General relativistic nonideal fluid equations for dark matter from a truncated cumulant expansion

A new truncation scheme based on the cumulant expansion of the one-particle phase-space distribution function for dark matter particles is developed. Extending the method of moments in relativistic kinetic theory, we derive evolution equations which supplement the covariant conservation of the energ...

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Bibliographic Details
Main Authors: Erschfeld, Alaric (Author) , Flörchinger, Stefan (Author) , Rupprecht, Maximilian (Author)
Format: Article (Journal)
Language:English
Published: 16 September 2020
In: Physical review
Year: 2020, Volume: 102, Issue: 6
ISSN:2470-0029
DOI:10.1103/PhysRevD.102.063520
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevD.102.063520
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.102.063520
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Author Notes:Alaric Erschfeld, Stefan Floerchinger, and Maximilian Rupprecht
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Summary:A new truncation scheme based on the cumulant expansion of the one-particle phase-space distribution function for dark matter particles is developed. Extending the method of moments in relativistic kinetic theory, we derive evolution equations which supplement the covariant conservation of the energy-momentum tensor and particle number current. Truncating the cumulant expansion we obtain a closed, covariant and hyperbolic system of equations which can be used to model the evolution of a general relativistic nonideal fluid. As a working example we consider a Friedmann-Lemaître-Robertson-Walker cosmology with dynamic pressure and solve for the time evolution of the effective equation of state parameter.
Item Description:Gesehen am 26.10.2020
Physical Description:Online Resource
ISSN:2470-0029
DOI:10.1103/PhysRevD.102.063520