Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3384
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dc.contributor.authorBANERJEE, NABAMITAen_US
dc.contributor.authorLodato, Ivanoen_US
dc.contributor.authorNEOGI, TURMOLIen_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), 066029.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3384-
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.96.066029en_US
dc.description.abstractWe consider three dimensional N = 4 flat supergravity, with an Abelian R-symmetry enhancing the gravitational phase space. We obtain the field configuration whose asymptotic symmetries at null infinity coincide with the centrally extended N = 4 super-Bondi-Metzner-Sachs (BMS) algebra. The killing spinors for this generic configuration are obtained together with the energy bounds imposed by supersymmetry. It is explicitly shown that the same algebra can be obtained as a flat (AdS radius →∞) limit of the combined (2,0) and (0,2) sectors of AdS supergravity.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectN=4 supersymmetricen_US
dc.subjectBMS3 algebrasen_US
dc.subjectAsymptotic symmetryen_US
dc.subjectAdS supergravityen_US
dc.subject2017en_US
dc.titleN=4 supersymmetric BMS3 algebras from asymptotic symmetry analysisen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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