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    Lecture 4

    Relativity of Simultaneity Revisited

    ct

    x

    O

    0=v

    A B C

    x

    ct

    O

    0v

    A B C

    vtxxi+=

    ct

    x

    Two events simultaneous in one inertial frame are not simultaneous

    in any other inertial frame moving relative to the first.

    OR

    Clocks synchronized in one inertial frame are not synchronizedin any other inertial frame moving relative to the first.

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    Lecture 4

    Lorentz Transformation

    Requirements:

    Transformation must be linear in both space and timecoordinates

    Transformation must reduce to Galilean transformationfor sufficiently small values of the relative speed between

    two inertial frames

    Mathematically, we have

    btaxx

    tbxax

    =

    +=

    abv =

    0=x

    0=x

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    Lecture 4

    Lorentz Transformation-Cont d

    Now, consider the motion of a light pulse originating at the

    origin of both inertial frames

    tcx

    ctx

    =

    =

    tbacbtctatc

    tbactbtcact

    )()(

    )()(

    ==

    +=+=

    bac

    c

    t

    t

    c

    bac

    =

    =

    +

    )( 222

    2222

    vca

    bcac

    =

    =

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    Lecture 4

    Lorentz Transformation-Cont d

    2

    21

    1)(

    c

    v

    av

    =

    abtxaabtxax

    btaxaxxaxtb

    +=+=

    ==

    )1(

    )(

    22atx

    b

    at +

    =

    21

    2

    22

    22

    22222/1

    /1

    /1

    11

    1

    c

    v

    v

    cv

    cv

    cv

    v

    cv

    b

    a=

    =

    =

    Lorentz factor

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    Lecture 4

    Lorentz Transformation-Cont d

    To summarize

    )(

    )(

    2c

    xvtt

    zzyy

    tvxx

    +=

    =

    =

    +=

    )(

    )(

    2c

    vxtt

    zzyy

    vtxx

    =

    =

    =

    =

    =+=

    22c

    vxttx

    c

    vt

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    Lecture 4

    x

    ct ct

    x

    OO

    The time axis in S follows:

    ))(/(

    0)(

    ctcvvtx

    vtxx

    ==

    =

    xct )/1( =

    The spatial axis in S follows:

    2

    2

    /

    0)/(

    cvxt

    cvxtt

    =

    =

    xct =

    Relationship between Inertial Frames

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    Lecture 4

    Coupling of Space and Time

    )(

    )(

    2

    c

    vxtt

    vtxx

    =

    =

    (x1, t1) (x2, t2)

    [ ]

    =

    =

    212

    1212

    121212

    )()(

    )()(

    c

    xxvtttt

    ttvxxxx

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    Lecture 4

    Length Contraction

    A rod is at rest in S, and lies along thex-axis. Let its two ends be

    denoted by space-time coordinates (x1, t1) and (x2, t2),then thelength of the rod is always measured as

    Now, what is the length of the rod as measured by an observer in

    S?

    x1 = (x1 vt)

    x2 = (x2 vt)

    L = x2(t) x

    1(t)

    x2 x1 = (x2 x1)

    L = Lp 1v

    2

    c2

    Lp= x2

    x1 Proper Length

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    Lecture 4

    Time Dilation

    A clock is at rest in S. Consider two events corresponding to

    different readings of the clock, (x, t1)and(x, t2).The timeinterval between the two events in Sis denoted by

    p=

    t2

    t1

    what is the time interval between the same two events as

    measured by an observer in S?

    Proper Time

    t1= ( t1 +

    v xc2 )

    t2= ( t2 +

    v xc

    2 )

    t2 t1 = ( t2 t1)

    =

    p

    1 v2

    c2

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    Lecture 4

    Relativistic Doppler Effect

    += xc

    vtt

    2

    += xc

    vtt

    2

    += )(2

    tc

    c

    vtt

    lightIf the time interval represents

    the period of the light wave,

    t=1

    f, t =

    1

    fp

    f =1 v

    c

    1+ vc

    fp

    fp :proper frequency, if the

    source of light is at rest

    in S.

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    Lecture 4

    Redshift and Blueshift

    beta valuec

    v= 21

    1

    =Lorentz factor

    We define z ( fp

    f) f

    1)1(

    1)1(2

    2

    ++

    +=

    z

    z

    f =1

    1+ fp

    z If

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    Lecture 4

    General formula for Doppler shift: f =fp

    1

    1 cos

    Transverse Doppler Effect

    t= t +v

    c2 x

    x = 0

    t = ( t )

    t=1

    f, t =

    1

    fpf =

    fp

    Transverse Doppler shift always represents

    redshift!

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    Lecture 4

    Reading Assignments

    Chapter 1, 1-6