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The Disordered Universe 2025: Open Effective Field Theories

High Energy Physics - Theory · Submitted 27 Oct 2026 · 87 references

Pith's verdict: A clear, well-organized pedagogical chapter on open EFTs for cosmology. It does not claim new results but is honest about its assumptions and limitations. The main soft spot—unquantified locality assumption—is acknowledged but not resolved, which limits its reach but not its value as a teaching resource.

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arXiv ID2610.36898 (version 1)
Pith IDFL3YBBFH, Pith's permanent record of this paper and its review
CitationAlessandro Fumagalli, Francesco Paronetto, Guilherme Leite Pimentel, Leonardo Stanzani, Lucas Vicente Garc\'ia-Consuegra, Mattia Varrone, Paolo Benincasa, Thomas Colas. "The Disordered Universe 2025: Open Effective Field Theories." arXiv:2610.36898 (2026). https://pith.science/paper/FL3YBBFH
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Referee report
The paper

The paper claims

The Schwinger-Keldysh formalism provides a systematic framework for constructing open effective field theories that capture dissipation and noise from unknown environments, demonstrated for inflation, gauge theories, and gravity.

The reading

This paper shows how the Schwinger-Keldysh (in-in) formalism can be extended to construct open effective field theories that systematically capture dissipation and noise from unobserved environments. It demonstrates the construction for scalar fields, then applies it to single-clock inflation, deriving the most general local open EFT operators consistent with symmetries. The resulting power spectra and bispectra exhibit characteristic signatures, such as regularized folded singularities and dissipation-enhanced equilateral non-Gaussianities, which could be smoking guns for open dynamics. The paper also outlines extensions to gauge theories and gravity, identifying key challenges like maintaining gauge invariance in open systems.

What carries the argument

The Schwinger-Keldysh (in-in) path integral with double branches φ_+ and φ_−, transformed to the Keldysh basis φ_r = (φ_+ + φ_−)/2 and φ_a = φ_+ − φ_−. The open effective action S_eff is decomposed into a unitary part S[φ_+]−S[φ_−] and an influence functional F[φ_+,φ_−], which is further organized in powers of φ_a. The non-equilibrium constraints (normalization, hermiticity, and positivity) restrict the allowed operators and provide positivity bounds on coefficients. For inflation, the building blocks are π_a and P_μ = ∂_μ(t+π_r), with the symmetry breaking pattern shift_+ × shift_− → shift_r.

Extended reading notes

Core claim

The central claim is that the influence functional of an open system can be systematically constructed in the Keldysh basis using only the non-equilibrium constraints (normalization, hermiticity, positivity) and the symmetry breaking pattern of the microscopic theory (e.g., time translations reduced to the diagonal subgroup). For single-clock inflation, the open effective action is built from building blocks π_a and ∂_μ(t+π_r), leading to a set of dissipative and stochastic operators at each order in π_a. The paper derives explicit Feynman rules in the Keldysh basis, computes the dissipative power spectrum and bispectrum, and shows that the bispectrum shape interpolates between equilateral (large dissipation) and folded (small dissipation) configurations, with the folded singularity regularized by dissipation. It also matches the open EFT to a concrete gauge-inflation model.

Load-bearing premise

The separation of scales that allows the effective theory to be local: the typical length and timescales of the environment must be much shorter than the Hubble radius.

Editorial extensions

If this is right

  • Observable primordial non-Gaussianities from dissipation are peaked in equilateral or folded configurations depending on γ/H, and the folded divergence is always regularized.
  • The open EFT of inflation predicts a specific scaling of the power spectrum with γ: ∆^2_ζ ∝ β_1 H^4 / f_π^4 in low dissipation, and ∝ √(H/γ) in high dissipation, which can match warm inflation when a fluctuation-dissipation relation holds.
  • Matching to a gauge-inflation model fixes the EFT coefficients in terms of microphysical parameters (m, M, f, ξ), providing a UV-complete example of the open EFT.
  • In the decoupling limit (ϵ ≪ 1), the open EFT of inflation reduces to a theory of a shift-symmetric scalar in rigid de Sitter with additional dissipative and stochastic operators.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The regularized folded singularity in the bispectrum provides a clean observational discriminant between open-system dynamics and non-Bunch-Davies initial states, which produce a true divergence.
  • The framework suggests that stochastic gravitational wave backgrounds could be generated by tidal deformations of an environment, offering a new source for gravitational-wave astrophysics.
  • The construction of open EFT for gauge theories using Stückelberg fields and 1-form symmetries might lead to a systematic classification of dissipative phases in cosmology, such as conducting versus insulating dark sectors.
Original abstract

Effective field theories (EFTs) offer a powerful method to unify diverse models under a small set of control parameters, allowing systematic expansions around well-established theories. While these techniques were traditionally developed for particle physics experiments with clean, isolated initial states, realistic macroscopic environments are often noisy and dissipative. Recognising the limitations of traditional EFTs has recently sparked intense progress at the interface of high-energy physics and condensed matter. These developments motivate a new approach to gravitation and cosmology, one that models the gravitational sector as evolving in the presence of an unobservable medium. Open Effective Field Theories provide a systematic, controllable framework for this endeavour. This chapter presents this versatile framework and illustrates how the Schwinger-Keldysh formalism captures the influence of unknown environments, manifesting as dissipation and noise, on observational probes. These notes are based on a series of lectures held during the La Ricotta Summer School "The Disordered Universe 2025" from 21 July to 1 August 2025.

The compiled record

The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-10-28: 1 request, 5,617 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.14 · human participants 0.04 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.02 · compares with prior results 0.25 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

Effective field theories (EFTs) offer a powerful method to unify diverse models under a small set of control parameters, allowing systematic expansions around well-established theories. While these techniques were traditionally developed for particle physics experiments with clean, isolated initial states, realistic macroscopic environments are often noisy and dissipative. Recognising the limitations of traditional EFTs has recently sparked intense progress at the interface of high-energy physics and condensed matter. These developments motivate a new approach to gravitation and cosmology, one that models the gravitational sector as evolving in the presence of an unobservable medium. Open Effective Field Theories provide a systematic, controllable framework for this endeavour. This chapter presents this versatile framework and illustrates how the Schwinger-Keldysh formalism captures the influence of unknown environments, manifesting as dissipation and noise, on observational probes. These notes are based on a series of lectures held during the La Ricotta Summer School "The Disordered Universe 2025" from 21 July to 1 August 2025.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Effective field theories (EFTs) offer a powerful method to unify diverse models under a small set of control parameters, allowing systematic expansions around well-established theories. background 1.00 0.05 0.05 asserted 1.00
s1 While these techniques were traditionally developed for particle physics experiments with clean, isolated initial states, realistic macroscopic environments are often noisy and dissipative. background 0.67 0.04 0.03 asserted 0.95
s2 Recognising the limitations of traditional EFTs has recently sparked intense progress at the interface of high-energy physics and condensed matter. background 0.97 0.04 0.04 asserted 1.00
s3 These developments motivate a new approach to gravitation and cosmology, one that models the gravitational sector as evolving in the presence of an unobservable medium. contribution 0.64 0.11 0.20 asserted 0.80
s4 Open Effective Field Theories provide a systematic, controllable framework for this endeavour. contribution 0.60 0.14 0.23 asserted 1.00
s5 This chapter presents this versatile framework and illustrates how the Schwinger-Keldysh formalism captures the influence of unknown environments, manifesting as dissipation and noise, on observational probes. contribution 0.95 0.51 0.24 asserted 1.00
s6 These notes are based on a series of lectures held during the La Ricotta Summer School "The Disordered Universe 2025" from 21 July to 1 August 2025. background 0.87 0.38 0.01 asserted 0.98

What kind of paper the classifier reports this is: method or tool 0.71 · evidence from argument 0.89.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

Figures
Figure 1. Comparison between a) the single-branch path integral contour used in the computation
Figure 2. In-in diagrammatics of tree-level three-point correlator. The “
Figure 3. Schematic setup of open systems. The system, made of the degree of freedom,
Figure 4. Classical and quantum open system correspondence. Classically, stochastic effects are
Figure 5. Illustration of the Schwinger-Keldysh path integral, where time is running from left to right
Figure 6. Feynman rules in the Keldysh basis. • Then, diagrams evaluation follows the exact same rules as in [7]. As seen from Eq. (3.80), external legs connecting to the conformal boundary η0 → 0 − are continuous, corresponding to φr insertions. An example is given in
Figure 7. The two diagrams to compute the interaction given in Eq. (
Figure 8. Shape function of the contact bispectrum generated by
Figure 9. The ϵr and ϵa transformations on the closed time path, where time is running from left to right in both contours and the arrows represent path ordering (time ordering in |in⟩ and anti-time￾ordering in ⟨in|). The ϵr transformation translates the “ + ” and “ − ” variables in the same direction while ϵa transformation does it in the opposite directions. While the ϵr transformation is preserved, the ϵa one is explicitly broken due to dissipative effects [40]. under general ϵ± translations. More precisely, the effective functional remains invariant under the translation (see the…
Figure 10. Shapes of the bispectrum at large dissipation
Figure 11. Shapes of the bispectrum at low dissipation
Figure 12. Amplitude in the equilateral configuration as a function of the dissipation parameter
Figure 13. Illustration of the lack of conservation of the system’s current. This effect is a mere

Figures reproduced from arXiv:2610.36898 by the authors.

References

Discussion

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