Zeta measures and Thermodynamic Formalism for temperature zero
Abstract
We address the analysis of the following problem: given a real H\"older potential f defined on the Bernoulli space and μf its equilibrium state, it is known that this shift-invariant probability can be weakly approximated by probabilities in periodic orbits associated to certain zeta functions. Given a H\"older function f>0 and a value s such that 0<s<1, we can associate a shift-invariant probability s such that for each continuous function k we have \[∫ k ds=Σn=1∞Σx∈ Fixnesfn(x)-nP(f)kn(x)nΣn=1∞Σx∈ Fixnesfn(x)-nP(f),\] where P(f) is the pressure of f, Fixn is the set of solutions of σn(x)=x, for any n∈ N, and fn(x) = f(x) + f(σ(x)) + f(σ2(x))+... + f(σn-1 (x)). We call s a zeta probability for f and s. It is known that s μf, when s 1. We consider for each value c the potential c f and the corresponding equilibrium state μc f. What happens with s when c goes to infinity and s goes to one? This question is related to the problem of how to approximate the maximizing probability for f by probabilities on periodic orbits. We study this question and also present here the deviation function I and Large Deviation Principle for this limit c ∞, s 1. We will make an assumption: c ∞, s 1 c(1-s)= L>0. We do not assume here the maximizing probability for f is unique.
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.