Lecture 2
Auburn University
MATH 2660 - Spring 2026
January 9, 2026

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\[ \vec{v}=\begin{bmatrix}a_1\\a_2\\\vdots\\a_n\end{bmatrix} \]
For some \(n\in\mathbb{N}\), the Euclidean space of dimension \(n\) is the set of all \(n\)-tuples \[ (a_1,a_2,\dots,a_n) \] where each \(a_i\in\mathbb{R}\).

Unconsciously, when we are given coordinates, we do something like this:
The last two steps are interchangeable: the order does not matter.
We now interpret \((2,-3)\) as an instruction for movement:
To emphasize that this object represents a vector, rather than a point, we often write \[ \vec{v}=\begin{bmatrix}a_1\\a_2\\\vdots\\a_n\end{bmatrix}\qquad\text{or}\qquad \vec{v} = \langle a_1, a_2, \dots, a_n\rangle. \] We write vectors vertically, as columns, for convenience and consistency—this choice will become clear later in the course.
In examples like \((2,-3)=2\vec{e}_1-3\vec{e}_2\), there are two kinds of quantities: the magnitudes (\(2\) and \(-3\)) and the directions (\(\vec{e}_1\) and \(\vec{e}_2\)).
In general, the vector \(\langle a_1,a_2,\dots,a_n \rangle\) in \(\mathbb{R}^n\) is the movement along each axis direction by the given magnitudes.
Equivalently, \[ \langle a_1,a_2,\dots,a_n \rangle =a_1\vec{e}_1+a_2\vec{e}_2+\cdots+a_n\vec{e}_n, \] where \(\vec{e}_i\) is the unit vector in the \(i\)th coordinate direction (the standard basis vector).
We define two fundamental operations for vectors \(\vec{v},\vec{w}\in\mathbb{R}^n\) and a scalar \(c\in\mathbb{R}\).
1. Vector addition \[ \vec{v}+\vec{w} = \begin{bmatrix}v_1\\ \vdots\\ v_n\end{bmatrix} + \begin{bmatrix}w_1\\ \vdots\\ w_n\end{bmatrix} = \begin{bmatrix}v_1+w_1\\ \vdots\\ v_n+w_n\end{bmatrix}. \]
2. Scalar multiplication \[ c\vec{v} = c\begin{bmatrix}v_1\\ \vdots\\ v_n\end{bmatrix} = \begin{bmatrix}cv_1\\ \vdots\\ cv_n\end{bmatrix}. \]
1. Vector addition: placing two vectors head-to-tail; equivalently, the sum is given by the diagonal of the parallelogram formed by the two vectors.
2. Scalar multiplication:
If \(c < 0\), the direction of the vector is reversed.
Suppose we are given vectors \(\vec{v}_1,\dots,\vec{v}_k\). A vector \(\vec{w}\) of the form \[ \vec{w}=c_1\vec{v}_1+\cdots+c_k\vec{v}_k \] is called a linear combination of \(\vec{v}_1,\dots,\vec{v}_k\) with coefficients \(c_1,\dots,c_k\in\mathbb{R}\).
Let \[ \vec{v}_1=\begin{bmatrix}2\\-3\end{bmatrix}, \qquad \vec{v}_2=\begin{bmatrix}1\\0.5\end{bmatrix}. \] Compute \(\vec{w}=3\vec{v}_1-2\vec{v}_2\).
First, \[ 3\vec{v}_1 = 3\begin{bmatrix}2\\-3\end{bmatrix} = \begin{bmatrix}6\\-9\end{bmatrix}. \]
Next, \[ -2\vec{v}_2 = -2\begin{bmatrix}1\\0.5\end{bmatrix} = \begin{bmatrix}-2\\-1\end{bmatrix}. \]
So \[ \vec{w} = \begin{bmatrix}6\\-9\end{bmatrix} + \begin{bmatrix}-2\\-1\end{bmatrix} = \begin{bmatrix}4\\-10\end{bmatrix}. \]