N. M. Hazel
University of Edinburgh
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Featured researches published by N. M. Hazel.
Nuclear Physics | 1995
D.R. Burford; Hoa Dung Ha Duong; Jonathan M. Flynn; Brian J. Gough; N. M. Hazel; J. Nieves; H.P. Shanahan
We present a unified method for analysing form factors in B -> pi l nu-bar_l and B -> K* gamma decays. The analysis provides consistency checks on the q^2 and 1/M extrapolations necessary to obtain the physical decay rates. For the first time the q^2 dependence of the form factors is obtained at the B scale. In the B -> pi l nu-bar_l case, we show that pole fits to f^+ may not be consistent with the q^2 behaviour of f^0, leading to a possible factor of two uncertainty in the decay rate and hence in the value of |V_{ub}|^2 deduced from it. For B -> K* gamma, from the combined analysis of form factors T_1 and T_2, we find the hadronisation ratio R_{K^*} of the exclusive B -> K* gamma to the inclusive b -> s gamma rates is of order 35% or 15% for constant and pole-type behaviour of T_2 respectively.
Physical Review Letters | 1994
S. P. Booth; K.C. Bowler; N. M. Hazel; David Henty; H. Hoeber; R.D. Kenway; D. G. Richards; H. P. Shanahan; J.N. Simone; Alan Simpson; Laurent Lellouch; J. Nieves; Christopher T. Sachrajda; Hartmut Wittig
We calculate the Isgur-Wise function by measuring the elastic scattering amplitude of a D meson in the quenched approximation on a
Physical Review D | 1995
K.C. Bowler; N. M. Hazel; H. Hoeber; R.D. Kenway; D.G. Richards; L. Lellouch; J. Nieves; C.T. Sachrajda; Hartmut Wittig
{24}^{3}
Nuclear Physics | 1996
Jonathan M. Flynn; J. Nieves; K.C. Bowler; N. M. Hazel; D.S Hent; H. Hoeber; R.D. Kenway; D.G. Richards; Brian J. Gough; Laurent Lellouch; H. P. Shanahan
\ifmmode\times\else\texttimes\fi{}48 lattice at \ensuremath{\beta}=6.2, using an O(a)-improved fermion action. Fitting the resulting chirally extrapolated Isgur-Wise function to Stechs relativistic-oscillator parametrization, we obtain a slope parameter
Physical Review D | 1995
K.C. Bowler; N. M. Hazel; H. Hoeber; R.D. Kenway; David G. Richards; L. Lellouch; J. Nieves; C.T. Sachrajda; Hartmut Wittig
{\mathrm{\ensuremath{\rho}}}^{2}
Physical Review Letters | 1994
K.C. Bowler; N. M. Hazel; David Henty; H. Hoeber; R.D. Kenway; David G. Richards; H. P. Shanahan; J.N. Simone; J.M. Flynn; Brian J. Gough
=1.
Physical Review D | 1995
K.C. Bowler; N. M. Hazel; David Henty; H. Hoeber; R.D. Kenway; D.G. Richards; H. P. Shanahan; J.N. Simone; Jonathan M. Flynn; Brian J. Gough
{2}_{\mathrm{\ensuremath{-}}3}^{+7}
Physical Review Letters | 1994
K.C. Bowler; N. M. Hazel; David Henty; H. Hoeber; R.D. Kenway; David G. Richards; H. P. Shanahan; J.N. Simone; J.M. Flynn; Brian J. Gough
. We then use this result, in conjunction with heavy-quark symmetry, to extract
Nuclear Physics | 1996
Jonathan M. Flynn; J. Nieves; K.C. Bowler; N. M. Hazel; D.S Hent; H. Hoeber; R.D. Kenway; David G. Richards; Brian J. Gough; Laurent Lellouch; H. P. Shanahan
{\mathit{V}}_{\mathit{c}\mathit{b}}
Physical Review D | 1994
K.C. Bowler; H. Hoeber; Brian J. Gough; R.D. Kenway; H. P. Shanahan; Jonathan M. Flynn; N. M. Hazel; David Henty; J.N. Simone; David G. Richards
from the measured B\ifmmode\bar\else\textasciimacron\fi{}\ensuremath{\rightarrow}