Holographic correlation functions at finite density and/or finite temperature
George Georgiou, Dimitrios Zoakos

TL;DR
This paper holographically computes scalar two-point functions at finite density and temperature, revealing how these correlators depend on thermodynamic parameters and matching expectations from conformal field theory and black hole thermodynamics.
Contribution
It provides a systematic expansion of holographic two-point functions at finite temperature and density, connecting them with OPE structures and thermodynamic properties of the dual black hole.
Findings
Correlators depend on temperature and chemical potential.
Agreement with OPE and thermodynamics of black holes.
Explicit behavior of correlators at large distances.
Abstract
We calculate holographically one and two-point functions of scalar operators at finite density and/or finite temperature. In the case of finite density and zero temperature we argue that only scalar operators can have non-zero VEVs. In the case in which both the chemical potential and the temperature are finite, we present a systematic expansion of the two-point correlators in powers of the temperature T and the chemical potential . The holographic result is in agreement with the general form of the OPE which dictates that the two-point function may be written as a linear combination of the Gegenbauer polynomials but with the coefficients depending now on both the temperature and the chemical potential, as well as on the CFT data. The leading terms in this expansion originate from the expectation values of the scalar operator , the R-current ${\cal…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
