Sigma(1385) Resonance Studies with STAR at sqrt{s_{NN}}=200 GeV
| dc.creator | Salur, Sevil | |
| dc.date | 2004-03-10 | |
| dc.date.accessioned | 2026-07-07T06:24:31Z | |
| dc.date.available | 2026-07-07T06:24:31Z | |
| dc.description | In p+p, d+Au, and Au+Au collisions at \sqrt{s_{NN}}=200 GeV with the STAR detector at RHIC, Σ(1385)\toΛ+πwere measured using two techniques; three-particle mixing and a hybrid mixing technique. We present results from both of these methods and compare the invariant mass spectra and the backgrounds. | |
| dc.description | NATO ASI Structure and Dynamics of Elementary Matter Conference Proceeding for Poster Presentation | |
| dc.identifier | https://arxiv.org/abs/hep-ex/0403016 | |
| dc.identifier | http://arxiv.org/abs/hep-ex/0403016 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/96570 | |
| dc.subject | High Energy Physics - Experiment | |
| dc.title | Sigma(1385) Resonance Studies with STAR at sqrt{s_{NN}}=200 GeV | |
| dc.type | text |