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# Content
1 An artificial neural network maps a point in the space of input observables to
2 some value of neural network output $x$. The neural network training error is
3 given by equation~\ref{eq:NNerrorFunc}. A given point in the vector space
4 spanned by the neural network input observables (denoted as ``feature space'')
5 contributes to the neural network training error $E$ by
6 \begin{equation}
7 E' = (1 - x)^2\cdot\rho^\tau + x^2\cdot\rho^{QCD}
8 \end{equation}
9 where $\rho^\tau (\rho^{QCD})$ denotes the training sample density of the
10 $\tau$ signal and QCD--jet background at that point in feature space.
11
12 The value $x$ assigned by the neural network to this region in feature space
13 should satisfy the requirement of minimal error:
14 \begin{align}
15 \frac{\partial E'}{\partial x} &= 0 \nonumber \\
16 0 &= -2(1-x)\cdot\rho^\tau+2x\cdot\rho^{QCD} \nonumber \\
17 x &= \frac{\rho^\tau} {\rho^\tau + \rho^{QCD}} \label{eq:probFracToX} \\
18 \rho^\tau &= x(\rho^\tau + \rho^{QCD}) \nonumber \\
19 \frac{\rho^{QCD}}{\rho^\tau} &= \frac{1}{x} - 1 \label{eq:rawTransformX}
20 \end{align}
21
22 N.B. that the ratio $\frac{\rho^{QCD}}{\rho^\tau}$ corresponds to the ratio of
23 the normalized probability density functions of signal and background input
24 observable distributions, i.e. $\int \rho^{\tau} d\vec x = 1$.
25
26 In the case of multiple neural networks, one can derive a formula that maps the
27 output $x_j$ of the neural network corresponding to decay mode $j$ according to
28 the ``prior probabilities'' $p_j^\tau (p_j^{QCD})$ for true $\tau$ lepton
29 hadronic decays (quark and gluon jets) to pass the preselection criteria and
30 be reconstructed with decay mode $j$.
31
32 By substituting $\rho^s \rightarrow \rho^s p_j^s$ for $s \in \{\tau, QCD\}$ in
33 equation~\ref{eq:probFracToX}, the output $x_j$ can be related to $p_j^\tau
34 (p_j^{QCD})$ by
35 \begin{equation}
36 x_j' = \frac{\rho^\tau \cdot p_j^\tau}
37 {\rho^\tau \cdot p_j^\tau + \rho^{QCD} \cdot p_j^{QCD} }
38 = \frac{p_j^\tau}
39 {p_j^\tau + \frac{\rho^{QCD}}{\rho^\tau} \cdot p_j^{QCD} }
40 \label{eq:probFracToXWithPriors}
41 \end{equation}
42
43 Substituting equation~\ref{eq:rawTransformX} into
44 equation~\ref{eq:probFracToXWithPriors} yields the transformation of the output
45 $x_j$ of the neural neural network corresponding to any selected decay mode $j$
46 to a single discriminator output $x_j'$ which for a given point on the optimal
47 performance curve should be independent of $j$.
48
49 \begin{equation}
50 x_j' = \frac{p_j^\tau}
51 {p_j^\tau + \left(\frac{1}{x_j}-1\right)\cdot p_j^{QCD} }
52 \end{equation}
53
54