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Dynamical analysis of a first order theory of bulk viscosity
General Relativity and Quantum Cosmology · Submitted 28 Aug 2018
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We provide stability properties, cosmological interpretation and thermodynamic features of the critical points.
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The abstract, sentence by sentence
We perform a global analysis of curved Friedmann-Robertson-Walker cosmologies in the presence of a viscous fluid. The fluid's bulk viscosity is governed by a first order theory recently proposed in [M. M. Disconzi, T. W. Kephart, and R. J. Scherrer, Phys. Rev. D 91, 043532 (2015)], and the analysis is carried out in a compactified parameter space with dimensionless coordinates. We provide stability properties, cosmological interpretation and thermodynamic features of the critical points.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We perform a global analysis of curved Friedmann-Robertson-Walker cosmologies in the presence of a viscous fluid. | contribution 0.98 | 0.95 | 0.06 | asserted 0.95 |
| s1 | The fluid's bulk viscosity is governed by a first order theory recently proposed in [M. M. Disconzi, T. W. Kephart, and R. | method 0.71 | 0.10 | 0.03 | asserted 0.99 |
| s2 | J. Scherrer, Phys. Rev. D 91, 043532 (2015)], and the analysis is carried out in a compactified parameter space with dimensionless coordinates. | method 0.96 | 0.67 | 0.05 | asserted 0.99 |
| s3 | We provide stability properties, cosmological interpretation and thermodynamic features of the critical points. | contribution 0.68 | 0.94 | 0.32 | asserted 0.98 |
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Original abstract
We perform a global analysis of curved Friedmann-Robertson-Walker cosmologies in the presence of a viscous fluid. The fluid's bulk viscosity is governed by a first order theory recently proposed in [M. M. Disconzi, T. W. Kephart, and R. J. Scherrer, Phys. Rev. D 91, 043532 (2015)], and the analysis is carried out in a compactified parameter space with dimensionless coordinates. We provide stability properties, cosmological interpretation and thermodynamic features of the critical points.
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