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State the domain of each of the following vector-valued functions: (a) \(\mathbf{r}(t)=\ln (t-1) \mathbf{i}+\sqrt{20-t} \mathbf{j}\) (b) \(\mathbf{r}(t)=\ln \left(t^{-1}\right) \mathbf{i}+\tan ^{-1} t \mathbf{j}+t \mathbf{k}\) (c) \(\mathbf{r}(t)=\frac{1}{\sqrt{1-t^{2}}} \mathbf{j}+\frac{1}{\sqrt{9-t^{2}}} \mathbf{k}\)

Short Answer

Expert verified
(a) Domain is (1, 20]; (b) Domain is (-∞, 0) ∪ (0, ∞); (c) Domain is (-1, 1) ∩ (-3, 3).

Step by step solution

01

Understanding the Function

The given function is \(\mathbf{r}(t) = \ln(t-1) \mathbf{i} + \sqrt{20-t} \mathbf{j}\). To find the domain, we need to find where each component is defined.
02

Analyzing Each Component

1. For \(\ln(t-1)\), the argument must be greater than 0. Thus, \(t-1 > 0\) or \(t > 1\). 2. For \(\sqrt{20-t}\), the expression under the square root must be non-negative. Therefore, \(20-t \geq 0\) or \(t \leq 20\).
03

Deriving the Domain for (a)

Combining both conditions, \(t > 1\) and \(t \leq 20\), the domain of the function \(\mathbf{r}(t)\) is \((1, 20]\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Domain of Functions
In mathematical analysis and calculus, the domain of a function is crucial for understanding where the function can be evaluated. For any function, the domain represents all the possible input values (usually represented as "x" or, in the case of vector-valued functions, "t") that can be used in the function to produce a valid result.

For vector-valued functions, each component can impose its own restrictions on the domain. Let's look at an example: the vector-valued function \( \mathbf{r}(t) = \ln(t-1) \mathbf{i} + \sqrt{20-t} \mathbf{j} \).The domain is found by considering the restrictions of each component of the function:
  • \( \ln(t-1) \): The natural logarithm requires that its input, \(t-1\), must be greater than zero. Therefore, \(t > 1\).
  • \( \sqrt{20-t} \): The square root function requires that its argument be non-negative, i.e., \(20-t \geq 0\) or \(t \leq 20\).
Combining these conditions, the domain of \( \mathbf{r}(t) \) is the interval \((1, 20] \). Understanding the domain involves analyzing these constraints and applying set theory to the conditions dictated by each function component.
Logarithmic Functions
Logarithmic functions are a cornerstone in mathematics, often denoted as \( \ln(x) \) for the natural logarithm with base \(e\), where \(e\approx 2.71828\). The domain of logarithmic functions must always be comprised of positive numbers, as the logarithm of non-positive numbers is undefined in real analysis.

For example, consider the logarithmic component in the function \( \ln(t-1) \). The condition for the logarithm to be defined is that \( t-1 > 0 \). This implies \( t > 1 \). The significance of this constraint is clear: it defines one boundary for the domain of any function it is part of. For any point inside this boundary, you can calculate the logarithm.

Key properties to remember about logarithms include:
  • \( \ln(ab) = \ln(a) + \ln(b) \)
  • \( \ln \left(\frac{a}{b}\right) = \ln(a) - \ln(b) \)
  • \( \ln(a^b) = b\ln(a) \)
These properties help manipulate and simplify expressions involving logarithms, assisting in solving equations and understanding function behavior.
Square Root Functions
Square root functions are one of the basic types of functions involving the radical sign. These functions are often written in the form \( \sqrt{x} \) and their domain typically includes only non-negative values of \(x\). This is because the square root of a negative number is not defined in the set of real numbers.

In our example with \( \sqrt{20-t} \), the expression under the square root must be non-negative, meaning \( 20-t \geq 0 \), leading to the condition \( t \leq 20 \). This condition ensures that the result of the square root is a real number.

Here’s what to remember:
  • The square root function will only output real numbers for non-negative inputs.
  • This property defines an upper or lower boundary for the domain, depending on the context.
  • In the vector-valued function \( \mathbf{r}(t) \), it introduced the restriction \( t \leq 20 \).
Understanding these conditions is pivotal when determining the domain of functions that include square root expressions.
Mathematical Analysis
Mathematical analysis involves a wide variety of concepts and techniques used to understand the behavior of functions, their limits, continuity, and derivatives. The study of vector-valued functions is a part of this broader discipline, dealing with functions whose values are vectors.

In examining the domain of vector-valued functions, mathematical analysis uses a combination of understanding individual function components and their constraints to determine the overall function's domain.

Consider the interplay of functions in \( \mathbf{r}(t) = \ln(t-1) \mathbf{i} + \sqrt{20-t} \mathbf{j} \):
  • The logarithmic function provides a lower bound \( t > 1 \).
  • The square root function provides an upper bound \( t \leq 20 \).
With analysis, we are able to logically combine these constraints to find the largest set of input values for which all components are defined. This logical approach facilitates deeper understanding and solutions to complex problems, embodying the essence of mathematical analysis in practice.

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Most popular questions from this chapter

Show that for a straight line \(\mathbf{r}(t)=\mathbf{r}_{0}+a_{0} t \mathbf{i}+\) \(b_{0} t \mathbf{j}+c_{0} t \mathbf{k}\) both \(\kappa\) and \(\tau\) are zero.

Name and sketch the graph of each of the following equations in three-space. $$ 9 x^{2}-y^{2}+9 z^{2}-9=0 $$

EXPL 48. In this exercise you will derive Kepler's First Law, that planets travel in elliptical orbits. We begin with the notation. Place the coordinate system so that the sun is at the origin and the planet's closest approach to the sun (the perihelion) is on the positive \(x\) -axis and occurs at time \(t=0\). Let \(\mathbf{r}(t)\) denote the position vector and let \(r(t)=\|\mathbf{r}(t)\|\) denote the distance from the sun at time \(t\). Also, let \(\theta(t)\) denote the angle that the vector \(\mathbf{r}(t)\) makes with the positive \(x\) -axis at time \(t\). Thus, \((r(t), \theta(t))\) is the polar coordinate representation of the planet's position. Let \(\mathbf{u}_{1}=\mathbf{r} / r=(\cos \theta) \mathbf{i}+(\sin \theta) \mathbf{j} \quad\) and \(\quad \mathbf{u}_{2}=(-\sin \theta) \mathbf{i}+(\cos \theta) \mathbf{j}\) Vectors \(\mathbf{u}_{1}\) and \(\mathbf{u}_{2}\) are orthogonal unit vectors pointing in the directions of increasing \(r\) and increasing \(\theta\), respectively. Figure 12 summarizes this notation. We will often omit the argument \(t\), but keep in mind that \(\mathbf{r}, \theta, \mathbf{u}_{1}\), and \(\mathbf{u}_{2}\) are all functions of \(t .\) A prime in. dicates differentiation with respect to time \(t\). (a) Show that \(\mathbf{u}_{1}^{\prime}=\theta^{\prime} \mathbf{u}_{2}\) and \(\mathbf{u}_{2}^{\prime}=-\theta^{\prime} \mathbf{u}_{1}\). (b) Show that the velocity and acceleration vectors satisfy $$ \begin{array}{l} \mathbf{v}=r^{\prime} \mathbf{u}_{1}+r \theta^{\prime} \mathbf{u}_{2} \\ \mathbf{a}=\left(r^{\prime \prime}-r\left(\theta^{\prime}\right)^{2}\right) \mathbf{u}_{1}+\left(2 r^{\prime} \theta^{\prime}+r \theta^{\prime \prime}\right) \mathbf{u}_{2} \end{array} $$ (c) Use the fact that the only force acting on the planet is the gravity of the sun to express a as a multiple of \(\mathbf{u}_{1}\), then explain how we can conclude that $$ \begin{aligned} r^{\prime \prime}-r\left(\theta^{\prime}\right)^{2} &=\frac{-G M}{r^{2}} \\ 2 r^{\prime} \theta^{\prime}+r \theta^{\prime \prime} &=0 \end{aligned} $$ (d) Consider \(\mathbf{r} \times \mathbf{r}^{\prime}\), which we showed in Example 8 was a constant vector, say D. Use the result from (b) to show that \(\mathbf{D}=r^{2} \theta^{\prime} \mathbf{k} .\) (e) Substitute \(t=0\) to get \(\mathbf{D}=r_{0} v_{0} \mathbf{k}\), where \(r_{0}=r(0)\) and \(v_{0}=\|\mathbf{v}(0)\|\). Then argue that \(r^{2} \theta^{\prime}=r_{0} v_{0}\) for all \(t\). (f) Make the substitution \(q=r^{\prime}\) and use the result from (e) to obtain the first-order (nonlinear) differential equation in \(q\) : $$ q \frac{d q}{d r}=\frac{r_{0}^{2} v_{0}^{2}}{r^{3}}-\frac{G M}{r^{2}} $$ (g) Integrate with respect to \(r\) on both sides of the above equation and use an initial condition to obtain $$ q^{2}=2 G M\left(\frac{1}{r}-\frac{1}{r_{0}}\right)+v_{0}^{2}\left(1-\frac{r_{0}^{2}}{r^{2}}\right) $$ (h) Substitute \(p=1 / r\) into the above equation to obtain $$ \frac{r_{0}^{2} v_{0}^{2}}{\left(\theta^{\prime}\right)^{2}}\left(\frac{d p}{d t}\right)^{2}=2 G M\left(p-p_{0}\right)+v_{0}^{2}\left(1-\frac{p^{2}}{p_{0}^{2}}\right) $$

find the tangential and normal components \(\left(a_{T}\right.\) and \(\left.a_{N}\right)\) of the acceleration vector at \(t .\) Then evaluate at \(t=t_{1} .\) $$ \mathbf{r}(t)=\left(t-\frac{1}{3} t^{3}\right) \mathbf{i}-\left(t+\frac{1}{3} t^{3}\right) \mathbf{j}+t \mathbf{k} ; t_{1}=3 $$

find the tangential and normal components \(\left(a_{T}\right.\) and \(\left.a_{N}\right)\) of the acceleration vector at \(t .\) Then evaluate at \(t=t_{1} .\) $$ \mathbf{r}(t)=t^{2} \mathbf{i}+t \mathbf{j} ; t_{1}=1 $$

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