Difference: ResultsWinter2016UUT (r2 vs. r1)

r2 - 09 Jan 2016 - 09:47 - DenisDerkach r1 - 21 Jul 2015 - 13:47 - DenisDerkach
  

Tree Level Fit results: Winter 2016

Tree Level Fit results: Summer 2015

It is possible to generalize the full UTfit beyond the Standard Model to all those NP models characterized by Minimal Flavour Violation, i.e. having quark mixing ruled only by the Standard Model CKM couplings ( http://arxiv.org/abs/hep-ph/0007085). In fact, in this case no additional weak phases are generated and several observables entering into the Standard Model fit (the tree-level processes and the measurement of angles through the use of time dependent CP asymmetries) are not affected by the presence of New Physics. The only sizable effect we are sensitive to is a shift of the Inami-Lim function of the top contribution in meson mixing. This means that in general ?K and ?md cannot be used in a common SM and MFV framework. Also the ratio ?md/?ms cannot be used in general, as ?ms can get additional NP contributions at large tan?. So, simply removing the information related to ?K, ?md and ?ms from the full UTfit, one can obtain a more precise determination of the Universal Unitarity Triangle, which is a common starting point for the Standard Model and any MFV model.

It is possible to generalize the full UTfit beyond the Standard Model to all those NP models characterized by Minimal Flavour Violation, i.e. having quark mixing ruled only by the Standard Model CKM couplings ( http://arxiv.org/abs/hep-ph/0007085). In fact, in this case no additional weak phases are generated and several observables entering into the Standard Model fit (the tree-level processes and the measurement of angles through the use of time dependent CP asymmetries) are not affected by the presence of New Physics. The only sizable effect we are sensitive to is a shift of the Inami-Lim function of the top contribution in meson mixing. This means that in general ?K and ?md cannot be used in a common SM and MFV framework. Also the ratio ?md/?ms cannot be used in general, as ?ms can get additional NP contributions at large tan?. So, simply removing the information related to ?K, ?md and ?ms from the full UTfit, one can obtain a more precise determination of the Universal Unitarity Triangle, which is a common starting point for the Standard Model and any MFV model.

  
ParameterInput valuePrediction
\bar{\rho} -0.141 \pm 0.023
\bar{\eta} -0.339 \pm 0.015
\rho -0.145 \pm 0.023
\eta -0.346 \pm 0.014
A -0.810 \pm 0.021
\lambda 0.22518 \pm 0.000870.22507 \pm 0.00064
\alpha, [^{\circ}] 92.5 \pm 5.5 \text{ and } 166.1 \pm 0.688.1 \pm 3.4
\beta, [^{\circ}] -24.2 \pm 1.6
\sin(2\beta) 0.679 \pm 0.0230.746 \pm 0.039
\gamma, [^{\circ}] -108.5 \pm 6.5 \text{ and } 71.4 \pm 6.566.9 \pm 3.0
CKM matrix thus looks like V_{CKM}=\left(\begin{array}{ccc} (0.97431 \pm 0.00013) & (0.22508 \pm 0.00066) & (0.00364 \pm 0.00012)e^{i(-67.5 \pm 3.5)^\circ}\\ ( -0.22491 \pm 0.00066)e^{i(0.0328 \pm 0.0021)^\circ} & (0.97347 \pm 0.00014)e^{i(-0.00175 \pm 0.00011)^\circ} & (0.04237 \pm 0.00062) \\ (0.00853 \pm 0.00031)e^{i(-21.50 \pm 0.83)^\circ} & ( -0.0403 \pm 0.0010)e^{i(1.026 \pm 0.043)^\circ} & (0.999143 \pm 0.000045)\end{array}\right)



Full fit result for \,\bar{\rho}
0.141 \pm 0.023
95% prob:[0.095, 0.190]
99% prob:[0.075, 0.219]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\bar{\eta}
0.339 \pm 0.015
95% prob:[0.309, 0.369]
99% prob:[0.293, 0.381]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\bar{\rho} - \bar{\eta}



EPS - PDF - PNG - JPG - GIF



Full fit result for \,\rho
0.145 \pm 0.023
95% prob:[0.097, 0.195]
99% prob:[0.077, 0.224]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\eta
0.346 \pm 0.014
95% prob:[0.318, 0.377]
99% prob:[0.305, 0.394]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,A
0.810 \pm 0.021
95% prob:[0.767, 0.854]
99% prob:[0.746, 0.876]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\lambda
0.22518 \pm 0.00087
95% prob:[0.22356, 0.22712]
99% prob:[0.22257, 0.22801]
EPS - PDF - PNG - JPG - GIF



Prediction for \,\lambda
0.22507 \pm 0.00064
95% prob:[0.22386, 0.22633]
99% prob:[0.22326, 0.22703]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\alpha, [^{\circ}]
92.5 \pm 5.5 \text{ and } 166.1 \pm 0.6
95% prob:[83.60, 102.60] U [162.30, 169.70]
99% prob:[80.00, 108.80] U [159.19, 171.60]
EPS - PDF - PNG - JPG - GIF



Prediction for \,\alpha, [^{\circ}]
88.1 \pm 3.4
95% prob:[81.5, 95.2]
99% prob:[78.2, 98.7]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\beta, [^{\circ}]
24.2 \pm 1.6
95% prob:[20.9, 27.6]
99% prob:[19.4, 29.3]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\sin(2\beta)
0.679 \pm 0.023
95% prob:[0.635, 0.729]
99% prob:[0.613, 0.755]
EPS - PDF - PNG - JPG - GIF



Prediction for \,\sin(2\beta)
0.746 \pm 0.039
95% prob:[0.669, 0.822]
99% prob:[0.630, 0.858]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\gamma, [^{\circ}]
-108.5 \pm 6.5 \text{ and } 71.4 \pm 6.5
95% prob:[-122.0, -95.9] U [57.7, 84.0]
99% prob:[-129.3, -89.4] U [50.7, 90.7]
EPS - PDF - PNG - JPG - GIF



Prediction for \,\gamma, [^{\circ}]
66.9 \pm 3.0
95% prob:[61.0, 73.0]
99% prob:[58.0, 75.9]
EPS - PDF - PNG - JPG - GIF
ParameterInput valueFull fit
\bar{\rho} -0.143 \pm 0.024
\bar{\eta} -0.341 \pm 0.015
\rho -0.147 \pm 0.024
\eta -0.35 \pm 0.015
A -0.815 \pm 0.029
\lambda 0.22519 \pm 0.000990.22497 \pm 0.00065
\alpha, [^{\circ}] 92.7 \pm 6.290.7 \pm 3.6
\beta, [^{\circ}] -21.67 \pm 0.87
\sin(2\beta) 0.68 \pm 0.0240.686 \pm 0.022
\gamma, [^{\circ}] 71.4 \pm 6.5 \text{ and } 71.4 \pm 6.567.2 \pm 3.6
The fit results for all the nine CKM elements are V_{CKM}=\left(\begin{array}{ccc} (0.9743 \pm 0.00015) & (0.22507 \pm 0.00066) & (0.00354 \pm 0.00017)e^{i(-67.3 \pm 3.6)^\circ}\\ ( -0.22496 \pm 0.00061)e^{i(0.0335 \pm 0.0026)^\circ} & (0.97347 \pm 0.00016)e^{i(-0.00178 \pm 0.00013)^\circ} & (0.0414 \pm 0.0014) \\ (0.00857 \pm 0.00037)e^{i(-21.66 \pm 0.87)^\circ} & ( -0.0406 \pm 0.0014)e^{i(1.033 \pm 0.044)^\circ} & (0.999129 \pm 0.00006)\end{array}\right)



Full fit result for \,\bar{\rho}
0.143 \pm 0.024
95% prob:[0.096, 0.193]
99% prob:[0.076, 0.222]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\bar{\eta}
0.341 \pm 0.015
95% prob:[0.312, 0.371]
99% prob:[0.292, 0.392]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\rho
0.147 \pm 0.024
95% prob:[0.098, 0.198]
99% prob:[0.078, 0.227]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\eta
0.35 \pm 0.015
95% prob:[0.320, 0.380]
99% prob:[0.306, 0.397]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,A
0.815 \pm 0.029
95% prob:[0.76, 0.873]
99% prob:[0.731, 0.902]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\lambda
0.22519 \pm 0.00099
95% prob:[0.2235, 0.2271]
99% prob:[0.2226, 0.228]
EPS - PDF - PNG - JPG - GIF



Full Fit result for \,\lambda
0.22497 \pm 0.00065
95% prob:[0.2239, 0.2264]
99% prob:[0.2232, 0.227]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\alpha, [^{\circ}]
92.7 \pm 6.2 \text{ and } 167.3 \pm 0.1
95% prob:[83.5, 102.9] U [161.2, 169.8]
99% prob:[78.8, 108.2] U [157.9, 171.5] U [179.5, 180]
EPS - PDF - PNG - JPG - GIF



Full Fit result for \,\alpha, [^{\circ}]
90.7 \pm 3.6
95% prob:[83.7, 98.7]
99% prob:[80.7, 103]
EPS - PDF - PNG - JPG - GIF



Full fit result for \,\beta, [^{\circ}]
21.67 \pm 0.87
95% prob:[20.0, 23.5]
99% prob:[19.2, 24.5]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\sin(2\beta)
0.68 \pm 0.024
95% prob:[0.635, 0.729]
99% prob:[0.613, 0.755]
EPS - PDF - PNG - JPG - GIF



Full Fit result for \,\sin(2\beta)
0.686 \pm 0.022
95% prob:[0.644, 0.732]
99% prob:[0.624, 0.756]
EPS - PDF - PNG - JPG - GIF



Fit Input for \,\gamma, [^{\circ}]
-108.5 \pm 6.5 \text{ and } 71.4 \pm 6.5
95% prob:[-122, -95.] U [57.8, 84.1]
99% prob:[-129, -89.] U [50.7, 90.7]
EPS - PDF - PNG - JPG - GIF



Full Fit result for \,\gamma, [^{\circ}]
67.2 \pm 3.6
95% prob:[59.5, 74.5]
99% prob:[55.2, 77.8]
EPS - PDF - PNG - JPG - GIF
r2 - 09 Jan 2016 - 09:47 - DenisDerkach r1 - 21 Jul 2015 - 13:47 - DenisDerkach

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