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In the region \(-\infty

Short Answer

Expert verified
The relationship is \(\tilde{V}(\alpha) = \frac{\tilde{\rho}(\alpha)}{\epsilon_0 (\alpha^2 + q^2)}. The potential at (x,0,0) is \(\frac{A}{\pi} \int_{-\infty}^{\infty} \frac{\sin kt}{k(k^2+q^2)} dk\).

Step by step solution

01

Understand the given charge-density wave

The charge-density wave is given by \( \rho(\textbf{r})= A \cos q x\). This wave only varies along the x-direction.
02

Expressing charge-density \(\rho(\textbf{r})\) in integral form

The wave \( \rho(\textbf{r})\) is represented as \(\rho(\textbf{r})=\frac{e^{i q x}}{\sqrt{2 \pi}} \int_{-\infty}^{\infty}\tilde{\rho}(\alpha) e^{i x z} d \alpha\).
03

Identifying the potential \(V(\textbf{r})\)

The potential \(V(\textbf{r})\) is given by \(V(\textbf{r})=\frac{e^{i q x}}{\sqrt{2 \pi}} \int_{-\infty}^{\infty}\tilde{V}(\alpha) e^{i x z} d \alpha\).
04

Relation between \(\tilde{V}(\alpha)\) and \(\tilde{\rho}(\alpha)\)

Using Poisson's equation in Fourier space, the potential and charge density are related by: \(abla^2 V = - \frac{\rho}{\epsilon_0}\).In Fourier space, \(\-k^2 \tilde{V}(k) = -\frac{\tilde{\rho}(k)}{\epsilon_0}\), where \(k = \sqrt{\alpha^2+\beta^2+\gamma^2} = \sqrt{\alpha^2+q^2}\), leading to \(\tilde{V}(\alpha) = \frac{\tilde{\rho}(\alpha)}{\epsilon_0 (\alpha^2 + q^2)}\).
05

Substituting the given \(\tilde{\rho}(\alpha)\) into the potential expression

The charge density given is \(\rho(\mathbf{r})= A \cos q x\), which in Fourier space (\( \tilde{\rho}(\alpha)\)) gives, mathematically, \(\frac{e^{i q x}}{\sqrt{2 \pi}} \tilde{\rho}(\alpha) e^{i x z}\). Substitution into Fourier transformed Poisson eq. gives: \(\tilde{V}(\alpha)=\frac{1}{\epsilon_0(\alpha^2+q^2)}\tilde{\rho}(\alpha)\).
06

Integrate over \(\alpha\)

Expressing potential at the point (x,0,0), substituting boundary (-t to t) limits for non-zero terms simplify: \(. Finally: V(x,0,0)= \frac{A}{\pi} \int_{-\infty}^{\infty} \frac{\sin (kt)}{k(k^2+q^2)} dk\).

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Key Concepts

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

Poisson's equation
Poisson's equation is a fundamental part of electrostatics. It relates the electric potential to the charge density in a region. The equation is given by: \[ abla^2 V = - \frac{\rho}{\text{ε}_0} \] where \(V\) is the electric potential, \(ρ\) is the charge density, and \(ε_0\) is the permittivity of free space. In simple terms, it means that if you know the charge distribution, you can find the resulting electric potential.
  • The Laplacian operator \( abla^2 \), appears in the equation. It measures the second spatial derivatives of the potential.
  • The term \( - \frac{\rho}{\text{ε}_0} \) signifies the source term; it shows how charges affect the potential field.
Fourier transform
The Fourier transform is a mathematical tool that transforms a function of time (or space) into a function of frequency (or wave number). It is very useful in solving differential equations, including Poisson's equation. The general form of the Fourier transform of a function \(f(x)\) is: \[ \tilde{f}(\beta) = \frac{1}{\text{π}} \bigint_{- \text{∞}}^{\text{∞}} f(x) e^{-ix\beta} dx \]Using the Fourier transform, Poisson's equation in the original (spatial) domain \( abla^2 V = - \frac{\rho}{\text{ε}_0} \) can be converted into the frequency domain: \[ - k^2 \tilde{V}(k) = - \frac{\tilde{\rho}(k)}{\text{ω}_0} \]This approach simplifies many problems, as it turns complicated differential equations into algebraic equations.
Electric potential
The electric potential \(V\) is a scalar quantity representing the electric potential energy per unit charge at a point in space. To find the electric potential caused by a charge distribution, you can use Poisson's equation: \[ abla^2 V = - \frac{\rho}{\text{ε}_0} \]In our specific problem, we are dealing with a charge-density wave: \[ \rho(\textbf{r}) = A \text{ cos} qx \]By using Poisson's equation in Fourier space, we relate the transformed potential and charge density: \[ \tilde{V}(\beta) = \frac{\tilde{\rho}(\beta)}{\text{ω}_0 (\beta^2 + q^2)} \]
  • This relationship can be reverted back into the spatial domain to get our electric potential.
  • The final result for the potential at point \((x, 0, 0)\) after integrating and simplifying is: \[ V(x, 0, 0) = \frac{A}{ \text{π}} \bigint_{-\text{∞}}^{\text{∞}} \frac{ \text{sin}(kt)}{k(k^2 + q^2)} dk \]

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Most popular questions from this chapter

(a) By applying the divergence theorem to the volume integral $$ \int_{V}\left[\phi\left(\nabla^{2}-m^{2}\right) \psi-\psi\left(\nabla^{2}-m^{2}\right) \phi\right] d V $$ obtain a Green's function expression, as the sum of a volume integral and a surface integral, for \(\phi\left(\mathbf{r}^{\prime}\right)\) that satisfies $$ \nabla^{2} \phi-m^{2} \phi=\rho $$ in \(V\) and takes the specified form \(\phi=f\) on \(S\), the boundary of \(V .\) The Green's function \(G\left(\mathbf{r}, \mathbf{r}^{\prime}\right)\) to be used satisfies $$ \nabla^{2} G-m^{2} G=\delta\left(\mathbf{r}-\mathbf{r}^{\prime}\right) $$ and vanishes when \(\mathbf{r}\) is on \(S .\) (b) When \(V\) is all space, \(G\left(\mathbf{r}, \mathbf{r}^{\prime}\right)\) can be written as \(G(t)=g(t) / t\) where \(t=\left|\mathbf{r}-\mathbf{r}^{\prime}\right|\) and \(g(t)\) is bounded as \(t \rightarrow \infty .\) Find the form of \(G(t)\). (c) Find \(\phi(\mathbf{r})\) in the half space \(x>0\) if \(\rho(\mathbf{r})=\delta\left(\mathbf{r}-\mathbf{r}_{1}\right)\) and \(\phi=0\) both on \(x=0\) and as \(r \rightarrow \infty\) .

The free transverse vibrations of a thick rod satisfy the equation $$ a^{4} \frac{\partial^{4} u}{\partial x^{4}}+\frac{\partial^{2} u}{\partial t^{2}}=0 $$ Obtain a solution in separated-variable form and, for a rod clamped at one end, \(x=0\), and free at the other, \(x=L\), show that the angular frequency of vibration \(\omega\) satisfies $$ \cosh \left(\frac{\omega^{1 / 2} L}{a}\right)=-\sec \left(\frac{\omega^{1 / 2} L}{a}\right) $$. (At a clamped end both \(u\) and \(\partial u / \partial x\) vanish, whilst at a free end, where there is no bending moment, \(\partial^{2} u / \partial x^{2}\) and \(\partial^{3} u / \partial x^{3}\) are both zero.)

Consider the PDE \(\mathcal{L} u(\mathbf{r})=\rho(\mathbf{r})\), for which the differential operator \(\mathcal{L}\) is given by $$ \mathcal{L}=\nabla \cdot[p(\mathbf{r}) \nabla]+q(\mathbf{r}) $$ where \(p(\mathbf{r})\) and \(q(\mathbf{r})\) are functions of position. By proving the generalised form of Green's theorem, $$ \int_{V}(\phi \mathcal{L} \psi-\psi \mathcal{L} \phi) d V=\oint_{S} p(\phi \nabla \psi-\psi \nabla \phi) \cdot \hat{\mathbf{n}} d S $$ show that the solution of the PDE is given by $$ u\left(\mathbf{r}_{0}\right)=\int_{V} G\left(\mathbf{r}, \mathbf{r}_{0}\right) \rho(\mathbf{r}) d V(\mathbf{r})+\oint_{S} p(\mathbf{r})\left[u(\mathbf{r}) \frac{\partial G\left(\mathbf{r}, \mathbf{r}_{0}\right)}{\partial n}-G\left(\mathbf{r}, \mathbf{r}_{0}\right) \frac{\partial u(\mathbf{r})}{\partial n}\right] d S(\mathbf{r}) $$ where \(G\left(\mathbf{r}, \mathbf{r}_{0}\right)\) is the Green's function satisfying \(\mathcal{L} G\left(\mathbf{r}, \mathbf{r}_{0}\right)=\delta\left(\mathbf{r}-\mathbf{r}_{0}\right)\).

(a) Find the form of the solution of Laplace's equation in plane polar coordinates \(\rho, \phi\) that takes the value \(+1\) for \(0<\phi<\pi\) and the value \(-1\) for \(-\pi<\phi<0\) when \(\rho=a\) (b) For a point \((x, y)\) on or inside the circle \(x^{2}+y^{2}=a^{2}\), identify the angles \(\alpha\) and \(\beta\) defined by $$ \alpha=\tan ^{-1} \frac{y}{a+x} \quad \text { and } \quad \beta=\tan ^{-1} \frac{y}{a-x} $$ Show that \(u(x, y)=(2 / \pi)(\alpha+\beta)\) is a solution of Laplace's equation that satisfies the boundary conditions given in (a). (c) Deduce a Fourier series expansion for the function $$ \tan ^{-1} \frac{\sin \phi}{1+\cos \phi}+\tan ^{-1} \frac{\sin \phi}{1-\cos \phi} $$.

Find the Green's function for the three-dimensional Neumann problem $$ \nabla^{2} \phi=0 \quad \text { for } z>0 \quad \text { and } \quad \frac{\partial \phi}{\partial z}=f(x, y) \quad \text { on } z=0 $$ Determine \(\phi(x, y, z)\) if $$ f(x, y)= \begin{cases}\delta(y) & \text { for }|x|

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