
Generalized solution of the paraxial equation
Tomasz Rado˙zycki∗
Faculty of Mathematics and Natural Sciences, College of Sciences, Institute of Physical Sciences,
Cardinal Stefan Wyszy´nski University, W´oycickiego 1/3, 01-938 Warsaw, Poland
A fairly general expression for a light beam is found as a solution of the paraxial Helmholtz
equation. It is achieved by exploiting appropriately chosen complex variables which entail the
separability of the equation. Next, the expression for the beam is obtained independently by super-
imposing shifted Gaussian beams, whereby the shift can be made either by a real vector (in which
case the foci of the Gaussian beams are located on a circle) or by a complex one. The solutions
found depend on several parameters, the specific choice of which allows to obtain beams with quite
different properties. For several selected parameter values figures are drawn, demonstrating the
spatial distribution of the energy density and phase. In special cases, the effect of a shift of the
intensity peak from one branch to another and phase singularities are observed.
I. INTRODUCTION
Within the scalar optics approximation a number of
monochromatic paraxial light beams of intriguing prop-
erties have been found. From the mathematical perspec-
tive, assuming the propagation along the z-axis, they are
described as solutions of the so-called paraxial equation:
4⊥ψ(r, z)+2ik∂zψ(r, z) = 0,(1)
where the stationary function ψ(r, z), called the envelope,
is related to the electric field via
E(r, z, t) = E0eik(z−ct)ψ(r, z),(2)
with E0representing a constant vector. The Laplace op-
erator 4⊥in (1) is the two-dimensional one acting in
the transverse plane only (here r= [x, y]). The symbol
∂zstands for the partial derivative ∂
∂z . The approxima-
tions leading to the form (1) have been discussed in detail
elsewhere [1, 2].
A commonly accepted fundamental solution of the
paraxial equation is the Gaussian beam, which in the
cylindrical coordinates has the form (apart from the nor-
malization constant):
ψ(r, ϕ, z) = w0
w(z)n+1rneinϕ (3)
×exp h−r2
w(z)2+ikr2
2R(z)−i(n+ 1)ψG(z)i
endowed (n6= 0) or not (n= 0) with orbital angular
momentum with respect to the propagation axis [2–12].
The basic parameters that characterize this beam (w0
– the waist radius, w(z) = w0p1+(z/zR)2– radius at
a distance z,R(z) = z(1 + (zR/z)2) – the wavefront-
curvature radius, zR=kw2
0/2 – the Rayleigh length
and ψG(z) = arctan(z/zR) – the Gouy’s phase) are well
known and need no further explanation. This beam, writ-
ten in a slightly modified although equivalent form, will
be of use in the present work (see (18)).
∗t.radozycki@uksw.edu.pl
Other beams of similar nature include Bessel-Gaussian
(BG) [12–15], modified BG [16–18], Laguerre-Gaussian
(LG) [2, 12, 15, 19–23], Kummer-Gaussian (KG) (i.e.,
Hypergeometric-Gaussian) [24, 25], or γbeams [26], the
latter containing no Gaussian fall-off factor. All of them
are cylindrical in the sense that the wave intensity dis-
plays axial symmetry. Equation (1) has also solutions of
another kind, which do not manifest cylindrical symme-
try. As examples, one can mention Hermite-Gaussian
(HG) beams [2, 27] of rectangular symmetry, or Airy
beams [28–30].
The literature on this subject is extremely vast due
to the important and broad applications of light beams,
especially those with nontrivial structure, ranging from
trapping and guiding of particles, through image pro-
cessing, optical communication, harmonics generation in
nonlinear optics, quantum cryptography, up to biology
and medicine.
Some attempts to obtain a more general description
and/or derivation of various paraxial beams have been
undertaken in the past [18, 31–35]. In this paper, we
wish to present, along these lines, somewhat more general
solution to the equation (1), which depends on several
parameters remaining at our disposal. These general so-
lution does not exhibit cylindrical symmetry (in the sense
spoken of above), except for some special cases. A partic-
ular choice of the parameters values enables on one hand
to recover some of the above-mentioned modes, and on
the other to obtain other modes with equally interesting
properties.
The solution in question will be obtained below in two
ways. First, in Section II, some specially defined substi-
tutions are used, which leads in two steps to the com-
plete separation of the paraxial equation. It is known
that the Helmholtz equation in 3 dimensions, owing to
the Robertson-Eisenhart condition [36, 37], turns out to
be separable in 11 orthogonal coordinate systems [38].
However, in order to obtain new solutions, in this work
complex variables will be employed.
Then, in Section III, it is demonstrated that, at least
for integer values of the parameter l(see (14)), these so-
lutions are superpositions of shifted zero-order Gaussian
beams [39] with some appropriately tailored weight func-
arXiv:2210.01088v1 [physics.optics] 3 Oct 2022