On the Flavor Problem in Strongly Coupled Theories - THEP Mainz
On the Flavor Problem in Strongly Coupled Theories - THEP Mainz
On the Flavor Problem in Strongly Coupled Theories - THEP Mainz
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98 Chapter 3. Solv<strong>in</strong>g <strong>the</strong> <strong>Flavor</strong> <strong>Problem</strong> <strong>in</strong> <strong>Strongly</strong> <strong>Coupled</strong> <strong>Theories</strong><br />
gR b<br />
0.12<br />
0.11<br />
0.10<br />
0.09<br />
0.08<br />
0.07<br />
99� CL<br />
95� CL<br />
68� CL<br />
�<br />
0.06<br />
�0.430 �0.425 �0.420 �0.415 �0.410<br />
�<br />
gL b<br />
gR b<br />
0.11<br />
0.10<br />
0.09<br />
0.08<br />
99� CL<br />
95� CL<br />
68� CL<br />
0.07<br />
�0.426 �0.424 �0.422 �0.420 �0.418 �0.416<br />
Figure 3.3: The plots show regions of 68%, 95% and 99% probability <strong>in</strong> <strong>the</strong> g b L − gb R<br />
plane. The best fit value is denoted with a cross and <strong>the</strong> experimental value with a<br />
star. The red colored regions <strong>in</strong>dicate <strong>the</strong> predicted values of a large set of parameter<br />
po<strong>in</strong>ts for <strong>the</strong> m<strong>in</strong>imal RS model <strong>in</strong> <strong>the</strong> left panel and for <strong>the</strong> RS model with custodial<br />
protection <strong>in</strong> <strong>the</strong> right panel.<br />
Insert<strong>in</strong>g <strong>the</strong> predicted SM values gb L = −0.42114 and gb R = 0.077420 [146, Table G3]<br />
for <strong>the</strong> left- and right-handed bottom-quark coupl<strong>in</strong>gs <strong>in</strong>to <strong>the</strong> relations (3.12), we<br />
obta<strong>in</strong> for <strong>the</strong> central values of <strong>the</strong> quantities <strong>in</strong> question<br />
R 0 b = 0.21474 , Ab = 0.935 , A 0,b<br />
FB = 0.1032 . (3.13)<br />
In comparison, <strong>the</strong> experimentally extracted values for <strong>the</strong> three “pseudo observables”<br />
read [146]<br />
R0 b = 0.21629 ± 0.00066 ,<br />
Ab = 0.923 ± 0.020 ,<br />
A 0,b<br />
FB = 0.0992 ± 0.0016 ,<br />
�<br />
gL b<br />
⎛<br />
1.00 −0.08<br />
⎞<br />
−0.10<br />
ρ = ⎝ −0.08 1.00 0.06 ⎠ , (3.14)<br />
−0.10 0.06 1.00<br />
where ρ is <strong>the</strong> correlation matrix. This reproduces <strong>the</strong> deviations listed <strong>in</strong> Table 3.1.<br />
In contrast to <strong>the</strong> orig<strong>in</strong>al analysis <strong>in</strong> [115, Sec. 6.4], <strong>the</strong> <strong>the</strong>oretical corrections to R 0 b<br />
pull <strong>the</strong> best fit value 3σ away from <strong>the</strong> experimental SM value, as can be seen <strong>in</strong> Figure<br />
3.3, <strong>in</strong> which <strong>the</strong> best fit is denoted by a cross and <strong>the</strong> experimental value by a star.<br />
A new physics contribution that would improve this situation needs a large positive<br />
correction to gb R of <strong>the</strong> order of 20% and no contribution to gb L ( while a small negative<br />
shift would also improve <strong>the</strong> fit). As becomes clear from (3.10) and (3.11), RS<br />
corrections reduce <strong>the</strong> SM value of both gb R and gb L <strong>in</strong> magnitude, which corresponds<br />
to a negative shift of gb R and a positive one for gb L , po<strong>in</strong>t<strong>in</strong>g <strong>in</strong> exactly <strong>the</strong> oppo-<br />
are smaller by a factor of roughly<br />
site direction. In addition, <strong>the</strong> corrections to g b R<br />
�