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Spin tensor and its role in non-equilibrium thermodynamics

  • It is shown that the description of a relativistic fluid at local thermodynamic equilibrium depends on the particular quantum stress-energy tensor operator chosen, e.g., the canonical or symmetrized Belinfante stress-energy tensor. We argue that the Belinfante tensor is not appropriate to describe a relativistic fluid whose macroscopic polarization relaxes slowly to thermodynamic equilibrium and that a spin tensor, like the canonical spin tensor, is required. As a consequence, the description of a polarized relativistic fluid involves an extension of relativistic hydrodynamics including a new antisymmetric rank-two tensor as a dynamical field. We show that the canonical and Belinfante tensors lead to different predictions for measurable quantities such as spectrum and polarization of particles produced in relativistic heavy-ion collisions.

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Metadaten
Author:Francesco BecattiniORCiDGND, Wojciech FlorkowskiORCiDGND, Enrico SperanzaORCiDGND
URN:urn:nbn:de:hebis:30:3-546700
DOI:https://doi.org/10.1016/j.physletb.2018.12.016
ISSN:1873-2445
ISSN:0370-2693
Parent Title (English):Physics Letters B
Publisher:Elsevier
Place of publication:Amsterdam [u.a.]
Document Type:Article
Language:English
Date of Publication (online):2018/12/18
Date of first Publication:2018/12/18
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2020/05/14
Volume:789.2019
Page Number:7
First Page:419
Last Page:425
HeBIS-PPN:465583415
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung 4.0