11-30 Two Beam Interferoemters

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    19.

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    Michelson Interferometer

    Sagnac Interferometer

    Fizeau Interferometer

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    L1

    L2

    =4(n1L1-n2L2)/

    Measuring the intensity of theoutput allows us to infer the values

    of physical parameters n, L or

    I0

    Iout

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    From 1980-1983 the meter was defined as1579800.299 wavelengths of light from a HeNelaser. How could you reproduce the standard

    meter in a lab?

    Scan one mirror as you count off twice thismany fringes. The distance it travels would be

    one meter

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    The output field varies depending on wavelength and on the path lengthdifference

    giving an output intensity (for r2=t2=1/2) of

    if one of the mirrors moves at constant velocity, such that

    The output signal will be modulated at a frequency

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    With the expression

    the wavelength of a source can bemeasured by comparing the modulationfrequency for that source to themodulation frequency of a knownreference

    If N=L/ is the number ofinterference fringes that are countedthe measurement error / is 1/Ngiving a resolving power of

    Output intensity as a function of time

    Schematic of a scanning Michelson interferometersource: Andrews and Demidov

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    L1

    L2

    =4(n1L1-n2L2)/

    Measuring the intensity of theoutput allows us to infer the values

    of physical parameters n, L or

    I0

    Iout

    vacuum chamber

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    How can you measure the index ofrefraction of air?

    L1

    L2

    =4(n1L1-n2L2)/

    I0

    Iout

    vacuum chamber

    count the fringes as air is let back into a vacuumchamber of known length in one arm

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    What do we mean by count the fringes?

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    04 -7500 -5000 -2500 0 2500 5000 7500 1!1

    -5000

    -2500

    2500

    5000

    fringe pattern of analigned Michelson withan arm length mismatch

    ofL

    fringe pattern of analigned Michelson withan arm length mismatch

    ofL+/10

    04 -7500 -5000 -2500 0 2500 5000 7500 1!1

    -5000

    -2500

    2500

    5000

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    How accurately can we count fringes?

    Shot noise produces noise that causes the intensity to fluctuate by

    where N=Pt/h is the number of photons detected in our measurement of

    time t. This is related to the phase shift on the side of a fringe by

    So the minimum detectable phase shift is

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    Veff =v

    vI= I/

    N

    0

    I

    dI

    d= I

    min =1N

    =

    h

    Pt

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    What is the smallest displacement of a Michelson mirror that can bemeasured by a 500 mW Nd:YAG laser with a wavelength of=1064nm in aone second measurement?

    12

    min =1

    N=

    h

    Pt

    =

    hc

    Pt

    = (6.63 1034 J s)(3 108 m/s)(1064 109 m)(500 103 W)(1 s)

    = 6 1010 radfrom =2(2L)/ for a Michelson interferometer

    Lmin=min/4=5x10-17 m

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    A detector with a finite size aperture wil tend toaverage out the fringes that are incident on thedetector. The effective visibility is

    and the actual detectable phase shift is

    act=min/Veff

    one could minimize the detector size to avoid thisproblem, but that would limit the detected power andhence decrease min. Alternatively if theinterferometer is well aligned, the fringes becomecourser than the detector 13

    Veff = vmax

    vmin

    vmax + vmin

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    What does the output interferencepattern look like when theinterferometer is aligned? When it

    is misaligned?

    L1

    L2

    =4(n1L1-n2L2)/

    I0

    Iout

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    Two counter-propagatingbeams interfere. Sincebeams travel the samepath (in opposite

    directions) this devicehas very good commonmode noise rejection, andis primarily sensitive topath length changes at

    high frequency

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    Consider the effect ofrotation on a squareSagnac interferometer

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    transit time is tt=4L/c, additional path lengthdue to rotation during that time is LLtt,so =16L2/c or =16A/, and is avery sensitive measure of rotation

    L

    note: to treat this problem properly requires a full relativistic treatment not considered here

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    An air wedge between two glassplates to generate fringes that have aspacing proportional to thewavelength

    To prevent aliasing on the m-elementdetector array we must have thenumber of fringes N=2d/ less thanm/2 giving a limit on d

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    Many configuration of amplitude splittinginterferometers exist that allow physicalquantities to be measured with extremesensitivity

    Even if all technical sources of noise can beeliminated, shot noise will still exist and limitthe sensitivity of any optical measurement

    Alignment, power, and measurement time allaffect the sensitivity of measurements madewith an interferometer

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