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Open EFT for Interacting Fermions from Holography

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arxiv 2403.10604 v2 pith:RFWA4QP5 submitted 2024-03-15 hep-th

Open EFT for Interacting Fermions from Holography

classification hep-th
keywords bulkblackcorrelatorsfermionsholeinteractingopenscattering
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We initiate the study of an open EFT for finite-temperature holographic systems with interacting fermions. In particular, we do this for Yukawa interactions in the bulk using the real-time formalism (grSK geometry). From the bulk perspective, this study corresponds to Yukawa scattering against a black hole, incorporating the effects of Hawking radiation. We derive an EFT in the exterior of the black hole and thus develop a Witten diagrammatic understanding of the scattering processes. This allows the explicit evaluation of boundary Schwinger-Keldysh (SK) correlators to arbitrary order, at tree-level in the bulk. Here we present explicitly the SK generating functional up to four-point functions. Finally, we represent the correlators in a column-vector representation that manifests microscopic unitarity and thermality, with all the statistical factors neatly folded in.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Dissipative hydrodynamic actions and horizon symmetries in gravity

    hep-th 2026-07 unverdicted novelty 6.0

    A new prescription computes the dissipative action for holographic hydrodynamics in AdS4 to first order in derivatives and reproduces known Green's functions via horizon diffeomorphisms.

  2. Imprint of the black hole interior on thermal four-point correlators

    hep-th 2025-12 conditional novelty 6.0

    Analytically continuing and smearing thermal four-point correlators turns them into flat-space scattering amplitudes at a bulk point inside the black hole.

  3. Loops Outside a Black Hole

    hep-th 2025-09 conditional novelty 6.0

    Conjecture reducing bulk loop discontinuity integrals in black hole Schwinger-Keldysh geometry to exterior real-time finite-temperature loop integrals, checked at one to three loops for low-point functions.