Basis

The bases for a linear space describe the space. Each member basis is independent.


Description

Bases are independent vectors that can be linearly combined to reach every other vector in a linear space. If a basis vector is removed, the space necessarily shrinks.

If the basis vectors are orthonormalized, they form an orthonormal basis. A convenient pair of orthonormal basis vectors in R2 are [1 0] and [0 1]. A convenient set of orthonormal basis vectors in R3 are [1 0 0], [0 1 0], and [0 0 1]. And so on.

A null space has no basis.

All non-null spaces have infinitely many possible bases to choose from, because the only requirement on a basis is that it be independent.


Change of Basis

A space can be linearly transformed to bring about a change of basis. This transformation can be expressed with a matrix. The inverse of that matrix then also expresses the inverse of the change of basis.

Such a change of basis has a linear scaling effect on space. The scaling factor is the determinant. If the determinant is 0, then the matrix expresses a transformation that removes one (or more) basis vector(s). Such a transformation effectively collapses the space to a lower dimension.

Any matrix that has basis is invertible, and therefore has a non-zero determinant.

Usage

If a matrix is diagonalizable, identifying the change of basis that transforms it into a diagonal matrix enables several efficient strategies for solving systems.

Some differentiation problems are more easily solved in polar coordinates than in Cartesian coordinates. The transformation of points is simple (i.e., r = √(x2 + y2), x = r*cosθ, and y = r*sinθ). The trick is that space was also transformed in the change of basis. The Jacobian is the determinant of the matrix describing the chain rule operations necessary.

    | ∂x ∂x |
    | ―― ―― |
    | ∂u ∂v |   ∂x ∂y   ∂x ∂y
det |       | = ―― ―― - ―― ――
    | ∂y ∂y |   ∂u ∂v   ∂v ∂u
    | ―― ―― |
    | ∂u ∂v |

Concretely, for the transformation of 2-dimensional polar coordinates to 2-dimensional Cartesian coordinates, the Jacobian is:

    | ∂x ∂x |       
    | ―― ―― |
    | ∂θ ∂r |       | cosθ -r*sinθ |
det |       | = det | sinθ  r*cosθ | = (cosθ)(r*cosθ) - (-r*sinθ)(sinθ) = r
    | ∂y ∂y |
    | ―― ―― |
    | ∂θ ∂r |

Therefore dxdy = rdrdθ.


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