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  4. Study of the reaction e[superscript +]e[superscript -]→J/ψπ[superscript +]π[superscript -] via initial-state radiation at BABAR

Study of the reaction e[superscript +]e[superscript -]→J/ψπ[superscript +]π[superscript -] via initial-state radiation at BABAR

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Author(s)
Dujmic, Denis
•
Sciolla, Gabriella
•
Cowan, Ray F
Date Issued
September 2012
Journal
Physical Review D
Publisher
American Physical Society
Citation
Lees, J. et al. “Study of the reaction e[superscript +]e[superscript -]→J/ψπ[superscript +]π[superscript -] via initial-state radiation at BABAR.” Physical Review D 86.5 (2012). © 2012 American Physical Society
Version
Final published version
Abstract
We study the process e[superscript +]e[superscript -]→J/ψπ[superscript +]π[superscript -] with initial-state-radiation events produced at the PEP-II asymmetric-energy collider. The data were recorded with the BABAR detector at center-of-mass energies 10.58 and 10.54 GeV, and correspond to an integrated luminosity of 454  fb[superscript -1]. We investigate the J/ψπ[superscript +]π[superscript -] mass distribution in the region from 3.5 to 5.5  GeV/c[superscript 2]. Below 3.7  GeV/c[superscript 2] the ψ(2S) signal dominates, and above 4  GeV/c[superscript 2] there is a significant peak due to the Y(4260). A fit to the data in the range 3.74–5.50  GeV/c[superscript 2] yields a mass value 4245±5(stat)±4(syst)  MeV/c[superscript 2] and a width value 114[subscript -15][superscript +16](stat)±7(syst)  MeV for this state. We do not confirm the report from the Belle Collaboration of a broad structure at 4.01  GeV/c[superscript 2]. In addition, we investigate the π[superscript +]π[superscript -] system which results from Y(4260) decay.
MIT Department
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/1721.1/76655
DOI of Published Version
https://doi.org/10.1103/PhysRevD.86.051102
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