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@@ -35,9 +35,9 @@ algorithm.
% Codewords, n, k, rate
%
One particularly important class of coding schemes is that of binary
linear block codes.
The information to be protected takes the form of a sequence of
Binary linear block codes form one particularly important class of
coding schemes.
The information to be protected is represented by a sequence of
binary symbols, which is split into separate blocks.
Each block is encoded, transmitted, and decoded separately.
The encoding step introduces redundancy by mapping input messages
@@ -45,10 +45,11 @@ $\bm{u} \in \mathbb{F}_2^k$ of length $k \in \mathbb{N}$ (called the
\textit{information length}) onto \textit{codewords} $\bm{x} \in
\mathbb{F}_2^n$ of length $n \in \mathbb{N}$ (called the
\textit{block length}) with $n > k$.
A measure of the amount of introduced redundancy is the \textit{code
rate} $R = k/n$.
We call the set of all codewords $\mathcal{C}$ the \textit{code}
\cite[Sec.~3.1.1]{ryan_channel_2009}.
The \textit{code rate} $R = k/n$ is a measure of the amount of
introduced redundancy.
We call the set of all codewords
$\mathcal{C} = \{\bm{x}^{(1)}, \bm{x}^{(2)}, \ldots, \bm{x}^{(2^k)}\}$
the \textit{code} \cite[Sec.~3.1.1]{ryan_channel_2009}.
%
% d_min and the [] Notation
@@ -77,7 +78,7 @@ $[n,k,d_\text{min}]$.
% Parity checks, H, and the syndrome
%
A particularly elegant way of describing the code space $C$ is the
A particularly elegant way of describing the code space $\mathcal{C}$ is the
notion of \textit{parity checks}.
Since $\lvert \mathcal{C} \rvert = 2^k$ and $\lvert \mathbb{F}_2^n
\rvert = 2^n$, there are $n-k$ conditions constrain the additional
@@ -86,17 +87,17 @@ These conditions, called parity checks, take the form of equations
over $\mathbb{F}_2^n$, linking the individual positions of each codeword.
We can arrange the coefficients of these equations in a
\textit{parity-check matrix} (\acs{pcm}) $\bm{H} \in
\mathbb{F}_2^{(n-k) \times n}$ and equivalently define the code as
\cite[Sec.~3.1.1]{ryan_channel_2009}
\mathbb{F}_2^{(n-k) \times n}$, $\text{rank}(\bm{H}) = n-k$, and
equivalently define the code as \cite[Sec.~3.1.1]{ryan_channel_2009}
\begin{align*}
\mathcal{C} = \left\{ \bm{x} \in \mathbb{F}_2^n :
\bm{H}\bm{x}^\text{T} = \bm{0} \right\}
\mathcal{C} := \text{kern}(\bm{H}) = \left\{ \bm{x} \in \mathbb{F}_2^n :
\bm{H}\bm{x}^\mathsf{T} = \bm{0} \right\}
.%
\end{align*}
Note that in general we may have linearly dependent parity checks,
In general, we have linearly dependent parity checks,
prompting us to define the \ac{pcm} as $\bm{H} \in
\mathbb{F}_2^{m\times n}$ with $\hspace{2mm} m \ge n-k$ instead.
The \textit{syndrome} $\bm{s} = \bm{H} \bm{v}^\text{T}$ describes
The \textit{syndrome} $\bm{s} = \bm{H} \bm{v}^\mathsf{T}$ describes
which parity checks a vector $\bm{v} \in \mathbb{F}_2^n$ violates.
The representation using the \ac{pcm} has the benefit of providing a
description of the code, the memory complexity of which does not grow
@@ -118,9 +119,9 @@ $\bm{y} \in \mathbb{R}^n$, and \textit{hard-decision} decoding, where
$\bm{y} \in \mathbb{F}_2^n$ \cite[Sec.~1.5.1.3]{ryan_channel_2009}.
Finally, the decoder is responsible for obtaining an estimate
$\hat{\bm{u}} \in \mathbb{F}_2^k$ of the original input message.
This is done by first finding an estimate $\hat{\bm{x}}$ of the sent
This can be done by first finding an estimate $\hat{\bm{x}}$ of the sent
codeword and undoing the encoding.
The decoding problem that we generally attempt to solve thus consists
The decoding problem that we attempt to solve thus consists
in finding the best estimate $\hat{\bm{x}}$ given $\bm{y}$.
\begin{figure}[t]
@@ -168,9 +169,9 @@ in finding the best estimate $\hat{\bm{x}}$ given $\bm{y}$.
%
Shannon's noisy-channel coding theorem is stated for codes whose block
length approaches infinity. This suggests that as the block length
becomes larger, the performance of the considered codes should
generally improve.
length $n$ approaches infinity.
This suggests that as the block length becomes larger, the
performance of the considered codes should generally improve.
However, the size of the \ac{pcm} of a linear block code grows
quadratically with $n$.
This would quickly render decoding intractable as we increase the
@@ -189,13 +190,14 @@ This is exactly the motivation behind \ac{ldpc} codes
These differ from ``classical codes'' in their decoding algorithms:
Classical codes are usually decoded using one-step hard-decision decoding,
whereas modern codes are suitable for iterative soft-decision
decoding \cite[Preface]{ryan_channel_2009}. The iterative decoding algorithms
decoding \cite[Preface]{ryan_channel_2009}.
For \ac{ldpc} codes, the iterative decoding algorithms
are generally defined in terms of message passing on the
\textit{Tanner graph} of a code. The Tanner graph is a bipartite
graph that constitutes an alternative representation of the \ac{pcm}.
We define two types of nodes: \acp{vn}, corresponding to codeword
We define two types of nodes: \Acp{vn}, corresponding to codeword
bits, and \acp{cn}, corresponding to individual parity checks.
We then construct the Tanner graph by connecting each \ac{cn} to
Then, we construct the Tanner graph by connecting each \ac{cn} to
the \acp{vn} that make up the corresponding parity check
\cite[Sec.~5.1.2]{ryan_channel_2009}.
\Cref{PCM and Tanner graph of the Hamming code} shows the Tanner
@@ -273,11 +275,11 @@ Mathematically, we represent a \ac{vn} using the index $i \in
and a \ac{cn} using the index $j \in \mathcal{J}
:= \left[ 0 : m-1 \right]$.
We can then encode the information contained in the graph by defining
the neighborhood of a variable node $i$ as
$\mathcal{N}_\text{V} (i) = \left\{ j \in \mathcal{J} : \bm{H}_{j,i}
the neighborhood of a \ac{vn} $i$ as
$\mathcal{N}_\text{V} (i) = \left\{ j \in \mathcal{J} : H_{j,i}
= 1 \right\}$
and that of a check node $j$ as
$\mathcal{N}_\text{C} (j) = \left\{ i \in \mathcal{I} : \bm{H}_{j,i}
and the neighborhood of a \ac{cn} $j$ as
$\mathcal{N}_\text{C} (j) = \left\{ i \in \mathcal{I} : H_{j,i}
= 1 \right\}$.
%
@@ -379,15 +381,15 @@ the numbers of ones, of their rows and columns are constant
Already during their introduction, regular \ac{ldpc} codes were shown to have
a minimum distance scaling linearly with the block length $n$ for
large values \cite[Ch.~2,~Theorem~1]{gallager_low_1960},
which leads to the fact that they do not exhibit an error floor under
\ac{ml} decoding.
Irregular codes, on the other hand, generally do exhibit an error floor,
while their redeeming quality is the ability to reach near-capacity
performance in the waterfall region \cite[Intro.]{costello_spatially_2014}.
which leads to a more favorable behavior of the error rate for high
signal-to-noise ratios.
Irregular codes, on the other hand, have more severe error floor behavior.
However, they have the the ability to reach near-capacity performance
in the waterfall region \cite[Intro.]{costello_spatially_2014}.
\subsection{Spatially-Coupled LDPC Codes}
A recent development in the field of \ac{ldpc} codes is that of
A more recent development in the field of \ac{ldpc} codes is that of
\ac{sc}-\ac{ldpc} codes.
Their key feature is that they combine the best properties of regular
and irregular codes.
@@ -399,11 +401,12 @@ waterfall region \cite[Intro.]{costello_spatially_2014}.
The essential property of \ac{sc}-\ac{ldpc} codes is that codewords
from different \textit{spatial positions}, which would ordinarily be sent
one after the other independently, are linked.
This is achieved by connecting some \acp{vn} of one spatial position to
\acp{cn} of another, resulting in a \ac{pcm} of the form
This is achieved by introducing edges between \acp{vn} of one spatial
position and \acp{cn} of another, resulting in a \ac{pcm} of the form
\cite[Eq.~1]{hassan_fully_2016}
%
\begin{align*}
\begin{align}
\label{eq:PCM}
\bm{H} =
\begin{pmatrix}
\bm{H}_0(1) & & \\
@@ -413,10 +416,11 @@ This is achieved by connecting some \acp{vn} of one spatial position to
& & \bm{H}_K(L) \\
\end{pmatrix}
,
\end{align*}
\end{align}
%
where $K \in \mathbb{N}$ is the \textit{coupling width} and $L \in
\mathbb{N}$ is the number of spatial positions.
The parts of the \ac{pcm} left empty in \Cref{eq:PCM} are filled with zeros.
This construction results in a Tanner graph as depicted in
\Cref{fig:sc-ldpc-tanner}.
@@ -513,7 +517,7 @@ Note that at the first few spatial positions some \acp{cn} have lower degrees.
This leads to more reliable information about the
\acp{vn} that, as we will see, is
later passed to subsequent spatial positions during decoding.
This is precisely the effect that leads to the good performance of
This is precisely the effect that leads to the improved performance of
\ac{sc}-\ac{ldpc} codes in the waterfall region \cite{costello_spatially_2014}.
\subsection{Iterative Decoding}
@@ -521,15 +525,14 @@ This is precisely the effect that leads to the good performance of
% Introduction
\ac{ldpc} codes are generally decoded using efficient iterative
algorithms, something that is possible due to their sparsity
\cite[Sec.~5.3]{ryan_channel_2009}.
The algorithm originally proposed alongside LDPC codes for this
purpose by Gallager in 1960 is now known as the \ac{spa}
Due to their sparse graphs, efficient iterative decoders exist for
\ac{ldpc} codes \cite[Sec.~5.3]{ryan_channel_2009}.
The decoding algorithm originally proposed alongside LDPC codes by
Gallager in 1960 is now known as the \ac{spa}
\cite[5.4.1]{ryan_channel_2009}, also called \acf{bp}.
The optimality criterion the \ac{spa} is built around is a
symbol-wise \ac{map} decision \cite[Sec.~5.4.1]{ryan_channel_2009}.
bit-wise \ac{map} decision \cite[Sec.~5.4.1]{ryan_channel_2009}.
The core idea of the resulting algorithm is to view \acp{cn}
and \acp{vn} as representing individual local codes.
A \ac{cn} represents a single parity check on the connected \acp{vn},
@@ -539,11 +542,11 @@ should agree on its value; it can therefore be understood as a repetition code.
The algorithm alternates between consolidating soft information about
the \acp{vn} in the \acp{cn}, and consolidating soft information about
the \acp{cn} in the \acp{vn}.
To this end, messages are passed back and forth along the edges of
the Tanner graph.
To this end, messages computed in the nodes are passed back and forth
along the edges of the Tanner graph.
$L_{i\rightarrow j}$ represents a message passed from \ac{vn} $i$ to
\ac{cn} j, $L_{i\leftarrow j}$ represents a message passed from
\ac{cn} j to \ac{vn} i.
\ac{cn} $j$, $L_{i\leftarrow j}$ represents a message passed from
\ac{cn} $j$ to \ac{vn} $i$.
The \acp{vn} additionally receive messages \cite[5.4.2]{ryan_channel_2009}
\begin{align*}
\tilde{L}_i = \log \frac{P(X=0 \vert Y=y)}{P(X=1 \vert Y=y)},
@@ -574,7 +577,7 @@ possible cycles and are thus especially problematic.
% Min-sum algorithm
A simplification of the \ac{spa} is the min-sum decoder. Here, the
A simplification of the \ac{spa} is the min-sum algorithm. Here, the
\ac{cn} update is approximated as \cite[Sec.~5.5.1]{ryan_channel_2009}
\begin{align*}
L_{i \leftarrow j} = \prod_{i' \in \mathcal{N}_\text{C}(j)\setminus \{i\}}
@@ -598,7 +601,7 @@ decoding of subsequent blocks \cite[Sec.~III.~C.]{hassan_fully_2016}.
\label{sec:Quantum Mechanics and Quantum Information Science}
Designing codes and decoders for \ac{qec} is generally performed on a
layer of abstraction far removed from the quantum mechanical
layer of mathematical abstraction far removed from the quantum mechanical
processes underlying the actual physics.
Nevertheless, having a fundamental understanding of the related
quantum mechanical concepts is useful to grasp the unique constraints
@@ -618,39 +621,41 @@ function and the observable world:
$\lvert \psi (x,t) \rvert^2$ is the \ac{pdf} of finding a particle at
position $x$ and time $t$ \cite[Sec.~1.2]{griffiths_introduction_1995}.
Note that this presupposes a normalization of $\psi$ such that
$\int_{-\infty}^{\infty} \lvert \psi(x,t) \rvert^2 dx = 1$.
\begin{align*}
\int_{-\infty}^{\infty} \lvert \psi(x,t) \rvert^2 dx = 1
.%
\end{align*}
% Dirac notation
Much of the related mathematics can be very elegantly expressed
using the language of linear algebra.
The so-called Bra-ket or Dirac notation is especially appropriate,
having been proposed by Paul Dirac in 1939 for the express purpose
of simplifying quantum mechanical notation \cite{dirac_new_1939}.
Two new symbols are defined, \emph{bra}s $\bra{\cdot}$ and
\emph{ket}s $\ket{\cdot}$.
The language of linear algebra allows one to express the related
mathematics particularly elegantly.
The so-called Bra-ket or Dirac notation, introducced
by Paul Dirac in 1939 for the express purpose of simplifying quantum
mechanical notation \cite{dirac_new_1939}, is especially appropriate.
Two new symbols are defined, \emph{bra} $\bra{\cdot}$ and
\emph{ket} $\ket{\cdot}$.
Kets denote column vectors, while bras denote their Hermitian conjugates.
For example, two vectors specified by the labels $a$ and $b$
respectively are written as $\ket{a}$ and $\ket{b}$.
For example, two vectors specified by the labels $a$ and $b$,
respectively, are written as $\ket{a}$ and $\ket{b}$.
Their inner product is $\braket{a\vert b}$.
% Expressing wave functions using linear algebra
The connection we will make between quantum mechanics and linear
algebra is that we will model the state space of a system as a
\emph{function space}, the Hilbert space $L_2$.
We will represent the state of a particle with wave function
$\psi(x,t)$ using the vector $\ket{\psi}$
\cite[Sec.~3.3]{griffiths_introduction_1995}.
\emph{function space}, namely the Hilbert space $L_2$.
The state of a particle with wave function $\psi(x,t)$ is represented
by the vector $\ket{\psi}$ \cite[Sec.~3.3]{griffiths_introduction_1995}.
% Operators
Another important notion is that of an \emph{operator}, a transformation
that takes a function as an input and returns another function as an
output \cite[Sec.~3.2.2]{griffiths_introduction_1995}.
that maps a function onto another function
\cite[Sec.~3.2.2]{griffiths_introduction_1995}.
A prominent example of this is the differential operator $\partial x$.
Operators are useful to describe the relations between different
quantities relating to a particle.
An example of this is the differential operator $\partial x$.
We define the \emph{commutator} of two operators $P_1$ and $P_2$ as
\begin{align*}
[P_1,P_2] = P_1P_2 - P_2P_1
@@ -669,22 +674,21 @@ We say the two operators \emph{commute} iff $[P_1,P_2] = 0$, and they
% Observable quantities
An \emph{observable quantity} $Q(x,p,t)$ is a quantity of a quantum
mechanical system that we can measure, such as the position $x$ or
An \emph{observable} $Q(x,p,t)$ is a quantity of a quantum
mechanical system that we can measure, e.g., the position $x$ or
momentum $p$ of a particle.
In general, such measurements are not deterministic, i.e.,
measurements on identically prepared states can yield different results.
There are some states, however, that are \emph{determinate} for a
specific observable: measuring those will always yield identical
observations \cite[Sec.~3.3]{griffiths_introduction_1995}.
However, some states are \emph{determinate} for a
specific observable: Measuring those will always yield identical
outcomes \cite[Sec.~3.3]{griffiths_introduction_1995}.
% General expression for expected value of observable quantity
If we know the wave function of a particle, we should be able to
compute the expected value $\braket{Q}$ of any observable quantity we wish.
It can be shown that for any $Q$, we can find a
corresponding Hermitian operator $\hat{Q}$ such that
\cite[Sec.~3.3]{griffiths_introduction_1995}
If the wave function of a particle is known, the expected value
$\braket{Q}$ of any observable quantity can be computed.
Indeed, for any $Q$, there exists a corresponding Hermitian operator
$\hat{Q}$ such that \cite[Sec.~3.3]{griffiths_introduction_1995}
\begin{align}
\label{eq:gen_expr_Q_exp}
\braket{Q} = \int_{-\infty}^{\infty} \psi^*(x,t) \hat{Q} \psi(x,t) dx
@@ -700,9 +704,9 @@ operator to $\hat{Q} = x$, we can write
= \int_{-\infty}^{\infty} x \lvert \psi(x,t) \rvert ^2 dx
.%
\end{align*}
Note that $\lvert \psi(x,t) \rvert^2 $ represents the \ac{pdf} of
finding a particle in a specific state. We immediately see that the
formula simplifies to the direct calculation of the expected value.
Note that $\lvert \psi(x,t) \rvert^2 $ is the \ac{pdf} of
finding a particle at position $x$. Hence, we immediately see that
the formula simplifies to the direct calculation of the expected value.
% Determinate states and eigenvalues
@@ -716,40 +720,40 @@ We begin by translating \Cref{eq:gen_expr_Q_exp} into linear algebra as
.%
\end{align}
\Cref{eq:gen_expr_Q_exp_lin} expresses an inherently probabilistic
relationship.
The determinate states are inherently deterministic.
relationship, whereas the determinate states are inherently deterministic.
To relate the two, we note that since determinate states should
always yield the same measurement results, the variance of the
observable should be zero.
observable must be zero.
We thus compute \cite[Eq.~3.116]{griffiths_introduction_1995}
\begin{align}
0 &\overset{!}{=} \braket{(Q - \braket{Q})^2}
= \braket{e_n \vert (\hat{Q} - \braket{Q})^2 e_n} \nonumber\\
&= \braket{(Q - \braket{Q})e_n \vert (\hat{Q} - \braket{Q})
&= \braket{(\hat{Q} - \braket{Q})e_n \vert (\hat{Q} - \braket{Q})
e_n} \nonumber\\
&= \lVert (Q - \braket{Q}) e_n \rVert^2 \nonumber\\[3mm]
&\hspace{-8mm}\Leftrightarrow (\hat{Q} - \braket{Q}) \ket{e_n} =
0 \nonumber\\
&= \lVert (\hat{Q} - \braket{Q}) e_n \rVert^2 \nonumber\\[3mm]
&\hspace{-14mm}\iff (\hat{Q} - \braket{Q}) \ket{e_n}
= 0 \nonumber\\
\label{eq:observable_eigenrelation}
&\hspace{-8mm}\Leftrightarrow \hat{Q}\ket{e_n}
&\hspace{-14mm}\iff \hat{Q}\ket{e_n}
= \underbrace{\braket{Q}}_{\lambda_n} \ket{e_n}
.%
\end{align}%
%
Because we have assumed the variance to be zero, the expected value
$\braket{Q}$ is now the deterministic measurement result
By setting the variance to zero, the expected value
$\braket{Q}$ becomes a deterministic measurement result
corresponding to the determinate state
$\ket{e_n},~n\in \mathbb{N}$.
We can see that the determinate states are the \emph{eigenstates} of
the observable operator $\hat{Q}$ and that the measurement values are
the corresponding \emph{eigenvalues} $\lambda_n$
The determinate states are precisely the \emph{eigenstates} of
the observable operator $\hat{Q}$, and the associated measurement
values are the corresponding \emph{eigenvalues} $\lambda_n$
\cite[Sec.~3.3]{griffiths_introduction_1995}.
% Determinate states as a basis
As we are modelling the wave function $\psi(x,t)$ as a vector
As we model the wave function $\psi(x,t)$ as a vector
$\ket{\psi}$, we can find a set of basis vectors to decompose it into.
We can use the determinate states for this purpose, expressing the state as%
In particular, we can use the determinate states for this purpose,
expressing the state as%
\footnote{
We only consider the case of having a \emph{discrete
spectrum} here, i.e., having a discrete set of eigenvalues and vectors.
@@ -787,7 +791,7 @@ $Q(x,t,p)$ using a corresponding operator $\hat{Q}$, which allows us
to compute the expected value as $\braket{Q} = \braket{\psi
\vert \hat{Q} \psi}$.
The eigenvectors of $\hat{Q}$ are the determinate states
$\ket{e_n},~n\in \mathbb{N}$ and the eigenvalues are the respective
$\ket{e_n},~n\in \mathbb{N}$, and the eigenvalues are the respective
measurement outcomes.
We can decompose an arbitrary state as $\ket{\psi} = \sum_{n=1}^{\infty} c_n
\ket{e_n}$, where $\lvert c_n \rvert ^2$ represents the probability
@@ -805,16 +809,16 @@ The measurements we considered in the previous section, for which
\Cref{eq:gen_expr_Q_exp_lin} holds, belong to the category of
\emph{projective measurements}.
For these, certain restrictions such as repeatability apply: the act
of measuring a quantum state should \emph{collapse} it onto one of
of measuring a quantum state \emph{collapses} it onto one of
the determinate states.
Further measurements should then yield the same value.
More general methods of modelling measurements exist, e.g., describing
Further measurements then yield the same value.
More general methods of modelling measurements exist, e.g.,
destructive measurements \cite[Box~2.5]{nielsen_quantum_2010}, but
they are not relevant to this work.
% Projection operators
We can model the collapse of the original state onto one of the
We model the collapse of the original state onto one of the
superimposed basis states as a \emph{projection}.
To see this, we use
\Cref{eq:determinate_basis,eq:observable_eigenrelation} to compute
@@ -833,9 +837,9 @@ the separate components as
using \emph{projection operators} \cite[Eq.~3.160]{griffiths_introduction_1995}
\begin{align*}
\hat{P}_n := \ket{e_n}\bra{e_n}, \hspace{3mm} n\in \mathbb{N}
.
,
\end{align*}%
These project a vector onto the subspace spanned by $\ket{e_n}$.
which project a vector onto the subspace spanned by $\ket{e_n}$.
% % Using projection operators to measure if a state has a component
% % along a basis vector
@@ -861,10 +865,9 @@ These project a vector onto the subspace spanned by $\ket{e_n}$.
% Intro
% TODO: Make sure `quantum gate` is proper terminology
A central concept for quantum computing is that of the \emph{qubit}.
We employ it analogously to the classical \emph{bit}.
For classical computers, we alter bits' states using \emph{gates}.
It takes the place of the classical \emph{bit}.
For classical computers, we alter the state of a bit using \emph{gates}.
We can chain multiple of these gates together to build up more complex logic,
such as half-adders or eventually a full processor.
In principle, quantum computers work in a similar fashion, only that
@@ -895,10 +898,10 @@ A qubit is defined to be a system with quantum state
\alpha \\
\beta
\end{pmatrix}
= \alpha \ket{0} + \beta \ket{1}
= \alpha \ket{0} + \beta \ket{1}, \hspace{5mm} \alpha,\beta \in \mathbb{C}
.%
\end{align}
The overall state of a composite quantum system is described using
The overall state of a multi-qubit quantum system is described using
the \emph{tensor product}, denoted as $\otimes$
\cite[Sec.~2.2.8]{nielsen_quantum_2010}.
Take for example the two qubits
@@ -927,9 +930,9 @@ i.e.,
.%
\end{split}
\end{align}
We call $\ket{x_0, \ldots, x_n}~, x_i \in \{0,1\}$ the
We call $\ket{x_0, \ldots, x_n},~x_i \in \{0,1\}$ the
\emph{computational basis states} \cite[Sec.~4.6]{nielsen_quantum_2010}.
To additionally simplify set notation, we define
To simplify set notation, we define
\begin{align*}
\mathcal{M}^{\otimes n} := \underbrace{\mathcal{M}\otimes \ldots
\otimes \mathcal{M}}_{n \text{ times}}
@@ -938,7 +941,7 @@ To additionally simplify set notation, we define
% Entanglement
States that are not able to be decomposed into such products
States that are not able to be decomposed into products of single-qubit states
are called \emph{entangled} \cite[Sec.~2.2.8]{nielsen_quantum_2010}.
An example of such states are the \emph{Bell states}
\begin{align*}
@@ -976,7 +979,7 @@ we now shift our focus to describing the evolution of their states.
We model state changes as operators.
Unlike classical systems, where there are only two possible states and
thus the only possible state change is a bit-flip, a general qubit
state as shown in \Cref{eq:gen_qubit_state} lives on a continuum of values.
state as shown in \Cref{eq:gen_qubit_state} lies on a continuum of values.
We thus technically also have an infinite number of possible state changes.
Fortunately, we can express any operator as a linear combination of the
\emph{Pauli operators} \cite[Sec.~2.2]{gottesman_stabilizer_1997}
@@ -1013,13 +1016,15 @@ Fortunately, we can express any operator as a linear combination of the
In fact, if we allow for complex coefficients, the $X$ and $Z$
operators are sufficient to express any other operator as a linear
combination \cite[Sec.~2.2]{roffe_quantum_2019}.
$I$ is the identity operator and $X$ and $Z$ are referred to as
Hereby, $I$ is the identity operator and $X$ and $Z$ are referred to as
\emph{bit-flips} and \emph{phase-flips} respectively.
We call the set $\mathcal{G}_n = \left\{ \pm I,\pm \mathrm{i}I, \pm
X,\pm \mathrm{i}X,
\pm Y,\pm \mathrm{i}Y, \pm Z, \pm \mathrm{i}Z \right\}^{\otimes n}$
the \emph{Pauli
group} over $n$ qubits.
We call the set
\begin{align}
\mathcal{G}_n = \left\{ \pm I,\pm \mathrm{i}I, \pm
X,\pm \mathrm{i}X,
\pm Y,\pm \mathrm{i}Y, \pm Z, \pm \mathrm{i}Z \right\}^{\otimes n}
\end{align}
the \emph{Pauli group} over $n$ qubits.
In the context of modifying qubit states, we also call operators \emph{gates}.
When working with multi-qubit systems, we can also apply Pauli gates
@@ -1049,7 +1054,7 @@ Other important operators include the \emph{Hadamard} and
\centering
\begin{align*}
\begin{array}{c}
CNOT\text{ Operator} \\
\text{CNOT Operator} \\
\hline\\
\ket{00} \mapsto \ket{00} \\
\ket{01} \mapsto \ket{01} \\
@@ -1060,7 +1065,9 @@ Other important operators include the \emph{Hadamard} and
\end{minipage}%
\end{figure}
\vspace{-4mm}
\noindent Many more operators relevant to quantum computing exist, but they are
\noindent The CNOT operator is a 2-qubit gate that applies a bit-flip to the
second qubit conditioned on the state of the first one.
Many more operators relevant to quantum computing exist, but they are
not covered here as they are not central to this work.
%%%%%%%%%%%%%%%%
@@ -1093,9 +1100,8 @@ The control connection is represented by a vertical line connecting
the gate to the corresponding qubit, where a filled dot is placed.
A controlled gate applies the respective operation only if the
control qubit is in state $\ket{1}$.
An example of this is the CNOT gate introduced in
\Cref{subsec:Qubits and Multi-Qubit States}, which is depicted in
\Cref{fig:cnot_circuit}.
\Cref{fig:cnot_circuit} depicts an example of this: The CNOT gate
introduced in \Cref{subsec:Qubits and Multi-Qubit States}.
\begin{figure}[t]
\centering
@@ -1117,7 +1123,7 @@ An example of this is the CNOT gate introduced in
% General motivation behind QEC
One of the major barriers on the road to building a functioning
One of the major barriers on the road to building a functioning and scalable
quantum computer is the inevitability of errors during quantum
computation. These arise due to the difficulty in sufficiently isolating the
qubits from external noise \cite[Sec.~1]{roffe_quantum_2019}.
@@ -1126,7 +1132,7 @@ with the environment act as small measurements, an effect called
\emph{decoherence} of the quantum state
\cite[Sec.~1]{gottesman_stabilizer_1997}.
\ac{qec} is one approach of dealing with this problem, by protecting
the quantum state in a similar fashion to information in classical error
a quantum state in a similar fashion to information in classical error
correction.
% The unique challenges of QEC
@@ -1146,9 +1152,10 @@ Three main restrictions apply \cite[Sec.~2.4]{roffe_quantum_2019}:
% General idea (logical vs. physical gates) + notation
Much like in classical error correction, in \ac{qec} information
is protected by mapping it onto codewords in a higher-dimensional space,
thereby introducing redundancy.
Much like in classical error correction, \ac{qec} protects information by
introducing redundancy.
The information, represented by a state in a low-dimensional space,
is mapped onto an encoded state in a higher-dimensional space.
To this end, $k \in \mathbb{N}$ \emph{logical qubits} are mapped onto
$n \in \mathbb{N}$ \emph{physical qubits}, $n>k$.
We circumvent the no-cloning restriction by not copying the state of any of
@@ -1169,8 +1176,9 @@ This is due to the \emph{backlog problem}
\cite[Sec.~II.G.3.]{terhal_quantum_2015}: There are certain gates
at which the effect of existing errors on single qubits may be
exacerbated by transforming them to multi-qubit errors.
We wish to correct the errors before passing qubits through such gates.
If the \ac{qec} system is not fast enough, there will be an increasing
If we ensure decoding with sufficiently low latency, we can correct
the errors before passing qubits through such gates.
However, if the \ac{qec} system is not fast enough, there will be an increasing
backlog of information at this point in the circuit, leading to an
exponential slowdown in computation.
@@ -1200,8 +1208,8 @@ Note that this code is only able to detect single $X$-type errors.
% Measuring stabilizers
To determine if an error occurred, we want to measure
whether a state belongs
To determine if an error occurred, we aim at to measuring whether a
state belongs
% TODO: Remove footnote?
% \footnote{
% It is possible for a state to not completely lie in either subspace.
@@ -1210,11 +1218,12 @@ whether a state belongs
% }
to $\mathcal{C}$ or $\mathcal{F}$.
As explained in \Cref{subsec:Observables}, physical measurements
can be mathematically described using operators whose eigenvalues
can be mathematically described using operators, whose eigenvalues
are the possible measurement results.
Here, we need an operator with two eigenvalues and the corresponding
eigenspaces should be $\mathcal{C}$ and $\mathcal{F}$ respectively.
For the two-qubit code, $Z_1Z_2$ is such an operator:
For the two-qubit repetition code, $Z_1Z_2 \in \mathcal{G}_2$ is such
an operator:
\begin{align}
Z_1Z_2 E \ket{\psi}_\text{L} &= (+1) E \ket{\psi}_\text{L}
\hspace*{3mm} \forall
@@ -1225,13 +1234,14 @@ For the two-qubit code, $Z_1Z_2$ is such an operator:
.%
\end{align}
$E \in \left\{ X,I \right\}$ is an operator describing a possible
error and $E \ket{\psi}_\text{L}$ is the resulting state after that error.
single-qubit error and $E \ket{\psi}_\text{L}$ is the resulting state
after that error.
By measuring the corresponding eigenvalue, we can determine if
$E\ket{\psi}_\text{L}$ lies in $\mathcal{C}$ or $\mathcal{F}$.
% TODO: If necessary, cite \cite[Sec.~3]{roffe_quantum_2019} for the
% non-compromising meausrement of the information
To do this without directly observing (and thus potentially
collapsing) the logical state $\ket{\psi}_\text{L}$, we prepare an
To do this without directly observing and, thus potentially
collapsing, the logical state $\ket{\psi}_\text{L}$, we prepare an
ancilla qubit with state $\ket{0}_\text{A}$ and entangle it with
$\ket{\psi}_\text{L}$ in such a way that the eigenvalue is indicated
by measuring the ancilla qubit instead.
@@ -1296,11 +1306,11 @@ This effect is referred to as error \emph{digitization}
% The stabilizer group
Operators such as $Z_1Z_2$ above are called \emph{stabilizers}.
More generally, an operator $P_i \in \mathcal{G}_n$ is called a stabilizer of an
More generally, an operator $P_i \in \mathcal{G}_n$ is a stabilizer of an
$\llbracket n, k, d_\text{min} \rrbracket$ code $\mathcal{C}$, if
\begin{itemize}
\item It stabilizes all logical states, i.e.,
$P_i\ket{\psi}_\text{L} = (+1)\ket{\psi}_\text{L} ~\forall~
$P_i\ket{\psi}_\text{L} = (+1)\ket{\psi}_\text{L}, ~\forall~
\ket{\psi}_\text{L} \in \mathcal{C}$.
\item It commutes with all other stabilizers $P_j$ of the code,
i.e., $[P_i, P_j] = 0$.
@@ -1316,8 +1326,8 @@ Formally, we define the \emph{stabilizer group} $\mathcal{S}$ as
[P_i,P_j] = 0 \forall i,j\right\}
.%
\end{align*}
We care in particular about the commuting properties of stabilizers
with respect to possible errors.
We care about the commuting properties of stabilizers with respect to
possible errors, in particular.
The measurement circuit for an arbitrary stabilizer $P_i$ modifies
the state as \cite[Eq.~29]{roffe_quantum_2019}
\begin{align*}
@@ -1350,6 +1360,7 @@ If a given error $E$ anticommutes with $P_i$, we have
\end{align*}
and measuring the ancilla $\text{A}_i$ corresponding to stabilizer
$P_i$ returns 1.
Similarly, if it commutes, the ancilla measurement returns 0.
%%%%%%%%%%%%%%%%
\subsection{Stabilizer Codes}
@@ -1357,9 +1368,10 @@ $P_i$ returns 1.
% Structure of a stabilizer code
For classical binary linear block codes, we use $n-k$ parity-checks
Stabilizer codes are the quantum analogue of classical binary linear
block codes, for which we use $n-k$ parity checks
to reduce the degrees of freedom introduced by the encoding operation.
Effectively, each parity-check defines a local code splitting the
Effectively, each parity check defines a local code splitting the
vector space in half, with only one part containing valid codewords.
The global code is the intersection of all local codes.
We can do the same in the quantum case.
@@ -1377,19 +1389,23 @@ operators $P_i$, each using a circuit as explained in
\Cref{subsec:Stabilizer Measurements}.
Note that this is an abstract representation of the syndrome extraction.
For the actual implementation in hardware, we can transform this into
a circuit that requires only CNOT and H-gates
a circuit that requires only CNOT and $H$-gates
\cite[Sec.~10.5.8]{nielsen_quantum_2010}.
% Logical operators
In order to modify the logical state encoded using the physical
qubits, we can use \emph{logical operators} \cite[Sec.~4.2]{roffe_quantum_2019}.
For each qubit, there are two logical operators, $X_i$ and $Z_j$.
These are operators that
For a $\llbracket n,k \rrbracket$ stabilizer code, there exist
logical operators generated by $2k$ representatives $X_i,
Z_j,~i,j\in[1:k]$ such that
\begin{itemize}
\item Commute with all the stabilizers in $\mathcal{S}$.
\item Anti-commute with one another, i.e., $[ \overline{X}_i,
\overline{Z}_i ]_{+} = \overline{X}_i \overline{Z}_i +
\item They commute with all stabilizers in $\mathcal{S}$.
\item For $i=j$, they anti-commute with one another, i.e., $[
\overline{X}_i, \overline{Z}_i ]_{+} = \overline{X}_i
\overline{Z}_i + \overline{Z}_i \overline{X}_i = 0$.
\item For $i\neq j$, they commute with one another, i.e., $[ \overline{X}_i,
\overline{Z}_i ] = \overline{X}_i \overline{Z}_i -
\overline{Z}_i \overline{X}_i = 0$.
\end{itemize}
We can also measure these operators to find out the logical state a
@@ -1399,22 +1415,22 @@ physical state corresponds to \cite[Sec.~2.6]{derks_designing_2025}.
% TODO: Do I have to introduce before that stabilizers only need X
% and Z operators?
We can represent stabilizer codes using a \emph{check matrix}
\cite[Sec.~10.5.1]{nielsen_quantum_2010}
We can represent stabilizer codes using a binary \emph{check matrix}
$\bm{H} \in \mathbb{F}_2^{(n-k)\times(2n)}$
\cite[Sec.~10.5.1]{nielsen_quantum_2010} with
\begin{align*}
\bm{H} = \left[
\begin{array}{c|c}
\bm{H}_X & \bm{H}_Z
\end{array}
\right]
,%
.%
\end{align*}
with $\bm{H} \in \mathbb{F}_2^{(n-k)\times(2n)}$.
This is similar to a classical \ac{pcm} in that it contains $n-k$
rows, each describing one constraint. Each constraint restricts an additional
degree of freedom of the higher-dimensional space we use to introduce
redundancy.
In contrast to the classical case, this matrix now has $2n$ columns,
In contrast to the classical case, this matrix has $2n$ columns,
as we have to consider both the $X$ and $Z$ type operators that make up
the stabilizers.
Take for example the Steane code \cite[Eq.~10.83]{nielsen_quantum_2010}.
@@ -1433,8 +1449,8 @@ We can describe it using the check matrix
\right]
.%
\end{align}
The first $n$ columns correspond to $X$ operators acting on the
corresponding physical qubit, the rest to the $Z$ operators.
The first $n$ columns correspond to $X$ stabilizers acting on the
corresponding physical qubit, the rest to the $Z$ stabilizers.
\begin{figure}[t]
\centering
@@ -1463,27 +1479,27 @@ corresponding physical qubit, the rest to the $Z$ operators.
% Intro
Stabilizer codes are especially practical to work with when they can
handle $X$ and $Z$ type errors independently.
Stabilizer codes are especially practical to work with when the
stabilizers can be split into one subset consisting only of
$Z$ stabilizers and one consisting only of $X$ stabilizers.
As $Z$ errors anti-commute with $X$ operators in the stabilizers and
vice versa, this property translates into being able to split the
stabilizers into a subset being made up of only $X$
operators and the rest only of $Z$ operators.
vice versa, this property translates into being able to correct $X$
or $Z$ errors independently.
We call such codes \ac{css} codes.
We can see this property in \Cref{eq:steane} in the check matrix
of the Steane code.
% Construction
We can exploit this separate consideration of $X$ and $Z$ errors in
We can exploit this separate consideration of $X$ and $Z$ stabilizers in
the construction of \ac{css} codes.
We combine two binary linear codes $\mathcal{C}_1$ and
$\mathcal{C}_2$, each responsible for correcting one type of error
$\mathcal{C}_2$, each responsible for correcting either $Z$ or $X$ errors
\cite[Sec.~10.5.6]{nielsen_quantum_2010}.
Using the dual code of $\mathcal{C}_2$ \cite[Eq.~3.4]{ryan_channel_2009}
\begin{align*}
\mathcal{C}_2^\perp := \left\{ \bm{x}' \in \mathbb{F}^2 :
\bm{x}' \bm{x}^\text{T} = 0 ~\forall \bm{x} \in \mathcal{C}_2 \right\}
\bm{x}' \bm{x}^\mathsf{T} = 0 ~\forall \bm{x} \in \mathcal{C}_2 \right\}
,%
\end{align*}
we define $\bm{H}_X$ as the \ac{pcm} of $\mathcal{C}_2^\perp$ and $\bm{H}_Z$
@@ -1501,7 +1517,7 @@ In order to yield a valid stabilizer code, $\mathcal{C}_1$ and
$\mathcal{C}_2$ must satisfy the commutativity condition
\begin{align}
\label{eq:css_condition}
\bm{H}_X \bm{H}_Z^\text{T} = \bm{0}
\bm{H}_X \bm{H}_Z^\mathsf{T} = \bm{0}
.%
\end{align}
We can ensure this by choosing $\mathcal{C}_1$ and $\mathcal{C}_2$
@@ -1516,15 +1532,15 @@ such that $\mathcal{C}_2 \subset \mathcal{C}_1$.
Various methods of constructing \ac{qec} codes exist
\cite{swierkowska_eccentric_2025}.
Topological codes, for example, encode information in the features of
a lattice and are intrinsically robust against local errors.
a lattice in a way that allows for local interactions between qubits.
Among these, the \emph{surface code} is the most widely studied.
Another example are concatenated codes, which nest one code within
another, allowing for especially simple and flexible constructions
\cite[Sec.~3.2]{swierkowska_eccentric_2025}.
An area of research that has recently seen more attention is that of
quantum \ac{ldpc} (\acs{qldpc}) codes.
They have much better encoding efficiency than, e.g., the surface
code, scaling up of which would be prohibitively expensive
They have much higher rate than, e.g., surface codes, scaling up of
which would be prohibitively expensive
\cite[Sec.~I]{bravyi_high-threshold_2024}.
% Bivariate Bicycle codes
@@ -1536,7 +1552,7 @@ $\bm{H}_Z$ are constructed from two matrices $\bm{A}$ and $\bm{B}$ as
\begin{align*}
\bm{H}_X = [\bm{A} \vert \bm{B}]
\hspace*{5mm} \text{and} \hspace*{5mm}
\bm{H}_Z = [\bm{B}^\text{T} \vert \bm{A}^\text{T}]
\bm{H}_Z = [\bm{B}^\mathsf{T} \vert \bm{A}^\mathsf{T}]
.%
\end{align*}
This way, we can guarantee the satisfaction of the commutativity
@@ -1576,16 +1592,17 @@ This necessitates a modification of the standard \ac{bp} algorithm
introduced in \Cref{subsec:Iterative Decoding}
\cite[Sec.~3.1]{yao_belief_2024}.
Instead of attempting to find the most likely codeword directly, the
algorithm will now try to find an error pattern $\hat{\bm{e}} \in
\mathbb{F}_2^n$ that satisfies
syndrome-based decoding algorithm tries to find an error pattern
$\hat{\bm{e}} \in \mathbb{F}_2^n$ that satisfies
\begin{align*}
\bm{H} \hat{\bm{e}}^\text{T} = \bm{s}
\bm{H} \hat{\bm{e}}^\mathsf{T} = \bm{s}
.%
\end{align*}
To this end, we initialize the channel \acp{llr} as
\begin{align*}
\tilde{L}_i = \log{\frac{P(X_i = 0)}{P(X_i = 1)}} = \log{\frac{1
- p_i}{p_i}}
\tilde{L}_i = \log{\frac{P(X_i = 0)}{P(X_i = 1)}} = \log{
\left( \frac{1 - p_i}{p_i} \right)
}
,%
\end{align*}
where $p_i$ is the prior probability of error of \ac{vn} $i$.
@@ -1642,7 +1659,7 @@ The resulting syndrome-based \ac{bp} algorithm is shown in
\right\}$
\EndFor
\If{$\bm{H}\hat{\bm{e}}^\text{T} = \bm{s}$}
\If{$\bm{H}\hat{\bm{e}}^\mathsf{T} = \bm{s}$}
\State \textbf{break}
\EndIf
@@ -1721,7 +1738,7 @@ This way, we obtain the \ac{ler}.
\mathbbm{1}\left\{ L^\text{total}_i \right\}$
\EndFor
\If{$\bm{H}\hat{\bm{e}}^\text{T} = \bm{s}$}
\If{$\bm{H}\hat{\bm{e}}^\mathsf{T} = \bm{s}$}
\State \textbf{break}
\Else
\State $i_\text{max} \leftarrow \argmax_{i \in \mathcal{I}'} \lvert L^\text{total}_i \rvert $

View File

@@ -16,19 +16,19 @@ using qubits.
While the use of error correcting codes may facilitate this, it also
introduces two new challenges \cite[Sec.~4]{gottesman_introduction_2009}:
\begin{itemize}
\item For realizing a quantum algorithm, we must be able to
\item To realize a quantum algorithm, we must be able to
perform operations on the encoded state in such a way that we
do not lose the protection against errors.
\item \ac{qec} systems, in particular the syndrome extraction
circuit, are themselves partially implemented in
quantum hardware.
In addition to the errors we have originally introduced them
for, these systems must be able to account for the fact they
are implemented on noisy hardware themselves.
for, these systems must therefore be able to account for the
fact they are implemented on noisy hardware themselves.
\end{itemize}
In the literature, both of these points are viewed under the umbrella
of \emph{fault-tolerant} quantum computing.
In this thesis, we focus only on the second aspect.
In this thesis, we focus on the second aspect.
It was recognized early on as a challenge of \ac{qec} that the correction
machinery itself may introduce new faults \cite[Sec.~III]{shor_scheme_1995}.
@@ -670,7 +670,7 @@ extraction round.
\begin{figure}[t]
\begin{gather*}
\hspace*{-33.3mm}%
\hspace*{-31.8mm}%
\begin{array}{c}
E_6 \\
\downarrow
@@ -844,10 +844,10 @@ violate the same set of detectors, i.e.,
\begin{align*}
\hspace{-15mm}
% tex-fmt: off
&& \bm{H} \bm{e}_1^\text{T} & \neq \bm{H} \bm{e}_2^\text{T} \\
\iff \hspace{-33mm} && \bm{H} \left( \bm{e}_1 - \bm{e}_2 \right)^\text{T} & \neq 0 \\
\iff \hspace{-33mm} && \bm{D} \bm{\Omega} \left( \bm{e}_1 - \bm{e}_2 \right)^\text{T} & \neq 0 \\
\iff \hspace{-33mm} && \bm{\Omega} \left( \bm{e}_1 - \bm{e}_2 \right)^\text{T} & \notin \text{kern} \{\bm{D}\}
&& \bm{H} \bm{e}_1^\mathsf{T} & \neq \bm{H} \bm{e}_2^\mathsf{T} \\
\iff \hspace{-33mm} && \bm{H} \left( \bm{e}_1 - \bm{e}_2 \right)^\mathsf{T} & \neq 0 \\
\iff \hspace{-33mm} && \bm{D} \bm{\Omega} \left( \bm{e}_1 - \bm{e}_2 \right)^\mathsf{T} & \neq 0 \\
\iff \hspace{-33mm} && \bm{\Omega} \left( \bm{e}_1 - \bm{e}_2 \right)^\mathsf{T} & \notin \text{kern} \{\bm{D}\}
% tex-fmt: on
.%
\end{align*}
@@ -938,10 +938,10 @@ triggered the measurements in the syndrome extraction round immediately
afterwards, but all subsequent ones as well.
To only see the effect of errors in the syndrome measurement round
immediately following them, we consider our newly defined detectors
instead of the measurements, that effectively compute the difference
between the measurements.
instead of the measurements.
These effectively compute the difference between the measurements.
Hereby, each error can only trigger syndrome bits that follow it.
Each error can only trigger syndrome bits that follow it.
This is reflected in the triangular structure of $\bm{\Omega}$ in
\Cref{eq:syndrome_matrix_ex}.
Combining the measurements into detectors according to
@@ -1121,7 +1121,7 @@ In fact, it was in this tool that the concept of the \ac{dem} was
first introduced.
One capability of stim, and \acp{dem} in general, that we did not
explain in detail about in this chapter, is the merging of error mechanisms.
explain in detail in this chapter, is the merging of error mechanisms.
Since \acp{dem} differentiate errors based on their effect on the
measurements and not on their Pauli type and location
\cite[Sec.~1.4.3]{higgott_practical_2024}, it is natural to group

View File

@@ -470,7 +470,7 @@ model and is difficult to predict beforehand.
The block-diagonal structure reflects the time-like locality
of the syndrome extraction circuit, with each block
corresponding to one syndrome measurement round.
Two consecutive windows are highlighted: the window size $W
Two consecutive windows are highlighted: The window size $W
\in \mathbb{N}$ controls the number of syndrome rounds
included in each window, while the step size $F \in
\mathbb{N}$ controls how many rounds separate the start of
@@ -701,7 +701,7 @@ estimates committed after decoding window $\ell$, we have to set
\begin{align*}
\left(\bm{s}\right)_{\mathcal{J}_\text{overlap}^{(\ell)}} =
\bm{H}_\text{overlap}^{(\ell)}
\left( \hat{\bm{e}}_\text{commit}^{(\ell)} \right)^\text{T}
\left( \hat{\bm{e}}_\text{commit}^{(\ell)} \right)^\mathsf{T}
.%
\end{align*}
@@ -986,7 +986,7 @@ Note that the decoding procedure performed on the individual windows
\State $\displaystyle\left(\hat{\bm{e}}^\text{total}\right)_{\mathcal{I}^{(\ell)}_\text{commit}} \leftarrow \hat{\bm{e}}^{(\ell)}_\text{commit}$
\State $\displaystyle\left(\bm{s}\right)_{\mathcal{J}_\text{overlap}^{(\ell)}}
\leftarrow \bm{H}_\text{overlap}^{(\ell)}
\left( \hat{\bm{e}}_\text{commit}^{(\ell)} \right)^\text{T}$
\left( \hat{\bm{e}}_\text{commit}^{(\ell)} \right)^\mathsf{T}$
\If{$\ell < n_\text{win} - 1$}
\State $L^{(\ell+1)}_{i\leftarrow j} \leftarrow
L^{(\ell)}_{i\leftarrow j}
@@ -1013,8 +1013,8 @@ the most reliable \ac{vn}, meaning we perform a hard decision and
remove it from the following decoding process.
This means that when moving from one window to the next, we now have
more information available: not just the \ac{bp} messages but also the
information about what \acp{vn} were decimated and to what values.
more information available: Not just the \ac{bp} messages but also the
Information about what \acp{vn} were decimated and to what values.
We call this \emph{decimation information} in the following.
We can extend \Cref{alg:warm_start_bp} by additionally passing the
decimation information after initializing the \ac{cn} to \ac{vn} messages.
@@ -1184,7 +1184,7 @@ decimation information after initializing the \ac{cn} to \ac{vn} messages.
% \State $\displaystyle\left(\hat{\bm{e}}^\text{total}\right)_{\mathcal{I}^{(\ell)}_\text{commit}} \leftarrow \hat{\bm{e}}^{(\ell)}_\text{commit}$
% \State $\displaystyle\left(\bm{s}\right)_{\mathcal{J}_\text{overlap}^{(\ell)}}
% \leftarrow \bm{H}_\text{overlap}^{(\ell)}
% \left( \hat{\bm{e}}_\text{commit}^{(\ell)} \right)^\text{T}$
% \left( \hat{\bm{e}}_\text{commit}^{(\ell)} \right)^\mathsf{T}$
% \If{$\ell < n_\text{win} - 1$}
% \State $L^{(\ell+1)}_{i\leftarrow j} \leftarrow
% L^{(\ell)}_{i\leftarrow j}
@@ -1404,7 +1404,7 @@ The fact that the $W = 5$ curve is already very close to the
whole-block decoder indicates that the marginal benefit of enlarging
the window saturates after a certain point.
Thus, from a practical standpoint, the choice of $W$ represents a
trade-off between decoding latency and accuracy: larger windows
trade-off between decoding latency and accuracy: Larger windows
delay the start of decoding by requiring more syndrome extraction
rounds to be collected upfront, while the diminishing returns above
$W = 4$ suggest that growing the window much further yields little
@@ -1511,7 +1511,7 @@ The dashed colored curves reproduce the cold-start results from
corresponding warm-start runs for the same window sizes
$W \in \{3, 4, 5\}$.
The remaining experimental parameters are unchanged:
the step size is fixed to $F = 1$,
The step size is fixed to $F = 1$,
the inner \ac{bp} decoder is allowed up to $200$ iterations per
window invocation, the black curve again gives the whole-block
reference, and the physical error rate is swept from $p = 0.001$ to
@@ -1707,7 +1707,7 @@ $n_\text{iter} \in [32, 512]$.
All curves decrease monotonically with the iteration budget, but
contrary to our expectation, none of them appears to fully saturate
within the swept range: even at $n_\text{iter} = 4096$, every curve
within the swept range: Even at $n_\text{iter} = 4096$, every curve
still exhibits a noticeable downward slope.
At $n_\text{iter} = 32$, the whole-block curve lies below both the
$W=4$ and $W=5$ sliding-window curves.
@@ -1729,7 +1729,7 @@ mirroring the behavior already observed in \Cref{fig:whole_vs_cold_vs_warm}.
These observations are largely consistent with the effective-iterations
hypothesis put forward above.
The whole-block decoder eventually overtaking every windowed scheme
matches the prediction made there: with a sufficiently large
matches the prediction made there: With a sufficiently large
iteration budget, the whole-block decoder reaches an error rate
that none of the windowed schemes can beat, because of the more global
nature of the considered constraints.
@@ -1767,7 +1767,7 @@ sliding-window approach is still at an advantage.
Having examined the effect of the window size $W$, we next turn to
the second windowing parameter, the step size $F$.
We carry out an investigation analogous to the one above:
we first compare warm- and cold-start decoding across the full range
We first compare warm- and cold-start decoding across the full range
of physical error rates at a fixed iteration budget, and then we
examine the dependence on the iteration budget at a fixed physical
error rate.
@@ -1994,7 +1994,7 @@ At fixed $F$, the warm-start approach lies below
cold-start across the entire sweep, and at fixed
warm or cold start, smaller $F$ produces a lower \ac{ler}.
Both gaps grow as the physical error rate decreases:
the curves at $F = 1$ separate further from those at $F = 2$ and $F = 3$,
The curves at $F = 1$ separate further from those at $F = 2$ and $F = 3$,
and the warm-start curves separate further from the cold-start ones.
In \Cref{fig:bp_f_over_iter}, all six curves again decrease
monotonically with the iteration budget, with no clear saturation
@@ -2016,7 +2016,7 @@ With $W$ held fixed, decreasing $F$ enlarges the overlap between
consecutive windows from $W - F$ to $W - F + 1$ syndrome measurement rounds, so
a smaller step size is beneficial for the same reason that a larger
window size is:
each \ac{vn} in an overlap region participates in more window
Each \ac{vn} in an overlap region participates in more window
invocations, and the warm-start modification effectively accumulates
iterations on it across these invocations.
The widening of the warm/cold gap towards low iteration counts and
@@ -2281,7 +2281,7 @@ This is the opposite of what we observed for plain \ac{bp}, where
warm-start improved upon cold-start at every parameter setting.
The gap between the warm- and cold-start curves additionally widens
as the physical error rate decreases:
at the lowest sampled rate $p = 0.001$, the per-round \ac{ler} of the
At the lowest sampled rate $p = 0.001$, the per-round \ac{ler} of the
warm-start runs is more than two orders of magnitude above that of
the corresponding cold-start runs.
In \Cref{fig:bpgd_w}, larger window sizes yield lower per-round
@@ -2300,13 +2300,13 @@ than its cold-start counterpart is surprising in light of the results
for plain \ac{bp}, where the warm-start modification was uniformly beneficial.
The dependence on the window size in \Cref{fig:bpgd_w} is, on its own,
consistent with the same explanation that we gave for
\Cref{fig:whole_vs_cold}: larger windows expose the inner decoder to
\Cref{fig:whole_vs_cold}: Larger windows expose the inner decoder to
a larger fraction of the constraints encoded in the detector error
matrix at the time of decoding, and this benefits both warm- and
cold-start decoding.
The dependence on the step size in \Cref{fig:bpgd_f}, however, is the
opposite of the corresponding dependence under plain \ac{bp}
(\Cref{fig:bp_f_over_p}): for warm-start, smaller $F$ now degrades performance
(\Cref{fig:bp_f_over_p}): For warm-start, smaller $F$ now degrades performance
rather than helps, even though smaller $F$ implies a larger overlap
in both cases.
@@ -2564,7 +2564,7 @@ the warm-start curves now show a clear reordering as $n_\text{iter}$
grows.
At low iteration budgets the warm-start ordering matches the
cold-start ordering, with $F = 1$ best and $F = 3$ worst, but at the
largest iteration budget this ordering is fully inverted: warm-start
largest iteration budget this ordering is fully inverted: Warm-start
$F = 1$ is now the worst and $F = 3$ the best.
% [Interpretation] Figure 4.11
@@ -2596,7 +2596,7 @@ decoding performance.
The same mechanism explains the inversion of the step-size ordering
in \Cref{fig:bpgd_iter_F}.
At low iteration budgets, the ordering is set by the same overlap
argument as for plain \ac{bp}: smaller $F$ implies a larger overlap
argument as for plain \ac{bp}: Smaller $F$ implies a larger overlap
between consecutive windows, more shared messages, and therefore
better warm-start performance.
At large iteration budgets, the ordering is set by the premature hard
@@ -2777,7 +2777,7 @@ since the decimation decisions were made based on the messages themselves.
\Cref{fig:bpgd_msg} repeats the experiment of \Cref{fig:bpgd_wf}
with the modified warm-start procedure that carries over only the
\ac{bp} messages.
All other experimental parameters are unchanged: the maximum number
All other experimental parameters are unchanged: The maximum number
of inner \ac{bp} iterations is $n_\text{iter} = 5000$, and the
physical error rate is swept from $p = 0.001$ to $p = 0.004$ in steps
of $0.0005$.
@@ -2810,7 +2810,7 @@ the warm-start regression observed in \Cref{fig:bpgd_wf},
and warm-start now consistently outperforms cold-start.
The dependence on the window size and the step size also recovers
the qualitative behavior we observed for plain \ac{bp} in
\Cref{fig:whole_vs_cold_vs_warm,fig:bp_f_over_p}: a larger overlap
\Cref{fig:whole_vs_cold_vs_warm,fig:bp_f_over_p}: A larger overlap
between consecutive windows, achieved either by enlarging $W$ or by
decreasing $F$, both improves the absolute decoding performance and
increases the warm-start advantage over cold-start.
@@ -2994,7 +2994,7 @@ cold-start curves across the entire range of $n_\text{iter}$ available to us.
\Cref{fig:bpgd_msg_iter} repeats the experiment of
\Cref{fig:bpgd_iter} with the modified warm-start procedure that
carries over only the \ac{bp} messages.
All other experimental parameters are unchanged: the physical error
All other experimental parameters are unchanged: The physical error
rate is fixed at $p = 0.0025$ and the iteration budget is swept over
$n_\text{iter} \in \{32, 128, 256, 512, 1024, 1536, 2048, 2560,
3072, 3584, 4096\}$.
@@ -3026,7 +3026,7 @@ initialization no longer freezes any \acp{vn} in the next window.
The dependence of this benefit on $W$ and $F$ also recovers the
pattern observed for plain \ac{bp} in
\Cref{fig:whole_vs_cold_vs_warm,fig:bp_f_over_p}:
larger overlap, achieved by larger $W$ or smaller $F$, yields more
Larger overlap, achieved by larger $W$ or smaller $F$, yields more
effective extra iterations and therefore a larger warm-start gain.
% BPGD conclusion
@@ -3048,7 +3048,7 @@ cold-start that follows the same behavior as for plain \ac{bp} with
regard to overlap.
A second observation specific to \ac{bpgd} is that its iteration
requirements are substantially larger than those of plain \ac{bp}:
the per-round \ac{ler} drops sharply only once the iteration budget
The per-round \ac{ler} drops sharply only once the iteration budget
is on the order of the number of \acp{vn} in each window.
Future work could include a softer treatment of the decimation state

View File

@@ -7,7 +7,7 @@ This thesis investigates decoding under \acp{dem} for fault-tolerant
\ac{qec}, with a focus on low-latency decoding methods for \ac{qldpc} codes.
The repetition of the syndrome measurements, especially under
consideration of circuit-level noise, leads to a significant increase
in decoding complexity: in our experiments on the $\llbracket
in decoding complexity: In our experiments on the $\llbracket
144,12,12 \rrbracket$ \ac{bb} code with $12$ syndrome extraction
rounds, the check matrix grows from 144 \acp{vn} and 72
\acp{cn} to 9504 \acp{vn} and 1008 \acp{cn}.
@@ -46,18 +46,18 @@ min-sum algorithm.
For standard min-sum \ac{bp}, the warm start is consistently
beneficial to the cold start, across the considered parameter ranges.
The size of the gain depends on the overlap between consecutive
windows: enlarging $W$ or shrinking $F$, both of which enlarge the
windows: Enlarging $W$ or shrinking $F$, both of which enlarge the
overlap, result in larger gains of the warm-start.
We observe that the underlying mechanism is an effective increase in
the number of \ac{bp} iterations spent on the \acp{vn} in the overlap
region: each such \ac{vn} is processed by multiple consecutive window
region: Each such \ac{vn} is processed by multiple consecutive window
invocations, and the warm start lets these invocations accumulate
iterations on the same \acp{vn} rather than restarting from scratch.
The gain was most pronounced at low numbers of maximum iterations, where
every additional iteration carries proportionally more information.
For \ac{bpgd}, we note that more information is available in the
overlap region of a window: in addition to the \ac{bp} messages,
overlap region of a window: In addition to the \ac{bp} messages,
there is information about which \acp{vn} were decimated and to what value.
Passing this decimation information to the next window in addition to
the messages turned out to worsen the performance considerably, which
@@ -66,7 +66,7 @@ overlap region.
Restricting the warm start to the \ac{bp} messages alone, removed this effect.
The resulting message-only warm start recovered a consistent
improvement over cold-start that followed the same qualitative
behaviour as for standard \ac{bp}: larger overlap, achieved by larger
behaviour as for standard \ac{bp}: Larger overlap, achieved by larger
$W$ or smaller $F$, yielded a larger gain, and the
performance difference is most pronounced at low numbers of maximum iterations.

View File

@@ -49,7 +49,7 @@ For both standard \ac{bp} and \ac{bpgd} decoding, the warm-start
initialization provides a consistent improvement across all examined
parameter settings.
We attribute this to an effective increase in \ac{bp} iterations on
variable nodes in the overlap regions: each such VN is processed by
variable nodes in the overlap regions: Each such VN is processed by
multiple consecutive windows, and warm-starting lets these
invocations accumulate iterations rather than restart from scratch.
Crucially, the warm-start modification incurs no additional

View File

@@ -91,9 +91,9 @@
%\thesisHeadOfInstitute{Prof. Dr.-Ing. Peter Rost\\Prof. Dr.-Ing.
% Laurent Schmalen}
\thesisSupervisor{Dr.-Ing. Hedongliang Liu\\ && M.Sc. Jonathan Mandelbaum}
\thesisStartDate{01.11.2025}
\thesisEndDate{04.05.2026}
\thesisSignatureDate{04.05.2026}
\thesisStartDate{Nov. 1st, 2025}
\thesisEndDate{May 4th, 2026}
\thesisSignatureDate{May 4th, 2026}
\thesisSignature{res/Unterschrift_AT_blue.png}
\thesisSignatureHeight{2.4cm}
\thesisLanguage{english}
@@ -109,9 +109,11 @@
\cleardoublepage
\pagenumbering{arabic}
\newgeometry{a4paper,left=3cm,right=3cm,top=2cm,bottom=2.5cm}
\addtocontents{toc}{\protect\vspace*{-9mm}}
\tableofcontents
\cleardoublepage
\restoregeometry
\input{chapters/1_introduction.tex}
\input{chapters/2_fundamentals.tex}
@@ -124,10 +126,10 @@
% \listoftables
% \include{abbreviations}
% \cleardoublepage
% \phantomsection
% \addcontentsline{toc}{chapter}{List of Abbreviations}
% \printacronyms
\cleardoublepage
\phantomsection
\addcontentsline{toc}{chapter}{List of Abbreviations}
\printacronyms
\bibliography{lib/cel-thesis/IEEEabrv,src/thesis/bibliography}