1993/11/24 by Hugh Shanahan, UKQCD Collaboration
Physics and Astronomy · #hep-lat
published as Nucl.Phys.Proc.Suppl. 34 (1994) 474-476 · 3 pages uuencoded postscript, to appear in the Proceedings of LATTICE 93 Dallas, Edinburgh Preprint 93/529
arxiv created 1993/11/24 · arxiv updated 2009/12/01
Preliminary results are presented on the calculation of the relevant form factor for the radiative decay B → K^* γ We find that the form factor is weakly dependent on the spectator quark mass. We compare the results obtained for a full chiral extrapolation and where this independence is assumed. Both results are found to be statistically consistent with the experimental data.