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A Mathematica based Version of the CKMfitter Package

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30 Chapter 5. Probing <strong>the</strong> Standard Model<br />

5.1.2 |Vus|<br />

The matrix element |Vus| has been extracted from semileptonic Kaon decays (Kl3),<br />

e. g. K + → π 0 e + νe. Its current world average (WA) is [9]:<br />

|Vus|Kl3 = 0.2257 ± 0.0021gauss . (5.2)<br />

|Vus| as well as |Vud| are <strong>the</strong> main inputs to constrain <strong>the</strong> Wolfenstein parameter λ.<br />

However, |Vus| depends on large <strong>the</strong>oretical uncertainties from <strong>the</strong> determination <strong>of</strong><br />

<strong>the</strong> form factor f+(0). O<strong>the</strong>r possibilities to determine |Vus| involve for instance<br />

leptonic Kaon and Pion decays, semileptonic Hyperon decays or hadronic τ decays.<br />

5.1.3 |Vcb|<br />

The magnitude <strong>of</strong> |Vcb| is determined from exclusive and inclusive measurements 1<br />

<strong>of</strong> semileptonic B-meson decays to charmed final states (b → clν). Because <strong>of</strong> <strong>the</strong>oretical<br />

uncertainties on <strong>the</strong> form factor calculation, <strong>the</strong> exclusive determination is<br />

less precise compared to <strong>the</strong> inclusive one and thus not used in this work. Due to<br />

<strong>the</strong> large statistics, <strong>the</strong> inclusive WA [9]:<br />

|Vcb|incl = (41.7 ± 0.7gauss) · 10 −3<br />

(5.3)<br />

is already below <strong>the</strong> 2% level. It is <strong>the</strong> main input to constrain <strong>the</strong> Wolfenstein<br />

parameter A.<br />

5.1.4 |Vub|<br />

Analogous to |Vcb|, <strong>the</strong> CKM matrix element |Vub| is determined from exclusive and<br />

inclusive measurements <strong>of</strong> b → ulν transitions. The inclusive determination suffers<br />

from large B → Xclν background and uses <strong>the</strong>refore phase space regions where <strong>the</strong><br />

charm background is kinematically suppressed. Hadronic effects enter in leading<br />

order (LO) via one non-perturbative shape function, which has been extracted from<br />

<strong>the</strong> photon energy spectrum in B → Xsγ. For <strong>the</strong> inclusive WA, <strong>the</strong> BLNP [28]<br />

calculation is chosen [29] 2 :<br />

|Vub| incl. = (4.48 ± 0.24gauss ± 0.39<strong>the</strong>o) · 10 −3 , (5.4)<br />

The <strong>the</strong>oretical error is obtained by adding linearly <strong>the</strong> contributions from weak<br />

annihilation, subleading shape functions and <strong>the</strong> Heavy-Quark Expansion (HQE)<br />

uncertainty on <strong>the</strong> b-quark mass.<br />

Direct measurements <strong>of</strong> exclusive channels depend significantly on form factor calculations.<br />

The form factors can be calculated using unquenched Lattice QCD (LQCD)<br />

or QCD Sum Rules, which still leads to larger <strong>the</strong>oretical uncertainties compared to<br />

<strong>the</strong> inclusive determination.<br />

1 Exclusive means <strong>the</strong> full reconstruction <strong>of</strong> a single mode, e. g. B + → ¯ D 0 e + νe, where inclusive<br />

measurements integrate over all possible final states, B → Xclν.<br />

2 The central value has been shifted after <strong>the</strong> ICHEP06 conference to 4.49 · 10 −3 .

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