ersten 3 Kapitel fertig.
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@ -180,14 +180,18 @@ continuous (given $d \ge 1$) as every $p_i$ gets blended in between $\tau_i$ and
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$\tau_{i+d}$ and out between $\tau_{i+1}$, and $\tau_{i+d+1}$ as can bee seen from the two coefficients
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in every step of the recursion.
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\improvement[inline]{Weitere Eigenschaften erwähnen:
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\newline Convex hull
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\newline $\sum_i N_i = 1$?
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\newline Bilder von Basisfunktionen zur Visualisierung.
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This means that all changes are only a local linear combination between the
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control--point $p_i$ to $p_{i+d+1}$ and consequently this yields to the
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convex--hull--property of B-Splines --- meaning, that no matter how we choose
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our coefficients, the resulting points all have to lie inside convex--hull of
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the control--points.
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\improvement[inline]{
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Bilder von Basisfunktionen zur Visualisierung.
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}
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For a given number of points $v_1,\dots,v_n$ we can then calculate
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the contributions $n_{i,j}~:=~N_{j,d,\tau}$ of each control point $p_j$ to get the
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the contributions \linebreak[4]$n_{i,j}~:=~N_{j,d,\tau}$ of each control point $p_j$ to get the
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projection from the control--point--space into the object--space:
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$$
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v_i = \sum_j n_{i,j} \cdot p_j = \vec{n}_i^{T} \vec{p}
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@ -264,16 +268,21 @@ however, is very generic and we introduce it here in a broader sense.
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The general shape of an evolutionary algorithm (adapted from
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\cite{back1993overview}) is outlined in Algorithm \ref{alg:evo}. Here, $P(t)$
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denotes the population of parameters in step $t$ of the algorithm. The
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population contains $\mu$ individuals $a_i$ that fit the shape of the parameters
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we are looking for. Typically these are initialized by a random guess or just
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zero. Further on we need a so--called *fitness--function* $\Phi : I \mapsto M$\improvement{Was ist $I,M$?\newline Bezug Genotyp/Phenotyp} that can take
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each parameter to a measurable space along a convergence--function $c : I \mapsto
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\mathbb{B}$ that terminates the optimization.
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population contains $\mu$ individuals $a_i$ from the possible individual--set
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$I$ that fit the shape of the parameters we are looking for. Typically these are
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initialized by a random guess or just zero. Further on we need a so--called
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*fitness--function* $\Phi : I \mapsto M$ that can take each parameter to a measurable
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space $M$ (usually $M = \mathbb{R}$) along a convergence--function $c : I \mapsto \mathbb{B}$
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that terminates the optimization.
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Biologically speaking the set $I$ corresponds to the set of possible *Genotypes*
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while $M$ represents the possible observable *Phenotypes*.
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The main algorithm just repeats the following steps:
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- **Recombine** with a recombination--function $r : I^{\mu} \mapsto I^{\lambda}$ to
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generate new individuals based on the parents characteristics.
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generate $\lambda$ new individuals based on the characteristics of the $\mu$
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parents.
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This makes sure that the next guess is close to the old guess.
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- **Mutate** with a mutation--function $m : I^{\lambda} \mapsto I^{\lambda}$ to
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introduce new effects that cannot be produced by mere recombination of the
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@ -332,9 +341,23 @@ least get suboptimal solutions fast, which then refine over time.
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## Criteria for the evolvability of linear deformations
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\label{sec:intro:rvi}
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\improvement[inline]{Nomenklatur. Was ist $\vec{U}$? Kurz Matrix--Darstellung
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des Problems & Rückgriff auf FFD-Kapitel.}
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As we have established in chapter \ref{sec:back:ffd}, we can describe a
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deformation by the formula
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$$
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V = UP
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$$
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where $V$ is a $n \times d$ matrix of vertices, $U$ are the (during
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parametrization) calculated deformation--coefficients and $P$ is a $m \times d$ matrix
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of control--points that we interact with during deformation.
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We can also think of the deformation in terms of differences from the original
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coordinates
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$$
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\Delta V = U \cdot \Delta P
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$$
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which is isomorphic to the former due to the linear correlation in the
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deformation. One can see in this way, that the way the deformation behaves lies
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solely in the entries of $U$, which is why the three criteria focus on this.
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### Variability
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@ -550,7 +573,8 @@ entfernen kann?}
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For our tests we chose different uniformly sized grids and added gaussian noise
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onto each control-point^[For the special case of the outer layer we only applied
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noise away from the object] to simulate different starting-conditions.
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noise away from the object, so the object is still confined in the convex hull
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of the control--points.] to simulate different starting-conditions.
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\unsure[inline]{verweis auf DM--FFD?}
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@ -148,7 +148,8 @@ Unless otherwise noted the following holds:
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\tightlist
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\item
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lowercase letters \(x,y,z\)\\
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refer to real variables and represent a point in 3D--Space.
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refer to real variables and represent the coordinates of a point in
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3D--Space.
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\item
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lowercase letters \(u,v,w\)\\
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refer to real variables between \(0\) and \(1\) used as coefficients
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@ -169,15 +170,15 @@ Unless otherwise noted the following holds:
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\improvement[inline]{Mehr Bilder}
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Many modern industrial design processes require advanced optimization
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methods due to the increased complexity. These designs have to adhere to
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more and more degrees of freedom as methods refine and/or other methods
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are used. Examples for this are physical domains like aerodynamic
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(i.e.~drag), fluid dynamics (i.e.~throughput of liquid) --- where the
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complexity increases with the temporal and spatial resolution of the
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simulation --- or known hard algorithmic problems in informatics
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(i.e.~layouting of circuit boards or stacking of 3D--objects). Moreover
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these are typically not static environments but requirements shift over
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time or from case to case.
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methods due to the increased complexity resulting from more and more
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degrees of freedom as methods refine and/or other methods are used.
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Examples for this are physical domains like aerodynamic (i.e.~drag),
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fluid dynamics (i.e.~throughput of liquid) --- where the complexity
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increases with the temporal and spatial resolution of the simulation ---
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or known hard algorithmic problems in informatics (i.e.~layouting of
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circuit boards or stacking of 3D--objects). Moreover these are typically
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not static environments but requirements shift over time or from case to
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case.
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Evolutionary algorithms cope especially well with these problem domains
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while addressing all the issues at hand\cite{minai2006complex}. One of
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@ -228,7 +229,7 @@ the original author used, namely \emph{regularity}, \emph{variability},
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and \emph{improvement potential}. We introduce these term in detail in
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Chapter \ref{sec:intro:rvi}. In the original publication the author
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could show a correlation between these evolvability--criteria with the
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quality and potential of such optimization.
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quality and convergence speed of such optimization.
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We will replicate the same setup on the same objects but use \acf{FFD}
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instead of \acf{RBF} to create a local deformation near the control
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@ -332,16 +333,20 @@ between \(\tau_i\) and \(\tau_{i+d}\) and out between \(\tau_{i+1}\),
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and \(\tau_{i+d+1}\) as can bee seen from the two coefficients in every
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step of the recursion.
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\improvement[inline]{Weitere Eigenschaften erwähnen:
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\newline Convex hull
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\newline $\sum_i N_i = 1$?
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\newline Bilder von Basisfunktionen zur Visualisierung.
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This means that all changes are only a local linear combination between
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the control--point \(p_i\) to \(p_{i+d+1}\) and consequently this yields
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to the convex--hull--property of B-Splines --- meaning, that no matter
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how we choose our coefficients, the resulting points all have to lie
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inside convex--hull of the control--points.
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\improvement[inline]{
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Bilder von Basisfunktionen zur Visualisierung.
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}
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For a given number of points \(v_1,\dots,v_n\) we can then calculate the
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contributions \(n_{i,j}~:=~N_{j,d,\tau}\) of each control point \(p_j\)
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to get the projection from the control--point--space into the
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object--space: \[
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contributions \linebreak[4]\(n_{i,j}~:=~N_{j,d,\tau}\) of each control
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point \(p_j\) to get the projection from the control--point--space into
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the object--space: \[
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v_i = \sum_j n_{i,j} \cdot p_j = \vec{n}_i^{T} \vec{p}
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\] or written for all points at the same time: \[
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\vec{v} = \vec{N} \vec{p}
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@ -420,14 +425,17 @@ broader sense.
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The general shape of an evolutionary algorithm (adapted from
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\cite{back1993overview}) is outlined in Algorithm \ref{alg:evo}. Here,
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\(P(t)\) denotes the population of parameters in step \(t\) of the
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algorithm. The population contains \(\mu\) individuals \(a_i\) that fit
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the shape of the parameters we are looking for. Typically these are
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initialized by a random guess or just zero. Further on we need a
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so--called \emph{fitness--function}
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\(\Phi : I \mapsto M\)\improvement{Was ist $I,M$?\newline Bezug Genotyp/Phenotyp}
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that can take each parameter to a measurable space along a
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convergence--function \(c : I \mapsto \mathbb{B}\) that terminates the
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optimization.
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algorithm. The population contains \(\mu\) individuals \(a_i\) from the
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possible individual--set \(I\) that fit the shape of the parameters we
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are looking for. Typically these are initialized by a random guess or
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just zero. Further on we need a so--called \emph{fitness--function}
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\(\Phi : I \mapsto M\) that can take each parameter to a measurable
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space \(M\) (usually \(M = \mathbb{R}\)) along a convergence--function
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\(c : I \mapsto \mathbb{B}\) that terminates the optimization.
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Biologically speaking the set \(I\) corresponds to the set of possible
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\emph{Genotypes} while \(M\) represents the possible observable
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\emph{Phenotypes}.
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The main algorithm just repeats the following steps:
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@ -435,8 +443,8 @@ The main algorithm just repeats the following steps:
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\tightlist
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\item
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\textbf{Recombine} with a recombination--function
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\(r : I^{\mu} \mapsto I^{\lambda}\) to generate new individuals based
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on the parents characteristics.\\
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\(r : I^{\mu} \mapsto I^{\lambda}\) to generate \(\lambda\) new
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individuals based on the characteristics of the \(\mu\) parents.\\
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This makes sure that the next guess is close to the old guess.
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\item
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\textbf{Mutate} with a mutation--function
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@ -507,8 +515,21 @@ deformations}\label{criteria-for-the-evolvability-of-linear-deformations}
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\label{sec:intro:rvi}
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\improvement[inline]{Nomenklatur. Was ist $\vec{U}$? Kurz Matrix--Darstellung
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des Problems & Rückgriff auf FFD-Kapitel.}
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As we have established in chapter \ref{sec:back:ffd}, we can describe a
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deformation by the formula \[
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V = UP
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\] where \(V\) is a \(n \times d\) matrix of vertices, \(U\) are the
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(during parametrization) calculated deformation--coefficients and \(P\)
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is a \(m \times d\) matrix of control--points that we interact with
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during deformation.
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We can also think of the deformation in terms of differences from the
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original coordinates \[
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\Delta V = U \cdot \Delta P
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\] which is isomorphic to the former due to the linear correlation in
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the deformation. One can see in this way, that the way the deformation
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behaves lies solely in the entries of \(U\), which is why the three
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criteria focus on this.
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\subsection{Variability}\label{variability}
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@ -730,8 +751,9 @@ entfernen kann?}
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For our tests we chose different uniformly sized grids and added
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gaussian noise onto each control-point\footnote{For the special case of
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the outer layer we only applied noise away from the object} to
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simulate different starting-conditions.
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the outer layer we only applied noise away from the object, so the
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object is still confined in the convex hull of the control--points.}
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to simulate different starting-conditions.
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\unsure[inline]{verweis auf DM--FFD?}
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@ -16,7 +16,7 @@
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\usepackage{color} %\colorbox
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\usepackage{dsfont} %\mathds
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\usepackage{draftwatermark}
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\SetWatermarkLightness{0.9} % default: 0.8
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\SetWatermarkLightness{0.95} % default: 0.8
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\usepackage{epigraph}
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% \usepackage{euler} % euler: uni, eucal: baake, ohne: standard
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\usepackage{eucal} % euler calligraphy
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