Selberg zeta function
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The Selberg zeta-function was introduced by Atle Selberg in the 1950s. It is analogous to the famous Riemann zeta function : where is the set of prime numbers. The Selberg zeta-function uses the lengths of simple closed geodesics to instead of the primes numbers.
For any hyperbolic surface of finite area there is an associated Selberg zeta-function; this function is a meromorphic function defined in the complex plane. The zeta function is defined in terms of the closed geodesics of the surface.
The zeros and poles of the Selberg zeta-function, Z(s), can be described in terms of spectral data of the surface.
The zeros are at the following points:
- For every cusp form with eigenvalue s0(1 − s0) there exists a zero at the point s0. The order of the zero equals the dimension of the corresponding eigenspace. (A cusp form is an eigenfunction to the Laplace-Beltrami operator which has Fourier expansion with zero constant term.)
- The zeta-function also has a zero at every pole of the determinant of the scattering matrix, φ(s). The order of the zero equals the order of the corresponding pole of the scattering matrix.
The zeta-function also has poles at , and can have zeros or poles at the points .
[edit] Selberg zeta-function for the modular group
For the case where the surface is , where Γ is the modular group, the Selberg zeta-function is of special interest. For this special case the Selberg zeta-function is intimately connected to the Riemann zeta-function.
In this case the scattering matrix is given by:
In particular, we see that if the Riemann zeta-function has a zero at s0, then the scattering matrix has a pole at s0 / 2, and hence the Selberg zeta-function has a zero at s0 / 2.
[edit] Bibliography
- Hejhal, D. A. The Selberg trace formula for PSL(2,R). Vol. 2, Springer-Verlag, Berlin, 1983.
- Iwaniec, H. Spectral methods of automorphic forms, American Mathematical Society, second edition, 2002.
- Venkov, A. B. Spectral theory of automorphic functions. Proc. Steklov. Inst. Math, 1982.
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