# The pointwise H\"older spectrum of general self-affine functions on an   interval

**Authors:** Pieter Allaart

arXiv: 1907.09660 · 2020-06-16

## TL;DR

This paper analyzes the multifractal spectrum of self-affine functions on an interval, including well-known examples like the Takagi function, and determines when the multifractal formalism accurately describes their pointwise regularity.

## Contribution

It provides explicit formulas for the pointwise Hölder spectrum of self-affine functions and identifies conditions under which the multifractal formalism holds or fails.

## Key findings

- Multifractal spectrum given by formalism when |d_k| ≥ |a_k| for some k
- Explicit pointwise Hölder exponents derived for certain cases
- Conditions identified for multifractal formalism validity

## Abstract

This paper gives the pointwise H\"older (or multifractal) spectrum of continuous functions on the interval $[0,1]$ whose graph is the attractor of an iterated function system consisting of $r\geq 2$ affine maps on $\mathbb{R}^2$. These functions satisfy a functional equation of the form $\phi(a_k x+b_k)=c_k x+d_k\phi(x)+e_k$, for $k=1,2,\dots,r$ and $x\in[0,1]$. They include the Takagi function, the Riesz-Nagy singular functions, Okamoto's functions, and many other well-known examples. It is shown that the multifractal spectrum of $\phi$ is given by the multifractal formalism when $|d_k|\geq |a_k|$ for at least one $k$, but the multifractal formalism may fail otherwise, depending on the relationship between the shear parameters $c_k$ and the other parameters. In the special case when $a_k>0$ for every $k$, an exact expression is derived for the pointwise H\"older exponent at any point. These results extend recent work by the author [Adv. Math. 328 (2018), 1-39] and S. Dubuc [Expo. Math. 36 (2018), 119-142].

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1907.09660/full.md

## References

22 references — full list in the complete paper: https://tomesphere.com/paper/1907.09660/full.md

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Source: https://tomesphere.com/paper/1907.09660