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Di-electron spectrum at mid-rapidity in p+p collisions at √s=200 GeV

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Author(s)
Balewski, Jan T.
•
Betancourt, Michael Joseph
•
Corliss, Ross Cameron
•
Hays-Wehle, James Prewitt
•
Leight, William Axel
•
Surrow, Bernd
•
Redwine, Robert P
•
Seele, Joseph Patrick
•
Steadman, Stephen G
•
van Nieuwenhuizen, Gerrit J
Date Issued
August 2012
Journal
Physical Review C
Publisher
American Physical Society
Citation
Adamczyk, L. et al. “Di-electron spectrum at mid-rapidity in p+p collisions at √s=200 GeV.” Physical Review C 86.2 (2012). ©2012 American Physical Society
Version
Final published version
Abstract
We report on the mid-rapidity mass spectrum of di-electrons and cross sections of pseudoscalar and vector mesons via e[superscript +]e[superscript −] decays, from √s=200 GeV p+p collisions, measured by the large-acceptance experiment STAR at the Relativistic Heavy Ion Collider. The ratio of the di-electron continuum to the combinatorial background is larger than 10% over the entire mass range. Simulations of di-electrons from light-meson decays and heavy-flavor decays (charmonium and open charm correlation) are found to describe the data. The extracted ω→e[superscript +]e[superscript −] invariant yields are consistent with previous measurements. The mid-rapidity yields (d N/dy) of φ and J/ψ are extracted through their di-electron decay channels and are consistent with the previous measurements of φ→K[superscript +]K[superscript −] and J/ψ→e[superscript +]e[superscript −]. Our results suggest a new upper limit of the branching ratio of the η→e[superscript +]e[superscript −] of 1.7×10[superscript −5] at the 90% confidence level.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/74209
DOI of Published Version
https://doi.org/10.1103/PhysRevC.86.024906
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