Chapter 16: Problem 8
Use the Divergence Theorem to find the outward flux of \(\mathbf{F}\) across the boundary of the region \(D .\) Sphere \(\mathbf{F}=x^{2} \mathbf{i}+x z \mathbf{j}+3 z \mathbf{k}\) \(D :\) The solid sphere \(x^{2}+y^{2}+z^{2} \leq 4\)
Short Answer
Expert verified
The outward flux is \(24\pi^2\).
Step by step solution
01
Understand the Divergence Theorem
The Divergence Theorem relates the flux of a vector field through a closed surface to a volume integral over the region bounded by the surface. It states: \[ \iint_{\partial D} \mathbf{F} \cdot \mathbf{n}\, dS = \iiint_{D} (abla \cdot \mathbf{F})\, dV \] where \(\partial D\) is the boundary of \(D\), \(\mathbf{F}\) is the vector field, and \(abla \cdot \mathbf{F}\) is the divergence of \(\mathbf{F}\).
02
Calculate the Divergence of \(\mathbf{F}\)
For the vector field \(\mathbf{F} = x^{2} \mathbf{i} + xz \mathbf{j} + 3z \mathbf{k}\), the divergence is given by: \(abla \cdot \mathbf{F} = \frac{\partial }{\partial x}(x^2) + \frac{\partial }{\partial y}(xz) + \frac{\partial }{\partial z}(3z)\). Calculate each partial derivative: \(\frac{\partial }{\partial x}(x^2) = 2x\), \(\frac{\partial }{\partial y}(xz) = 0\), and \(\frac{\partial }{\partial z}(3z) = 3\). Thus, \(abla \cdot \mathbf{F} = 2x + 0 + 3 = 2x + 3\).
03
Set Up the Volume Integral
The region \(D\) is the solid sphere given by \(x^2 + y^2 + z^2 \leq 4\). In spherical coordinates, this is described by \(0 \leq \rho \leq 2\), \(0 \leq \theta \leq 2\pi\), and \(0 \leq \phi \leq \pi\). The divergence \(2x + 3\) in spherical coordinates becomes \(2\rho \cos(\theta)\sin(\phi) + 3\). The volume element in spherical coordinates is \(\rho^2 \sin(\phi)\, d\rho \, d\theta \, d\phi\). The integral setup is: \[ \iiint_{D} (2x + 3)\, dV = \int_{0}^{\pi} \int_{0}^{2\pi} \int_{0}^{2} \left(2\rho \cos(\theta)\sin(\phi) + 3\right)\rho^2 \sin(\phi)\, d\rho \, d\theta \, d\phi \]
04
Evaluate the Volume Integral
First integrate with respect to \(\rho\): \[ \int_{0}^{2} \left(2\rho \cos(\theta)\sin(\phi) + 3\right)\rho^2 \sin(\phi)\, d\rho = \int_{0}^{2} (2\rho^3 \cos(\theta) \sin^2(\phi) + 3\rho^2 \sin(\phi))\, d\rho \] Calculate it: \[= \left. \frac{1}{2} \rho^4 \cos(\theta) \sin^2(\phi) + \rho^3 \sin(\phi) \right|_{0}^{2} = 8\cos(\theta) \sin^2(\phi) + 24\sin(\phi)\] Integrate with respect to \(\theta\): \[ \int_{0}^{2\pi} (8\cos(\theta) \sin^2(\phi) + 24\sin(\phi)) \, d\theta = \int_{0}^{2\pi} 8\cos(\theta) \sin^2(\phi)\, d\theta + \int_{0}^{2\pi} 24\sin(\phi) \, d\theta \] \(\int_{0}^{2\pi} 8\cos(\theta) \sin^2(\phi)\, d\theta\) evaluates to zero, and \(\int_{0}^{2\pi} 24\sin(\phi)\, d\theta = 48\pi\sin(\phi)\). Now integrate with respect to \(\phi\): \[ \int_{0}^{\pi} 48\pi\sin(\phi)\, \sin(\phi)\, d\phi = 48\pi \int_{0}^{\pi} \sin^2(\phi)\, d\phi \] Use the identity \(\sin^2(\phi) = \frac{1 - \cos(2\phi)}{2}\): \[= 48\pi \int_{0}^{\pi} \frac{1 - \cos(2\phi)}{2}\, d\phi = 48\pi\left[\frac{\phi}{2} - \frac{\sin(2\phi)}{4}\right]_{0}^{\pi} = 48\pi\left(\frac{\pi}{2}\right) = 24\pi^2\]
05
Conclusion
The outward flux of the vector field \(\mathbf{F}\) through the boundary of the region \(D\) is \(24\pi^2\).
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Outward Flux
The concept of outward flux is crucial in understanding how a vector field behaves as it passes through a surface. Imagine a closed surface, like the boundary of a sphere. The outward flux measures the flow of a vector field across this surface, pointing outwards.
- It's like measuring the total fluid that would cross the surface if you thought of the vector field as representing a fluid's velocity.
- The Divergence Theorem, sometimes referred to as Gauss's theorem, assists in calculating this flux by connecting it to a volume integral over the region the surface encloses.
- The mathematical expression for the outward flux through a closed surface is given by the surface integral \( \iint_{\partial D} \mathbf{F} \cdot \mathbf{n}\, dS \), where \( \mathbf{n} \) is the outward normal vector on the surface.
Vector Field
A vector field is essentially a function that associates a vector to every point in space. It's remarkable because it can represent varying phenomena such as wind patterns, magnetic fields, or in our case, a mathematical construct to help in calculations.
- The vector field in the problem, \( \mathbf{F} = x^{2} \mathbf{i} + xz \mathbf{j} + 3z \mathbf{k} \), constructs lines of vector representations throughout space.
- The components \( x^2 \mathbf{i}, xz \mathbf{j}, \text{and} 3z \mathbf{k} \) represent the influence in the x, y, and z directions respectively.
Spherical Coordinates
Spherical coordinates provide an alternate way to describe points in three-dimensional space, especially useful for objects like spheres or shells.
- They include three parameters: \( \rho \) (the radial distance), \( \theta \) (the azimuthal angle), and \( \phi \) (the polar angle).
- In spherical coordinates, a point is represented in terms of distance from the origin \( \rho \), rotated angle from the positive x-axis \( \theta \), and the angle from the positive z-axis \( \phi \).