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PhysRevLett.118.181601.pdf
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AMER PHYSICAL SOCCitation
Chiral Shock Waves 2017, 118 (18) Physical Review LettersJournal
Physical Review LettersRights
© 2017 American Physical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We study the shock waves in relativistic chiral matter. We argue that the conventional Rankine-Hugoinot relations are modified due to the presence of chiral transport phenomena. We show that the entropy discontinuity in a weak shock wave is quadratic in the pressure discontinuity when the effect of chiral transport becomes sufficiently large. We also show that rarefaction shock waves, which do not exist in usual nonchiral fluids, can appear in chiral matter. The direction of shock wave propagation is found to be completely determined by the direction of the vorticity and the chirality of fermions. These features are exemplified by shock propagation in dense neutrino matter in the hydrodynamic regime.ISSN
0031-90071079-7114
PubMed ID
28524671Version
Final published versionSponsors
JSPS KAKENHI [16K17703]; MEXT-Supported Program for the Strategic Research Foundation at Private Universities, "Topological Science" [S1511006]; U.S. Department of Energy [DE-FG02-04ER41338]Additional Links
http://link.aps.org/doi/10.1103/PhysRevLett.118.181601ae974a485f413a2113503eed53cd6c53
10.1103/PhysRevLett.118.181601
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