✦ LIBER ✦

Lattice-constrained parametrizations of form factors for semileptonic and rare radiative B decays

✍ Scribed by L. Del Debbio; J.M. Flynn; L. Lellouch; J. Nieves

Book ID: 114290650
Publisher: Elsevier Science
Year: 1998
Tongue: English
Weight: 206 KB
Volume: 63
Category: Article
ISSN: 0920-5632
DOI: 10.1016/s0920-5632(97)00777-9

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Lattice-constrained parametrizations of

Lattice-constrained parametrizations of form factors for semileptonic and rare radiative B decays

✍ Luigi Del Debbio; Jonathan M Flynn; Laurent Lellouch; Juan Nieves 📂 Article 📅 1998 🏛 Elsevier Science 🌐 English ⚖ 196 KB

Heavy quark mass dependence of semilepto

Heavy quark mass dependence of semileptonic form factors for B decays

✍ S. Aoki; M. Fukugita; S. Hashimoto; K.-I. Ishikawa; N. Ishizuka; Y. Iwasaki; K. 📂 Article 📅 1998 🏛 Elsevier Science 🌐 English ⚖ 230 KB

Anomalous dimension matrix for radiative

Anomalous dimension matrix for radiative and rare semileptonic B decays up to three loops

✍ Paolo Gambino; Martin Gorbahn; Ulrich Haisch 📂 Article 📅 2003 🏛 Elsevier Science 🌐 English ⚖ 318 KB

Semileptonic decays of b-meson and effec

Semileptonic decays of b-meson and effects of form factor

✍ Yoshiki Kizukuri 📂 Article 📅 1982 🏛 Elsevier Science 🌐 English ⚖ 154 KB

Form factors for B → πlνl and B → K∗γ de

Form factors for B → πlνl and B → K∗γ decays on the lattice

✍ D.R. Burford; H.D. Duong; J.M. Flynn; B.J. Gough; N.M. Hazel; J. Nieves; H.P. Sh 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 627 KB

Next-to-leading order calculations of th

Next-to-leading order calculations of the radiative and semileptonic rare B decays in the standard model and comparison with data

✍ A. Ali 📂 Article 📅 2003 🏛 Elsevier Science 🌐 English ⚖ 584 KB

We review some selected rare B decays calculated in next-to-leading order accuracy in the Standard Model (SM). These include the radiative decays B → (Xs, K \* , ρ)γ and the semileptonic decays B → (Xs, K, K \* ) + -, for which new data from the BABAR and BELLE collaborations have been presented at