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Find the indefinite integral. $$ \int\left(\sec ^{2} t \mathbf{i}+\frac{1}{1+t^{2}} \mathbf{j}\right) d t $$

Short Answer

Expert verified
The indefinite integral is \(\tan(t)\mathbf{i}+\arctan(t)\mathbf{j}+C\), where \(C\) is the constant of integration.

Step by step solution

01

Identify the integrals

Split the integral into two separate parts for each vector. One integral will be for \(\sec ^{2} t \mathbf{i}\) and another for \(\frac{1}{1+t^{2}} \mathbf{j}\)
02

Calculate the first integral

Integral of \(\sec ^{2} t\) is given by the trigonometric identity \(\int \sec^2 t \, dt = \tan(t)\). So, \(\int\sec ^{2} t \mathbf{i} dt = \tan(t)\mathbf{i}\)
03

Calculate the second integral

Integral of \(\frac{1}{1+t^{2}}\) is given as \(\arctan(t)\) according to standard integrals. So, \(\int\frac{1}{1+t^{2}}\mathbf{j} dt = \arctan(t)\mathbf{j}\)
04

Combine the results

Combine the results of the two integrals to get the final solution.

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Key Concepts

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

Integration
Integration is a fundamental concept in calculus that involves finding the integral, or antiderivative, of a function. This process is the reverse of differentiation, where we are given the rate of change and need to discover the original function. Indefinite integrals, like the one presented in our textbook exercise, do not have set limits of integration and are represented with a constant of integration, typically denoted as 'C'.

Understanding integration allows us to solve various problems, such as calculating areas under curves, averaging functions, and in physics, it aids in determining the position of an object knowing its velocity over time. The indefinite integral essentially represents a family of functions, all of which are possible antiderivatives of the original function.
Trigonometric Integrals
Trigonometric integrals involve integrating functions that contain trigonometric expressions, such as sine, cosine, secant, or tangent. These integrals often require specific techniques and identities for simplification before the integral can be easily evaluated. In our exercise's Step 2, the integration of \(\sec^{2}(t)\) is simplified by using the well-known identity \(\int \sec^2(t)\, dt = \tan(t)\).

There's a rich collection of formulas dealing with trigonometric integrals, and mastering them is crucial for students tackling calculus problems. Integrating trigonometric functions often requires substitution techniques or recognition of patterns aligned with standard integral formulas. Learning to identify such patterns can significantly simplify the integration process.
Antiderivatives
An antiderivative of a function is another function that differentiates to give the first function. In other words, it's a process of finding the original function given its derivative. When we take the indefinite integral of a function, we are essentially looking for its antiderivatives. Each function can have an infinite number of antiderivatives, differing only by a constant. The textbook exercise provides an example of finding antiderivatives: Step 2 resolves \(\sec^2(t)\) into \(\tan(t)\), while Step 3 transforms \(\frac{1}{1+t^2}\) into \(\arctan(t)\). These antiderivatives are pivotal in constructing the integral function that represents the cumulative sum of the original function's rate of change over an interval.
Vector Calculus
Vector calculus extends basic calculus concepts into a multidimensional setting. It's utilized in physics and engineering to handle quantities that have both magnitude and direction, called vectors. In the solved exercise, we see vector calculus in action as the integral is performed on a vector-valued function, which has both \(\mathbf{i}\) and \(\mathbf{j}\) components representing different dimensions.

Steps 1 and 4 of the solution emphasize important aspects of vector calculus: each component of the vector can be integrated separately, and the results can then be combined into a single vector expression. This piecewise integration is vital in applications such as calculating work done by a force field, fluid flow, or even the trajectory of objects in space.

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Most popular questions from this chapter

Find the vectors \(T\) and \(N\), and the unit binormal vector \(\mathbf{B}=\mathbf{T} \times \mathbf{N}\), for the vector-valued function \(\mathbf{r}(t)\) at the given value of \(t\). $$ \mathbf{r}(t)=2 \cos t \mathbf{i}+2 \sin t \mathbf{j}+\frac{t}{2} \mathbf{k} $$ $$ t_{0}=\frac{\pi}{2} $$

You are asked to verify Kepler's Laws of Planetary Motion. For these exercises, assume that each planet moves in an orbit given by the vector- valued function \(\mathbf{r}\). Let \(\boldsymbol{r}=\|\mathbf{r}\|\), let \(\boldsymbol{G}\) represent the universal gravitational constant, let \(M\) represent the mass of the sun, and let \(m\) represent the mass of the planet. Prove Kepler's Third Law: The square of the period of a planet's orbit is proportional to the cube of the mean distance between the planet and the sun.

Use a computer algebra system to graph the space curve. Then find \(\mathbf{T}(t), \mathrm{N}(t), a_{\mathbf{T}}\), and \(a_{\mathrm{N}}\) at the given time \(t\). Sketch \(\mathrm{T}(t)\) and \(\mathrm{N}(t)\) on the space curve. $$ \mathbf{r}(t)=t \mathbf{i}+3 t^{2} \mathbf{j}+\frac{t^{2}}{2} \mathbf{k} \quad t=2 $$

Use a computer algebra system to graph the space curve. Then find \(\mathbf{T}(t), \mathrm{N}(t), a_{\mathbf{T}}\), and \(a_{\mathrm{N}}\) at the given time \(t\). Sketch \(\mathrm{T}(t)\) and \(\mathrm{N}(t)\) on the space curve. $$ \mathbf{r}(t)=4 t \mathbf{i}+3 \cos t \mathbf{j}+3 \sin t \mathbf{k} \quad t=\frac{\pi}{2} $$

Sketch the space curve and find its length over the given interval. Function \(\quad\) Interval \(\mathbf{r}(t)=\left\langle\cos t+t \sin t, \sin t-t \cos t, t^{2}\right\rangle \quad\left[0, \frac{\pi}{2}\right]\)

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