Holographic KMS relations at finite density
R. Loganayagam, Krishnendu Ray, Shivam K. Sharma, Akhil Sivakumar

TL;DR
This paper extends the holographic Schwinger-Keldysh framework to charged black branes, enabling the study of real-time correlators at finite density and temperature, and confirms the KMS relations for fermionic fields.
Contribution
It introduces a holographic prescription for real-time correlators in charged black brane backgrounds, verifying KMS relations for fermionic probes at finite density.
Findings
Derived Schwinger-Keldysh correlators satisfy KMS relations with Fermi-Dirac factors.
Extended the Dirac equation solutions in a boundary derivative expansion.
Validated the prescription using charged Dirac probe fields.
Abstract
We extend the holographic Schwinger-Keldysh prescription introduced in arXiv:1812.08785 to charged black branes, with a view towards studying Hawking radiation in these backgrounds. Equivalently we study real-time fluctuations of the dual CFT held at finite temperature and finite chemical potential. We check our prescription using charged Dirac probe fields. We solve the Dirac equation in a boundary derivative expansion extending the results in arXiv:2011.07039. The Schwinger-Keldysh correlators derived using this prescription automatically satisfy the appropriate KMS relations with Fermi-Dirac factors.
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