Linear systems of equations are the basic tool in NLA.
They appear as:
From school we know about linear equations.
A linear system of equations can be written in the form
\begin{align*} &2 x + 3 y = 5\quad &\longrightarrow \quad &2x + 3 y + 0 z = 5\\ &2 x + 3z = 5\quad &\longrightarrow\quad &2 x + 0 y + 3 z = 5\\ &x + y = 2\quad &\longrightarrow\quad & 1 x + 1 y + 0 z = 2\\ \end{align*}
$$ \begin{pmatrix} 2 & 3 & 0 \\ 2 & 0 & 3 \\ 1 & 1 & 0 \\ \end{pmatrix}\begin{pmatrix} x \\ y \\ z \end{pmatrix} = \begin{pmatrix} 5 \\ 5 \\ 2 \end{pmatrix} $$ or simply $$ A u = f, $$
where $A$ is a $3 \times 3$ matrix and $f$ is right-hand side
If the system $Au = f$ has
more equations than unknowns it is called overdetermined system (generically, no solution)
less equations than unknowns it is called underdetermined system (solution is non-unique, to make it unique additional assumptions have to be made)
A solution to the linear system of equations with a square matrix $A$
$$A u = f$$
exists, iff
or
In different applications, the typical size of the linear systems can be different.
We take a continious problem, discretize it on a mesh with $N$ elements and get a linear system with $N\times N$ matrix.
Example of a mesh around A319 aircraft
(taken from GMSH website).
The main difficulty is that these systems are big: millions or billions of unknowns!
Q: how to work with such matrices?
A: fortunately, those matrices are structured and require $\mathcal{O}(N)$ parameters to be stored.
The most widespread structure are sparse matrices: such matrices have only $\mathcal{O}(N)$ non-zeros!
Example (one of the famous matrices around for $n = 5$):
$$ \begin{pmatrix} 2 & -1 & 0 & 0 & 0 \\ -1 & 2 & -1 & 0 & 0 \\ 0 & -1 & 2 & -1 & 0 \\ 0 & 0 &-1& 2 & -1 \\ 0 & 0 & 0 & -1 & 2 \\ \end{pmatrix} $$
Important: forget about determinants and the Cramer rule (it is good for $2 \times 2$ matrices still)!
The main tool is variable elimination.
\begin{align*} &2 y + 3 x = 5 \quad&\longrightarrow \quad &y = 5/2 - 3/2 x \\ &2 x + 3z = 5 \quad&\longrightarrow\quad &z = 5/3 - 2/3 x\\ &x + y = 2 \quad&\longrightarrow\quad & 5/2 + 5/3 - (3/2 + 2/3) x = 2,\\ \end{align*}
and that is how you find $x$ (and all previous ones).
This process is called Gaussian elimination and is one of the most widely used algorithms.
$$ x_1 = f_1 - (a_{12} x_2 + \ldots + a_{1n} x_n)/a_{11}, $$
and then substitute this into the equations $2, \ldots, n$.
Then we eliminate $x_2$ and so on from the second equation.
The important thing is that the pivots (that we divide over) are not equal to $0$.
In the backward step:
Gaussian elimination is the computation of one of the most important matrix decompositions: LU-decomposition.
Definition: LU-decomposition of the square matrix $A$ is the representation
$$A = LU,$$
where $L$ is lower triangular and $U$ is upper triangular matrix (i.e. elements strictly above the diagonal are zero, elements strictly below the diagonal are zero)
This factorization is non-unique, so it is typical to require that the matrix $L$ has ones on the diagonal.
Main goal of the LU decomposition is to solve linear system, because
$$ A^{-1} f = (L U)^{-1} f = U^{-1} L^{-1} f, $$
and this reduces to the solution of two linear systems forward step $$ L y = f, $$ and backward step $$ U x = y. $$
Does $LU$ decomposition always exist?
Each elimination step requires $\mathcal{O}(n^2)$ operations.
Thus, the cost of the naive algorithm is $\mathcal{O}(n^3)$.
Think a little bit: Can Strassen algorithm help here?
We can try to compute block version of LU-decomposition:
$$\begin{pmatrix} A_{11} & A_{12} \\ A_{21} & A_{22} \end{pmatrix} = \begin{pmatrix} L_{11} & 0 \\ L_{21} & L_{22} \end{pmatrix} \begin{pmatrix} U_{11} & U_{12} \\ 0 & U_{22} \end{pmatrix} $$
There are two basic operations: compute LU-factorization of half-matrices + matrix-by-matrix product.
The LU-decomposition algorithm does not fail
if we do not divide by zero at every step of the Gaussian elimination.
Q: when it is so, for which class of matrices?
A: it is true for strictly regular matrices.
Definition. A matrix $A$ is called strictly regular, if all of its principal minors (i.e, submatrices in the first $k$ rows and $k$ columns) are non-singular.
In this case, there always exists an LU-decomposition. The reverse is also true (check!).
Proof. If there is an LU-decomposition, then the matrix is strictly regular
This follows from the fact that to get a minor you multiply a corresponding submatrix of $L$ by a corresponding submatrix of $U$,
and they are non-singular (since non-singularity of triangular matrices is equivalent to the fact that their diagonal elements are not equal to zero).
The other way can be proven by induction. Suppose that we know that for all $(n-1) \times (n-1)$ matrices will non-singular minors LU-decomposition exists.
Then, consider the block form $$ A = \begin{pmatrix} a & c^{\top} \\ b & D \end{pmatrix}, $$ where $D$ is $(n-1) \times (n-1)$.
Then we do "block elimination":
$$ \begin{pmatrix} 1 & 0 \\ -z & I \end{pmatrix} \begin{pmatrix} a & c^{\top} \\ b & D \end{pmatrix}= \begin{pmatrix} a & c^{\top} \\ 0 & A_1 \end{pmatrix}, $$
where $z = \frac{b}{a}, \quad A_1 = D - \frac{1}{a} b c^{\top}$.
We can show that $A_1$ is also strictly regular, thus it has (by induction) the LU-decomposition:
$$
A_1 = L_1 U_1,
$$
And that gives the $LU$ decomposition of the original matrix.
Corollary: If $L$ is unit triangular (ones on the diagonal), then $LU$-decomposition is unique.
Proof: Indeed, $L_1 U_1 = L_2 U_2$ means $L_2^{-1} L_1 = U_2 U_1^{-1}$. $L_2^{-1} L_1 $ is lower triangular with ones on the diagonal. $U_2 U_1^{-1}$ is upper triangular. Thus, $L_2^{-1} L_1 = U_2 U_1^{-1} = I$ and $L_1 = L_2$, $U_1 = U_2$.
Strictly regular matrices have LU-decomposition.
An important subclass of strictly regular matrices is the class of Hermitian positive definite matrices
Definition. A matrix $A$ is called positive definite if for any $x: \Vert x \Vert \ne 0$ we have
$$ (x, Ax) > 0. $$
Claim: A Hermitian positive definite matrix $A$ is strictly regular and has Cholesky factorization of the form
$$A = RR^*,$$
where $R$ is a lower triangular matrix.
Let us try to prove this fact (on the whiteboard).
It is sometimes referred to as "square root" of the matrix.
In many cases, computing LU-decomposition once is a good idea!
Once the decomposition is found (it is $\mathcal{O}(n^3)$), then solving linear systems with $L$ and $U$ costs only $\mathcal{O}(n^2)$ operations.
Check: Solving linear systems with triangular matrices is easy (why?). How we compute the $L$ and $U$ factors?
What happens, if the matrix is not strictly regular (or the pivots in the Gaussian elimination are really small?).
There is classical $2 \times 2$ example of a matrix with a bad LU decomposition.
The matrix we look at is
$$ A = \begin{pmatrix} \varepsilon & 1 \\ 1 & 1 \end{pmatrix} $$
Let us do some demo here.
import numpy as np
eps = 1e-18#1.12e-16
a = [[eps, 1],[1.0, 1]]
a = np.array(a)
a0 = a.copy()
n = a.shape[0]
L = np.zeros((n, n))
U = np.zeros((n, n))
for k in range(n): #Eliminate one row
L[k, k] = 1
for i in range(k+1, n):
L[i, k] = a[i, k] / a[k, k]
for j in range(k+1, n):
a[i, j] = a[i, j] - L[i, k] * a[k, j]
for j in range(k, n):
U[k, j] = a[k, j]
print('L * U - A:\n', np.dot(L, U) - a0)
L
L * U - A: [[ 0.00000000e+00 0.00000000e+00] [-1.11022302e-16 -1.00000000e+00]]
array([[1.e+00, 0.e+00], [1.e+18, 1.e+00]])
We can do pivoting, i.e. permute rows and columns to maximize $A_{kk}$ that we divide over.
The simplest but effective strategy is the row pivoting: at each step, select the index that is maximal in modulus, and put it onto the diagonal.
It gives us the decomposition
$$A = P L U,$$ where $P$ is a permutation matrix.
What makes row pivoting good?
It is made good by the fact that
$$ | L_{ij}|<1, $$ but the elements of $U$ can grow, up to $2^n$! (in practice, this is very rarely encountered).
Can you come up with a matrix where the elements of $U$ grow as much as possible?
There is a fundamental problem of solving linear systems which is independent on the algorithm used.
It occures when elements of a matrix are represented as floating point numbers or there is some measurement noise.
Let us illustrate this issue on the following example.
import numpy as np
import matplotlib.pyplot as plt
%matplotlib inline
import seaborn as sns
sns.set_style("whitegrid")
sns.set_context("talk")
n = 15
a = [[1.0/(i + j + 1) for i in range(n)] for j in range(n)]
a = np.array(a)
rhs = np.random.randn(n) #Right-hand side
x = np.linalg.solve(a, rhs) #This function computes LU-factorization and solves linear system
#And check if everything is fine
er = np.linalg.norm(a.dot(x) - rhs) / np.linalg.norm(rhs)
print(er)
plt.plot(x)
0.36794870513685535
[<matplotlib.lines.Line2D at 0x1a1d986208>]
As you see, the error grows with larger $n$, and we have to find out why.
Important point is that it is not a problem of the algorithm: it is a problem of representing
the matrix in the memory. The error occurs in the moment when the matrix elements are evaluated approximately.
What was the problem in the previous example?
Why the error grows so quickly?
And here is one of the main concepts of numerical linear algebra: the concept of condition number of a matrix.
But before that we have to define the inverse.
The inverse of a matrix $A$ is defined as a matrix $X$ denoted by $A^{-1}$ such that
$$ AX = XA = I, $$
where $I$ is the identity matrix (i.e., $I_{ij} = 0$ if $i \ne j$ and $1$ otherwise).
The computation of the inverse is linked to the solution of linear systems. Indeed, $i$-th column of the product gives
$$
A x_i = e_i,
$$
where $e_i$ is the $i$-th column of the identity matrix. Thus, we can apply Gaussian elimination to solve this system. Moreover, if there are no divisions by zero in this process (and the pivots do not depend on the right-hand side), then it is possible to solve the system.
If we have computed $A^{-1}$, the solution of linear system
$$Ax = f$$
is just $x = A^{-1} f$.
Indeed,
$$ A(A^{-1} f) = (AA^{-1})f = I f = f. $$
To study, why there can be such big errors in a solution (see the example above on the Hilbert matrix) we need an important auxiliary result.
Neumann series:
If matrix $F$ is such that $\Vert F \Vert < 1$ holds, then the matrix $(I - F)$ is invertible and
$$(I - F)^{-1} = I + F + F^2 + F^3 + \ldots = \sum_{k=0}^{\infty} F^k.$$
Note that it is a matrix version of the geometric progression.
Question: What norm is considered here? What is the "best possible" norm here?
The proof is constructive. First of all, prove that the series $\sum_{k=0}^{\infty} F^k$ converges.
Like in the scalar case, we have
$$
(I - F) \sum_{k=0}^N F^k = (I - F^{N+1}) \rightarrow I, \quad N \to +\infty
$$
Indeed, $$ \| (I - F^{N+1}) - I\| = \|F^{N+1}\| \leqslant \|F\|^{N+1} \to 0, \quad N\to +\infty. $$
We can also estimate the norm of the inverse: $$ \left\Vert \sum_{k=0}^N F^k \right\Vert \leq \sum_{k=0}^N \Vert F \Vert^k \Vert I \Vert \leq \frac{\Vert I \Vert}{1 - \Vert F \Vert} $$
Using this result, we can estimate, how the perturbation of the matrix influences the inverse matrix. We assume that the perturbation $E$ is small in the sense that $\Vert A^{-1} E \Vert < 1$. Then $$(A + E)^{-1} = \sum_{k=0}^{\infty} (-A^{-1} E)^k A^{-1}$$ and moreover, $$ \frac{\Vert (A + E)^{-1} - A^{-1} \Vert}{\Vert A^{-1} \Vert} \leq \frac{\Vert A^{-1} \Vert \Vert E \Vert \Vert I \Vert}{1 - \Vert A^{-1} E \Vert}. $$ As you see, the norm of the inverse enters the estimate.
Now consider the perturbed linear system: $$ (A + \Delta A) \widehat{x} = f + \Delta f. $$
$$
\begin{split}
\widehat{x} - x &= (A + \Delta A)^{-1} (f + \Delta f) - A^{-1} f =\\
&= \left((A + \Delta A)^{-1} - A^{-1}\right)f + (A + \Delta A)^{-1} \Delta f = \\
&= \Big[\sum_{k=0}^{\infty} (-A^{-1} \Delta A)^k\Big] A^{-1} f + \Big[\sum_{k=0}^{\infty} (A^{-1} \Delta A)^k \Big] A^{-1} \Delta f,
\end{split}
$$
therefore
$$
\begin{split}
\frac{\Vert \widehat{x} - x \Vert}{\Vert x \Vert} \leq
&\frac{\Vert A \Vert \Vert A^{-1} \Vert}{1 - \|A^{-1}\Delta A\|} \Big(\frac{\Vert\Delta A\Vert}{\Vert A \Vert} + \frac{\Vert \Delta f \Vert}{ \Vert f \Vert}\Big) \leq \\
\leq
&\frac{\Vert A \Vert \Vert A^{-1} \Vert}{1 - \|A\|\|A^{-1}\|\frac{\|\Delta A\|}{\|A\|}} \Big(\frac{\Vert\Delta A\Vert}{\Vert A \Vert} + \frac{\Vert \Delta f \Vert}{ \Vert f \Vert}\Big) \equiv \\
\equiv &\frac{\mathrm{cond}(A)}{1 - \mathrm{cond}(A)\frac{\|\Delta A\|}{\|A\|}} \Big(\frac{\Vert\Delta A\Vert}{\Vert A \Vert} + \frac{\Vert \Delta f \Vert}{ \Vert f \Vert}\Big)
\end{split}
$$
The crucial role is played by the condition number $\mathrm{cond}(A) = \Vert A \Vert \Vert A^{-1} \Vert$.
The larger the condition number, the less number of digits we can recover. Note, that the condition number is different for different norms.
Note, that if $\Delta A = 0$, then $$ \frac{\Vert \widehat{x} - x \Vert}{\Vert x \Vert} \leq \mathrm{cond}(A) \frac{\|\Delta f\|}{\|f\|} $$
The spectral norm of the matrix is equal to largest singular value, and the singular values of the inverse matrix are equal to the inverses of the singular values. Thus, the condition number is equal to the ratio of the largest singular value and the smallest singular value. $$ \mathrm{cond}_2 (A) = \|A\|_2 \|A^{-1}\|_2 = \frac{\sigma_{\max}}{\sigma_{\min}} $$
We can also try to test how tight is the estimate, both with ones in the right-hand side, and with a random vector in the right-hand side. The results are strickingly different
import numpy as np
import matplotlib.pyplot as plt
%matplotlib inline
n = 1000
a = [[1.0/(i + j + 1) for i in range(n)] for j in range(n)]
a = np.array(a)
rhs = np.ones(n) #Right-hand side
f = np.linalg.solve(a, rhs)
#And check if everything is fine
er = np.linalg.norm(a.dot(f) - rhs) / np.linalg.norm(rhs)
cn = np.linalg.cond(a, 2)
print('Error:', er, 'Condition number:', cn)
Error: 2.217472233227586e-06 Condition number: 4.492167979846466e+20
And with random right-hand side...
import numpy as np
import matplotlib.pyplot as plt
%matplotlib inline
n = 100
a = [[1.0/(i + j + 1) for i in range(n)] for j in range(n)]
a = np.array(a)
rhs = np.random.randn(n) #Right-hand side
f = np.linalg.solve(a, rhs)
#And check if everything is fine
er = np.linalg.norm(a.dot(f) - rhs) / np.linalg.norm(rhs)
cn = np.linalg.cond(a)
print('Error:', er, 'Condition number:', cn)
u, s, v = np.linalg.svd(a)
rhs = np.random.randn(n)
plt.plot(u.T.dot(rhs))
Error: 9.745096544698619 Condition number: 4.073996146476839e+19
[<matplotlib.lines.Line2D at 0x1a1e27a278>]
Can you think about an explanation?
Important class of problems are overdetermined linear systems, when the number of equations is greater, than the number of unknowns. The simplest example that you all know, is linear fitting, fitting a set of 2D points by a line.
Then, a typical way is to minimize the residual (least squares)
$$\Vert A x - b \Vert_2 \rightarrow \min$$
The optimality condition is $0\equiv \nabla \left(\|Ax-b\|_2^2\right)$, where $\nabla$ denotes gradient. Therefore,
$$ 0 \equiv \nabla \left(\|Ax-b\|_2^2\right) = 2(A^*A x - A^*b) = 0. $$
Thus, $$ \quad A^* A x = A^* b $$ The matrix $A^* A$ is called Gram matrix and the system is called normal equation.
This is not a good way to do it, since the condition number of $A^* A$ is a square of condition number of $A$ (check why).
Matrix $A^* A$ can be singular in general case.
Therefore, we need to introduce the concept of pseudoinverse matrix $A^{\dagger}$ such that
solution to the linear least squares problem can formally be written as
$$x = A^{\dagger} b.$$
The matrix $$A^{\dagger} = \lim_{\alpha \rightarrow 0}(\alpha I + A^* A)^{-1} A^*$$ is called Moore-Penrose pseudoinverse of the matrix $A$.
If matrix $A$ has full column rank, then $A^* A$ is non-singular and we get $A^{\dagger} = \lim_{\alpha \rightarrow 0}(\alpha I + A^* A)^{-1} A^* = (A^* A)^{-1} A^*$.
If matrix $A$ is squared and non-singular we get $A^{\dagger} = \lim_{\alpha \rightarrow 0}(\alpha I + A^* A)^{-1} A^* = (A^* A)^{-1} A^* = A^{-1} A^{-*} A^* = A^{-1}$ - standard inverse of $A$
If $A$ has linearly dependent columns, then $A^\dagger b$ gives solution that has minimal Euclidean norm
Let $A = U \Sigma V^*$ be the SVD of $A$. Then,
$$A^{\dagger} = V \Sigma^{\dagger} U^*,$$
where $\Sigma^{\dagger}$ consists of inverses of non-zero singular values of $A$. Indeed,
$$A^{\dagger} = \lim_{\alpha \rightarrow 0}(\alpha I + A^* A)^{-1} A^* = \lim_{\alpha \rightarrow 0}( \alpha VV^* + V \Sigma^2 V^*)^{-1} V \Sigma U^* = \lim_{\alpha \rightarrow 0}( V(\alpha I + \Sigma^2) V^*)^{-1} V \Sigma U^* = V \lim_{\alpha \rightarrow 0}(\alpha I + \Sigma^2)^{-1} \Sigma U^* = V \Sigma^{\dagger} U^*,$$
Is to use the $QR$ decomposition.
Any matrix can be factored into a product
$$ A = Q R, $$ where $Q$ is unitary, and $R$ is upper triangular (details in the next lectures).
Then, if $A$ has full column rank, then
$$ x = A^{\dagger}b = (A^*A)^{-1}A^*b = ((QR)^*(QR))^{-1}(QR)^*b = (R^*Q^*QR)^{-1}R^*Q^*b = R^{-1}Q^*b. $$ Thus, finding optimal $x$ is equivalent to solving
$$ Rx = Q^* b. $$
Since $R$ is upper triangular, the solving of this linear system costs $\mathcal{O}(n^2)$. Also it is more stable, than using the pseudo-inverse matrix directly.
Instead of solving $A^* A x = A^* b$,
we introduce a new variable $r = Ax - b$ and then have
$$A^* r = 0, \quad r = Ax - b,$$
or in the block form
$$ \begin{pmatrix} 0 & A^* \\ A & -I \end{pmatrix} \begin{pmatrix} x \\ r \end{pmatrix} = \begin{pmatrix} 0 \\ b \end{pmatrix}, $$
the total size of the system is $(n + m)$ square, and the condition number is the same as for $A$ (by the way, how we define the condition number of a rectangular matrix?)
Consider a two-dimensional example. Suppose we have a linear model $$y = ax + b$$ and noisy data $(x_1, y_1), \dots (x_n, y_n)$. Then the linear system on coefficients will look as follows $$ \begin{split} a x_1 &+ b &= y_1 \\ &\vdots \\ a x_n &+ b &= y_n \\ \end{split} $$ or in a matrix form $$ \begin{pmatrix} x_1 & 1 \\ \vdots & \vdots \\ x_n & 1 \\ \end{pmatrix} \begin{pmatrix} a \\ b \end{pmatrix} = \begin{pmatrix} y_1 \\ \vdots \\ y_n \\ \end{pmatrix}, $$ which represents overdetermined system.
%matplotlib inline
import numpy as np
import matplotlib.pyplot as plt
a_exact = 1.
b_exact = 2.
n = 10
xi = np.arange(n)
yi = a_exact * xi + b_exact + 2*np.random.random(n)
A = np.array([xi, np.ones(n)])
coef = np.linalg.pinv(A).T.dot(yi) # coef is [a, b]
plt.plot(xi, yi, 'o', label='$(x_i, y_i)$')
plt.plot(xi, coef[0]*xi + coef[1], label='Least Squares')
plt.legend(loc='best')
<matplotlib.legend.Legend at 0x1a1e5d7a20>
A typical 3D-problem requires a $100 \times 100 \times 100$ discretization
This gives a linear system with $10^6$ unknowns, right-hand side takes $8$ megabytes of memory
This matrix has $10^6 \times 10^6 = 10^{12}$ elements, takes $8$ terabytes of memory.
Fortunately, the matrices in real-life are not dense, but have certain structure: