# Complexity of circulant graphs with non-fixed jumps, its arithmetic   properties and asymptotics

**Authors:** Alexander Mednykh, Ilya Mednykh

arXiv: 1812.04484 · 2018-12-12

## TL;DR

This paper derives explicit formulas and asymptotic behavior for the number of spanning trees in a family of circulant graphs with non-fixed jumps, revealing their arithmetic properties and connections to Mahler measures.

## Contribution

It provides a new explicit formula for spanning trees in circulant graphs with non-fixed jumps and explores their arithmetic and asymptotic properties.

## Key findings

- Explicit formula for spanning trees involving Chebyshev polynomials
- Representation of complexity as p * n * a(n)^2 with integer sequence a(n)
- Asymptotic formula linked to Mahler measure of Laurent polynomials

## Abstract

In the present paper, we investigate a family of circulant graphs with non-fixed jumps $$G_n=C_{\beta n}(s_1, \ldots,s_k,\alpha_1n,\ldots,\alpha_\ell n),\, 1\le s_1<\ldots<s_k\le[\frac{\beta n}{2}],\, 1\le \alpha_1< \ldots<\alpha_\ell\le[\frac{\beta}{2}].$$ Here $n$ is an arbitrary large natural number and integers $s_1, \ldots,s_k,\alpha_1, \ldots,\alpha_\ell$ are supposed to be fixed.   First, we present an explicit formula for the number of spanning trees in the graph $G_n.$ This formula is a product of $\beta s_k-1$ factors, each given by the $n$-th Chebyshev polynomial of the first kind evaluated at the roots of some prescribed polynomial of degree $s_k.$ Next, we provide some arithmetic properties of the complexity function. We show that the number of spanning trees in $G_n$ can be represented in the form $\tau(n)=p \,n \,a(n)^2,$ where $a(n)$ is an integer sequence and $p$ is a prescribed natural number depending of parity of $\beta$ and $n.$ Finally, we find an asymptotic formula for $\tau(n)$ through the Mahler measure of the Laurent polynomials differing by a constant from $2k-\sum\limits_{i=1}^k(z^{s_i}+z^{-s_i}).$

## Full text

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## References

37 references — full list in the complete paper: https://tomesphere.com/paper/1812.04484/full.md

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Source: https://tomesphere.com/paper/1812.04484