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Relativistic hydrodynamics with spin

  • A newly proposed framework of perfect-fluid relativistic hydrodynamics for particles with spin 1/2 is briefly reviewed. The hydrodynamic equations follow entirely from the conservation laws for energy, momentum, and angular momentum. The incorporation of the angular-momentum conservation requires that the spin polarization tensor ωμν is introduced. It plays a role of a Lagrange multiplier conjugated to the spin tensor Sλ,μν. The space-time evolution of the spin polarization tensor depends on the specific form chosen for the spin tensor.

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Metadaten
Author:Wojciech FlorkowskiORCiDGND, Bengt FrimanORCiD, Amaresh JaiswalORCiD, Radoslaw RyblewskiORCiD, Enrico SperanzaORCiDGND
URN:urn:nbn:de:hebis:30:3-776125
DOI:https://doi.org/10.1016/j.nuclphysa.2018.10.010
ISSN:0375-9474
Parent Title (English):Nuclear Physics A
Publisher:Elsevier
Place of publication:Amsterdam
Document Type:Article
Language:English
Date of Publication (online):2019/01/22
Date of first Publication:2019/01/22
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2023/10/05
Tag:heavy-ion collisions; relativistic hydrodynamics; spin polarization
Volume:982
Page Number:4
First Page:523
Last Page:526
HeBIS-PPN:513178465
Institutes:Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - CC BY-NC-ND - Namensnennung - Nicht kommerziell - Keine Bearbeitungen 4.0 International