dc.contributor.author | Walker, M. | |
dc.contributor.author | van Nieuwenhuizen, Gerrit Jan | |
dc.contributor.author | Stevens, Justin | |
dc.contributor.author | Balewski, Jan T. | |
dc.contributor.author | Corliss, Ross | |
dc.contributor.author | Hays-Wehle, James Prewitt | |
dc.contributor.author | Leight, William Axel | |
dc.date.accessioned | 2015-02-19T16:52:05Z | |
dc.date.available | 2015-02-19T16:52:05Z | |
dc.date.issued | 2014-10 | |
dc.date.submitted | 2014-10 | |
dc.identifier.issn | 03702693 | |
dc.identifier.uri | http://hdl.handle.net/1721.1/94636 | |
dc.description.abstract | We report on a polarization measurement of inclusive [J over ψ] mesons in the di-electron decay channel at mid-rapidity at 2<p[subscript T]<6 GeV/c in p+p collisions at √s = 200 GeV. Data were taken with the STAR detector at RHIC. The [J over ψ] polarization measurement should help to distinguish between different models of the [J over ψ] production mechanism since they predict different p[subscript T] dependences of the [J over ψ] polarization. In this analysis, [J over ψ] polarization is studied in the helicity frame. The polarization parameter λ[subscript θ] measured at RHIC becomes smaller towards high p[subscript T], indicating more longitudinal [J over ψ] polarization as p[subscript T] increases. The result is compared with predictions of presently available models. | en_US |
dc.description.sponsorship | United States. Dept. of Energy. Office of Science | en_US |
dc.description.sponsorship | National Science Foundation (U.S.) | en_US |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.relation.isversionof | http://dx.doi.org/10.1016/j.physletb.2014.10.049 | en_US |
dc.rights | Creative Commons Attribution | en_US |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | en_US |
dc.source | Elsevier | en_US |
dc.title | [J over ψ] polarization in p+p collisions at √s = 200 TeV in STAR | en_US |
dc.type | Article | en_US |
dc.identifier.citation | “[J over ψ] polarization in p+p collisions at √s = 200 TeV in STAR.” Physics Letters B 739 (December 2014): 180–188. | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Laboratory for Nuclear Science | en_US |
dc.contributor.mitauthor | Walker, M. | en_US |
dc.contributor.mitauthor | van Nieuwenhuizen, Gerrit Jan | en_US |
dc.contributor.mitauthor | Stevens, Justin | en_US |
dc.contributor.mitauthor | Balewski, Jan T. | en_US |
dc.contributor.mitauthor | Corliss, Ross | en_US |
dc.contributor.mitauthor | Hays-Wehle, James Prewitt | en_US |
dc.contributor.mitauthor | Leight, William Axel | en_US |
dc.relation.journal | Physics Letters B | en_US |
dc.eprint.version | Final published version | en_US |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
dc.identifier.orcid | https://orcid.org/0000-0002-5515-4563 | |
dc.identifier.orcid | https://orcid.org/0000-0002-0816-200X | |
dspace.mitauthor.error | true | |
mit.license | PUBLISHER_CC | en_US |
mit.metadata.status | Complete | |