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]
Shifted polyharmonic Maass forms for PSL(2,Z) by Nickolas Andersen and others. Introduction, depth-one eigenfunction conditions; the paper uses its own Laplacian sign convention
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 requirefor 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]
Shifted polyharmonic Maass forms for PSL(2,Z) by Nickolas Andersen and others. Introduction, equations 1.1–1.2 and growth hypothesis
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 obeysThe 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]
Polyharmonic Maass forms for PSL(2,Z) by Jeffrey C. Lagarias and Robert C. Rhoades. Introduction and harmonic-depth convention
A global depth-two example comes from the finite part of a completed nonholomorphic Eisenstein series. Near , writewhere 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 , satisfyingThe integral condition describes the cusp at infinity; other groups require the corresponding condition in coordinates at each cusp.[ref]
Rigorous computation of Maass cusp forms of squarefree level by Andrei Seymour-Howell. Section 2.1, definition specialized to level one and stated Laplacian sign
Translation invariance gives a Fourier series. When , its decaying modes have the formwhere 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]
Rigorous computation of Maass cusp forms of squarefree level by Andrei Seymour-Howell. Section 2.4, even and odd Fourier expansions, rewritten in complex exponential notation
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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