Published February 1, 2009 | Version v1
Journal article

Radiative corrections on the B→P form factors with chiral current in the light-cone sum rules

  • 1. Department of Physics, Chongqing University, Chongqing 400030 (China)
  • 2. Institute of High Energy Physics and Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences, P.O. Box 918(4), Beijing 100049 (China)

Description

Based on the approach of the vector form factor FB→π,K+(q2) in our previous papers, we extend the calculation of the radiative corrections to the B→P (P stands π, K, and all light pseudoscalar mesons) scalar and tensor form factors FB→P0,T(q2) with chiral current in the light-cone sum rules (LCSRs). The most uncertain twist-3 contributions to the B→P form factors can be naturally eliminated through a properly designed correlator. We present the next-leading-order formulas of FB→P+,0,T(q2) with the b-quark pole mass that is universal. It has been shown that our results are simpler and less uncertain under the same parameter regions since we only need to calculate the next-leading order on the twist-2 part from the obtained LCSR. Second, we obtain fB→π+,0(0)=0.260-0.040+0.059, fB→πT(0)=0.276-0.039+0.052, fB→K+,0(0)=0.334-0.069+0.094, and fB→KT(0)=0.379-0.077+0.092 at q2=0 and the SUf(3)-breaking effects are discussed too.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
79
Journal Issue
3
Journal Page Range
p. 034013-034013.15
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41010734
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
B QUARKS; CHIRALITY; FORM FACTORS; LIGHT CONE; MASS; PSEUDOSCALAR MESONS; RADIATIVE CORRECTIONS; SUM RULES
Descriptors DEC
BEAUTY PARTICLES; BOSONS; CORRECTIONS; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; HADRONS; MESONS; PARTICLE PROPERTIES; QUARKS; SPACE-TIME

Optional Information

Notes
(c) 2009 The American Physical Society