In the weight-zero convention, a Maass form for a discrete subgroup is a smooth function on the upper half-plane, invariant under , satisfying a hyperbolic Laplacian eigenvalue equation and specified growth conditions at the cusps:
Additional conditions specify a cuspidal or square-integrable class. The sign of is a convention and must be stated.[ref]
The constant function is an invariant eigenfunction with and moderate growth, but is not cuspidal: its average along a horizontal period is nonzero. A Maass cusp form has zero such constant term at each cusp. The eigenfunction condition allows nonholomorphic automorphic forms, connecting arithmetic symmetries with spectral geometry.
A shifted polyharmonic Maass form is a smooth automorphic function that satisfies a generalized eigenfunction equation for a hyperbolic Laplacian. In weight zero, choose the convention and require
for an integer , together with automorphy and the specified growth conditions at each cusp. Moderate growth means at most polynomial growth in cusp coordinates. The weight- version replaces by the corresponding Weight-k hyperbolic Laplacian and uses the weight- transformation law.[ref]
The least possible is the exact depth. For this is an ordinary eigenfunction condition; higher depth allows a chain of generalized eigenfunctions. It is not merely an equation with a different eigenvalue. The cited paper uses the opposite Laplacian sign, so its eigenvalue parameter is the negative of the one used here.
For an illuminating construction, let a nonholomorphic Eisenstein series satisfy . At a regular value , differentiate in . The function obeys
The first right-hand side is nonzero, so this gives depth two. Parameter differentiation introduces a generalized eigenfunction while preserving automorphy.[ref]
In the integer-depth convention, a polyharmonic Maass form is a smooth automorphic function annihilated by a positive integer power of its weight-appropriate hyperbolic Laplacian, with specified growth at the cusps. In weight zero, using , the equation is . It is the zero-shift case of a shifted polyharmonic Maass form. Exact depth is the least such integer . Some refined conventions also use half-integer depths, so the convention must be stated.[ref]
A global depth-two example comes from the finite part of a completed nonholomorphic Eisenstein series. Near , write
where is a nonzero constant and . Comparing constant Laurent coefficients gives , hence but . The finite part is automorphic and has moderate growth.[ref]
This demonstrates why higher depth is substantive: the space contains functions that are not harmonic but become harmonic after one application of the Laplacian. Merely solving a local differential equation is insufficient; automorphy and cusp growth remain part of the definition.
A Maass cusp form is a nonzero Maass form with vanishing constant term of an automorphic form at every cusp. For weight zero on the modular group , it is a smooth, -invariant function on the upper half-plane, square-integrable on a fundamental domain with measure , satisfying
The integral condition describes the cusp at infinity; other groups require the corresponding condition in coordinates at each cusp.[ref]
Translation invariance gives a Fourier series. When , its decaying modes have the form
where is a Modified Bessel function of the second kind. The absent term expresses cuspidality. The Fourier coefficients must also satisfy the full automorphic symmetry.[ref]
The constant function is a useful test: it satisfies the symmetry and has eigenvalue zero, but its horizontal average is , so it is not a Maass cusp form. The extra condition isolates oscillating eigenfunctions connecting arithmetic symmetry with spectral geometry.

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