Dominant spin-orbit effects in radiative decays gamma(3S) -> gamma + chi(bJ)(1P)

A.M. Badalian, B.L.G. Bakker

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Abstract

We show that there are two reasons why the partial width for the transition Γ
Original languageEnglish
Article number074001
JournalPhysical Review D
Volume86
Issue number7
DOIs
Publication statusPublished - 2012

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