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Study of e+ e- → ωX(3872) and γX(3872) from 4.66 to 4.95 GeV
Inst High Energy Phys, Beijing 100049, Peoples R China.
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. Uppsala Univ, Box 516, SE-75120 Uppsala, Sweden.ORCID iD: 0000-0001-6280-3851
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. Uppsala Univ, Box 516, SE-75120 Uppsala, Sweden.ORCID iD: 0000-0002-6945-716x
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Nuclear Physics. Natl Ctr Nucl Res, PL-02093 Warsaw, Poland;Uppsala Univ, Box 516, SE-75120 Uppsala, Sweden.ORCID iD: 0000-0003-4937-2270
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Number of Authors: 6562024 (English)In: Physical Review D: covering particles, fields, gravitation, and cosmology, ISSN 2470-0010, E-ISSN 2470-0029, Vol. 110, no 1, article id 012006Article in journal (Refereed) Published
Abstract [en]

Using data samples with an integrated luminosity of 4.5 fb(-1) collected by the BESIII detector at center-of-mass energies ranging from 4.66 GeV to 4.95 GeV, we study the processes of e(+) e(-) -> omega X(3872) and e(+) e(-) -> gamma X(3872). With the e(+) e(-) -> X(3872) process, the branching fraction ratio R = B(X(3872)->gamma J/psi)/B(X(3872)pi(+)pi(-)J/psi is measured to be 0.38 +/- 0.20(stat) +/- 0.01(syst) (R < 0.83 at 90% confidence level). In addition, we measure the ratio of the average cross section of e(+) e(-) -> omega X(3872) to e(+) e(-) -> omega chi(c1)(omega chi(c2)) to be sigma(omega X(3872))/sigma(omega Xc1)(sigma(omega X(3872))/sigma(omega Xc2)) = 5.2 +/- 1.0(stat) +/- 1.9(syst)(5.5 +/- 1.1(stat) +/- 2.4(syst)). Finally, we search for the process of e(+) e(-) -> gamma X(3872), and no obvious signal is observed. The upper limit on the ratio of the average cross section of e(+) e(-) -> gamma X(3872) to e(+) e(-) -> gamma X(3872) is set as sigma(gamma X)(3872)/sigma(omega X(3872)) < 0.23 at 90% confidence level.

Place, publisher, year, edition, pages
AMER PHYSICAL SOC , 2024. Vol. 110, no 1, article id 012006
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Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-550220DOI: 10.1103/PhysRevD.110.012006ISI: 001397782100001OAI: oai:DiVA.org:uu-550220DiVA, id: diva2:1937538
Funder
Swedish Research Council
Note

For complete list of authors see http://dx.doi.org/10.1103/PhysRevD.110.012006

Available from: 2025-02-13 Created: 2025-02-13 Last updated: 2025-02-13Bibliographically approved

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Adlarson, PatrikJohansson, TordKupsc, AndrzejSchönning, KarinThorén, ViktorWolke, Magnus
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