Inflation as a response to protect the Holographic Principle

TL;DR

This paper proposes a model where cosmic inflation occurs as a mechanism to uphold the holographic principle, specifically the Fischler-Susskind bound, in a closed universe with a two-fluid system.

Contribution

It introduces a novel inflationary model driven by holographic considerations, linking the early universe expansion to holographic bound preservation.

Findings

Inflation can be triggered by holographic bound constraints.

Conditions for exponential expansion compatible with observations are discussed.

A two-fluid closed universe model supports holographically motivated inflation.

Abstract

A model where the inflationary phase emerges as a response to protect the Fischler-Susskind holographic bound is described. A two fluid model in a closed universe inflation picture is assumed, and a discussion on conditions under which is possible to obtain an additional exponential expansion phase as those currently observed is given.