Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3383
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dc.contributor.authorBANERJEE, NABAMITAen_US
dc.contributor.authorDutta, Suvankaren_US
dc.contributor.authorJain, Akashen_US
dc.date.accessioned2019-07-01T05:39:12Z
dc.date.available2019-07-01T05:39:12Z
dc.date.issued2017-09en_US
dc.identifier.citationPhysical Review D, 96(6), 065004.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3383-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.96.065004en_US
dc.description.abstractWe study dynamics of an (anomalous) Galilean superfluid up to first order in derivative expansion, both in parity-even and parity-odd sectors. We construct a relativistic system—null superfluid, which is a null fluid (introduced in N. Banerjee, S. Dutta, and A. Jain Akash, [Phys. Rev. D 93, 105020 (2016).]) with a spontaneously broken global U(1) symmetry. A null superfluid is in one-to-one correspondence with a Galilean superfluid in one lower dimension; i.e., they have the same symmetries, thermodynamics, constitutive relations and are related to each other by a mere choice of basis. The correspondence is based on null reduction, which is known to reduce the Poincaré symmetry of a theory to Galilean symmetry in one lower dimension. To perform this analysis, we use off-shell formalism of (super)fluid dynamics, adopting it appropriately to null (super)fluids. We also verify these results via c→∞ limit of a parent relativistic system.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectFirst orderen_US
dc.subjectGalilean superfluiden_US
dc.subjectDynamicsen_US
dc.subjectGalilean superfluiden_US
dc.subjectrelativistic systemen_US
dc.subject2017en_US
dc.titleFirst order Galilean superfluid dynamicsen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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