The Hyperfine Spin Splittings In Heavy Quarkonia

Abstract

The hyperfine spin splittings in heavy quarkonia are studied using the recently developed renormalization group improved spin-spin potential which is independent of the scale parameter μ. The calculated energy difference between the J/ and the ηc fits the experimental data well, while the predicted energy difference Mp between the center of the gravity of 13P0,1,2 states and the 11P1 state of charmonium has the correct sign but is somewhat larger than the experimental data. This is not surprising since there are several other contributions to Mp, which we discuss, that are of comparable size ( 1 MeV) that should be included, before precise agreement with the data can be expected. The mass differences of the '-ηc', (1S)-ηb, (2S)-ηb', and Bc*-Bc are also predicted.

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