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1.1 |
An artificial neural network maps a point in the space of input observables to
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some value of neural network output $x$. The neural network training error is
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given by equation~\ref{eq:NNerrorFunc}. A given point in the vector space
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1.2 |
spanned by the neural network input observables (denoted as ``feature space'')
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contributes to the neural network training error $E$ by
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friis |
1.1 |
\begin{equation}
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E' = (1 - x)^2\cdot\rho^\tau + x^2\cdot\rho^{QCD}
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\end{equation}
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1.2 |
where $\rho^\tau (\rho^{QCD})$ denotes the training sample density of the
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$\tau$ signal and QCD--jet background at that point in feature space.
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friis |
1.1 |
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friis |
1.2 |
The value $x$ assigned by the neural network to this region in feature space
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should satisfy the requirement of minimal error:
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1.1 |
\begin{align}
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\frac{\partial E'}{\partial x} &= 0 \nonumber \\
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0 &= -2(1-x)\cdot\rho^\tau+2x\cdot\rho^{QCD} \nonumber \\
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x &= \frac{\rho^\tau} {\rho^\tau + \rho^{QCD}} \label{eq:probFracToX} \\
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\rho^\tau &= x(\rho^\tau + \rho^{QCD}) \nonumber \\
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\frac{\rho^{QCD}}{\rho^\tau} &= \frac{1}{x} - 1 \label{eq:rawTransformX}
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\end{align}
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N.B. that the ratio $\frac{\rho^{QCD}}{\rho^\tau}$ corresponds to the ratio of
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the normalized probability density functions of signal and background input
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observable distributions, i.e. $\int \rho^{\tau} d\vec x = 1$.
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In the case of multiple neural networks, one can derive a formula that maps the
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output $x_j$ of the neural network corresponding to decay mode $j$ according to
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friis |
1.2 |
the ``prior probabilities'' $p_j^\tau (p_j^{QCD})$ for true $\tau$ lepton
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hadronic decays (quark and gluon jets) to pass the preselection criteria and
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be reconstructed with decay mode $j$.
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friis |
1.1 |
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By substituting $\rho^s \rightarrow \rho^s p_j^s$ for $s \in \{\tau, QCD\}$ in
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1.2 |
equation~\ref{eq:probFracToX}, the output $x_j$ can be related to $p_j^\tau
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(p_j^{QCD})$ by
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friis |
1.1 |
\begin{equation}
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x_j' = \frac{\rho^\tau \cdot p_j^\tau}
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{\rho^\tau \cdot p_j^\tau + \rho^{QCD} \cdot p_j^{QCD} }
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= \frac{p_j^\tau}
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{p_j^\tau + \frac{\rho^{QCD}}{\rho^\tau} \cdot p_j^{QCD} }
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\label{eq:probFracToXWithPriors}
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\end{equation}
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friis |
1.2 |
Substituting equation~\ref{eq:rawTransformX} into
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equation~\ref{eq:probFracToXWithPriors} yields the transformation of the output
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$x_j$ of the neural neural network corresponding to any selected decay mode $j$
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to a single discriminator output $x_j'$ which for a given point on the optimal
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performance curve should be independent of $j$.
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friis |
1.1 |
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\begin{equation}
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x_j' = \frac{p_j^\tau}
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{p_j^\tau + \left(\frac{1}{x_j}-1\right)\cdot p_j^{QCD} }
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\end{equation}
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