Light Beams in High-Order Modes
A recent project that we have been working on involves the geometric phase that results from cyclic changes in the modes of a higher-order Gaussian beam. A set of the beam modes of a Gaussian beam carry orbital angular momentum. Patrick Crawford (Summer 2002), Matt Pysher (Summer 2002), Henry Sztul (Spring 2000 and 2001) and PJ Haglin (Summer 2000) have been working on this project. We have done the first measurements of this phase for optical beams. An article on this work appeared recently in Physical Review Letters [PRL 90, 203901 (2003)].
When you have a collimated beam of light the wave equation in three
dimensions becomes the paraxial wave equation. This equation can be solved in
either Cartesian or cylindrical coordinates. The solution in Cartesian
coordinates gives a family of solutions expressed in terms of Hermite
polynomials multiplied by a Gaussian envelope. These Hermite-Gauss solutions (or
modes) are categorized by their indices (n,m) and "order" N=n+m. The
Hermite-Gauss (HGnm) of order zero, HG00 is the usual output of an ordinary laser (TEM00):
All
the points on a transverse plane
have the same phase:

That is, if we show the surfaces containing points that have the same phase
(e.g. crests, like in the figure), these surfaces are planes separated by a
wavelength. Higher order solutions have more complex profiles, like HG10:
HG20:
and HG30:
. Hermite-Gauss modes do
not carry orbital angular momentum.
The solutions of the paraxial wave equation in cylindrical coordinates give
rise to a family of modes, expressed in terms of the product of a Laguerre
polynomial of radial index p and axial index l, a Gaussian
envelope and a phase term that depends on the product of the transverse angular
coordinate and the radial index l. Light beams in Laguerre-Gauss (LGpl)
beams carry orbital angular momentum ( l h/2p
per photon) . The lowest order mode LG00 is the same as the
HG00. The first order modes LG0+1
and LG0-1 have intensity profiles that are radially
symmetric , with zero intensity in the center:
. When the light
beam in this mode is projected on a screen it looks like a "doughnut:"
. But more interesting is
the phase structure of this wave. The phase winds as a function of the angle:
points at opposite sides of the doughnut are 180 degrees out of phase, and
points 90 degrees from each other with respect to the center are 90 degrees out
of phase. In a transverse plane, the phase smoothly advances with angle,
counter-clockwise for LG0+1 and
clockwise for LG0-1. One way to represent this phase
structure is the following figure:
. Points of equal color
have the same phase. Another view is shown below, where the phase of the wave on
a transverse cut is shown. The red dots mark the intersection of the wave with
the transverse plane: see how the phase advances in a circle around the center
of the plane.

Since the center has "all phases" it is a phase singularity. This explains why the intensity
of the beam is zero at that point. If we were
to show the points of equal phase as the wave propagates, from a
right-handed corkscrew spiral for LG0+1
we would get:
, and for a left-handed
corkscrew spiral for LG0-1 :
. It is important to
understand that the light is not following a helical path. The phase of
the light is
changing in such a way that it describes a helix, as shown in the figure below. The contour
plot gives the intensity distribution of the doughnut. Points of the beam that
have the same phase (e.g., crests in the figure) describe a helix. The pitch of
the helix is one wavelength.

The orbital angular momentum arises from this phase structure. The local linear momentum density of the wave (p=e0ExB) has an axial component. For an expanding Gaussian beam in the lowest order (TEM00 or LG00) the linear momentum has radial and longitudinal components, as shown below.

For a beam with orbital angular momentum, the spiral phase front gives rise to an axial component of the linear momentum.

Thus, an integration of the angular momentum (L=rxp) over the entire profile gives rise to a component of angular momentum along the propagation direction [For more on this see L. Allen and M. Padgett, Optics Communications 184, 67-71 (2000) and G.A. Turnbull et al. Optics Communications 127, 183-188 (1996).].
We can make these beams in the laboratory in different ways. The easiest way involves using a computer-generated hologram. If we calculate the interference pattern generated by combining LG00 and LG0+1,

and print out an fringe pattern in binary form, we get a "forked" pattern, shown below. The fork reveals the phase singularity.

If we photo-reduce this image, we can use it as a diffraction grating. If we then shine a laser beam onto it we get

We can verify the first order is indeed the LG0+1 mode by interfering it with the zero order LG00:

[If you want to generate your own doughnuts click here.]
Our interference experiments can get fancier but also much more fun. If we set up a Mach Zehnder interferometer, like the one shown below
and put the forked grating before the first beam splitter, we
will have copies of the interference pattern shown above traveling both arms of
the interferometer. We can align the mirrors so that after the interferometer we
have the modes LG00 and LG0+1
superimposed. Then... we expand the LG00 mode by placing a
lens in the corresponding arm of the interferometer (you can do this also in a
Michelson interferometer). If both interfering beams were LG00
the pattern would be concentric circles:
, but if the unexpanded
beam is in the LG0+1 mode then the
interference pattern looks like a spiral:
. If we change the
length of one of the arms get the ...Mesmerizer!
(Short mpg video made by Henry Sztul.).
So far we have discussed first order modes. Second order modes such as LG0+2
also have a doughnut profile but with a phase that winds twice as fast as the LG0+1
mode. The points of equal phase wind about the axis forming a double helix:
. An interference
pattern with an expanding reference beam yields a double spiral: .
HG modes can be transformed into LG modes and vice versa using "mode transformers." These are made of cylindrical lenses. They exploit the Gouy phase to insert the proper phases that convert one set of modes into the other. The possibility of making these conversions was first reported by Allen and co-workers [L.Allen, M.W. Beijersberger, R.J.C. Spreew and J.P. Woerdman, Phys. Rev. A 45, 8185-9 (1992)]. For first order modes we have the following identities:

One "equation" can quickly become the other by inserting a 90-degree phase between HG10 and HG01. The transformation is made via the Gouy phase shift. This phase is a little known "secret" of wave propagation. It arises when a light wave goes through a waist after being focused by a lens, as shown below.

We have measured this phase using the Mach-Zehnder interferometer shown above. We interfere an LG00 beam with a copy of itself that is being focused by a positive lens. We then move the camera before and after the focal plane of the lens. One can see that the phase between the two waves changes as we go through the waist of the beam being focused. You can see it for yourself in this mpg video made by Henry Sztul.
Further readings:
"An Experiment to Observe the Intensity and Phase Structure of Laguerre-Gaussian Laser Modes," M. Padgett, J. Arlt, and N. Simpson, American Journal of Physics 64, 77-82 (1996).
"Light with a Twist in its Tail," M. Padgett and L. Allen, Contemporary Physics, 41, 275-285 (2000).
"Astigmatic Mode Converters and the Transfer of Orbital Angular Momentum," M.W. Beijersbergen, L. Allen, H.E.L.O. van der Veen and J.P. Woerdman, Optics Communications 96, 123-132 (1993).
[The background image is a double spiral interference pattern produced by a LG02 mode taken by P.R. Crawford (2002).]
This work has received support by an award from Research Corporation: "Geometric Phase of Optical Beams Possessing Angular Momentum" (2000-2002) and from NSF grant RUI-9988004.
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