2 ()− ∇Ψ+V()rΨ= 2mdoe.carleton.ca/~tjs/475_pdf_02/snew4.pdf · 2002. 9. 9. · Lecture 4:...

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Lecture 4: Wave Packets September, 2000 1 LECTURE 4 – WAVE PACKETS 1.2 Comparison between QM and Classical Electrons Classical physics (particle) Quantum mechanics (wave) electron is a point particle electron is wavelike motion described by a m F * * = for energy E, motion described by wavefunction F = -V (r) ( 29 (29 E , = Ψ = Ψ - ϖ ϖ ! * & t j e r t r (29 (29 Ψ = Ψ + Ψ - E r V & ! * 2 2 2m - energy potential r V where (29 (29 (29 (29 (29 ) 0 take , simplicity (for const. r V 0 F : electrons free" " consider now shall We , E 2 1 , * r position at electron finding of density y probabilit account into taken are electron on the acting forces the where is this - energy) (potential - r V charges governing equation al differenti - other from fields electric to due F typically 2 = = = = = = = Ψ Ψ Ψ r V k p mv E mv p r & & & ! ! & & & & ϖ

Transcript of 2 ()− ∇Ψ+V()rΨ= 2mdoe.carleton.ca/~tjs/475_pdf_02/snew4.pdf · 2002. 9. 9. · Lecture 4:...

  • Lecture 4: Wave Packets September, 2000 1

    LECTURE 4 – WAVE PACKETS

    1.2 Comparison between QM and Classical Electrons Classical physics (particle) Quantum mechanics (wave) electron is a point particle electron is wavelike motion described by amF

    ** = for energy E, motion described by wavefunction

    F = -∇ V (r )

    ( ) ( ) E , =Ψ=Ψ − ωω !*& tjertr

    ( ) ( ) Ψ=Ψ+Ψ∇− ErV &!* 22

    2m- energy potential rV where

    ( )

    ( ) ( )

    ( ) ( ) )0 take,simplicity(for const.rV 0F :electrons free""consider now shall We

    ,E 2

    1,

    *r

    positionat electron finding ofdensity y probabilit

    account into taken areelectron on the acting

    forces the whereis this- energy) (potential - rV

    charges

    governingequation aldifferenti - other from fields electric todue Ftypically

    2

    ==∴=

    ====

    Ψ⋅Ψ

    Ψ

    rV

    kpmvEmvp

    r

    &&&

    !!

    &&

    &

    &

    ω

  • Lecture 4: Wave Packets September, 2000 2

    Wavepackets and localized electrons For free electrons we have to solve Schrodinger equation for V(r) = 0 and previously found: We can’t conclude anything about the location of the electron! However, when dealing with real electrons, we usually have some idea where they are located! How can we reconcile this with the Schrodinger equation? Can it be correct? We will try to represent a localized electron as a wave pulse or wavepacket. A pulse (or packet) of probability of the electron existing at a given location. In other words, we need a wave function which is finite in space at a given time (i.e. t=0). Ψ(x) λo λ ∆x Particle behavior is observation of the evolution of the packet as a whole. Wave effects are an observation of the individual frequency components of the “packet”. From Fourier transform concepts, the wavepacket can be represented as a superposition of waves with different k (the spatial frequency). Just like forming a voltage pulse from temporal (time) frequency (ω or f) components. A Fourier Transform can be defined in time and a localized (in time) packet created using a frequency spectrum (communications theory).

    ( ) ( ).everywhere C*

    waveplane travelling- ,2=Ψ⋅Ψ∴

    =Ψ −⋅ trkjCetr ω&

    &

    *

    ( )

    ωωπ

    =

    π=ω

    ω∞

    ∞−

    ω∞

    ∞−

    de)(g2

    1)t(f

    dte)t(f2

    1g

    ti

    ti

  • Lecture 4: Wave Packets September, 2000 3

    We can do the same for a spatial function. A k “spectrum” will produce a spatially localized wave “packet”.

    ψ (k) is the spatial frequency spectrum of ψ(x). A k “spectrum” will produce a spatially localized wave “packet”. ψ(k) ∆k k ko

    It is found from Fourier math that the more tightly confined the wavepacket is in x, the broader the spread in k, and vice-versa, This is equivalent to needing high frequency components for a small rise time in a voltage pulse.

    dxex

    dkektx

    jkx

    tkxj

    −∞

    ∞−

    −∞

    ∞−

    Ψ=

    )0,(2

    1(k) where

    (13) )(2

    1),( i.e., )(

    πψ

    ψπ

    ω

    space.k in sizepacket k the and sizepacket theisx position,

    packet theis xfrequency, spatial e"packet wav" average theis 2

    k where o

    ∆∆

    = ooλπ

    principle.y uncertaint thecalled -h px 2p

    k

    later) derivation (Formal 2xk :result ansformFourier tr

    ≥∆⋅∆≥∆⋅∆∴

    ≥∆⋅∆

    π

    π

    !

  • Lecture 4: Wave Packets September, 2000 4

    Formation of a wave packet by superposition of two different waves of slightly different frequencies:

    As the number of waves increases, the wave packet becomes more localized in space.

    Note that the wavepacket does not change its shape as time passes if all the components have the same phase velocity.

    Let’s define the shift in space of the packet in time ∆t as

    tk

    x ∆∂∂=∆ ω

    Velocity of wavepacket: tdk

    dx ∆=∆ ω ∴

    dk

    d

    t

    xVgroup

    ω=∆∆= (16)

  • Lecture 4: Wave Packets September, 2000 5

    where Vgroup is the group velocity the velocity the packet moves at not the velocity of the individual phases. It represents the velocity of the particle. If the phase velocities are constant and the group velocity equals the phase velocity the packet moves with out changing shape, we call this “no dispersion”. However, if the phase velocity differs we can get packet distortion and dispersion of the packet.

    Dispersion is a very important phenomenon present in several types of wave propagation. In particular, it appears in the case of EM waves propagating through matter (Optical fibers).

  • Lecture 4: Wave Packets September, 2000 6

    Compare:

    For a free electron we have Em

    k == ω!!2

    22

    ∴ M

    E

    m

    k

    dk

    dso

    m

    k 2

    2

    2

    === !! ωω (17)

    Using Classical Physics:

    M

    EV

    mVE

    2

    2

    2

    =∴=

    and we find that the energy carried at group velocity is analogous to the kinetic energy of the particle at same velocity.