Minakshisundaram–Pleijel zeta function

Minakshisundaram–Pleijel zeta function

The Minakshisundaram–Pleijel zeta function is a zeta function encoding the eigenvalues of the Laplacian of a compact Riemannian manifold. It was introduced by Subbaramiah Minakshisundaram and Åke Pleijel (1949). The case of a compact region of the plane was treated earlier by Carleman (1935).

Contents

Definition

For a compact Riemannian manifold M of dimension N with eigenvalues \lambda_1, \lambda_2, \ldots of the Laplace–Beltrami operator Δ the zeta function is given for \operatorname{Re}(s) sufficiently large by

 Z(s) = \operatorname{Tr}(\Delta^{-s}) = \sum_{n=1}^{\infty} \vert \lambda_{n} \vert^{-s}.

(where if an eigenvalue is zero it is omitted in the sum). The manifold may have a boundary, in which case one has to prescribe suitable boundary conditions, such as Dirichlet or Neumann boundary conditions.

More generally one can define

 Z(P, Q, s) = \sum_{n=1}^{\infty} \frac{f_n(P)f_n(Q)}{ \lambda_{n}^s}

for P and Q on the manifold, where the fn are normalized eigenfunctions. This can be analytically continued to a meromorphic function of s for all complex s, and is holomorphic for PQ. The only possible poles are simple poles at the points s = N/2, N/2−1, N/2−2,..., 1/2,−1/2, −3/2,... for N odd, and at the points s = N/2, N/2−1, N/2−2, ...,2, 1 for N even. If N is odd then Z(P,Q,s) vanishes for s = 0, −1, −2,... The function Z(s) can be recovered from this by integrating Z(P, P, s) over the whole manifold M:

\displaystyle Z(s) = \int_M Z(P,P,s)dP

Heat kernel

The analytic continuation of the zeta function can be found by expressing it in terms of the heat kernel

 K(P,Q,t) = \sum_{n=1}^{\infty} f_n(P)f_n(Q) e^{- \lambda_{n}t}

as the Mellin transform

 Z(P,Q,s) = \frac{1}{\Gamma(s)} \int_0^\infty K(P,Q,t) t^{s-1} dt

The poles of the zeta function can be found from the asymptotic behavior of the heat kernel as t→0.

Example

If the manifold is a circle of dimension N=1, then the eigenvalues of the Laplacian are n2 for integers n. The zeta function

Z(s) = \sum_{n\ne 0}\frac{1}{(n^2)^s} = 2\zeta(2s)

where ζ is the Riemann zeta function.

References


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