Mimar Sinan Güzel Sanatlar Üniversitesi Açık Bilim, Sanat Arşivi

Açık Bilim, Sanat Arşivi, Mimar Sinan Güzel Sanatlar Üniversitesi tarafından doğrudan ve dolaylı olarak yayınlanan; kitap, makale, tez, bildiri, rapor gibi tüm akademik kaynakları uluslararası standartlarda dijital ortamda depolar, Üniversitenin akademik performansını izlemeye aracılık eder, kaynakları uzun süreli saklar ve yayınların etkisini artırmak için telif haklarına uygun olarak Açık Erişime sunar.

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dc.contributor.authorBahtiyar, H.
dc.contributor.authorCan, K. U.
dc.contributor.authorErkol, G.
dc.contributor.authorOka, M.
dc.contributor.authorTakahashi, T. T.
dc.date.accessioned2025-01-09T20:12:25Z
dc.date.available2025-01-09T20:12:25Z
dc.date.issued2018
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.98.114505
dc.identifier.urihttps://hdl.handle.net/20.500.14124/8618
dc.description.abstractWe evaluate the spin-3/2 -> spin-1/2 electromagnetic transitions of the doubly charmed baryons on 2 + 1 flavor, 32(3) x 64 PACS-CS lattices with a pion mass of 156(9) MeV/c(2). A relativistic heavy quark action is employed to minimize the associated systematic errors on charm-quark observables. We extract the magnetic dipole, M1, and the electric quadrupole, E2, transition form factors. In order to make a reliable estimate of the M1 form factor, we carry out an analysis by including the effect of excited-state contributions. We find that the M1 transition is dominant and light degrees of freedom (u/d- or s-quark) play the leading role. E2 form factors, on the other hand, are found to be negligibly small, which in turn, have a minimal effect on the helicity and transition amplitudes. We predict the decay widths and lifetimes of Xi(cc)*(+,++) and Omega(cc)*(+) based on our results. Finite size effects on these ensembles are expected to be around 1%. Differences in kinematical and dynamical factors with respect to the N gamma -> Delta transition are discussed and compared to nonlattice determinations while keeping possible systematic artifacts in mind. A comparison to acy Omega(c)gamma -> Omega(c)* transition and a discussion on systematic errors related to the choice of heavy quark action are also given. Results we present here are particularly suggestive for experimental facilities such as LHCb, PANDA, Belle II, and BESIII to search for further states.en_US
dc.description.sponsorshipScientific and Technological Research Council of Turkey (TUBITAK) [114F261]; KAKENHI [25247036, 16K05365]; Grants-in-Aid for Scientific Research [16K05365] Funding Source: KAKENen_US
dc.description.sponsorshipThe unquenched gauge configurations employed in our analysis were generated by PACS-CS Collaboration [39]. We used a modified version of the Chroma software system [59] along with QUDA [60,61]. K. U. C. thanks Dr. Balint Joo for his guidance on the Chroma software system and Dr. Yusuke Namekawa for discussions on Tsukuba action and his comments on the manuscript. This work is supported in part by The Scientific and Technological Research Council of Turkey (TUBITAK) under Project No. 114F261 and in part by KAKENHI under Contracts No. 25247036 and No. 16K05365.en_US
dc.language.isoengen_US
dc.publisherAmer Physical Socen_US
dc.relation.ispartofPhysical Review Den_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.titleRadiative transitions of doubly charmed baryons in lattice QCDen_US
dc.typearticleen_US
dc.authoridBahtiyar, Huseyin/0000-0001-5952-1677
dc.authoridCan, Kadir Utku/0000-0002-7052-1421
dc.authoridTakahashi, Toru/0000-0002-8476-9751
dc.authoridOka, Makoto/0000-0003-3206-3770
dc.authoridErkol, Guray/0000-0002-7814-7681
dc.departmentMimar Sinan Güzel Sanatlar Üniversitesien_US
dc.identifier.doi10.1103/PhysRevD.98.114505
dc.identifier.volume98en_US
dc.identifier.issue11en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.identifier.wosqualityQ1
dc.identifier.wosWOS:000452980500005
dc.identifier.scopus2-s2.0-85059481980
dc.identifier.scopusqualityQ1
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.snmzKA_20250105


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