TY - JOUR
T1 - High power [Formula presented] of [Formula presented] in [Formula presented]-flavored widths and [Formula presented] limit
AU - Bigi, I.
AU - Shifman, Mikhail "Misha"
AU - Uraltsev, N.
AU - Vainshtein, Arkady
PY - 1997
Y1 - 1997
N2 - The leading term in the semileptonic width of heavy flavor hadrons depends on the fifth power of the heavy quark mass. We present an analysis where this power can be self-consistently treated as a free parameter [Formula presented] and the width can be studied in the limit [Formula presented] The resulting expansion elucidates why the small velocity (SV) treatment is relevant for the inclusive semileptonic [Formula presented] transition. The extended SV limit (ESV limit) is introduced. The leading terms in the perturbative [Formula presented] expansion enhanced by powers of [Formula presented] are automatically resummed by using the low-scale Euclidean mass. The large-[Formula presented] treatment explains why the scales of order [Formula presented] are appropriate. On the other hand, the scale cannot be too small since the factorially divergent perturbative corrections associated with running of [Formula presented] show up. Both requirements are met if we use the short-distance mass normalized at a scale around [Formula presented] A convenient definition of such low-scale operator-product-expansion-compatible masses is briefly discussed.
AB - The leading term in the semileptonic width of heavy flavor hadrons depends on the fifth power of the heavy quark mass. We present an analysis where this power can be self-consistently treated as a free parameter [Formula presented] and the width can be studied in the limit [Formula presented] The resulting expansion elucidates why the small velocity (SV) treatment is relevant for the inclusive semileptonic [Formula presented] transition. The extended SV limit (ESV limit) is introduced. The leading terms in the perturbative [Formula presented] expansion enhanced by powers of [Formula presented] are automatically resummed by using the low-scale Euclidean mass. The large-[Formula presented] treatment explains why the scales of order [Formula presented] are appropriate. On the other hand, the scale cannot be too small since the factorially divergent perturbative corrections associated with running of [Formula presented] show up. Both requirements are met if we use the short-distance mass normalized at a scale around [Formula presented] A convenient definition of such low-scale operator-product-expansion-compatible masses is briefly discussed.
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U2 - 10.1103/PhysRevD.56.4017
DO - 10.1103/PhysRevD.56.4017
M3 - Article
AN - SCOPUS:0000138917
SN - 1550-7998
VL - 56
SP - 4017
EP - 4030
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 7
ER -