Lecture physical optics

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    EM I&II

    The energy transported by a large number ofphotonsis, on the average,equivalent to the energy transferred by a classicalelectromagnetic wave.

    The dual nature of light is evidenced by the fact that itpropagates throughspace in awave-like fashion and yet displaysparticlelike behavior duringthe processes ofemission and absorption.

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    3.1 Basic Laws of Electromagnetic Theory

    Charge & Fields

    Electric Field E

    A point charge qexperiences a force , theEfield at the position of the charge is:

    EF

    EqFE

    Magnetic Field B

    A movingcharge experience force , whichis depended on its velocity and magnetic

    field as:

    MF

    BVqFM

    q

    V

    B

    Moving charge in both Eand Bfields experiences:

    BVqEqF

    Electric

    current

    Time-varying

    EfieldElectric

    charge

    Time-varying

    Bfield

    Efield Bfield

    E E

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    3.1.1 Faradays Induction Law

    Convert magnetism into electricity

    ---- Michael Faraday 1822

    Swing of galvanometer

    when switch close/open

    A changing magnetic

    field generates a current

    (induced electromotiveforceemf).

    When constant,

    When constant,A

    tBAemf /

    B

    tABemf /

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    3.1.1 Faradays Induction Law

    Flux of the magnetic fieldthrough the wire loop

    cosBABAABM

    When constant, When constant,A

    tBAemf /B

    tABemf /

    Thefluxof the field: the product of field andarea where the penetration is perpendicular.

    More generally, ifBvaries in space

    AM SdB

    The induced emf developed around the loop

    dt

    demf M

    Very generally, an emfis a potential difference per unit charge,which corresponds to work done per unit charge, which is force per

    unit charge times distance, which is electric field times distance

    c

    ldEemf

    Thus,

    c A

    SdBdt

    dldE

    c A

    Sd

    t

    BldE

    or

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    3.1.2 Gauss's Law - Electric

    The relationship between the flux of theelectric fieldand the sourcesof that flux, charge.

    The flux ofEfield through an imaginary

    closed area A is:

    AE SdE

    If no sources or sinks of the Efield withinthe region encompassed by A, the net flux

    through the surface equals zero.

    qin vacuum centered inside a sphericalsurface of radius r.

    A AE EdSdSEEis constant overA AE rEdSE

    24

    By Coulombs Law:2

    04

    1

    r

    qE

    so

    0q

    E Electric flux of single point-charge

    Multiple charges: qE0

    1

    and A qSdE

    0

    1

    Gausss Law

    Continuously distributed charges: A V dVSdE 01

    V: volumeenclosed by A

    E

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    Electric Permittivity

    2212

    0 /108542.8 mNC

    Electric permittivity offreespace(vacuum)

    Conceptually, the permittivity embodies the electrical behavior of the

    medium: in a sense, it is a measure of the degree to which the material

    is permeated by the electric field in which it is immersed.

    Indeed, permittivity is often measured by a procedure in which thematerial under study is placed within a capacitor.

    Relative permittivity ordielectric constant:

    0 EK KE is defined as /0 and it is unitless.

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    3.1.3 Gauss's Law - Magnetic

    NO isolated magnetic poles

    Any closed surface in a region ofmagnetic field would accordingly have

    an equal number of lines of entering

    and emerging from it because there is

    no monopoles.

    B

    The flux of magnetic field throughsuch a surface is zero.

    A

    M SdB 0

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    3.1.4 Ampres Circular Law

    Magnetic field of a straight

    wire carrying a current iis:

    riB 2/0

    Suppose magnetic charge qm,analogy to electric charge

    Magnetic force = qmB in the direction ofB.

    The work done by carrying the monopole alongl: lBqW m

    The total work done is: lBqm

    In this case, riBB 2/0 so rBqlBqlBq mmm 2 Substitute riB 2/0 work done becomes iqm 0

    Hence, ilB 0 To be summed over any closed path surrounding i.

    Hecht

    ???

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    3.1.4 Ampres Circular Law

    ilB 0 0l C ildB 0

    Ampres Law

    It relates line integral of tangent to a closed curve C, with

    the total current ipassing within the confines ofC.

    B

    For the current with a nonuniform cross section:

    C A SdJldB

    0 here open surface A is bounded by C.

    The quantity 0 is called the permeability of free space

    and it is defined as 227 /104 CsN

    The permeability of a medium where the current

    imbedded in:

    0 MK KM: the dimensionless relative permeability.

    Hecht

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    3.1.4 Ampres Circular Law

    C A SdJldB

    0A1: 0JA2: no net current0J

    ???

    Moving charges are not the only source of a magnetic field.

    Capacitor:

    A

    QE

    as the charge varies, the electric field changes

    Taking the derivative of both sides

    A

    i

    t

    E

    Effective current density

    Maxwell hypothesized the existence ofdisplacementcurrent density.

    t

    EJD

    Rewrite Ampres Law as

    C A

    Sdt

    EJldB

    )(

    Note: a time-varying field will be accompanied by a

    field even whenE

    B

    0J

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    3.1.5 Maxwells Equations

    C A Sdt

    EJldB

    )(

    A SdB 0

    A V dVSdE 01

    c A

    Sdt

    BldE

    Free space

    0

    0

    0

    0

    J

    C A Sdt

    E

    ldB

    00

    A SdB 0

    A SdE 0

    c A

    Sdt

    BldE

    Eaffects Bwhile Bin turn affects E

    Symmetries of Math and Physics!

    Youre beautiful!

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    3.1.5 Maxwells Equations

    Differential form see Appendix 1 Hecht

    Forfree space, in Cartesian coordinates

    C A

    Sdt

    EldB

    00

    A SdB 0

    A

    SdE 0

    c ASd

    t

    BldE

    Faraday

    Ampere

    Gauss

    Magnetic field of a straight

    wire carrying a current iis:

    riB 2/0 ???

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    3.2 Electromagnetic Waves: application of Maxwell equations

    Time-varying E-field generatesperpendicularB-field

    Time-varying B-field generatesperpendicularE-field

    Consider an accelerating charge

    At the instant the charge begins to move, the Efield is altered and the time-

    varying Efield induces a Bfield.

    The charge is accelerating. Hence the induced Bfield is time-dependent.

    The time-varying Bfield generates an Efield.

    The process continues with Eand Bcoupled in the form of pulse.

    c A

    Sdt

    BldE

    C A

    Sdt

    EldB

    00

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    3.2 Electromagnetic Waves: application of Maxwell equations

    Second differential equations in Cartesian coordinates

    Note: each and every component of the

    electromagnetic field (Ex, Ey, Ez, Bx, By, Bz)obeys the scalar differential wave equation

    2

    2

    22

    2

    2

    2

    2

    21

    tvzyx

    With00

    /1 v

    22182732212

    00/1012.11)/104)(/1085.8( msCkgmkgmCs

    Thus, in free spacethe speed of all electromganetic waves would be

    smv /1031 8

    00

    Light of speed in vacuum smc /1099792458.28

    Latin: celer- fast

    3 2 1 T W

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    3.2.1 Transverse Waves

    2

    2

    002

    tEE

    0

    z

    E

    y

    E

    x

    E zyx

    Explain transverse wave property of light by EM theory

    For example, plane wave propagating in the positive x-direction in vacuum

    The electric field intensity should be a solution of

    and is constant over each of an infinite set of planes perpendicular

    to the x-axis. Hence, it is a function only ofxand t.E

    ),( txEE

    Back to Maxwell Eqs

    0

    x

    Ex),( txEE

    0xE

    xE constant

    No such traveling wave advancing

    in the + x-direction.

    Thus, the EM wave has no Efield component in the direction ofpropagation. The E-field associated with the plane wave is transverse.

    Transverse E-field Many directions (polarizations)

    For plane or linearly polarized waves, E-vector is fixed. For example, y-axis.

    ),(

    txEjE y

    A SdE 0

    3 2 1 T W

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    3.2.1 Transverse Waves

    ),( txEjE y

    t

    B

    x

    Ezy

    The time-dependent B-fieldonly have a component in

    the z-direction.

    In free space, the plane electromagnetic

    wave is transverse.

    Harmonic wave: ])/(cos[),( 0 cxtEtxE yy with a propagation speed ofc.

    The associated magnetic flux density is:

    dtx

    EB

    y

    z

    So, ])/(cos[1

    ),(])/sin[ 00

    cxtEctxBordtcxt

    c

    EB yz

    y

    z

    And zy cBE

    Note:

    Eyand Bzdiffer only by a scalar.

    They have same time-dependence. They are in-phase at all points in space.

    They are mutually perpendicular.

    Their cross-product Ex Bpoints in the propagation direction.

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    3.3 Energy and Momentum

    EM transports energy and momentum. i.e. light from star

    3.3.1 The Poynting Vector

    Radian energy per unit volume orenergy density, u.

    Energy density of the E-field (considering the plates of a charged capacitor)

    20

    2

    EuE

    Energy density of the B-field (considering a current-carrying toroid)

    2

    02

    1BuB

    For plane EM wave:00

    /1

    candcBE

    So, we have BE uu The energy streaming through space in the form ofan electromagnetic wave is shared equally between

    the constituent electric and magnetic fields.

    Further,

    2

    0

    2

    0

    1,, BuEuuuu

    BE

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    3.3.1 The Poynting Vector

    To represent the flow of electromagnetic energy associated with a traveling

    wave, let Ssymbolize the transport of energy per unit time (the power) acrossa unit area. Shas a unit of W/m2 SI system.

    An EM wave traveling with a speed cthroughan area A.

    uctA

    tAucS

    Energy in cylindrical

    volume

    or EBS0

    1

    Poynting vector

    BEcSorBES

    0

    2

    0

    1

    Direction: the energy flows in the direction of the propagation of the wave.

    Magnitude: the power per unit area crossing a surface whose normal is parallel to S

    Example: Harmonic, linearly polarized plane wave traveling through free space inthe direction of k

    )cos()cos(00 trkBBandtrkEE

    )(cos20002 trkBEcS

    Instantaneous flow of energy per unit areaper unit time

    00/1 candcBE

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    Averaging Harmonic Functions

    More practically, due to the extremely rapid changing ofS, we need to take anaveraging procedure to measure S.

    Time-averaged value of some function f(t) over an interval T:

    2/

    2/)(

    1)(

    Tt

    TtTdttf

    Ttf

    For harmonic function:

    )(1

    ))(1

    11

    2/2/

    )2/(2/(

    2/

    2/

    2/

    2/

    TiTiti

    T

    ti

    TtiTti

    T

    ti

    Tt

    Tt

    Tt

    Tt

    titi

    T

    ti

    eeeTie

    eeTi

    e

    eTi

    dteT

    e

    ti

    T

    ti

    eT

    T

    e

    )2/

    2/sin

    (

    sinc u

    u = , 2, 3..

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    3.3.2 Irradiance

    The amount of light illuminating a surface is called irradiance, Ithe averageenergy per unit area per unit time.

    How to measure I?The time-averaged value (T>>) of the magnitude of the Poynting vector,

    T is a measure ofI.

    Harmonic Wave:

    )(cos20002 trkBEcS T Tfor

    T

    2/1cos2

    000

    2

    2BE

    cS T

    or 20

    0

    2E

    cSI

    T

    The irradiance is proportional to the square

    of the amplitude of the electric field.

    Alternatively,TT

    EcIandBc

    I 2020

    Radian flux (optical power), W: the time rate of flow of radiant energy

    Radiant flux density W/m2: radian flux incident on or exiting from a unit area surface

    EBS0

    1

    00/1 candcBE

    A di

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    Magnetic Field due to Conduction Current

    24

    Io

    dd

    r

    s r

    B

    Biot-Savart Law

    Refers to magnetic field due tothecurrent-carrying conductor

    o

    = 4 x 10-7 T.m / A

    permeability of free space

    Unit vector

    Appendix:

    A di

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    Magnetic Field due to Conduction Current

    To find the total field, sum up thecontributions from all the currentelements Ids

    24

    Io d r

    s rB

    Integration over the entire

    current distribution

    Vector sum

    Useful to high-symmetry currents

    2

    4

    Io

    dd

    r

    s rB

    Appendix:

    A di

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    Example 1: B for a Circular Loop of Wire

    Magnetic field at the centerof a current loop

    r

    I

    r

    IB

    r

    r

    r

    rds

    2

    2

    4

    2

    00

    22

    rI

    24

    Io

    d

    r

    s rB

    Appendix:

    A di

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    Example 2: B for a Long, Straight Conductor

    The thin, straight wire

    is carrying a constant

    current

    Integrating over all the

    current elements gives

    2

    1

    1 2

    4

    4

    Isin

    Icos cos

    o

    o

    B da

    a

    sin

    d dx s r k

    Appendix:

    A di

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    B for a Long, Straight Conductor, Direction

    aI

    aIB

    22

    400

    2

    1

    1 2

    4

    4

    Isin

    Icos cos

    o

    o

    B d

    a

    a

    From previous results

    Now let 1=0, 2=, we have

    back

    Appendix:

    A di

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    Energy density of the E-field (considering the plates of a charged capacitor) 20

    2EuE

    The work to move a charge element dq from the negative plate to the

    positive plate is equal to Vdq, where Vis the voltage on the capacitor.

    C=Q/V

    (1)

    (2)

    (3)

    (4)

    (5)

    Appendix:

    Appendix:

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    The instantaneous power which must be suppliedto initiate the current in the inductor is

    The energy density (energy/volume)

    Energy density of the B-field (considering a current-carrying toroid) 2

    02

    1BuB

    (1)

    (2)

    (3)

    back

    Appendix:

    Appendi

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    Field Due to a Long Straight Wire

    Want to calculate themagnetic field at adistance rfrom the center

    of a wire carrying asteady current I

    The current is uniformlydistributed through the

    cross section of the wire

    Appendix:

    Appendix

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    Field Due to a Long Straight Wire

    Outside of the wire, r> R

    Inside the wire, we need I, the current insidethe amperian circle

    2

    2

    ( ) I

    I

    o

    o

    d B r

    B

    r

    B s

    2

    2

    2

    2

    2

    ( ) I ' I ' I

    I

    o

    o

    rd B r R

    B r

    R

    B s

    Appendix:

    Appendix:

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    Field Due to a Long Straight Wire

    The field is proportional

    to rinside the wire

    The field varies as 1/r

    outside the wire Both equations are

    equal at r= R

    Appendix: