# Conditioning of linear systems

## Contents

# 2.8. Conditioning of linear systems#

We are ready to consider the conditioning of solving the square linear system \(\mathbf{A}\mathbf{x}=\mathbf{b}\). In this problem, the data are \(\mathbf{A}\) and \(\mathbf{b}\), and the solution is \(\mathbf{x}\). Both data and result are multidimensional, so we will use norms to measure their magnitudes.

The motivation for the definition of relative condition number in Chapter 1 was to quantify the response of the result to perturbations of the data. For simplicity, we start by allowing perturbations to \(\mathbf{b}\) only while \(\mathbf{A}\) remains fixed.

Let \(\mathbf{A}\mathbf{x}=\mathbf{b}\) be perturbed to

The condition number should be the relative change in the solution divided by relative change in the data,

We can bound \(\| \mathbf{h} \|\) in terms of \(\| \mathbf{d} \|\):

where we have applied \(\mathbf{A}\mathbf{x}=\mathbf{b}\) and (2.7.6). Since also \(\mathbf{b}=\mathbf{A}\mathbf{x}\) implies \(\| \mathbf{b} \|\le \| \mathbf{A} \|\, \| \mathbf{x} \|\), we derive

It is possible to show that this bound is tight, in the sense that the inequalities are in fact equalities for some choices of \(\mathbf{b}\) and \(\mathbf{d}\). This result motivates a new definition.

The **matrix condition number** of an invertible square matrix \(\mathbf{A}\) is

This value depends on the choice of norm; a subscript on \(\kappa\) such as \(1\), \(2\), or \(\infty\) is used if clarification is needed. If \(\mathbf{A}\) is singular, we define \(\kappa(\mathbf{A}) = \infty\).

## Main result#

The matrix condition number (2.8.1) is equal to the condition number of solving a linear system of equations. Although we derived this fact above only for perturbations of \(\mathbf{b}\), a similar statement holds when \(\mathbf{A}\) is perturbed.

Using a traditional \(\Delta\) notation for the perturbation in a quantity, we can write the following.

If \(\mathbf{A}(\mathbf{x} + \Delta \mathbf{x}) = \mathbf{b} + \Delta \mathbf{b}\), then

If \((\mathbf{A}+\Delta \mathbf{A}) (\mathbf{x} + \Delta \mathbf{x}) = \mathbf{b}\), then

in the limit \(\| \Delta \mathbf{A} \| \to 0\).

Note that for any induced matrix norm,

A condition number of 1 is the best we can hope for—in that case, the relative perturbation of the solution has the same size as that of the data. A condition number of size \(10^t\) indicates that in floating-point arithmetic, roughly \(t\) digits are lost (i.e., become incorrect) in computing the solution \(\mathbf{x}\). And if \(\kappa(\mathbf{A}) > \epsilon_\text{mach}^{-1}\), then for computational purposes the matrix is effectively singular.

```
A = [ 1/(i+j) for i in 1:6, j in 1:6 ]
κ = cond(A)
```

```
5.109816296610315e7
```

Because \(\kappa\approx 10^8\), it’s possible to lose nearly 8 digits of accuracy in the process of passing from \(\mathbf{A}\) and \(\mathbf{b}\) to \(\mathbf{x}\). That fact is independent of the algorithm; it’s inevitable once the data are expressed in finite precision.

Let’s engineer a linear system problem to observe the effect of a perturbation. We will make sure we know the exact answer.

```
x = 1:6
b = A*x
```

```
6-element Vector{Float64}:
4.407142857142857
3.564285714285714
3.013095238095238
2.6174603174603175
2.317279942279942
2.0807359307359308
```

Now we perturb the system matrix and vector randomly by \(10^{-10}\) in norm.

```
ΔA = randn(size(A)); ΔA = 1e-10*(ΔA/opnorm(ΔA));
Δb = randn(size(b)); Δb = 1e-10*normalize(Δb);
```

We solve the perturbed problem using pivoted LU and see how the solution was changed.

```
new_x = ((A+ΔA) \ (b+Δb))
Δx = new_x - x
```

```
6-element Vector{Float64}:
-5.471659263400763e-5
0.0009283239117472419
-0.004843432603480302
0.010718598499813048
-0.010580070933729147
0.0038388020192696715
```

Here is the relative error in the solution.

```
@show relative_error = norm(Δx) / norm(x);
```

```
relative_error = norm(Δx) / norm(x) = 0.0017093353064577405
```

And here are upper bounds predicted using the condition number of the original matrix.

```
println("Upper bound due to b: $(κ*norm(Δb)/norm(b))")
println("Upper bound due to A: $(κ*opnorm(ΔA)/opnorm(A))")
```

```
Upper bound due to b: 0.0006723667712613617
Upper bound due to A: 0.004566989872745153
```

Even if we didn’t make any manual perturbations to the data, machine roundoff does so at the relative level of \(\macheps\).

```
Δx = A\b - x
@show relative_error = norm(Δx) / norm(x);
@show rounding_bound = κ*eps();
```

```
relative_error = norm(Δx) / norm(x) = 1.2278255878021855e-9
rounding_bound = κ * eps() = 1.134607140820324e-8
```

Larger Hilbert matrices are even more poorly conditioned:

```
A = [ 1/(i+j) for i=1:14, j=1:14 ];
κ = cond(A)
```

```
3.870898056087325e17
```

Note that \(\kappa\) exceeds \(1/\macheps\). In principle we therefore may end up with an answer that has relative error greater than 100%.

```
rounding_bound = κ*eps()
```

```
85.95120295689817
```

Let’s put that prediction to the test.

```
x = 1:14
b = A*x
Δx = A\b - x
@show relative_error = norm(Δx) / norm(x);
```

```
relative_error = norm(Δx) / norm(x) = 2.3271868502658917
```

As anticipated, the solution has zero accurate digits in the 2-norm.

## Residual and backward error#

Suppose that \(\mathbf{A}\mathbf{x}=\mathbf{b}\) and \(\tilde{\mathbf{x}}\) is a computed estimate of the solution \(\mathbf{x}\). The most natural quantity to study is the error, \(\mathbf{x}-\tilde{\mathbf{x}}\). Normally we can’t compute it because we don’t know the exact solution. However, we can compute something related.

For the problem \(\mathbf{A}\mathbf{x}=\mathbf{b}\), the **residual** at a solution estimate \(\tilde{\mathbf{x}}\) is

Obviously, a zero residual means that \(\tilde{\mathbf{x}}=\mathbf{x}\), and we have the exact solution. What happens more generally? Note that \(\mathbf{A}\tilde{\mathbf{x}}=\mathbf{b}-\mathbf{r}\). That is, \(\tilde{\mathbf{x}}\) solves the linear system problem for a right-hand side that is changed by \(-\mathbf{r}\). This is precisely what is meant by backward error.

Hence residual and backward error are the same thing for a linear system. What is the connection to the (forward) error? We can reconnect with (2.8.2) by the definition \(\mathbf{h} = \tilde{\mathbf{x}}-\mathbf{x}\), in which case

Thus (2.8.2) is equivalent to

Equation (2.8.5) says that the gap between relative error and the relative residual is a multiplication by the matrix condition number.

When solving a linear system, all that can be expected is that the backward error, not the error, is small.

## Exercises#

⌨ Refer to Demo 2.8.3 for the definition of a Hilbert matrix. Make a table of the values of \(\kappa(\mathbf{H}_n)\) in the 2-norm for \(n=2,3,\ldots,16\). Speculate as to why the growth of \(\kappa\) appears to slow down at \(n=13\).

⌨ The purpose of this problem is to verify, like in Demo 2.8.3, the error bound

\[\frac{\| \mathbf{x}-\tilde{\mathbf{x} \|}}{\| \mathbf{x} \|} \le \kappa(\mathbf{A}) \frac{\| \mathbf{h} \|}{\| \mathbf{b} \|}.\]Here \(\tilde{\mathbf{x}}\) is a numerical approximation to the exact solution \(\mathbf{x}\), and \(\mathbf{h}\) is an unknown perturbation caused by machine roundoff. We will assume that \(\| \mathbf{d} \|/\| \mathbf{b} \|\) is roughly

`eps()`

.For each \(n=10,20,\ldots,70\) let

`A = matrixdepot("prolate",n,0.4)`

and let \(\mathbf{x}\) have components \(x_k=k/n\) for \(k=1,\ldots,n\). Define`b=A*x`

and let \(\tilde{\mathbf{x}}\) be the solution produced numerically by backslash.Make a table including columns for \(n\), the condition number of \(\mathbf{A}\), the observed relative error in \(\tilde{\mathbf{x}}\), and the right-hand side of the inequality above. You should find that the inequality holds in every case.

⌨ Exercise 2.3.7 suggests that the solutions of linear systems

\[\begin{split}\mathbf{A} = \begin{bmatrix} 1 & -1 & 0 & \alpha-\beta & \beta \\ 0 & 1 & -1 & 0 & 0 \\ 0 & 0 & 1 & -1 & 0 \\ 0 & 0 & 0 & 1 & -1 \\ 0 & 0 & 0 & 0 & 1 \end{bmatrix}, \quad \mathbf{b} = \begin{bmatrix} \alpha \\ 0 \\ 0 \\ 0 \\ 1 \end{bmatrix}\end{split}\]become less accurate as \(\beta\) increases. Using \(\alpha=0.1\) and \(\beta=10,100,\ldots,10^{12}\), make a table with columns for \(\beta\), \(|x_1-1|\), and the condition number of the matrix.

⌨ Let \(\mathbf{A}_n\) denote the \((n+1)\times(n+1)\) version of the Vandermonde matrix in Equation (2.1.2) based on the equally spaced interpolation nodes \(t_i=i/n\) for \(i=0,\ldots,n\). Using the 1-norm, graph \(\kappa(\mathbf{A}_n)\) as a function of \(n\) for \(n=4,5,6,\ldots,20\), using a log scale on the \(y\)-axis. (The graph is nearly a straight line.)

⌨ The matrix \(\mathbf{A}\) in (2.6.1) has unpivoted LU factors given in (2.6.2) as a function of parameter \(\epsilon\). For \(\epsilon = 10^{-2},10^{-4},\ldots,10^{-10}\), make a table with columns for \(\epsilon\), \(\kappa(\mathbf{A})\), \(\kappa(\mathbf{L})\), and \(\kappa(\mathbf{U})\). (This shows that solution via unpivoted LU factorization is arbitrarily unstable.)

✍ Define \(\mathbf{A}_n\) as the \(n\times n\) matrix \(\displaystyle\begin{bmatrix} 1 & -2 & & &\\ & 1 & -2 & & \\ & & \ddots & \ddots & \\ & & & 1 & -2 \\ & & & & 1 \end{bmatrix}.\)

**(a)**Write out \(\mathbf{A}_2^{-1}\) and \(\mathbf{A}_3^{-1}\).**(b)**Write out \(\mathbf{A}_n^{-1}\) in the general case \(n>1\). (If necessary, look at a few more cases in Julia until you are certain of the pattern.) Make a clear argument why it is correct.**(c)**Using the \(\infty\)-norm, find \(\kappa(\mathbf{A}_n)\).✍

**(a)**Prove that for \(n\times n\) nonsingular matrices \(\mathbf{A}\) and \(\mathbf{B}\), \(\kappa(\mathbf{A}\mathbf{B})\le \kappa(\mathbf{A})\kappa(\mathbf{B})\).**(b)**Show by means of an example that the result of part (a) cannot be an equality in general.✍ Let \(\mathbf{D}\) be a diagonal \(n\times n\) matrix, not necessarily invertible. Prove that in the 1-norm,

\[\kappa(\mathbf{D}) = \frac{\max_i |D_{ii}|}{\min_i |D_{ii}|}.\](Hint: See Exercise 2.7.10.)