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dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorCoppage, Don
dc.contributor.authorGardner, J.
dc.contributor.authorHensel, Carsten
dc.contributor.authorMoulik, Tania
dc.contributor.authorWilson, Graham Wallace
dc.date.accessioned2014-10-27T15:55:04Z
dc.date.available2014-10-27T15:55:04Z
dc.date.issued2006-07-14
dc.identifier.citationV. M. Abazov et al. (D0 Collaboration). (2006). "Direct Limits on the B(0)(s) Oscillation Frequency." Physical Review D, 97(2):021802. http://dx.doi.org/10.1103/PhysRevLett.97.021802.
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/1808/15391
dc.descriptionThis is the publisher's version, also available electronically from http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.97.021802.
dc.description.abstractWe report results of a study of the B(0)(s) oscillation frequency using a large sample of B(0)(s) semileptonic decays corresponding to approximately 1  fb(−1) of integrated luminosity collected by the D0 experiment at the Fermilab Tevatron Collider in 2002–2006. The amplitude method gives a lower limit on the B(0)(s) oscillation frequency at 14.8  ps(−1) at the 95% C.L. At Δms=19  ps(−1), the amplitude deviates from the hypothesis A=0 (1) by 2.5 (1.6) standard deviations, corresponding to a two-sided C.L. of 1% (10%). A likelihood scan over the oscillation frequency, Δms, gives a most probable value of 19  ps(−1) and a range of 17<Δms<21  ps(−1) at the 90% C.L., assuming Gaussian uncertainties. This is the first direct two-sided bound measured by a single experiment. If Δms lies above 22  ps(−1), then the probability that it would produce a likelihood minimum similar to the one observed in the interval 16–22  ps(−1) is (5.0±0.3)%.
dc.publisherAmerican Physical Society
dc.titleDirect Limits on the B(0)(s) Oscillation Frequency
dc.typeArticle
kusw.kuauthorBaringer, Philip S.
kusw.kuauthorBean, Alice
kusw.kuauthorCoppage, Don
kusw.kuauthorGardner, J.
kusw.kuauthorHensel, Carsten
kusw.kuauthorMoulik, Tania
kusw.kuauthorWilson, Graham Wallace
kusw.kudepartmentPhysics and Astronomy
dc.identifier.doi10.1103/PhysRevLett.97.021802
kusw.oaversionScholarly/refereed, publisher version
kusw.oapolicyThis item meets KU Open Access policy criteria.
dc.rights.accessrightsopenAccess


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