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An upper bound on the denominator of Eisenstein classes in Bianchi manifolds

Romain Branchereau

Abstract

A general conjecture of Harder relates the denominator of the Eisenstein cohomology of certain locally symmetric spaces to special values of $L$-functions. In this paper we consider the locally symmetric space $\operatorname{SL}_2(\mathcal{O}) \backslash \mathbb{H}_3$ where $\mathcal{O}$ is the ring of integers of an imaginary quadratic field $K$ and $\mathbb{H}_3$ is the hyperbolic $3$-space. Tobias Berger proves a lower bound on the denominator of the Eisenstein cohomology in certain cases. The goal of this paper is to show how results of Ito and Sczech can be used to prove an upper bound on the denominator in terms of a special value of a Hecke $L$-function. When the class number of $K$ is one, we combine this result with Berger's result to obtain the exact denominator.

An upper bound on the denominator of Eisenstein classes in Bianchi manifolds

Abstract

A general conjecture of Harder relates the denominator of the Eisenstein cohomology of certain locally symmetric spaces to special values of -functions. In this paper we consider the locally symmetric space where is the ring of integers of an imaginary quadratic field and is the hyperbolic -space. Tobias Berger proves a lower bound on the denominator of the Eisenstein cohomology in certain cases. The goal of this paper is to show how results of Ito and Sczech can be used to prove an upper bound on the denominator in terms of a special value of a Hecke -function. When the class number of is one, we combine this result with Berger's result to obtain the exact denominator.
Paper Structure (28 sections, 24 theorems, 267 equations, 3 figures, 2 tables)

This paper contains 28 sections, 24 theorems, 267 equations, 3 figures, 2 tables.

Key Result

Theorem 1

(Theorem mainthm) We have the upper bound (in the sense of divisibility) on the denominator

Figures (3)

  • Figure 1: The embedding of $\mathcal{H}_r$ by $\iota_{r,v}$ is a horosphere in $\mathbb{H}_3$, tangent to the plane $v=0$ at the cusp $r$. As $v$ increases, the radius of the sphere decreases. Hence we can see the boundary components as horospheres at infinity.
  • Figure 2: The equivalence $[a,\gamma a] \sim [b , \gamma b ]$.
  • Figure 3: The equivalence $[a,b] \sim [\gamma a , \gamma b ]$.

Theorems & Definitions (51)

  • Theorem
  • Corollary
  • Remark 1.1
  • Proposition 2.1
  • Remark 2.1
  • Proposition 2.2: Sczech
  • Proposition 2.3
  • proof
  • Proposition 2.4
  • proof
  • ...and 41 more