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On the Flavor Problem in Strongly Coupled Theories - THEP Mainz

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4.4. Cross Section and Asymmetry <strong>in</strong> <strong>the</strong> M<strong>in</strong>imal RS Model 161<br />

mix<strong>in</strong>g with QCD pengu<strong>in</strong> operators gives for P = V, A,<br />

�<br />

�<br />

˜C P q¯q(mt) =<br />

2 η2/7<br />

+<br />

3η4/7 3<br />

˜C P q¯q(MKK) , (4.56)<br />

where η ≡ αs(MKK)/αs(mt) is <strong>the</strong> ratio of strong coupl<strong>in</strong>g constants evaluated at<br />

<strong>the</strong> relevant scales MKK and mt. The impact of RG effects is however limited, as<br />

can be seen from evaluat<strong>in</strong>g (4.56) us<strong>in</strong>g αs(MZ) = 0.139, MKK = 1 TeV, and mt =<br />

173.1 GeV, so that η = 0.803 at one-loop order. We obta<strong>in</strong><br />

˜C P q¯q(mt) = 1.07 ˜ C P q¯q(MKK) , (4.57)<br />

which makes for an effect of <strong>the</strong> order of a few percent. We anticipate, that <strong>the</strong><br />

t channel contributions are suppressed, because <strong>the</strong>y always feel <strong>the</strong> localization of<br />

<strong>the</strong> up quarks, which yields an exponential suppression due to <strong>the</strong> zero mode profiles<br />

and will <strong>the</strong>refore neglect renormalization group effects for <strong>the</strong> correspond<strong>in</strong>g Wilson<br />

coefficients.<br />

Restrict<strong>in</strong>g ourselves to <strong>the</strong> corrections proportional to αs and suppress<strong>in</strong>g relative<br />

O(1) factors as well as numerically sublead<strong>in</strong>g terms, one f<strong>in</strong>ds from <strong>the</strong> ZMA expansion<br />

of <strong>the</strong> Wilson coefficients of <strong>the</strong> results given <strong>in</strong> (4.55) that <strong>the</strong> coefficient<br />

functions S (0)<br />

quark like<br />

S (0)<br />

uū,RS<br />

A (0)<br />

uū,RS<br />

ij,RS<br />

∼ αsπ<br />

M 2 KK<br />

and A(0)<br />

ij,RS <strong>in</strong>troduced <strong>in</strong> (4.50) and (4.52) scale <strong>in</strong> <strong>the</strong> case of <strong>the</strong> up<br />

�<br />

A=L,R<br />

αsπ<br />

∼ −<br />

M 2 L<br />

KK<br />

F 2 (ctA ) , (4.58)<br />

� �<br />

q=t,u<br />

�<br />

F 2 (cqR ) − F 2 (cqL )<br />

�<br />

+ 1<br />

3<br />

where ctL ≡ cQ3 , ctR ≡ cu3 , cuL ≡ cQ1 , and cuR ≡ cu1 .<br />

�<br />

A=L,R<br />

F 2 (ctA )F 2 (cuA )<br />

�<br />

, (4.59)<br />

As a consequence of <strong>the</strong> composite character of <strong>the</strong> top, its bulk mass parameters are<br />

typically ctA > −1/2, while <strong>the</strong> up quark, be<strong>in</strong>g mostly elementary is located close to<br />

<strong>the</strong> UV brane. The relevant F 2 (cqA ) factors can <strong>the</strong>refore be approximated by<br />

F 2 (ctA ) ≈ 1 + 2ctA , F 2 (cuA ) ≈ (−1 − 2cuA ) eL(2cu A +1) , (4.60)<br />

with A = L, R, as elaborated <strong>in</strong> Section 2.4. The difference of bulk mass parameters<br />

for light quarks (cuL − cuR ) is typically small and positive, whereas (ctL − ctR ) can<br />

be of O(1) and is usually negative, because <strong>the</strong> localization parameter of <strong>the</strong> SU(2)L<br />

doublet also enters <strong>the</strong> mass formula for <strong>the</strong> bottom quark (2.158), which typically<br />

results <strong>in</strong> ctR > ctL . Us<strong>in</strong>g <strong>the</strong> above approximations and expand<strong>in</strong>g <strong>in</strong> powers of

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