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B→K Transition Form Factor with Tensor Current within the kT Factorization Approach

B→K Transition Form Factor with Tensor Current within the kT Factorization Approach
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摘要 We apply the kT factorization approach to deal with the B→K transition form factor with tensor current in the large recoil regions. Main uncertainties for the estimation are discussed and we obtain FT^B→K (0) = 0.25±0.01±0.02, where the first error is caused by the uncertainties from the pionic wavefunctions and the second is from that of the B-meson wavefunctions. This result is consistent with the light-cone sum rule results obtained in the literature. We apply the kT factorization approach to deal with the B→K transition form factor with tensor current in the large recoil regions. Main uncertainties for the estimation are discussed and we obtain FT^B→K (0) = 0.25±0.01±0.02, where the first error is caused by the uncertainties from the pionic wavefunctions and the second is from that of the B-meson wavefunctions. This result is consistent with the light-cone sum rule results obtained in the literature.
机构地区 Department of Physics
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第2期436-439,共4页 中国物理快报(英文版)
基金 Supported in part by the National Natural Science Foundation of China under Grant No 10575140, Chongqing University, and the National Basic Research Programme of China under Grant No 2003CB716300.
关键词 PULSARS x-ray spectra relativity and gravitation REDSHIFT pulsars, x-ray spectra, relativity and gravitation, redshift
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