Fluid Dynamics of Relativistic Quantum Dust

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dc.creatorElze, H. -Th.
dc.date2002-01-02
dc.date.accessioned2026-07-07T10:52:34Z
dc.date.available2026-07-07T10:52:34Z
dc.descriptionThe microscopic transport equations for free fields are solved using the Schwinger function. Thus, for general initial conditions, the evolution of the energy-momentum tensor is obtained, incorporating the quantum effects exactly. The result for relativistic fermions differs from classical hydrodynamics, which is illustrated for Landau and Bjorken type initial conditions in this model of exploding primordial matter. Free fermions behave like classical dust concerning hydrodynamic observables. However, quantum effects which are present in the initial state are preserved.
dc.description5 pages; LaTeX
dc.identifierhttps://arxiv.org/abs/hep-ph/0201007
dc.identifierhttp://arxiv.org/abs/hep-ph/0201007
dc.identifierJ.Phys.G28:2235,2002
dc.identifierdoi:10.1088/0954-3899/28/8/308
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185197
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.subjectQuantum Physics
dc.titleFluid Dynamics of Relativistic Quantum Dust
dc.typetext

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