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 Chapter 3 Electromagnetic Theory, Photons, and Light Lecture 5

Lecture5_Ch3_EMwaves

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  • Chapter 3

    Electromagnetic Theory, Photons,and Light

    Lecture 5

  • Maxwell equations

    AC SdBdtdldE 0S SdB qSdES 1

    Gausss

    Gausss

    Faradays

    Ampre-Maxwells

    ACSd

    tEJldB

    Lorentz force: BvqEqF

    +fields are defined through interaction with charges

    In matter

  • Maxwell equations: free space, no chargesCurrent J and charge are zero

    AC SddtBdldE

    0S SdB 0S SdE

    AC SdtEldB

    00There is remarkable symmetry between electric and magnetic fields!

    Integral form of Maxwell equations in free space:

    no magnetic charges

    no electric charges

    changing magnetic field creates changing electric fieldchanging electric field creates changing magnetic field

  • Maxwell equations: differential form(free space)

    0 E

    0 B

    tBE

    tEB

    00

    Notation: kzj

    yi

    x

    2

    2

    2

    2

    2

    22

    zyx

    Laplacian:

    0)(

    zE

    yE

    xEEdivE zyx

    ky

    Ex

    Ej

    xE

    zEi

    zE

    yEE xyzxyz

    tB

    zE

    yE xyz

    tB

    xE

    zE yzx

    tB

    yE

    xE zxy

    )(EcurlE

  • Electromagnetic waves

    (free space)

    tBE

    tEB

    00

    Changing E field creates B fieldChanging B field creates E field

    Is it possible to create self-sustaining EM field?

    Can manipulate mathematically into:

    2

    2

    002

    tEE

    2

    2

    002

    tBB

  • Electromagnetic waves

    2

    2

    002

    tEE

    2

    2

    002

    tBB

    2

    2

    2

    2

    2

    22

    zyx

    kx

    jx

    ix

    2

    2

    002

    2

    2

    2

    2

    2

    2

    2

    002

    2

    2

    2

    2

    2

    2

    2

    002

    2

    2

    2

    2

    2

    tE

    zE

    yE

    xE

    tE

    zE

    yE

    xE

    tE

    zE

    yE

    xE

    zzzz

    yyyy

    xxxx

    2

    2

    002

    2

    2

    2

    2

    2

    2

    2

    002

    2

    2

    2

    2

    2

    2

    2

    002

    2

    2

    2

    2

    2

    tB

    zB

    yB

    xB

    tB

    zB

    yB

    xB

    tB

    zB

    yB

    xB

    zzzz

    yyyy

    xxxx

    Resembles wave equation: 22

    22

    2

    2

    2

    2

    22 1

    tzyx

    v

    Each component of the EM field obeys the scalar wave equation, provided that

    00

    1v

  • Light - electromagnetic wave?

    00

    1vMaxwell in ~1865 found that EM wave must move at speed

    At that time permittivity 0 and permeability 0 were known from electric/magnetic force measurements and Maxwell calculated

    km/s 740,3101

    00

    vSpeed of light was also measured by Fizeau in 1849: 315,300 km/s

    Maxwell wrote: This velocity is so nearly that of light, that it seems we have strong reason to conclude that light itself (including radiant heat, and other radiations if any) is an electromagnetic disturbance in the form of waves propagated through the electromagnetic field according to electromagnetic laws.

    Exact value of speed of light: c = 2.997 924 58 108 m/sceler (lat. - fast)

  • Electromagnetic waveAssume: reference frame is chosen so that E=(Ex,0,0)

    longitudinal wave, propagates along x

    0 E

    0 B

    tBE

    tEB

    00

    0

    xEx Ex does not vary with x

    This cannot be a wave!

    Conclusion: it must be transverse wave, i.e. Ex=0. Similarly Bx=0.

    Since E is perpendicular to x, we must specify its direction as a function of time

    Direction of vector E in EM wave is called polarization

    Simple case: polarization is fixed, i.e. direction of E does not change

    0

    zE

    yE

    xE zyx

  • Polarized electromagnetic waveWe are free to chose y-axis so that E field propagating along x is polarized along y: (0, Ey ,0).

    0 E

    0 B

    tBE

    tEB

    00

    tB

    zE

    yE xyz

    tB

    xE

    zE yzx

    tB

    yE

    xE zxy

    tB

    xE zy

    Also: Bx=By=const (=0)

    E-field of wave has only y componentB-field of wave has only z component(for polarized wave propagating along x)

    In free space, the plane EM wave is transverse

  • Harmonic polarized electromagnetic wave

    cxtEtxE yy /cos, 0Harmonic functions are solution for wave equation:

    polarized along y axis propagates along x axis

    tB

    xE zy

    dtxEB yzFind B:

    cxtEc

    txB yz /cos1, 0

    zy cBE This is true for any wave:- amplitude ratio is c- E and B are in-phase

  • Harmonic polarized electromagnetic wave

    * direction of propagation is in the direction of cross-product:

    BE

    * EM field does not move in space, only disturbance does.Changing E field creates changing B field and vice versa

    Electromagnetic waves

  • Energy of EM wave

    It was shown (in Phys 272) that field energy densities are:

    20

    2EuE

    202

    1 BuB

    Since E=cB and c=(00)-1/2:BE uu

    - the energy in EM wave is shared equally between electric and magnetic fields

    Total energy: 20

    20

    1 BEuuu BE (W/m2)

  • The Poynting vector

    EM field contains energy that propagates through space at speed cEnergy transported through area A in time t: uAct

    EBEBcBEcEcuctAtuAcS

    00

    000

    20

    11

    Energy S transported by a wave through unit area in unit time:

    E c2

    The Poynting vector:

    BES

    0

    1

    power flow per unit area for a wave, direction of propagation is direction of S.

    (units: W/m2)

    John Henry Poynting (1852-1914)

  • The Poynting vector: polarized harmonic wave

    BES

    0

    1Polarized EM wave: trkEE cos0 trkBB cos0

    Poynting vector:

    trkBES 2000 cos1This is instantaneous value: S is oscillating

    Light field oscillates at ~10 15 Hz -most detectors will see average value of S.

  • Irradiance

    trkBES 2000 cos1Average value for periodic function: need to average one period only.It can be shown that average of cos2 is: 21cos2

    Tt

    20

    000

    0 221 EcBES

    T

    And average power flow per unit time:

    Irradiance:20

    0

    2EcSI

    T

    Alternative eq-ns:

    TTBcEcI 2

    0

    20

    Usually mostly E-field component interacts with matter, and we will refer to E as optical field and use energy eq-ns with E

    Irradiance is proportional to the square of the amplitude of the E field

    For linear isotropic dielectric:

    TEI 2v

    Optical power radiant flux total power falling on some area (Watts)

    (used to be called Intensity)

  • Spherical wave: inverse square lawSpherical waves are produced by point sources. As you move away from the source light intensity drops

    trkr

    tr vcos, ASpherical wave eq-n:

    trkr

    EE

    cos0 trkr

    BB

    cos0

    trkr

    Br

    ES

    200

    0

    cos1

    202

    0 12

    Er

    cSIT

    Inverse square law: the irradiance from a point source drops as 1/r2

  • Radiation pressure

    Using classical EM theory Maxwell showed that radiation pressure equals the energy density of the EM waves:

    2

    0

    20

    21

    2BEu

    P ucS ctSt P

    This is the instantaneous pressure that would be exerted on a perfectly absorbing surface by a normally incident beam

    Average pressure: cI

    ctS

    t TT

    P (N/m2)

    * for reflecting surface pressure doubles

  • Radiation pressure applicationStar wars episode 2

    http://www.livescience.com/32593-how-do-solar-sails-work-.html

    NASA to Launch World's Largest Solar Sail in November 2014: Sunjammerhttp://www.sunjammermission.com

  • Example problemA laser pointer emits light at 630 nm in xy plane at =450 to axis x(counter clock-wise). The light is polarized along axis z , beam cross-section is A=1 mm2 and its power is P=1 mW.1. Write an equation of E and B components of this EM wave for the region of the beam.

    x

    y

    z trkEE cos0Find : c22 Find k: sincos2 jik Find E0:

    Irradiance: 2002EcI

    AP

    00 2 AcPE k2 00 AcPE

    tcrjiAcPE 2sincos2cosk2 0

    Electric field:

    B

    E