Expand Solve the system:
2 x + 3 y = 8 2x + 3y = 8 2 x + 3 y = 8 and x − y = 1 x - y = 1 x − y = 1
In matrix form: ( 2 3 1 − 1 ) ( x y ) = ( 8 1 ) \begin{pmatrix} 2 & 3 \\ 1 & -1 \end{pmatrix} \begin{pmatrix} x \\ y \end{pmatrix} = \begin{pmatrix} 8 \\ 1 \end{pmatrix} ( 2 1 3 − 1 ) ( x y ) = ( 8 1 )
det ( A ) = ( 2 ) ( − 1 ) − ( 3 ) ( 1 ) = − 5 \det(A) = (2)(-1) - (3)(1) = -5 det ( A ) = ( 2 ) ( − 1 ) − ( 3 ) ( 1 ) = − 5
A − 1 = 1 − 5 ( − 1 − 3 − 1 2 ) = ( 0.2 0.6 0.2 − 0.4 ) A^{-1} = \dfrac{1}{-5}\begin{pmatrix} -1 & -3 \\ -1 & 2 \end{pmatrix} = \begin{pmatrix} 0.2 & 0.6 \\ 0.2 & -0.4 \end{pmatrix} A − 1 = − 5 1 ( − 1 − 1 − 3 2 ) = ( 0.2 0.2 0.6 − 0.4 )
( x y ) = ( 0.2 0.6 0.2 − 0.4 ) ( 8 1 ) = ( 2.2 1.2 ) \begin{pmatrix} x \\ y \end{pmatrix} = \begin{pmatrix} 0.2 & 0.6 \\ 0.2 & -0.4 \end{pmatrix} \begin{pmatrix} 8 \\ 1 \end{pmatrix} = \begin{pmatrix} 2.2 \\ 1.2 \end{pmatrix} ( x y ) = ( 0.2 0.2 0.6 − 0.4 ) ( 8 1 ) = ( 2.2 1.2 )
So x = 11 5 x = \frac{11}{5} x = 5 11 and y = 6 5 y = \frac{6}{5} y = 5 6 .
Every linear transformation T : R 2 → R 2 T: \mathbb{R}^2 \to \mathbb{R}^2 T : R 2 → R 2 can be represented by a 2 × 2 2 \times 2 2 × 2 Matrix M M M such that T ( v ) = M v T(\mathbf{v}) = M\mathbf{v} T ( v ) = M v . The images of the standard basis vectors ( 1 0 ) \begin{pmatrix} 1 \\ 0 \end{pmatrix} ( 1 0 ) and ( 0 1 ) \begin{pmatrix} 0 \\ 1 \end{pmatrix} ( 0 1 ) form the columns of M M M .
A reflection maps every point to its mirror image across a specified line. The determinant of any reflection matrix is − 1 -1 − 1 (orientation is reversed).
Reflection in the x x x -axis:
R_x = \begin`\{pmatrix}` 1 & 0 \\ 0 & -1 \end`\{pmatrix}` Reflection in the y y y -axis:
R_y = \begin`\{pmatrix}` -1 & 0 \\ 0 & 1 \end`\{pmatrix}` Reflection in the line y = x y = x y = x :
R_{y=x} = \begin`\{pmatrix}` 0 & 1 \\ 1 & 0 \end`\{pmatrix}` Reflection in the line y = − x y = -x y = − x :
R_{y=-x} = \begin`\{pmatrix}` 0 & -1 \\ -1 & 0 \end`\{pmatrix}` Reflection in the line y = ( tan θ ) x y = (\tan\theta)\,x y = ( tan θ ) x (a line through the origin making angle θ \theta θ With the positive x x x -axis):
R_\theta = \begin`\{pmatrix}` \cos 2\theta & \sin 2\theta \\ \sin 2\theta & -\cos 2\theta \end`\{pmatrix}` An anticlockwise rotation about the origin through an angle θ \theta θ is represented by:
R_\theta = \begin`\{pmatrix}` \cos\theta & -\sin\theta \\ \sin\theta & \cos\theta \end`\{pmatrix}` Key properties of rotation matrices:
det ( R θ ) = cos 2 θ + sin 2 θ = 1 \det(R_\theta) = \cos^2\theta + \sin^2\theta = 1 det ( R θ ) = cos 2 θ + sin 2 θ = 1 (area-preserving, orientation-preserving)R θ − 1 = R − θ = R θ T R_\theta^{-1} = R_{-\theta} = R_\theta^T R θ − 1 = R − θ = R θ T (rotation matrices are orthogonal)R α R β = R α + β R_\alpha R_\beta = R_{\alpha + \beta} R α R β = R α + β (composition of rotations adds angles)Common rotations:
Angle Matrix 90 ∘ 90^\circ 9 0 ∘ ( 0 − 1 1 0 ) \begin{pmatrix} 0 & -1 \\ 1 & 0 \end{pmatrix} ( 0 1 − 1 0 ) 180 ∘ 180^\circ 18 0 ∘ ( − 1 0 0 − 1 ) \begin{pmatrix} -1 & 0 \\ 0 & -1 \end{pmatrix} ( − 1 0 0 − 1 ) 270 ∘ 270^\circ 27 0 ∘ ( 0 1 − 1 0 ) \begin{pmatrix} 0 & 1 \\ -1 & 0 \end{pmatrix} ( 0 − 1 1 0 ) 60 ∘ 60^\circ 6 0 ∘ ( 1 2 − 3 2 3 2 1 2 ) \begin{pmatrix} \frac{1}{2} & -\frac{\sqrt{3}}{2} \\ \frac{\sqrt{3}}{2} & \frac{1}{2} \end{pmatrix} ( 2 1 2 3 − 2 3 2 1 ) 45 ∘ 45^\circ 4 5 ∘ ( 2 2 − 2 2 2 2 2 2 ) \begin{pmatrix} \frac{\sqrt{2}}{2} & -\frac{\sqrt{2}}{2} \\ \frac{\sqrt{2}}{2} & \frac{\sqrt{2}}{2} \end{pmatrix} ( 2 2 2 2 − 2 2 2 2 )
An enlargement with scale factor k k k about the origin scales all distances by ∣ k ∣ |k| ∣ k ∣ and, if k < 0 k \lt 0 k < 0 Also rotates by 180 ∘ 180^\circ 18 0 ∘ .
E_k = \begin`\{pmatrix}` k & 0 \\ 0 & k \end`\{pmatrix}` det ( E k ) = k 2 \det(E_k) = k^2 det ( E k ) = k 2 So the area scale factor is k 2 k^2 k 2 .For k = 1 k = 1 k = 1 This is the identity transformation. For k = − 1 k = -1 k = − 1 This is equivalent to a rotation of 180 ∘ 180^\circ 18 0 ∘ about the origin. Stretches. A stretch parallel to the x x x -axis with scale factor k k k :
S_x = \begin`\{pmatrix}` k & 0 \\ 0 & 1 \end`\{pmatrix}` A stretch parallel to the y y y -axis with scale factor k k k :
S_y = \begin`\{pmatrix}` 1 & 0 \\ 0 & k \end`\{pmatrix}` For a stretch parallel to the x x x -axis, det ( S x ) = k \det(S_x) = k det ( S x ) = k So the area scale factor is ∣ k ∣ |k| ∣ k ∣ . If 0 < k < 1 0 \lt k \lt 1 0 < k < 1 The figure is compressed; if k > 1 k \gt 1 k > 1 It is expanded.
Shears. A horizontal shear with shear factor k k k fixes every point on the x x x -axis and shifts Other points horizontally in proportion to their y y y -coordinate:
H_x = \begin`\{pmatrix}` 1 & k \\ 0 & 1 \end`\{pmatrix}` A vertical shear with shear factor k k k :
H_y = \begin`\{pmatrix}` 1 & 0 \\ k & 1 \end`\{pmatrix}` For any shear matrix, det = 1 \det = 1 det = 1 So area is preserved. The x x x -axis (for H x H_x H x ) or y y y -axis (for H y H_y H y ) is point-wise invariant.
If transformation A A A is applied first, followed by transformation B B B The composite transformation is represented by the product B A BA B A (note the order: right to left).
v ′ = B ( A v ) = ( B A ) v \mathbf{v}' = B(A\mathbf{v}) = (BA)\mathbf{v} v ′ = B ( A v ) = ( B A ) v Example. A rotation of 90 ∘ 90^\circ 9 0 ∘ anticlockwise followed by a reflection in the x x x -axis:
\begin`\{pmatrix}` 1 & 0 \\ 0 & -1 \end`\{pmatrix}` \begin`\{pmatrix}` 0 & -1 \\ 1 & 0 \end`\{pmatrix}` = \begin`\{pmatrix}` 0 & -1 \\ -1 & 0 \end`\{pmatrix}` This is equivalent to a single reflection in the line y = − x y = -x y = − x .
Worked Example: Composite Transformation Find the image of the point ( 2 , 3 ) (2, 3) ( 2 , 3 ) under a rotation of 90 ∘ 90^\circ 9 0 ∘ anticlockwise about the origin Followed by a reflection in the line y = x y = x y = x .
Rotation matrix:
R 90 = ( 0 − 1 1 0 ) R_{90} = \begin{pmatrix} 0 & -1 \\ 1 & 0 \end{pmatrix} R 90 = ( 0 1 − 1 0 ) Reflection in y = x y = x y = x :
R y = x = ( 0 1 1 0 ) R_{y=x} = \begin{pmatrix} 0 & 1 \\ 1 & 0 \end{pmatrix} R y = x = ( 0 1 1 0 ) Composite (reflection applied after rotation):
M = R y = x ⋅ R 90 = ( 0 1 1 0 ) ( 0 − 1 1 0 ) = ( 1 0 0 − 1 ) M = R_{y=x} \cdot R_{90} = \begin{pmatrix} 0 & 1 \\ 1 & 0 \end{pmatrix}\begin{pmatrix} 0 & -1 \\ 1 & 0 \end{pmatrix} = \begin{pmatrix} 1 & 0 \\ 0 & -1 \end{pmatrix} M = R y = x ⋅ R 90 = ( 0 1 1 0 ) ( 0 1 − 1 0 ) = ( 1 0 0 − 1 ) This is a reflection in the x x x -axis! Apply to ( 2 , 3 ) (2, 3) ( 2 , 3 ) :
( 1 0 0 − 1 ) ( 2 3 ) = ( 2 − 3 ) \begin{pmatrix} 1 & 0 \\ 0 & -1 \end{pmatrix}\begin{pmatrix} 2 \\ 3 \end{pmatrix} = \begin{pmatrix} 2 \\ -3 \end{pmatrix} ( 1 0 0 − 1 ) ( 2 3 ) = ( 2 − 3 ) The image is ( 2 , − 3 ) (2, -3) ( 2 , − 3 ) .
Inverse of a composite. Since ( B A ) − 1 = A − 1 B − 1 (BA)^{-1} = A^{-1}B^{-1} ( B A ) − 1 = A − 1 B − 1 To undo a composite transformation, The individual inverses are applied in reverse order.
An invariant point under transformation M M M is a point v \mathbf{v} v such that M v = v M\mathbf{v} = \mathbf{v} M v = v I.e. ( M − I ) v = 0 (M - I)\mathbf{v} = \mathbf{0} ( M − I ) v = 0 . The set of invariant points forms the null space of M − I M - I M − I .
For any 2 × 2 2 \times 2 2 × 2 transformation matrix, the origin is always invariant.
An invariant line is a line that is mapped onto itself (though individual points on the line may move along it). A line through the origin with direction vector d \mathbf{d} d is invariant if M d = λ d M\mathbf{d} = \lambda \mathbf{d} M d = λ d for some scalar λ \lambda λ Which means d \mathbf{d} d is an Eigenvector of M M M .
A line is point-wise invariant (every point is fixed) if and only if every point on it is an invariant point, meaning the line lies entirely in the null space of M − I M - I M − I .
Not all invariant lines are point-wise invariant. For example, a stretch parallel to the x x x -axis ( k 0 0 1 ) \begin{pmatrix} k & 0 \\ 0 & 1 \end{pmatrix} ( k 0 0 1 ) leaves the x x x -axis point-wise invariant and also leaves the y y y -axis invariant as a line (each point ( 0 , y ) (0, y) ( 0 , y ) maps to itself), but it leaves every line parallel to the x x x -axis invariant as a line (points slide along it), not point-wise.
For a reflection, the mirror line is point-wise invariant and the line perpendicular to it through the origin is invariant as a set (points are reflected across the mirror line but remain on the perpendicular line).
For any 2 × 2 2 \times 2 2 × 2 matrix M M M representing a linear transformation of the plane, the area scale Factor is ∣ det ( M ) ∣ |\det(M)| ∣ det ( M ) ∣ . This means:
If ∣ det ( M ) ∣ = 1 |\det(M)| = 1 ∣ det ( M ) ∣ = 1 The transformation preserves area (e.g. Rotations, reflections). If ∣ det ( M ) ∣ = k 2 |\det(M)| = k^2 ∣ det ( M ) ∣ = k 2 The area of any region is multiplied by k 2 k^2 k 2 (e.g. Enlargement by scale factor k k k ). If det ( M ) = 0 \det(M) = 0 det ( M ) = 0 The transformation is singular and collapses the plane to a line or point. This extends to 3 × 3 3 \times 3 3 × 3 matrices where ∣ det ( M ) ∣ |\det(M)| ∣ det ( M ) ∣ is the volume scale factor.
When a linear transformation acts on a vector, the vector is generally rotated and scaled. Certain special vectors, called eigenvectors , are only scaled (stretched or compressed) by the transformation, not rotated. The factor by which an eigenvector is scaled is the corresponding eigenvalue .
Let A A A be an n × n n \times n n × n matrix. A scalar λ \lambda λ is an eigenvalue of A A A if there exists a non-zero vector v \mathbf{v} v (the corresponding eigenvector ) such that:
A v = λ v A\mathbf{v} = \lambda \mathbf{v} A v = λ v Equivalently: ( A − λ I ) v = 0 (A - \lambda I)\mathbf{v} = \mathbf{0} ( A − λ I ) v = 0 .
For a non-trivial solution v ≠ 0 \mathbf{v} \neq \mathbf{0} v = 0 to exist, we require:
det ( A − λ I ) = 0 \det(A - \lambda I) = 0 det ( A − λ I ) = 0 The equation det ( A − λ I ) = 0 \det(A - \lambda I) = 0 det ( A − λ I ) = 0 is the characteristic equation of A A A . For a 2 × 2 2 \times 2 2 × 2 Matrix A = ( a b c d ) A = \begin{pmatrix} a & b \\ c & d \end{pmatrix} A = ( a c b d ) :
\det\begin`\{pmatrix}` a - \lambda & b \\ c & d - \lambda \end`\{pmatrix}` = (a - \lambda)(d - \lambda) - bc = 0 Expanding:
λ 2 − ( a + d ) λ + ( a d − b c ) = 0 \lambda^2 - (a + d)\lambda + (ad - bc) = 0 λ 2 − ( a + d ) λ + ( a d − b c ) = 0 Notice that a + d = t r ( A ) a + d = \mathrm{tr}(A) a + d = tr ( A ) (the trace of A A A ) and a d − b c = det ( A ) ad - bc = \det(A) a d − b c = det ( A ) . Therefore:
λ 2 − t r ( A ) λ + det ( A ) = 0 \lambda^2 - \mathrm{tr}(A)\lambda + \det(A) = 0 λ 2 − tr ( A ) λ + det ( A ) = 0 For a 3 × 3 3 \times 3 3 × 3 matrix, the characteristic equation is a cubic:
det ( A − λ I ) = − λ 3 + t r ( A ) λ 2 − S λ + det ( A ) = 0 \det(A - \lambda I) = -\lambda^3 + \mathrm{tr}(A)\lambda^2 - S\lambda + \det(A) = 0 det ( A − λ I ) = − λ 3 + tr ( A ) λ 2 − S λ + det ( A ) = 0 Where S S S is the sum of the principal 2 × 2 2 \times 2 2 × 2 minors (the sum of the determinants of the matrices obtained by deleting each row and the corresponding column).
Fundamental properties of eigenvalues:
The sum of the eigenvalues equals the trace: λ 1 + λ 2 + ⋯ + λ n = t r ( A ) \lambda_1 + \lambda_2 + \cdots + \lambda_n = \mathrm{tr}(A) λ 1 + λ 2 + ⋯ + λ n = tr ( A ) . The product of the eigenvalues equals the determinant: λ 1 λ 2 ⋯ λ n = det ( A ) \lambda_1 \lambda_2 \cdots \lambda_n = \det(A) λ 1 λ 2 ⋯ λ n = det ( A ) . A matrix is invertible if and only if none of its eigenvalues is zero. The eigenvalues of A k A^k A k are λ 1 k , λ 2 k , … , λ n k \lambda_1^k, \lambda_2^k, \ldots, \lambda_n^k λ 1 k , λ 2 k , … , λ n k . Once an eigenvalue λ \lambda λ is known, the corresponding eigenvectors are found by solving:
( A − λ I ) v = 0 (A - \lambda I)\mathbf{v} = \mathbf{0} ( A − λ I ) v = 0 This is a homogeneous system. Since det ( A − λ I ) = 0 \det(A - \lambda I) = 0 det ( A − λ I ) = 0 The rows of A − λ I A - \lambda I A − λ I are linearly dependent, and the system has infinitely many solutions forming a one-dimensional subspace (a line through the origin) for each distinct eigenvalue.
Important: Eigenvectors are determined only up to a non-zero scalar multiple. Any non-zero Multiple of an eigenvector is also an eigenvector for the same eigenvalue.
When the characteristic equation has a repeated root (a repeated eigenvalue), the matrix may or may not be diagonalisable.
Geometric multiplicity ≤ \leq ≤ algebraic multiplicity. The algebraic multiplicity of an eigenvalue is its multiplicity as a root of the characteristic equation. The geometric multiplicity is the dimension of the corresponding eigenspace (the number of linearly independent eigenvectors for that eigenvalue).A matrix is diagonalisable if and only if the geometric multiplicity of each eigenvalue equals its algebraic multiplicity. If the geometric multiplicity is strictly less than the algebraic multiplicity, the matrix is defective and cannot be diagonalised. For a 2 × 2 2 \times 2 2 × 2 matrix with a repeated eigenvalue λ \lambda λ :
If A = λ I A = \lambda I A = λ I Then every non-zero vector is an eigenvector (geometric multiplicity = 2 = 2 = 2 ), and A A A is diagonalisable (it is already diagonal). If A ≠ λ I A \neq \lambda I A = λ I but has a repeated eigenvalue, the geometric multiplicity is 1 1 1 and A A A is not diagonalisable. For a 3 × 3 3 \times 3 3 × 3 matrix, the characteristic equation is a cubic polynomial in λ \lambda λ . The cubic can have three distinct real roots, one repeated and one distinct real root, or one real root and two complex conjugate roots. Since the IB course works over R \mathbb{R} R Only real eigenvalues and eigenvectors are considered.