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dc.contributor.authorDubbs, Alexander Joseph
dc.contributor.authorEdelman, Alan
dc.contributor.authorKoev, Plamen
dc.contributor.authorVenkataramana, Praveen
dc.date.accessioned2015-01-14T18:45:15Z
dc.date.available2015-01-14T18:45:15Z
dc.date.issued2013-08
dc.date.submitted2013-04
dc.identifier.issn00222488
dc.identifier.urihttp://hdl.handle.net/1721.1/92863
dc.description.abstractWe introduce a “broken-arrow” matrix model for the β-Wishart ensemble, which improves on the traditional bidiagonal model by generalizing to non-identity covariance parameters. We prove that its joint eigenvalue density involves the correct hypergeometric function of two matrix arguments, and a continuous parameter β > 0. If we choose β = 1, 2, 4, we recover the classical Wishart ensembles of general covariance over the reals, complexes, and quaternions. Jack polynomials are often defined as the eigenfunctions of the Laplace-Beltrami operator. We prove that Jack polynomials are in addition eigenfunctions of an integral operator defined as an average over a β-dependent measure on the sphere. When combined with an identity due to Stanley, we derive a definition of Jack polynomials. An efficient numerical algorithm is also presented for simulations. The algorithm makes use of secular equation software for broken arrow matrices currently unavailable in the popular technical computing languages. The simulations are matched against the cdfs for the extreme eigenvalues. The techniques here suggest that arrow and broken arrow matrices can play an important role in theoretical and computational random matrix theory including the study of corners processes. We provide a number of simulations illustrating the extreme eigenvalue distributions that are likely to be useful for applications. We also compare the n → ∞ answer for all β with the free-probability prediction.en_US
dc.description.sponsorshipSan Jose State University (Woodward Fund for Applied Mathematics)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (SOLAR Grant No. 1035400)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (SOLAR Grant No. DMS-1035400)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (SOLAR Grant No. DMS-1016086)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (NSF GRFP)en_US
dc.language.isoen_US
dc.publisherAmerican Institute of Physics (AIP)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1063/1.4818304en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceMIT web domainen_US
dc.titleThe beta-Wishart ensembleen_US
dc.typeArticleen_US
dc.identifier.citationDubbs, Alexander, Alan Edelman, Plamen Koev, and Praveen Venkataramana. “The Beta-Wishart Ensemble.” Journal of Mathematical Physics 54, no. 8 (2013): 083507. © 2013 AIP.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Mathematicsen_US
dc.contributor.mitauthorDubbs, Alexander Josephen_US
dc.contributor.mitauthorEdelman, Alanen_US
dc.contributor.mitauthorVenkataramana, Praveenen_US
dc.relation.journalJournal of Mathematical Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsDubbs, Alexander; Edelman, Alan; Koev, Plamen; Venkataramana, Praveenen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7676-3133
dspace.mitauthor.errortrue
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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