Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G....

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Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs

Transcript of Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G....

Page 1: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Interferometric Measurement of Spatial Wigner Functions

of LightBryan Killett

Brian J. SmithM. G. Raymer

Funded by the NSF through the REU

and ITR programs.

Page 2: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

What is a spatial Wigner function?

2)()Pr( xx

2

)()Pr(

dxexk xikx

x

BUT - can we define a “joint probability density” function?

In other words, something like: Pr(x,kx).

x

x

Pk where

Given a normalized wave function (x), we know how to construct single-variable probability densities:

Page 3: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

What is a spatial Wigner function?

A straightforward definition of Pr(x,kx) would have to…

2. Allow for a physical interpretation at every point. Therefore,

Pr(x,kx) needs to be non-negative everywhere.

1. Integrate to unity and satisfy the following relations:

UNCERTAINTY PRINCIPLE!

dxkxk xx ),Pr()Pr(

xx dkkxx ),Pr()Pr(

The spatial Wigner function corresponding to (x) is simply a function that fulfills the above condition.

Page 4: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

The spatial Wigner function:

')'()'(),( '2* dxexxxxkxW xikx

x

This function has some other interesting properties:

A single integral along the x axis gives the probability density for kx and vice-versa for the other axis.

A double integral over all x and all kx results in unity.

- It is sometimes negative! Thus, we call it a quasiprobability distribution.

- It is uniquely related to (x) so a measurement of W(x,kx) can be transformed to reveal (x). (not merely (x)2 !)

Page 5: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How do we measure W(x,kx)?

Top Mirror

Output Beam

Input Beam

Page 6: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

The “Top Mirror” rotates the field.

Clockwise(CW) Beam

Counter-Clockwise (CCW) Beam

x

y

y

xx

yx

y

Top Mirror Top Mirror

Page 7: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Image Rotation Mirrors

Top MirrorOn Camera:

Page 8: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How do we measure W(x,kx)?

)()(

Setup Classical

xEx

Only one output is measured.

Input Beam

Page 9: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How does the interferometer work?

Input Beam

)'(0 xE

)'()'( 0 xExE

Page 10: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How does the interferometer work?

)'()'( 0 xxExE

Input Beam

)'(0 xE

)'()'( 0 xExE

Page 11: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How does the interferometer work?

'xikxe

Input Beam

)'(0 xE

)'()'( 0 xxExE

Page 12: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How does the interferometer work?

'0'

021 )'()'()'( xikxik

outputxx exxEexxExE

)'()'()'( xExExE CCWCWoutput

Input Beam

)'(0 xE

)'()'( 0 xxExE 'xikxe

Page 13: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

How does the interferometer work?

'0'

021 )'()'()'( xikxik

outputxx exxEexxExE

),(CC 21 xkxWI

'0'

021 )'()'()'( xikxik

outputxx exxEexxExE

The detector measures total power, which is the intensity ofthe output beam integrated over the face of the detector:

')'(2dxxEI output

')'()'( '2*0021 dxexxExxECC xikx

Page 14: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: TEM-00

(This mode is producedfrom a laser with standard

spherical mirror resonators.)

Page 15: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: TEM-00

Theory Experiment

Page 16: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: TEM-10

(This mode is producedfrom a laser with standard

spherical resonators.)(This mode is produced

from a laser with standardspherical mirror

resonators.)

Page 17: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: TEM-10

Notice that W(x,kx)is negative at some

points.

Theory Experiment

Page 18: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: Two Beam Interference

Glass plate

Page 19: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: Two Beam Interference

Theory Experiment

Page 20: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Wigner Results: Simulated Decoherence Effects

Experiment(No Decoherence)

Experiment(With Decoherence)

Page 21: Interferometric Measurement of Spatial Wigner Functions of Light Bryan Killett Brian J. Smith M. G. Raymer Funded by the NSF through the REU and ITR programs.

Future work

• Examine single photon states like the Schrodinger Cat state.

• Analyze the effect of scattering and decoherence on the spatial Wigner function.

• Bell inequalities/entanglement measurements with two interferometers.

See also a paper by our collaborators:“Direct Measurement of the spatialWigner function with area-integrated detection” in Optics Letters Vol 28, #15, by E. Mukamel et. al.