| dc.contributor.author | The BESIII collaboration | en_US |
| dc.contributor.author | Kolcu, Onur Buğra | en_US |
| dc.date.accessioned | 2019-10-29T17:49:40Z | |
| dc.date.available | 2019-10-29T17:49:40Z | |
| dc.date.issued | 2015 | |
| dc.identifier.issn | 1550-7998 | |
| dc.identifier.uri | https://dx.doi.org/10.1103/PhysRevD.91.032002 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12294/2243 | |
| dc.description.abstract | Using data samples collected at center-of-mass energies s=4.23, 4.26, and 4.36 GeV with the BESIII detector operating at the BEPCII storage ring, we search for the production of the charmoniumlike state Y(4140) through a radiative transition followed by its decay to ?J/?. No significant signal is observed and upper limits on ?[e+e-??Y(4140)]·B(Y(4140)??J/?) at the 90% confidence level are estimated as 0.35, 0.28, and 0.33 pb at s=4.23, 4.26, and 4.36 GeV, respectively. © 2015 American Physical Society. | en_US |
| dc.language.iso | eng | en_US |
| dc.publisher | American Physical Society | en_US |
| dc.relation.ispartof | Physical Review D - Particles, Fields, Gravitation and Cosmology | en_US |
| dc.identifier.doi | 10.1103/PhysRevD.91.032002 | en_US |
| dc.identifier.doi | 10.1103/PhysRevD.91.032002 | |
| dc.rights | info:eu-repo/semantics/openAccess | en_US |
| dc.title | Search for the y (4140) via e+e- ???J /? at s =4.23, 4.26 and 4.36 GeV | en_US |
| dc.type | article | en_US |
| dc.department | İstanbul Arel Üniversitesi, Meslek Yüksekokulu, Optisyenlik Programı | en_US |
| dc.identifier.volume | 91 | en_US |
| dc.identifier.issue | 3 | en_US |
| dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
