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dc.creatorAdam, J
dc.creatorAdamczyk, L
dc.creatorAdams, JR
dc.creatorAdkins, JK
dc.creatorAgakishiev, G
dc.creatorAggarwal, MM
dc.creatorAhammed, Z
dc.creatorAjitanand, NN
dc.creatorAlekseev, I
dc.creatorAnderson, DM
dc.creatorAoyama, R
dc.creatorAparin, A
dc.creatorArkhipkin, D
dc.creatorAschenauer, EC
dc.creatorAshraf, MU
dc.creatorAtetalla, F
dc.creatorAttri, A
dc.creatorAverichev, GS
dc.creatorBai, X
dc.creatorBairathi, V
dc.creatorBarish, K
dc.creatorBassill, AJ
dc.creatorBehera, A
dc.creatorBellwied, R
dc.creatorBhasin, A
dc.creatorBhati, AK
dc.creatorBielcik, J
dc.creatorBielcikova, J
dc.creatorBland, LC
dc.creatorBordyuzhin, IG
dc.creatorBrandenburg, JD
dc.creatorBrandin, AV
dc.creatorBrown, D
dc.creatorBryslawskyj, J
dc.creatorBunzarov, I
dc.creatorButterworth, J
dc.creatorCaines, H
dc.creatorCalderón De La Barca Sánchez, M
dc.creatorCampbell, JM
dc.creatorCebra, D
dc.creatorChakaberia, I
dc.creatorChaloupka, P
dc.creatorChang, FH
dc.creatorChang, Z
dc.creatorChankova-Bunzarova, N
dc.creatorChatterjee, A
dc.creatorChattopadhyay, S
dc.creatorChen, JH
dc.creatorChen, X
dc.creatorChen, X
dc.creatorCheng, J
dc.creatorCherney, M
dc.creatorChristie, W
dc.creatorContin, G
dc.creatorCrawford, HJ
dc.creatorDas, S
dc.creatorDedovich, TG
dc.creatorDeppner, IM
dc.creatorDerevschikov, AA
dc.creatorDidenko, L
dc.creatorDilks, C
dc.creatorDong, X
dc.creatorDrachenberg, JL
dc.creatorDunlop, JC
dc.creatorEfimov, LG
dc.creatorElsey, N
dc.creatorEngelage, J
dc.creatorEppley, G
dc.creatorEsha, R
dc.creatorEsumi, S
dc.creatorEvdokimov, O
dc.creatorEwigleben, J
dc.creatorEyser, O
dc.creatorFatemi, R
dc.creatorFazio, S
dc.creatorFederic, P
dc.creatorFedericova, P
dc.creatorFedorisin, J
dc.creatorFilip, P
dc.creatorFinch, E
dc.creatorFisyak, Y
dc.creatorFlores, CE
dc.creatorFulek, L
dc.creatorGagliardi, CA
dc.creatorGalatyuk, T
dc.creatorGeurts, F
dc.creatorGibson, A
dc.creatorGrosnick, D
dc.creatorGunarathne, DS
dc.creatorGuo, Y
dc.creatorGupta, A
dc.creatorGuryn, W
dc.creatorHamad, AI
dc.creatorHamed, A
dc.creatorHarlenderova, A
dc.creatorHarris, JW
dc.creatorHe, L
dc.creatorHeppelmann, S
dc.creatorHeppelmann, S
dc.creatorHerrmann, N
dc.date.accessioned2020-12-14T18:23:40Z
dc.date.available2020-12-14T18:23:40Z
dc.date.issued2018-09-25
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.doihttp://dx.doi.org/10.34944/dspace/4379
dc.identifier.other30312102 (pubmed)
dc.identifier.urihttp://hdl.handle.net/20.500.12613/4397
dc.description.abstract©) between 40 and 60 MeV/c. The absolute cross section of the excess depends weakly on centrality, while those from a theoretical model calculation incorporating an in-medium broadened ρ spectral function and radiation from a quark gluon plasma or hadronic cocktail contributions increase dramatically with an increasing number of participant nucleons. Model calculations of photon-photon interactions generated by the initial projectile and target nuclei describe the observed excess yields but fail to reproduce the pT2 distributions. © 2018 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the »https://creativecommons.org/licenses/by/4.0/» Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP 3 . We report first measurements of e+e- pair production in the mass region 0.4<Mee<2.6 GeV/c2 at low transverse momentum (pT<0.15 GeV/c) in noncentral Au+Au collisions at sNN=200 GeV and U+U collisions at sNN=193 GeV. Significant enhancement factors, expressed as ratios of data over known hadronic contributions, are observed in the 40%-80% centrality of these collisions. The excess yields peak distinctly at low pT with a width (âpT2â
dc.format.extent132301-
dc.language.isoen
dc.relation.haspartPhysical Review Letters
dc.relation.isreferencedbyAmerican Physical Society (APS)
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectSTAR Collaboration
dc.titleLow- pT e+e- Pair Production in Au +Au Collisions at sNN =200 GeV and U + U Collisions at sNN =193 GeV at STAR
dc.typeArticle
dc.type.genreJournal Article
dc.relation.doi10.1103/PhysRevLett.121.132301
dc.ada.noteFor Americans with Disabilities Act (ADA) accommodation, including help with reading this content, please contact scholarshare@temple.edu
dc.date.updated2020-12-14T18:23:35Z
refterms.dateFOA2020-12-14T18:23:40Z


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