Holographic Fluctuation-Dissipation Relations in Finite Density Systems

Fuente: arXiv
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Autore principale: Sharma, Shivam K.
Natura: Preprint
Pubblicazione: 2025
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author Sharma, Shivam K.
author_facet Sharma, Shivam K.
contents Using real-time holography, we investigate fluctuation-dissipation relations in holographic systems at finite density. In the bulk, it corresponds to the study of scattering of a charged scalar field against a charged black hole background, leading to an exterior field theory outside the AdS Reissner-Nordström black hole. This theory captures dissipation (from infalling Quasi-normal modes) and fluctuations (from Hawking radiation). Here, we also develop a Witten diagrammatic framework for computing $n$-point functions for interacting charged scalars. From the boundary perspective, it gives real-time correlations of the dual CFT held at finite temperature and finite chemical potential. Our results yield (non)-linear holographic fluctuation-dissipation relations at small but finite density, which are shown to recover the correct behaviour in the zero-density limit.
format Preprint
id arxiv_https___arxiv_org_abs_2501_17852
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Holographic Fluctuation-Dissipation Relations in Finite Density Systems
Sharma, Shivam K.
High Energy Physics - Theory
Statistical Mechanics
General Relativity and Quantum Cosmology
Using real-time holography, we investigate fluctuation-dissipation relations in holographic systems at finite density. In the bulk, it corresponds to the study of scattering of a charged scalar field against a charged black hole background, leading to an exterior field theory outside the AdS Reissner-Nordström black hole. This theory captures dissipation (from infalling Quasi-normal modes) and fluctuations (from Hawking radiation). Here, we also develop a Witten diagrammatic framework for computing $n$-point functions for interacting charged scalars. From the boundary perspective, it gives real-time correlations of the dual CFT held at finite temperature and finite chemical potential. Our results yield (non)-linear holographic fluctuation-dissipation relations at small but finite density, which are shown to recover the correct behaviour in the zero-density limit.
title Holographic Fluctuation-Dissipation Relations in Finite Density Systems
topic High Energy Physics - Theory
Statistical Mechanics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2501.17852