Please use this identifier to cite or link to this item: http://earchive.tpu.ru/handle/11683/64874
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dc.contributor.authorAaij, Roelen
dc.contributor.authorBeteta, Carlos Abellanen
dc.contributor.authorAdeva, Bernardoen
dc.contributor.authorShapkin, Mikhail Mikhaylovichen
dc.contributor.authorPanshin, Gennady Leonidovichen
dc.contributor.authorStrokov, Sergey Aleksandrovichen
dc.date.accessioned2021-03-21T16:52:28Z-
dc.date.available2021-03-21T16:52:28Z-
dc.date.issued2019-
dc.identifier.citationAmplitude Analysis of B±→π±K+K− Decays / R. Aaij, C. A. Beteta, B. Adeva [et al.] // Physical Review Letters. — 2019. — Vol. 123, iss. 23. — [231802, 11 p.].en
dc.identifier.urihttp://earchive.tpu.ru/handle/11683/64874-
dc.description.abstractThe first amplitude analysis of the B±→π±K+K− decay is reported based on a data sample corresponding to an integrated luminosity of 3.0  fb−1 of pp collisions recorded in 2011 and 2012 with the LHCb detector. The data are found to be best described by a coherent sum of five resonant structures plus a nonresonant component and a contribution from ππ↔KK S-wave rescattering. The dominant contributions in the π± K∓ and K+ K− systems are the nonresonant and the B±→ρ(1450)0π± amplitudes, respectively, with fit fractions around 30%. For the rescattering contribution, a sizable fit fraction is observed. This component has the largest CP asymmetry reported to date for a single amplitude of (−66±4±2)%, where the first uncertainty is statistical and the second systematic. No significant CP violation is observed in the other contributions.en
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.ispartofPhysical Review Letters. 2019. Vol. 123, iss. 23en
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightsAttribution-NonCommercial 4.0 Internationalen
dc.rights.urihttps://creativecommons.org/licenses/by-nc/4.0/-
dc.sourcePhysical Review Lettersen
dc.titleAmplitude Analysis of B±→π±K+K− Decaysen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dcterms.audienceResearchesen
local.description.firstpage231802-
local.filepathreprint-nw-34590.pdf-
local.filepathhttps://doi.org/10.1103/PhysRevLett.123.231802-
local.identifier.bibrecRU\TPU\network\34590-
local.identifier.perskeyRU\TPU\pers\40978-
local.identifier.perskeyRU\TPU\pers\37442-
local.issue23-
local.localtypeСтатьяru
local.volume123-
dc.identifier.doi10.1103/PhysRevLett.123.231802-
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