Matrix Representation of Linear Transformations
To express a linear transformation as a matrix, one constructs a matrix 'A' using the coefficients that define the transformation. For instance, a transformation T that maps (x, y) to (3x + 2y, 5y) can be represented by the matrix A = [3 2; 0 5]. Multiplying this matrix by a vector [x; y] yields the new coordinates of the transformed point. The matrix multiplication process involves taking the dot product of the rows of the matrix with the column vector to produce the resulting vector.Classifying Linear Transformations by Their Matrices
Different linear transformations are distinguished by their respective matrix representations. Reflections are typified by matrices that contain '1's and '-1's to mirror an image across a line or plane, which remains invariant. Rotations, which leave the origin fixed, are described by orthogonal matrices that include trigonometric functions of the rotation angle, indicating a counterclockwise rotation for positive angles. Scaling transformations are represented by diagonal matrices with scaling factors along the principal axes, altering the size of the geometric figures, while shearing matrices contain non-zero off-diagonal elements that skew the figure.Determining Area Changes and Composite Transformations
The area of a shape changes under certain linear transformations, such as scaling. The determinant of the transformation matrix, denoted as det(A), quantifies the area scaling factor. A positive determinant indicates a preservation of orientation and a scaling of the area by the determinant's absolute value, while a negative determinant reflects a change in orientation, such as a reflection. For multiple transformations applied in succession, the overall transformation can be represented by the product of the matrices corresponding to each transformation. This resultant matrix, known as the composite matrix, provides a single-step transformation that is equivalent to the sequential application of the original transformations.Applying Linear Transformations to Geometric Figures
Linear transformations are practically applied to geometric figures by transforming the coordinates of their vertices. For example, applying the matrix A = [1.2 0; 0 -2] to the vertices of a triangle will stretch it horizontally by a factor of 1.2 and reflect it vertically. The new vertex coordinates are obtained through matrix multiplication, and the change in area is determined by the determinant of A. Successive transformations, such as a reflection followed by a rotation, can be combined into a single matrix, streamlining the process of calculating the final position of the figure.Extending Linear Transformations to Higher Dimensions
The principles of linear transformations in two dimensions extend naturally to three dimensions, where they are represented by 3×3 matrices. This extension allows for a broader range of transformations, including translations, which require the use of homogeneous coordinates and 4×4 matrices to be represented linearly. Rotations in three dimensions can occur around any axis, and these are described by matrices that incorporate the sine and cosine of the rotation angles. Understanding 3D transformations requires a grasp of concepts such as eigenvectors and eigenvalues, which are essential in analyzing the properties of these transformations.