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Relativistic flux tube model calculation of the Isgur-Wise function

Journal Article · · Physical Review, D (Particles Fields); (United States)
;  [1]
  1. Department of Physics, University of Wisconsin, Madison, Wisconsin 53706 (United States)

The relativistic flux tube model is used to calculate the Isgur-Wise (IW) functions describing the exclusive semileptonic decays of [ital [bar B]] and [ital [bar B]][sub [ital s]] mesons. The light quark mass dependence is investigated and the predicted universal function agrees well with the results of lattice simulations, and with the experimental data. Recent experimental measurements of the [ital [bar B]][r arrow][ital D][sup *][ital l][bar [nu]][sub [ital l]] decay distribution yield the Cabibbo-Kobayashi-Maskawa element [ital V][sub [ital b][ital c]]=0.035[plus minus]0.001. The IW function slope and second derivative at the zero recoil point are predicted to be [xi][prime](1)=[minus]0.93[plus minus]0.04 and [xi][prime][prime](1)=1.7[plus minus]0.1 for a range of light quark masses. The importance of including higher derivatives in analyses of experiment is emphasized.

DOE Contract Number:
AC02-76ER00881
OSTI ID:
6579686
Journal Information:
Physical Review, D (Particles Fields); (United States), Journal Name: Physical Review, D (Particles Fields); (United States) Vol. 51:5; ISSN PRVDAQ; ISSN 0556-2821
Country of Publication:
United States
Language:
English