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A Mathematica based Version of the CKMfitter Package

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2 Chapter 1. Introduction<br />

Unfortunately, <strong>the</strong> Standard Model cannot answer all questions, e. g. evidences for<br />

dark matter from <strong>the</strong> measurement <strong>of</strong> <strong>the</strong> cosmic microwave backround radiation imply<br />

<strong>the</strong> existence <strong>of</strong> non-SM particles. Fur<strong>the</strong>rmore, <strong>the</strong> observed matter-antimatter<br />

asymmetry <strong>of</strong> <strong>the</strong> Universe requires additional CP-violating effects. There are many<br />

New Physics (NP) models, like Supersymmetric Models (SUSY) and Grand Unified<br />

Theories (GUTs), that can solve, in principle <strong>the</strong>se and o<strong>the</strong>r problems. Probing<br />

<strong>the</strong> consistency <strong>of</strong> <strong>the</strong>se models with experimental data is also a part <strong>of</strong> <strong>the</strong> global<br />

CKM matrix analysis.<br />

The <strong>CKMfitter</strong> package [4] provides a global analysis tool, which allows to constrain<br />

<strong>the</strong> CKM matrix parameters within <strong>the</strong> Standard Model and its possible extensions.<br />

In <strong>the</strong> framework <strong>of</strong> <strong>the</strong> frequentist approach Rfit, <strong>the</strong> consistency <strong>of</strong> recent experimental<br />

results and its <strong>the</strong>oretical predictions are probed. The s<strong>of</strong>tware package has<br />

been mainly written in FORTRAN using <strong>the</strong> MINUIT minimization package. Over<br />

<strong>the</strong> years, <strong>the</strong> complexity <strong>of</strong> <strong>the</strong> fit problems has increased substantially. Depending<br />

on <strong>the</strong> fit problem, a fit can last up to <strong>the</strong> order <strong>of</strong> days.<br />

In this <strong>the</strong>sis, a <strong>Ma<strong>the</strong>matica</strong> <strong>based</strong> version <strong>of</strong> <strong>the</strong> <strong>CKMfitter</strong> package is introduced.<br />

It has been initiated and commenced by Jérôme Charles. Beside <strong>of</strong> <strong>Ma<strong>the</strong>matica</strong>,<br />

which provides a framework for symbolic calculations, a slim and effective<br />

minimization routine is implemented. During this work, <strong>the</strong> final structure <strong>of</strong> <strong>the</strong><br />

source code with a userfriendly environment accrued and fundamental <strong>the</strong>ory packages<br />

were coded. They include <strong>the</strong> <strong>the</strong>oretical predictions <strong>of</strong> additional NP models<br />

beyond <strong>the</strong> SM. Important developments are also <strong>the</strong> routine for <strong>the</strong> treatment <strong>of</strong><br />

numerical input tables and <strong>the</strong> possibility <strong>of</strong> having different <strong>the</strong>oretical frameworks<br />

in one <strong>the</strong>ory package. A talk on <strong>the</strong> <strong>Ma<strong>the</strong>matica</strong> <strong>based</strong> <strong>CKMfitter</strong> version has<br />

been presented at <strong>the</strong> DPG Frühjahrstagung 2006 in Dortmund [5].<br />

After one year <strong>of</strong> development, a lot <strong>of</strong> important fits, for instance <strong>the</strong> Standard<br />

Global CKM Fit, can be performed using <strong>the</strong> <strong>Ma<strong>the</strong>matica</strong> <strong>based</strong> version <strong>of</strong> <strong>CKMfitter</strong>.<br />

For example, all SM and some NP fit results presented by Stephane T’Jampens<br />

at <strong>the</strong> International Conference on High Energy Physics 2006 (ICHEP06) in Moscow,<br />

have been produced with <strong>the</strong> new <strong>Ma<strong>the</strong>matica</strong> <strong>based</strong> <strong>CKMfitter</strong> version.<br />

The <strong>the</strong>sis is organized as follows. Chapter 2 gives a brief introduction to <strong>the</strong><br />

Standard Model and <strong>the</strong> CKM matrix. Fur<strong>the</strong>rmore, a review <strong>of</strong> <strong>the</strong> relevant <strong>the</strong>ory<br />

<strong>of</strong> neutral meson oscillation and CP violation is presented. After an overview about<br />

<strong>the</strong> original <strong>CKMfitter</strong> package and its statistical approach Rfit in Chapter 3, <strong>the</strong><br />

development <strong>of</strong> <strong>CKMfitter</strong> in a <strong>Ma<strong>the</strong>matica</strong> environment is described in Chapter 4.<br />

Up-to-date plots and results <strong>of</strong> <strong>the</strong> global CKM matrix analysis are presented in<br />

Chapter 5 for <strong>the</strong> Standard Model and in Chapter 6 in <strong>the</strong> framework <strong>of</strong> two New<br />

Physics models. A user guide and a development tutorial for <strong>the</strong> <strong>Ma<strong>the</strong>matica</strong> <strong>based</strong><br />

version <strong>of</strong> <strong>CKMfitter</strong> can be found in <strong>the</strong> appendices.

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