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PreprintCC BY 4.0arXiv

Homogeneous and Isotropic Linearized Gravity as a Caldeira--Leggett System

Abstract

We show that the homogeneous and isotropic sector of linearized gravity coupled to arbitrary additional degrees of freedom takes the Caldeira-Leggett form, provided their action contains no metric time derivatives at second order in perturbations. These additional degrees of freedom constitute the model's harmonic reservoir. Eliminating them yields a generalized Langevin equation for the metric perturbation, with their influence condensed in the reservoir's spectral density. This equivalence also yields a natural setting for reduced quantization of the perturbation and stochastic gravitational dynamics. We analyze the resulting dynamics with Laplace methods, extending results presented in other open-system settings.

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BibTeX
@misc{calzada2026homogeneous,
  title = {{Homogeneous and Isotropic Linearized Gravity as a Caldeira--Leggett System}},
  author = {Pelayo V. Calzada and Pedro Bargueño},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2607.28209},
  eprint = {2607.28209},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.28209},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Homogeneous and Isotropic Linearized Gravity as a Caldeira--Leggett System
AU  - Pelayo V. Calzada
AU  - Pedro Bargueño
PY  - 2026
DA  - 2026/09/16
PB  - arXiv
DO  - 10.48550/arxiv.2607.28209
UR  - https://arxiv.org/abs/2607.28209
AB  - We show that the homogeneous and isotropic sector of linearized gravity coupled to arbitrary additional degrees of freedom takes the Caldeira-Leggett form, provided their action contains no metric time derivatives at second order in perturbations. These additional degrees of freedom constitute the model's harmonic reservoir. Eliminating them yields a generalized Langevin equation for the metric perturbation, with their influence condensed in the reservoir's spectral density. This equivalence also yields a natural setting for reduced quantization of the perturbation and stochastic gravitational dynamics. We analyze the resulting dynamics with Laplace methods, extending results presented in other open-system settings.
ER  -