Problem 3
Question
A vector \(\mathbf{u}\) for which \(\|\mathbf{u}\|=1\) is called a(n) _____ vector.
Step-by-Step Solution
Verified Answer
Unit vector
1Step 1: Understand the Problem
Determine the concept that describes a vector with a magnitude (or norm) of 1.
2Step 2: Recall Key Definitions
Recall that a vector whose norm (or length) is 1 is called a 'unit vector'. Mathematically, if \(\|\mathbf{u}\| = 1\)\, then \(\mathbf{u}\) is a unit vector.
3Step 3: Conclusion
Based on the definition, conclude that a vector with a norm of 1 is called a unit vector.
Key Concepts
vector magnitudenorm of a vectorunit vector
vector magnitude
A vector's magnitude provides information about the length or size of the vector. It is sometimes also referred to as the 'length' or 'norm' of the vector.
For a vector \(\boldsymbol{v} \) in a 2-dimensional or 3-dimensional space, its magnitude is computed using the Pythagorean Theorem. Let's say \(\boldsymbol{v} = (v_1, v_2)\) in 2D or \(\boldsymbol{v} = (v_1, v_2, v_3)\) in 3D. The magnitude \(\boldsymbol{\text{of v}}\) can be calculated as:
\[\text{In 2D:} \|\boldsymbol{v}\| = \sqrt{v_1^2 + v_2^2}\ \] \[ \text{In 3D:} \|\boldsymbol{v}\| = \sqrt{v_1^2 + v_2^2 + v_3^2}\ \]
The result will always be a non-negative number.
Understanding vector magnitude is crucial in fields like physics, engineering, and computer graphics to measure distances and define directions.
For a vector \(\boldsymbol{v} \) in a 2-dimensional or 3-dimensional space, its magnitude is computed using the Pythagorean Theorem. Let's say \(\boldsymbol{v} = (v_1, v_2)\) in 2D or \(\boldsymbol{v} = (v_1, v_2, v_3)\) in 3D. The magnitude \(\boldsymbol{\text{of v}}\) can be calculated as:
\[\text{In 2D:} \|\boldsymbol{v}\| = \sqrt{v_1^2 + v_2^2}\ \] \[ \text{In 3D:} \|\boldsymbol{v}\| = \sqrt{v_1^2 + v_2^2 + v_3^2}\ \]
The result will always be a non-negative number.
Understanding vector magnitude is crucial in fields like physics, engineering, and computer graphics to measure distances and define directions.
norm of a vector
The norm of a vector usually refers to its magnitude or length in a given vector space. It is a function that assigns a strictly positive length or size to each vector in the space, except for the zero vector, which has a norm of zero.
There are different types of norms, but the most common one is the Euclidean norm, represented as \(\boldsymbol{\text{\|v\|}}\). For a vector \(\boldsymbol{v} = (v_1, v_2, ..., v_n)\):
\[\text{Euclidean norm:} \|v\| = \sqrt{v_1^2 + v_2^2 + ... + v_n^2} \]
Other types of norms include the Manhattan norm (or L1 norm), which is the sum of the absolute values of the components:
\[\boldsymbol{\text{Manhattan norm:}} \|v\|_1 = |v_1| + |v_2| + ... + |v_n| \]
And the infinity norm, which is the maximum absolute value among the vector's components:
\[\boldsymbol{\text{Infinity norm:}} \|v\|_\text{∞} = \text{max}(|v_1|, |v_2|, ..., |v_n|) \]
The Euclidean norm is the most commonly used and referred to simply as the 'norm' or 'magnitude' of the vector.
There are different types of norms, but the most common one is the Euclidean norm, represented as \(\boldsymbol{\text{\|v\|}}\). For a vector \(\boldsymbol{v} = (v_1, v_2, ..., v_n)\):
\[\text{Euclidean norm:} \|v\| = \sqrt{v_1^2 + v_2^2 + ... + v_n^2} \]
Other types of norms include the Manhattan norm (or L1 norm), which is the sum of the absolute values of the components:
\[\boldsymbol{\text{Manhattan norm:}} \|v\|_1 = |v_1| + |v_2| + ... + |v_n| \]
And the infinity norm, which is the maximum absolute value among the vector's components:
\[\boldsymbol{\text{Infinity norm:}} \|v\|_\text{∞} = \text{max}(|v_1|, |v_2|, ..., |v_n|) \]
The Euclidean norm is the most commonly used and referred to simply as the 'norm' or 'magnitude' of the vector.
unit vector
A unit vector is a vector that has a magnitude (or norm) of exactly 1. Unit vectors are often used to represent direction, as they retain the vector's direction but have a standard length.
If you have a vector \(\boldsymbol{v}\) that is not a unit vector, you can convert it into one by dividing the vector by its magnitude:
\[\text{Unit vector} \ \boldsymbol{\text{u}} = \ \frac{\boldsymbol{v}}{\boldsymbol{\text{\|v\|}}} \]
Here, \(\boldsymbol{v} \) is your original vector, and \(\boldsymbol{\text{\|v\|}} \) is its magnitude.
For example, if \(\boldsymbol{v} = (3, 4) \), the magnitude is \(\boldsymbol{\text{\|v\|}} = 5 \), and the unit vector \(\boldsymbol{u} \) is:
\[\boldsymbol{u} = \frac{(3, 4)}{5} = (0.6, 0.8) \]
Unit vectors are denoted with a hat, such as \(\boldsymbol{\text{\hat{i}}} \) and \(\boldsymbol{\text{\hat{j}}} \) in two dimensions, representing the x and y directions, respectively.
Understanding unit vectors is essential because they simplify mathematical computations and are used in various fields like physics, computer graphics, and navigation.
If you have a vector \(\boldsymbol{v}\) that is not a unit vector, you can convert it into one by dividing the vector by its magnitude:
\[\text{Unit vector} \ \boldsymbol{\text{u}} = \ \frac{\boldsymbol{v}}{\boldsymbol{\text{\|v\|}}} \]
Here, \(\boldsymbol{v} \) is your original vector, and \(\boldsymbol{\text{\|v\|}} \) is its magnitude.
For example, if \(\boldsymbol{v} = (3, 4) \), the magnitude is \(\boldsymbol{\text{\|v\|}} = 5 \), and the unit vector \(\boldsymbol{u} \) is:
\[\boldsymbol{u} = \frac{(3, 4)}{5} = (0.6, 0.8) \]
Unit vectors are denoted with a hat, such as \(\boldsymbol{\text{\hat{i}}} \) and \(\boldsymbol{\text{\hat{j}}} \) in two dimensions, representing the x and y directions, respectively.
Understanding unit vectors is essential because they simplify mathematical computations and are used in various fields like physics, computer graphics, and navigation.
Other exercises in this chapter
Problem 2
If \(\mathbf{v}\) is a vector, then \(\mathbf{v}+(-\mathbf{v})=\) _____
View solution Problem 3
\(\sin \frac{2 \pi}{3}=\)________; \(\cos \frac{4 \pi}{3}=\) ________.
View solution Problem 4
If \(\mathbf{v}=3 \mathbf{w},\) then the two vectors \(\mathbf{v}\) and \(\mathbf{w}\) are _________.
View solution Problem 4
Simplify: \(e^{2} \cdot e^{5}=\) ________ ;\(\left(e^{4}\right)^{3}=\) __________.
View solution