Inflationary Cosmology as flow of integrable weights

Fuente: arXiv
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1. Verfasser: Gomez, Cesar
Format: Preprint
Veröffentlicht: 2024
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author Gomez, Cesar
author_facet Gomez, Cesar
contents We identify the algebra of gauge invariant observables in de Sitter as the subalgebra of the type $III_1$ factor $A_{dS}$, associated to de Sitter, defined as the centralizer of any integrable weight on $A_{dS}$. These algebras are for any integrable weight type $II_{\infty}$ factors admitting a crossed product representation with respect to modular automorphisms. In this context we define Inflationary Cosmology as the flow of integrable weights and the dual automorphism as the flow generator. Using some basic properties of integrable weights we show that any type $II_1$ dS algebra cannot be represented as the $ε=0$ limit ( for $ε$ the slow roll parameter ) of the gauge invariant algebra defined by any integrable weight. This strongly indicates that the pure dS algebra defined as the $ε=0$ limit is algebraically non existent.
format Preprint
id arxiv_https___arxiv_org_abs_2407_20671
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Inflationary Cosmology as flow of integrable weights
Gomez, Cesar
High Energy Physics - Theory
We identify the algebra of gauge invariant observables in de Sitter as the subalgebra of the type $III_1$ factor $A_{dS}$, associated to de Sitter, defined as the centralizer of any integrable weight on $A_{dS}$. These algebras are for any integrable weight type $II_{\infty}$ factors admitting a crossed product representation with respect to modular automorphisms. In this context we define Inflationary Cosmology as the flow of integrable weights and the dual automorphism as the flow generator. Using some basic properties of integrable weights we show that any type $II_1$ dS algebra cannot be represented as the $ε=0$ limit ( for $ε$ the slow roll parameter ) of the gauge invariant algebra defined by any integrable weight. This strongly indicates that the pure dS algebra defined as the $ε=0$ limit is algebraically non existent.
title Inflationary Cosmology as flow of integrable weights
topic High Energy Physics - Theory
url https://arxiv.org/abs/2407.20671