Observation of the decay D-0 -> rho - mu + nu(mu)
dc.authorid | Onur Buğra Kolcu / 0000-0002-9177-1286 | en_US |
dc.authorid | Serkant Ali Çetin / 0000-0001-5050-8441 | |
dc.authorscopusid | Serkant Ali Çetin / 34567544400 | |
dc.authorwosid | Serkant Ali Çetin / AGF-0147-2022 | |
dc.authorwosid | Onur Buğra Kolcu / P-4990-2015 | |
dc.contributor.author | Ablikim, M. | |
dc.contributor.author | Achasov, M. N. | |
dc.contributor.author | Adlarson, P. | |
dc.contributor.author | Ahmed, S. | |
dc.contributor.author | Albrecht, M. | |
dc.contributor.author | Çetin, Serkant Ali | |
dc.contributor.author | Kolcu, Onur Buğra | |
dc.date.accessioned | 2022-01-10T07:05:28Z | |
dc.date.available | 2022-01-10T07:05:28Z | |
dc.date.issued | 2021 | en_US |
dc.department | İstinye Üniversitesi | en_US |
dc.description.abstract | By analyzing an e(+)e(-) annihilation data sample corresponding to an integrated luminosity of 2.93 fb(- 1) collected at a center-of-mass energy of 3.773 GeV with the BESIII detector, we measure the branching fraction of the D-0 ->rho(-) mu(+)nu(mu) decay for the first time. We obtain BD0 ->rho(-) mu(+)nu(mu) = (1.35 +/- 0.09(stat) +/- 0.09(syst)) x 10(-3). Using the world average of BD0 ->(rho)- epsilon(+)nu(epsilon), we find a branching fraction ratio of BD0 ->rho(-) mu(+)nu(mu)/ BD0 ->rho(-)e(+) nu(epsilon) = 0.90 +/- 0.11, which agrees with the theoretical expectation of lepton flavor universality within the uncertainty. Combining the world average of BD+->rho(0)mu+(.nu)(mu) and the lifetimes of D0(+), we obtain a partial decay width ratio of Gamma D-0 ->rho(-)mu(+)nu mu/2 Gamma D-0 ->rho(0)mu(+)nu(mu) ) = 0.71 +/- 0.14, which is consistent with the isospin symmetry expectation of unity within 2.1s. For the reported values of BD0 ->rho(-) mu(+)nu(mu)/BD0 ->rho(-)e+nu(e) and Gamma D-0 ->rho(-) mu(+nu)(mu) /2 Gamma(+)(D) ->rho(0)mu(+) nu(mu), the uncertainty is the quadratic sum of the statistical and systematic uncertainties. | en_US |
dc.identifier.doi | 10.1103/PhysRevD.104.L091103 | en_US |
dc.identifier.issn | 2470-0010 | en_US |
dc.identifier.issn | 2470-0029 | en_US |
dc.identifier.issue | 104 | en_US |
dc.identifier.uri | https://doi.org/10.1103/PhysRevD.104.L091103 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12713/2384 | |
dc.identifier.volume | 9 | en_US |
dc.identifier.wos | WOS:000725012100033 | en_US |
dc.identifier.wosquality | Q1 | en_US |
dc.indekslendigikaynak | Web of Science | en_US |
dc.institutionauthor | Çetin, Serkant Ali | |
dc.institutionauthor | Kolcu, Onur Buğra | |
dc.language.iso | en | en_US |
dc.publisher | AMER PHYSICAL SOC | en_US |
dc.relation.ispartof | PHYSICAL REVIEW D | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.subject | D+ | en_US |
dc.subject | Semileptonic-B | en_US |
dc.title | Observation of the decay D-0 -> rho - mu + nu(mu) | en_US |
dc.type | Article | en_US |