
doi: 10.1007/bf02172464
Let \(h(d)\) denote the class number (in the narrow sense) of indefinite binary quadratic forms of discriminant \(d>0\) (\(d\equiv 0\) or \(1\bmod 4\), \(d\) not a square). The growth of \(h(d)\) for \(d\to \infty\) is well known to be quite erratic due to the irregular growth behaviour of the fundamental unit \(\varepsilon(d)\) of the corresponding real quadratic field. In consequence of this the growth of \(\sum_{d\leq X} h(d)\) for \(X\to \infty\) is hard to estimate. However, a different mode of enumeration of the \(h(d)\) according to the size of \(\varepsilon(d)\) leads to the sum \(\sum_{\varepsilon(d)\leq X}h(d)\) whose asymptotic behaviour can be determined by means of the Selberg zeta-function since this sum is closely related with the distribution of norms of primitive hyperbolic elements of \(SL_2(\mathbb{Z})\). The author introduces an additional summation condition and proves: There exists an absolute constant \(C>0\) such that \[ \sum_{\substack{ \varepsilon(d)\leq X\\ h(d)< C\sqrt{d}/ \log^2d }} h(d)= O(X\log^3 X) \quad\text{for}\quad X\to \infty. \]
class number, Selberg zeta functions and regularized determinants; applications to spectral theory, Dirichlet series, Eisenstein series, etc. (explicit formulas), Spectral theory; trace formulas (e.g., that of Selberg), quadratic field, asymptotic behaviour, binary quadratic forms, Selberg zeta-function, Class numbers of quadratic and Hermitian forms, Asymptotic results on arithmetic functions, fundamental unit, distribution of norms of primitive hyperbolic elements
class number, Selberg zeta functions and regularized determinants; applications to spectral theory, Dirichlet series, Eisenstein series, etc. (explicit formulas), Spectral theory; trace formulas (e.g., that of Selberg), quadratic field, asymptotic behaviour, binary quadratic forms, Selberg zeta-function, Class numbers of quadratic and Hermitian forms, Asymptotic results on arithmetic functions, fundamental unit, distribution of norms of primitive hyperbolic elements
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