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Observation of e+eωχbJ(1P) and Search for Xbωϒ(1S) at s near 10.75 GeV

I. Adachi et al. (Belle II Collaboration)
Phys. Rev. Lett. 130, 091902 – Published 3 March 2023
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Abstract

We study the processes e+eωχbJ(1P) (J=0, 1, or 2) using samples at center-of-mass energies s=10.701, 10.745, and 10.805 GeV, corresponding to 1.6, 9.8, and 4.7fb1 of integrated luminosity, respectively. These data were collected with the Belle II detector during special operations of the SuperKEKB collider above the ϒ(4S) resonance. We report the first observation of ωχbJ(1P) signals at s=10.745GeV. By combining Belle II data with Belle results at s=10.867GeV, we find energy dependencies of the Born cross sections for e+eωχb1,b2(1P) to be consistent with the shape of the ϒ(10753) state. These data indicate that the internal structures of the ϒ(10753) and ϒ(10860) states may differ. Including data at s=10.653GeV, we also search for the bottomonium equivalent of the X(3872) state decaying into ωϒ(1S). No significant signal is observed for masses between 10.45 and 10.65GeV/c2.

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  • Received 29 August 2022
  • Accepted 25 January 2023

DOI:https://doi.org/10.1103/PhysRevLett.130.091902

Published by the American Physical Society under the terms of the 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 SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

  1. Physical Systems
Particles & Fields

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Vol. 130, Iss. 9 — 3 March 2023

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  • Figure 1
    Figure 1

    Distributions of (left) γϒ(1S) and (right) π+ππ0 masses in data at s=10.701, 10.745, and 10.805 GeV with fit results overlaid.

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  • Figure 2
    Figure 2

    Energy dependence of the Born cross sections for (left) e+eωχb1 and (right) e+eωχb2. Circles show the measurements reported here, triangles are the results of the Belle experiment [41]. Error bars represent combined statistical and systematic uncertainties. Curves show the fit results and various components of the fit function.

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  • Figure 3
    Figure 3

    Distributions of ωϒ(1S) mass from data at s=10.653, 10.701, 10.745, and 10.805 GeV. The red dash-dotted histograms are from simulated events e+eγXb[ωϒ(1S)] with the Xb mass fixed at 10.6GeV/c2 and yields fixed at the upper limit values.

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