Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/6802
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dc.contributor.authorBHATTACHARJEE, ARINDAMen_US
dc.contributor.authorNeetuen_US
dc.date.accessioned2022-05-06T05:43:34Z
dc.date.available2022-05-06T05:43:34Z
dc.date.issued2022-03en_US
dc.identifier.citationPhysical Review D, 105(6), 066012.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.105.066012en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/6802
dc.description.abstractOur goal is to find a matrix model with BMS3 constraints built in. These constraints are imposed through loop equations. We solve them using a free field realization of the algebra and write down the partition function in eigenvalue form. We comment on the nature of this partition function and its relations with integrable systems.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectVirasoro constrainten_US
dc.subjectSgravitational wavesen_US
dc.subjectGeneral relativityen_US
dc.subjectIntegrabilityen_US
dc.subjectEquationsen_US
dc.subjectOriginen_US
dc.subject2022-APR-WEEK4en_US
dc.subjectTOC-MAY2022en_US
dc.subject2022en_US
dc.titleMatrix model with 3D BMS constraintsen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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