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Gravitational EFT for dissipative open systems

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arxiv 2412.21136 v1 pith:KEQGJILH submitted 2024-12-30 hep-th astro-ph.COcond-mat.stat-mechgr-qchep-ph

classification hep-thastro-ph.COcond-mat.stat-mechgr-qchep-ph
keywords dissipativegravityenvironmentdynamicalapplyconstructioncoupledfield
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We elaborate on the effective field theory (EFT) construction for dissipative open systems coupled to dynamical gravity, in light of recent developments on the EFT of dissipative hydrodynamics (HydroEFT). Our construction is based on the Schwinger-Keldysh formalism and its symmetries as well as microscopic unitarity. A key aspect of dynamical gravity is that gravity couples to all degrees of freedom universally, hence the EFT has to take into account the energy-momentum tensor of the environment to which the energy escapes from the dissipative system of interest. We incorporate this effect by modeling the environment based on HydroEFT, assuming validity of the derivative expansion of the environment sector. For illustration, we apply our EFT recipe to a dissipative scalar field coupled to dynamical gravity that can be used, e.g., for dissipative inflation. In particular we quantify impacts of fluctuations in the environment sector on the scalar dynamics. We also apply the same framework to dissipative gravity, discussing dissipative gravitational waves and the generalized second law of black hole thermodynamics.

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Cited by 2 Pith papers

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

  1. Emergent structures in open EFTs

    hep-th 2025-09 conditional novelty 5.0 of 10

    Breaking the advanced (r minus a) symmetry in Schwinger-Keldysh open EFTs forces deformed identities among the equations of motion, and the paper gives an explicit deformed diffeomorphism identity for open gravity.

  2. Lectures on Open Systems and Cosmology

    hep-th 2026-07 unverdicted novelty 1.0 of 10

    A pedagogical review that presents the density-matrix/master-equation formalism and the Schwinger–Keldysh path integral in one notation and applies them to inflation; it claims no new result.

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