Schwinger-Keldysh effective field theory for stable and causal relativistic hydrodynamics
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Publication:6198558
DOI10.1007/JHEP01(2024)162arXiv2309.00511OpenAlexW4391262010WikidataQ129284296 ScholiaQ129284296MaRDI QIDQ6198558
Publication date: 20 March 2024
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2309.00511
Cites Work
- Unnamed Item
- Entropy current and equilibrium partition function in fluid dynamics
- Relativistic viscous hydrodynamics, conformal invariance, and holography
- Relativistic magnetohydrodynamics
- Constraints on superfluid hydrodynamics from equilibrium partition functions
- Stable and causal relativistic Navier-Stokes equations
- Stability and causality in dissipative relativistic fluids
- Effective action for relativistic hydrodynamics: fluctuations, dissipation, and entropy inflow
- Topological sigma models \& dissipative hydrodynamics
- Effective field theory of dissipative fluids
- Emergent supersymmetry in local equilibrium systems
- Dissipative hydrodynamics in superspace
- One-form superfluids \& magnetohydrodynamics
- Ghostbusters: unitarity and causality of non-equilibrium effective field theories
- First-order relativistic hydrodynamics is stable
- Hydrodynamic equations and correlation functions
- On thermal fluctuations and the generating functional in relativistic hydrodynamics
- Lectures on hydrodynamic fluctuations in relativistic theories
- Relativistic theories of dissipative fluids
- A stable and causal model of magnetohydrodynamics
- Relativistic Fluid Dynamics in and out of Equilibrium
- Heat waves
- Irreversibility and Generalized Noise
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