Selberg zeta function
From Wikipedia, the free encyclopedia
From Wikipedia, the free encyclopedia
The Selberg zeta-function was introduced by Atle Selberg (1956). It is analogous to the famous Riemann zeta function
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where is the set of prime numbers. The Selberg zeta-function uses the lengths of simple closed geodesics instead of the prime numbers. If is a subgroup of SL(2,R), the associated Selberg zeta function is defined as follows,
or
where p runs over conjugacy classes of prime geodesics (equivalently, conjugacy classes of primitive hyperbolic elements of ), and N(p) denotes the length of p (equivalently, the square of the bigger eigenvalue of p).
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:
The zeta-function also has poles at , and can have zeros or poles at the points .
The Ihara zeta function is considered a p-adic (and a graph-theoretic) analogue of the Selberg zeta function.
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 determinant of the scattering matrix is given by:
In particular, we see that if the Riemann zeta-function has a zero at , then the determinant of the scattering matrix has a pole at , and hence the Selberg zeta-function has a zero at .[citation needed]
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