- Selberg zeta function
The Selberg zeta-function was introduced by
Atle Selberg in the 1950s. It is analogous to the famousRiemann zeta function : where is the set of prime numbers. The Selberg zeta-function uses the lengths of simpleclosed geodesic s 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 thecomplex plane . The zeta function is defined in terms of the closedgeodesic s 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 there exists a zero at the point . The order of the zero equals the dimension of the corresponding eigenspace. (A cusp form is an eigenfunction to theLaplace-Beltrami operator which hasFourier expansion with zero constant term.)
# The zeta-function also has a zero at every pole of the determinant of the scattering matrix, . 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 .
Selberg zeta-function for the modular group
For the case where the surface is , where 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 , then the scattering matrix has a pole at , and hence the Selberg zeta-function has a zero at .
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.
Wikimedia Foundation. 2010.