Recall that 𝐑 denotes the real number line. 𝐑2 denotes the 2-dimensional plane of all column vectors of height 2 (i.e. (xy) ); 𝐑3 denotes the 3-dimensional space of all column vectors of height 3 (i.e. (xyz) ; and more generally, 𝐑n denotes the n -dimensional space of all column vectors of height n (i.e. (x1x2⋮xn) ).
02. Matrices: examples
02. Examples
Vectors in the plane
In the last video, we saw that a 2-by-2 matrix of numbers (abcd) defines a geometric transformation of the plane 𝐑2 : (xy)↦(ax+bycx+dy).
Just as the coordinates (xy) encode points in the plane, we should think of the matrix (abcd) as encoding a transformation of the plane. In this lecture, we will take a range of examples and see what the corresponding transformation looks like.
Example 1
Let M=(1000) . If I apply M to v=(xy) then I get Mv=(1000)(xy)=(x0).

Example 2
Consider the action of (1001) . This sends (xy) to (xy) ; this transformation leaves everything as it was: it is called the identity transformation. We call this matrix the identity matrix, and we often write this matrix as I ; it plays the role of the number 1 in the algebra of matrices.
Useful lemma
Let M=(abcd) , let e1=(10) and e2=(01) . Then
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Me1 is the first column of M , i.e. (ac) .
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Me2 is the second column of M , i.e. (bd) .

We'll call e1,e2 basis vectors, which basically means that any other vector can be written as a combination of e1 and e2 in a unique way. More on this in MATH220.
We'll just check it for Me1 : Me1=(abcd)(10)=(a+0c+0)=(ac).
Example 3
Take M=(0110) .
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Where does e1 go? It goes to the first column of M , which is e2 .
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Where does e2 go? It goes to the second column of M , which is e1 .
So e1 and e2 get switched. This corresponds to a reflection in the line y=x :

Let's check that the line y=x is indeed fixed by the action of M . The vectors (xx) (and only these ones) lie on this line, so let's compute: M(xx)=(xx),
Example 4
Take M=(0-110) .
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Where does e1 go? It goes to the first column of M , which is e2 .
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Where does e2 go? It goes to the second column of M , which is -e1 .

We see that this looks like a 90 degree (π/2 radian) rotation. This makes sense, because the matrix (cosθ-sinθsinθcosθ) for a rotation by an angle θ specialises to M when θ=π/2 , because cos(π/2)=0 and sin(π/2)=1 .
Example 5
Take M=(1101) . We have
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e1↦e1 ,
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e2↦(11) .
So e1 is fixed, but e2 is slanted over in the x -direction. In fact, the whole y -axis gets slanted in the x -direction, for example if we compute M(02) we get (22)

Example 6
As one final example, we'll take M=(-316-15) . What on earth does this correspond to? I claim that it corresponds to a shear in a different direction. How can we find the fixed direction?
If v=(xy) points in the direction fixed by M then v=Mv (that's what it means to be fixed). Therefore (xy)=(-316-15)(xy).
In other words, the first entries of v and Mv must coincide, and so must the second entries. This gives us a pair of linear simultaneous equations: x=-3x+16y,y=-x+5y.
Not all matrices have fixed directions, but if they do then this method will find it.
Outlook
In the next video, we will take a look at bigger matrices and higher-dimensional spaces.