57. Linear Transformation

A function 𝑇:𝑛𝑚 between vector spaces is a linear transformation if it preserves vector addition and scalar multiplication.

57.1. The two axioms

For any vectors 𝑎,𝑏𝑛 and scalar 𝑐:

1. Additivity

𝑇(𝑎+𝑏)=𝑇(𝑎)+𝑇(𝑏)

2. Homogeneity (scalar multiplication)

𝑇(𝑐𝑎)=𝑐𝑇(𝑎)

The two combine into a single condition: 𝑇(𝑐𝑎+𝑑𝑏)=𝑐𝑇(𝑎)+𝑑𝑇(𝑏) for all scalars and vectors.

Example

𝑇:22 defined by 𝑇([𝑥𝑦])=[2𝑥3𝑦] is linear.

Check additivity: 𝑎=[12], 𝑏=[31]:

𝑇(𝑎)+𝑇(𝑏)=[26]+[63]=[89]𝑇(𝑎+𝑏)=𝑇([43])=[89]

Check homogeneity: 𝑐=3, 𝑎=[12]:

𝑐𝑇(𝑎)=3[26]=[618]𝑇(𝑐𝑎)=𝑇([36])=[618]

57.2. Consequences

Linearity forces 𝑇 to be very rigid. From the two axioms:

57.3. Equivalent definition: matrix–vector product

Every linear transformation can be written as 𝑇(𝑥)=𝐴𝑥 for some matrix 𝐴 — see Matrix Representation. This means linear transformation 𝑛𝑚𝑚×𝑛 matrix.

57.4. Non-examples

57.5. See also