2017
DOI: 10.5506/aphyspolbsupp.10.1139
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Relativistic Hydrodynamics of Particles with Spin 1/2

Abstract: The formulation of relativistic hydrodynamics for massive particles with spin 1 /2 is shortly reviewed. The proposed framework is based on the Wigner function treated in a semi-classical approximation or, alternatively, on a classical treatment of spin 1 /2. Several theoretical issues regarding the choice of the energy-momentum and spin tensors used to construct the hydrodynamic framework with spin are discussed in parallel.

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Cited by 10 publications
(13 citation statements)
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“…For a similar observation in the NJL model see e.g. [37]. All low-energy effective models have in common that they have a physical UV scale above which they loose predictive power.…”
Section: A Masses and Fluctuation Scalesmentioning
confidence: 71%
“…For a similar observation in the NJL model see e.g. [37]. All low-energy effective models have in common that they have a physical UV scale above which they loose predictive power.…”
Section: A Masses and Fluctuation Scalesmentioning
confidence: 71%
“…A particularly appealing theoretical explanation of this effect invokes a direct coupling between the thermal vorticity and polarization, which is realized in the global equilibrium state of a rotating medium [4,5]. Recently, a new framework for relativistic perfect fluid hydrodynamics of spin-polarized media was presented [6,7,8,9], which extends the work of Refs. [4,5] to systems in local equilibrium.…”
Section: Introductionmentioning
confidence: 81%
“…On top of their evolution one has to solve Eqs. (8) for the normalized components of the polarization tensor.…”
Section: Evolution Equations For Spin-polarized Fluidsmentioning
confidence: 99%
“…In the next section we study Eqs. (11), (13), (14), (15) and (8) in the case where the equilibrium is achieved only locally.…”
Section: Evolution Equations For Spin-polarized Fluidsmentioning
confidence: 99%