Holographic Description of Heavy-Quark Potentials in an Inflationary Braneworld Scenario
Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz

TL;DR
This paper explores how heavy-quark potentials behave in an inflationary braneworld scenario using gauge/gravity duality, revealing a confining phase influenced by the Hubble parameter and brane tension.
Contribution
It introduces a holographic model of heavy-quark potentials in an inflating braneworld, connecting cosmological parameters with confinement properties.
Findings
Heavy-quark potential exhibits a confining phase.
Confinement depends on the ratio of Hubble parameter to brane tension.
The model links cosmological inflation to gauge theory confinement.
Abstract
We study heavy-quark potential in an inflationary braneworld scenario. The scenario we consider is an (Euclidean) inflating braneworld embedded in a static Euclidean . Using gauge/gravity duality we obtain a confining phase depending on the ratio between the Hubble parameter in the braneworld and the brane tension .
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