Gaussian Beams as Background Fields
When solving for the scattered field, the background wave type can be set to a predefined Gaussian beam from within the Settings of The Electromagnetic Waves, Frequency Domain Interface. In the paraxial approximation the background field for a Gaussian beam propagating along the z-axis is defined below,
,
where w0 is the beam radius, p0 is the focal plane on the z-axis, Ebg0 is the background electric field amplitude and the spot radius for different positions along the propagation axis is given by
.
defines the radius of curvature for the phase of the field and the so called Gouy phase shift is given by
.
The equations above are expressed using the Rayleigh range z0 and the transverse coordinate ρ, defined by
.
Note that the time-harmonic ansatz in COMSOL is ejωt and with this convention, the beam above propagates in the +z-direction. The equations are modified accordingly for beams propagating along the other coordinate axes.
The background field for a Gaussian beam is defined in a similar way for 2D components. In the particular case where the beam propagates along the x-axis, the background field is defined as
.
For a beam propagating along the y-axis, the coordinates x and y are interchanged.
Notice that the expressions above for Gaussian beams are not solutions to the Helmholtz equation, but to the so called paraxial approximation of the Helmholtz equation. This means that these equations become less accurate the smaller the spot radius is and should not be used when the spot radius is of the same size as or smaller than the wavelength.
To circumvent the problem that the paraxial approximation formula is not a solution to the Helmholtz equation, a plane wave expansion can be used to approximate a Gaussian beam. Since each plane wave is a solution to Helmholtz equation, also the expansion is a solution to Helmholtz equation.
The plane wave expansion approximates the Gaussian distribution in the focal plane
where the beam is assumed to be propagating in the z-direction, the focal plane is spanned by the x and y coordinates, e is the unit magnitude transverse polarization in the focal plane, l and m denote the indices for the wave vectors, the index n accounts for the two polarizations per wave vector klm, almn is the amplitude, un(klm) is the unit magnitude polarization, and r is the position vector.
Multiplying with the conjugate of the exponential factor above and the polarization factor un(klm) and applying a surface integral over the entire focal plane allows us to extract the amplitudes as
,
where kt,lm is the magnitude of the transverse wave vector component.