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The Hindered M1 Radiative Decay Υ(2S) → η_b(1S)γ from Lattice NRQCD

dc.creatorHughes, Ciaran
dc.creatorDowdall, Rachel J
dc.creatorDavies, Christine TH
dc.creatorHorgan, Ronald Raymond
dc.creatorvon, Hippel Georg
dc.creatorWingate, Matthew Bowen
dc.date.accessioned2018-11-24T23:18:24Z
dc.date.available2015-09-21T11:09:27Z
dc.date.available2018-11-24T23:18:24Z
dc.date.issued2015-11-03
dc.identifierhttps://www.repository.cam.ac.uk/handle/1810/251080
dc.identifier.urihttp://repository.aust.edu.ng/xmlui/handle/123456789/3268
dc.description.abstractWe present a calculation of the hindered M1 Υ(2S) → η_b(1S)γ decay rate using lattice nonrelativistic QCD. The calculation includes spin-dependent relativistic corrections to the NRQCD action through O(v⁶ ) in the quark’s relative velocity, relativistic corrections to the leading order current which mediates the transition through the quark’s magnetic moment, radiative corrections to the leading spin-magnetic coupling and for the first time a full error budget. We also use gluon field ensembles at multiple lattice spacing values, all of which include u, d, s and c quark vacuum polarisation. Our result for the branching fraction is B(Υ(2S) → η_b(1S)γ) = 5.4(1.8) × 10‾⁴ , which agrees with the current experimental value.
dc.languageen
dc.publisherAPS
dc.publisherPhysical Review D
dc.titleThe Hindered M1 Radiative Decay Υ(2S) → η_b(1S)γ from Lattice NRQCD
dc.typeArticle


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