Selberg integral: Difference between revisions
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Latest revision as of 08:33, 30 January 2025
Template:Short description In mathematics, the Selberg integral is a generalization of Euler beta function to n dimensions introduced by Atle Selberg.[1][2]
Selberg's integral formula
When , we have
Selberg's formula implies Dixon's identity for well poised hypergeometric series, and some special cases of Dyson's conjecture. This is a corollary of Aomoto.
Aomoto's integral formula
Aomoto proved a slightly more general integral formula.[3] With the same conditions as Selberg's formula,
A proof is found in Chapter 8 of Template:Harvtxt.[4]
Mehta's integral
When ,
It is a corollary of Selberg, by setting , and change of variables with , then taking .
This was conjectured by Template:Harvtxt, who were unaware of Selberg's earlier work.[5]
It is the partition function for a gas of point charges moving on a line that are attracted to the origin.[6]
In particular, when , the term on the right is .
Macdonald's integral
Template:Harvtxt conjectured the following extension of Mehta's integral to all finite root systems, Mehta's original case corresponding to the An−1 root system.[7]
The product is over the roots r of the roots system and the numbers dj are the degrees of the generators of the ring of invariants of the reflection group. Template:Harvtxt gave a uniform proof for all crystallographic reflection groups.[8] Several years later he proved it in full generality, making use of computer-aided calculations by Garvan.[9]