 Hermite-Gaussian optical mode

A Hermite-Gaussian optical mode is a separable paraxial field pattern whose transverse dependence is a product of Hermite polynomials and a Gaussian beam envelope. In an ideal aligned optical resonator with suitable spherical mirrors, these patterns form a family of transverse optical cavity modes. The two nonnegative integer orders $m,n$ count the straight nodal lines along the chosen transverse axes. The primary photonics notes give the mode fields and their order-dependent phase advance.^[ref]

At a common waist plane, choose a unit-normalized scalar fieldHere $H_j$ uses the physicists' Hermite polynomial convention, with $H_0(s)=1$, $H_1(s)=2s$ and $H_2(s)=4s^2-2$. The normalization follows fromAfter the two coordinate substitutions, $\iint u_{mn}^{\ast }{u}_{pq}dxdy={\delta }_{mp}{\delta }_{nq}$. Thus coefficients in a common-plane expansion can be recovered by inner products; the modes are orthogonal field patterns, not independent bright spots.

For $(m,n)=(1,0)$, intensity is proportional to $x^2{e}^{-2(x^2+y^2)/w_0^2}$, so its maxima lie at $x=\pm w_0/\sqrt{2}$, $y=0$. At $w_0=100\mu \mathrm{m}$, the bright lobes are about $141.4\mu \mathrm{m}$ apart. The field changes sign across $x=0$, although an intensity camera records positive intensity on both sides. For $(2,0)$, the nodal lines instead lie at $x=\pm w_0/2$. These patterns are illustrated in transverse optical cavity mode using individually peak-normalized images; equal peak intensity is different from equal integrated power.

A second-moment width of a Hermite-Gaussian optical mode distinguishes these multi-lobed beams quantitatively. Applying the Hermite polynomial recurrence inside the normalized integrals givesFor order $(1,0)$, the RMS widths are $\sqrt{3}{w}_0/2$ horizontally and $w_0/2$ vertically, despite the same envelope parameter $w_0$. Reporting a fitted single-lobe radius without its definition can obscure this difference.

During propagation the beam radius and wavefront curvature evolve, and the Gouy phase is multiplied by $m+n+1$. Consequently, transverse order contributes to the resonator's frequency condition and to confocal transverse-mode degeneracy. A proposed experiment scans the resonator while imaging a specified plane, then interferes its output with a reference field to test the phase reversal across a node. An intensity fit alone does not establish a pure coherent mode: mixtures, astigmatism, finite apertures and degeneracy can alter what is observed.