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Towards an effective action for relativistic dissipative hydrodynamics
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Towards an effective action for relativistic dissipative hydrodynamics
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We propose an effective action for first order relativistic dissipative hydrodynamics that can be used to evaluate n-point symmetrized correlation functions, taking into account thermal fluctuations of the hydrodynamic variables.
Forward citations
Cited by 3 Pith papers
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A generalized Chaplygin-type solid unifies dark matter and dark energy via an early pressureless phase transitioning to a late solid phase that supports acceleration and produces distinct low-redshift perturbation signatures.
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Non-Gaussian hydrodynamic fluctuations in an expanding relativistic fluid
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