Lecture12(Dispersion)

28
Wave Phenomena Physics 15c Lecture 12 Dispersion (H&L Sections 2.6)

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dispersion

Transcript of Lecture12(Dispersion)

  • Wave PhenomenaPhysics 15c

    Lecture 12Dispersion

    (H&L Sections 2.6)

  • What We Did Last Time

    ! Defined Fourier integral

    ! f(t) and F() represent a function in time/frequency domains! Analyzed pulses and wave packets

    ! Time resolution t and bandwidth related by! Proved for arbitrary waveform

    ! Rate of information transmission bandwidth! Diracs (t) a limiting case of infinitely fast pulse! Connection with Heisenbergs Uncertainty Principle in QM

    ( ) ( ) i tf t F e d

    =

    1( ) ( )2

    i tF f t e dt

    =

    12

    t >

  • Goals For Today

    ! Discuss dispersive waves! When velocity is not constant for different ! Waveform changes as it travels! Dispersion relation: dependence of k on

    ! Define group velocity! How fast can you send signals if the wave velocity is not

    constant?

  • Mass-Spring Transmission Line

    ! In Lecture #5, we had

    ! We ignored the gravity by making the strings very long

    nn1 n+1

    2

    1 12 ( ) ( )n s n n s n ndm k kdt

    +=

    0nmgL

    L What if we didnt make this approximation?

  • Wave Equation

    ! Equations of motion is now

    ! Usual Taylor-expansion trick

    ! Divide by (x)

    ! Wave equation:

    2

    1 12 ( ) ( )n s n n s n n ndm k kdt

    mgL

    + =

    2 22

    2 2

    ( , ) ( , ( , )) ( )sx t x tm k x

    t xmL

    x g t =

    2 2

    2 2

    ( , ) ( , ) ( , )l lx t x tK g

    tx t

    x L =

    2 22 2

    02 2

    ( , ) ( , ) ( , )wx t x tc x t

    t x =

    wl

    Kc

    =

    0gL

    =

    Natural frequency of pendulum

  • Solution

    ! Assume

    ! As before, we can write the solution as

    2 22 2

    02 2

    ( , ) ( , ) ( , )wx t x tc x t

    t x =

    ( , ) ( ) i tx t a x e =2

    2 2 202

    ( )( ) ( )i t i t i twd a xa x e c e a x e

    dx = Wave eqn.

    2 220

    2 2

    ( ) ( )w

    d a x a xdx c

    = SHO-like if 2 20 0 >

    ( )( , ) i kx tx t Ae =2 2

    0

    w

    kc

    =but with

    This is the difference

  • Dispersion Relation

    ! Normal-mode solutions are still! What changed is the relationship between k and

    ! A.k.a. dispersion relation

    ! NB: there are different types of dispersive waves! We are looking at just one example here

    ! Dispersion relation determines how the waves propagate in time and space

    ( )( , ) i kx tx t e =

    ( )w

    kc =

    2 20( )

    w

    kc

    =

    Non-dispersive waves

    Dispersive waves

    Well study how

  • Phase Velocity

    ! To calculate the propagation velocity of! We follow the point where the phase kx t is constant

    ! Phase velocity is the velocity of pure sine waves! Easily calculated from the dispersion relation

    ( )0( , )

    i kx tx t e =

    kx t C =C tx

    k

    = dx

    dt k

    = Phase velocity cp

    ( ) const.p wc c = =( )w

    kc =

    2 20( )

    w

    kc

    =

    Non-dispersive

    Dispersive2 2

    0

    ( )p wc c

    =

    No longerconstant!

  • Dispersing Pulses

    ! Imagine a pulse being sent over a distance! On non-dispersive medium, the pulse shape is unchanged

    ! That was because all normal modes had the same cp! On dispersive medium, the pulse shape must change

    ! The pulse gets dispersed! Hence the name: dispersion

    ! Dispersion makes poor media for communication

  • Dispersion Relation

    ! Dispersive waves have no solution for < 0! It has a low frequency cut-off at 0

    ! Phase velocity goes to infinity at cut-off! Wait! Isnt it unphysical? What happened to Relativity?

    k

    0

    wc k =

    2 20wc k =

    pc

    0

    wc

    2 20

    wp

    cc

    =

  • Finite-Length Signal

    ! Phase velocity cp is the speed of pure sine waves! But pure sine waves dont carry information! Relativity forbids superluminal transfer of information

    ! Lets think about a finite-length pulse

    ! Problem: this medium cant carry waves with ! We need to make a pulse that does not contain frequencies

    below the cut-off

    ( )f t ( )F

    t

    T

    0

    0