Observation of h_b(1P)->eta_b(1S)gamma

TL;DR

This paper reports the first observation of the radiative transition h_b(1P) to eta_b(1S) gamma, measuring eta_b(1S) properties and hyperfine splittings, revealing significant deviations from previous measurements and enhancing understanding of bottomonium states.

Contribution

First observation of h_b(1P) to eta_b(1S) gamma transition with precise measurements of eta_b(1S) mass, width, and hyperfine splitting using Belle data.

Findings

Measured eta_b(1S) mass: 9401.0 MeV/c^2

Observed hyperfine splitting: 59.3 MeV/c^2

Branching fraction: 49.8%

Abstract

We report the first observation of the radiative transition h_b(1P)->eta_b(1S)gamma, where the h_b(1P) is produced in Upsilon(5S)->h_b(1P)pi+pi- dipion transitions. We measure the eta_b(1S) mass to be (9401.0+-1.9+1.4-2.4)MeV/c^2 with a width of (12.4+5.5-4.6+11.5-3.4)MeV and a decay branching fraction of BF[h_b(1P)->eta_b(1S)gamma]=(49.8+-6.8+10.9-5.2)%. The measured eta_b(1S) mass corresponds to a hyperfine splitting of (59.3+-1.9+2.4-1.4)MeV/c^2. This value deviates significantly from the current world average obtained from measurements of Upsilon(3S)->eta_b(1S)gamma and Upsilon(2S)->eta_b(1S)gamma reactions. We also report updated results for the h_b(1P) mass (9899.0+-0.4+-1.0)MeV/c^2 and its hyperfine splitting (0.8+-1.1)MeV/c^2. These measurements are performed using a 121.4fb^-1 data sample collected at the peak of the Upsilon(5S) resonance with the Belle detector at the KEKB asymmetric-energy e+e- collider.