/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 41 A particle of mass \(m\) moves a... [FREE SOLUTION] | 91Ó°ÊÓ

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A particle of mass \(m\) moves along one of two "paths" through space and time connecting the points \((x, t)=(0,0)\) and \((x, t)=(D, T)\). One path is quadratic in time, i.e. \(x_{1}(t)=\frac{1}{2} a t^{2}\) where \(a\) is a constant. The second path is linear in time, i.e. \(x_{2}(t)=v t\) where \(v\) is a constant. The correct classical path is the quadratic path, that is \(x_{1}(t)\). a. Find the acceleration \(a\) for the correct classical path. Use freshman physics to find the force \(F=m a=-d V / d x\) and then the potential energy function \(V(x)\) in terms of \(m, D\), and \(T\). Also find the velocity \(v\) for the linear (i.e. incorrect classical) path. b. Calculate the classical action \(S[x(t)]=\int_{0}^{T}\left[\frac{1}{2} m \dot{x}^{2}-V(x)\right] d t\) for each of the two paths \(x_{1}(t)\) and \(x_{2}(t)\). Confirm that \(S_{1} \equiv S\left[x_{1}(t)\right]

Short Answer

Expert verified
The quadratic path has a lower classical action than the linear path, which confirms it as the classical path. For small particles moving macroscopic distances, the motion's quantum mechanical nature depends on \(\Delta S/\hbar\).

Step by step solution

01

Establish Equations of Motion

For the quadratic path, we know `x_1(t)` is given as \(x_1(t) = \frac{1}{2} a t^2\). For the linear path, \(x_2(t) = v t\). Here, our aim is to find the acceleration \(a\) for the quadratic path and the velocity \(v\) for the linear path.
02

Calculate Acceleration for Quadratic Path

Since the final position at time \(T\) is \(D\), for \(x_1(t) = \frac{1}{2} a t^2\), we have \(D = \frac{1}{2} a T^2\). Solving for \(a\), we get \(a = \frac{2D}{T^2}\).
03

Calculate Velocity for Linear Path

For the linear path, the final position is \(D = v T\). Solving for \(v\), we get \(v = \frac{D}{T}\).
04

Determine the Force and Potential Energy

The force is given by \(F = ma = m \left(\frac{2D}{T^2}\right)\). Since \(F = -\frac{dV}{dx}\), by integrating \(F\) with respect to \(x\), the potential energy function \(V(x)\) is given by \(V(x) = -m \left(\frac{2D}{T^2} \right) x + C\). By setting \(V(0) = 0\), we find that \(C = 0\).
05

Classical Action for Quadratic Path

For \(x_1(t)\), we compute the kinetic energy as \(\frac{1}{2} m \left( a t \right)^2 = \frac{1}{2} m \left( \frac{2D}{T^2} t \right)^2\). The classical action \(S_1\) is \(\int_0^T \left[ \frac{1}{2} m \left( \frac{2D}{T^2} t \right)^2 - \left( -m \frac{2D}{T^2} x \right) \right] dt\). Solve this integral for \(S_1\).
06

Classical Action for Linear Path

For \(x_2(t)\), compute \(\frac{1}{2} m v^2 = \frac{1}{2} m \left( \frac{D}{T} \right)^2\) and \(V(x) = -m \left(\frac{2D}{T^2} \right) xt\). Solve the integral \(\int_0^T \left[ \frac{1}{2} m \left( \frac{D}{T} \right)^2 - V(x) \right] dt\) to find \(S_2\).
07

Compute \(\Delta S\) and \(\Delta S/ \hbar\)

Calculate the difference \(\Delta S = S_2 - S_1\). For a nanoparticle and electron moving \(1 \text{ mm}\) in \(1 \text{ ms}\), use components from each particle, calculate \(\frac{\Delta S}{\hbar}\), and determine whether the motion should be considered quantum mechanical or classical based on the action's scale.

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Key Concepts

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

Classical Path
In classical mechanics, the concept of a "Classical Path" refers to the trajectory that a particle follows through space and time based on the principles established by Isaac Newton. The problem here looks at two hypothetical paths—a quadratic path and a linear path—to illustrate this concept.
A classical path is not just any path; it is the path that minimizes the action, a principle attributed to Pierre Maupertuis and championed by later scientists such as Lagrange and Hamilton. For two endpoints in space and time, the correct classical path, according to the principle of least action, is one that takes into consideration forces acting on the particle and results in a specified acceleration.
  • Quadratic Path: This problem cuts to the heart of classical dynamics by introducing a path described by a quadratic equation, where the position is a function of time squared, as in \( x_1(t) = \frac{1}{2} a t^2 \). This path signifies a particle experiencing constant acceleration.
  • Determining Forces: The acceleration \( a = \frac{2D}{T^2} \) is key to understanding the forces at play. Recognizing the force gives insight into potential energy and enables us to verify the correctness of the classical path using Newton's second law: \( F = ma \).
By solving for the correct classical path, students grasp how certain physical conditions derive the trajectory a particle must follow classically.
Action Calculation
The action, a pivotal concept in classical mechanics, is quantified as the integral of the Lagrangian over time. It helps students understand which path out of potential candidates is physically plausible. In this exercise, we compare the classical action calculated for both the quadratic and linear paths to confirm which one requires less action. This involves using the Lagrangian, \( L = T - V \), where \( T \) is kinetic energy and \( V \) is potential energy, and then integrating it over time.
For the quadratic path, the action is:
  • \( S_1 = \int_0^T \left[ \frac{1}{2} m \left( \frac{2D}{T^2} t \right)^2 - \left(-m \frac{2D}{T^2} x \right) \right] dt \)

For the linear (incorrect) path, the action is different:
  • \( S_2 = \int_0^T \left[ \frac{1}{2} m \left( \frac{D}{T} \right)^2 - V(x) \right] dt\)

The classical path is, by definition, the one with the smaller action (i.e., \( S_1 < S_2 \)). This disciplinary approach ingrains a deeper understanding of why nature "prefers" one path over another—adhering to the principle that action is minimized.
Quantum Mechanical Motion
When investigating whether a particle's motion is quantum mechanical, the calculation of \( \Delta S / \hbar \) becomes essential. \( \hbar \) is the reduced Planck's constant, which is notably small. Thus, only when \( \Delta S \) is comparable to or smaller than \( \hbar \) does quantum mechanical behavior emerge.
For example, in the textbook exercise, we account for a particle that moves 1 mm in 1 ms and compute this ratio for a nanoparticle and an electron. These two entities yield different results due to their substantial difference in masses and sizes:
  • Nano-Particle: Given its considerable mass, the action difference \( \Delta S \) divided by \( \hbar \) usually indicates more classical behavior.
  • Electron: With a much smaller mass, the action difference is often comparable to \( \hbar \), indicating more significant quantum effects.
Understanding which case depicts quantum mechanical motion enriches the student's grasp of how scale and environment could dictate the nature of motion.

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Most popular questions from this chapter

Let \(\left|a^{\prime}\right\rangle\) and \(\left|a^{\prime \prime}\right\rangle\) be eigenstates of a Hermitian operator \(A\) with eigenvalues \(a^{\prime}\) and \(a^{\prime \prime}\), respectively \(\left(a^{\prime} \neq a^{\prime \prime}\right)\). The Hamiltonian operator is given by $$ H=\left|a^{\prime}\right\rangle \delta\left\langle a^{\prime \prime}|+| a^{\prime \prime}\right\rangle \delta\left\langle a^{\prime}\right| $$ where \(\delta\) is just a real number. a. Clearly, \(\left|a^{\prime}\right\rangle\) and \(\left|a^{\prime \prime}\right\rangle\) are not eigenstates of the Hamiltonian. Write down the eigenstates of the Hamiltonian. What are their energy eigenvalues? b. Suppose the system is known to be in state \(\left|a^{\prime}\right\rangle\) at \(t=0\). Write down the state vector in the Schrödinger picture for \(t>0\). c. What is the probability for finding the system in \(\left|a^{\prime \prime}\right\rangle\) for \(t>0\) if the system is known to be in state \(\left|a^{\prime}\right\rangle\) at \(t=0\) ? d. Can you think of a physical situation corresponding to this problem?

Consider an electron confined to the interior of a hollow cylindrical shell whose axis coincides with the \(z\)-axis. The wave function is required to vanish on the inner and outer walls, \(\rho=\rho_{a}\) and \(\rho_{b}\), and also at the top and bottom, \(z=0\) and \(L\). a. Find the energy eigenfunctions. (Do not bother with normalization.) Show that the energy eigenvalues are given by $$ E_{l m n}=\left(\frac{\hbar^{2}}{2 m_{e}}\right)\left[k_{m n}^{2}+\left(\frac{l \pi}{L}\right)^{2}\right] \quad(l=1,2,3, \ldots, m=0,1,2, \ldots) $$ where \(k_{m n}\) is the \(n\)th root of the transcendental equation $$ J_{m}\left(k_{m n} \rho_{b}\right) N_{m}\left(k_{m n} \rho_{a}\right)-N_{m}\left(k_{m n} \rho_{b}\right) J_{m}\left(k_{m n} \rho_{a}\right)=0 . $$ b. Repeat the same problem when there is a uniform magnetic field \(\mathbf{B}=B \hat{\mathbf{z}}\) for \(0<\) \(\rho<\rho_{a} .\) Note that the energy eigenvalues are influenced by the magnetic field even though the electron never "touches" the magnetic field. c. Compare, in particular, the ground state of the \(B=0\) problem with that of the \(B \neq 0\) problem. Show that if we require the ground-state energy to be unchanged in the presence of \(B\), we obtain "flux quantization" $$ \pi \rho_{a}^{2} B=\frac{2 \pi N \hbar c}{e} \quad(N=0, \pm 1, \pm 2, \ldots) $$

Consider the Hamiltonian of a spinless particle of charge \(e\). In the presence of a static magnetic field, the interaction terms can be generated by $$ \mathbf{p}_{\text {operator }} \rightarrow \mathbf{p}_{\text {operator }}-\frac{e \mathbf{A}}{c} $$ where \(\mathbf{A}\) is the appropriate vector potential. Suppose, for simplicity, that the magnetic field \(\mathbf{B}\) is uniform in the positive \(z\)-direction. Prove that the above prescription indeed leads to the correct expression for the interaction of the orbital magnetic moment \((e / 2 m c) \mathbf{L}\) with the magnetic field \(\mathbf{B}\). Show that there is also an extra term proportional to \(B^{2}\left(x^{2}+y^{2}\right)\), and comment briefly on its physical significance.

A box containing a particle is divided into a right and a left compartment by a thin partition. If the particle is known to be on the right (left) side with certainty, the state is represented by the position eigenket \(|R\rangle(|L\rangle)\), where we have neglected spatial variations within each half of the box. The most general state vector can then be written as $$ |\alpha\rangle=|R\rangle\langle R \mid \alpha\rangle+|L\rangle\langle L \mid \alpha\rangle $$ where \(\langle R \mid \alpha\rangle\) and \(\langle L \mid \alpha\rangle\) can be regarded as "wave functions." The particle can tunnel through the partition; this tunneling effect is characterized by the Hamiltonian $$ H=\Delta(|L\rangle\langle R|+| R\rangle\langle L|) $$ where \(\Delta\) is a real number with the dimension of energy. a. Find the normalized energy eigenkets. What are the corresponding energy eigenvalues? b. In the Schrödinger picture the base kets \(|R\rangle\) and \(|L\rangle\) are fixed, and the state vector moves with time. Suppose the system is represented by \(|\alpha\rangle\) as given above at \(t=0 .\) Find the state vector \(\left|\alpha, t_{0}=0 ; t\right\rangle\) for \(t>0\) by applying the appropriate time-evolution operator to \(|\alpha\rangle\). c. Suppose at \(t=0\) the particle is on the right side with certainty. What is the probability for observing the particle on the left side as a function of time? d. Write down the coupled Schrödinger equations for the wave functions \(\langle R| \alpha, t_{0}=\) \(0 ; t\rangle\) and \(\left\langle L \mid \alpha, t_{0}=0 ; t\right\rangle\). Show that the solutions to the coupled Schrödinger equations are just what you expect from (b). e. Suppose the printer made an error and wrote \(H\) as $$ H=\Delta|L\rangle\langle R| $$ By explicitly solving the most general time-evolution problem with this Hamiltonian, show that probability conservation is violated.

A particle of mass \(m\) in one dimension is bound to a fixed center by an attractive \(\delta\)-function potential: $$ V(x)=-\lambda \delta(x) \quad(\lambda>0) . $$ At \(t=0\), the potential is suddenly switched off (that is, \(V=0\) for \(t>0\) ). Find the wave function for \(t>0\). (Be quantitative! But you need not attempt to evaluate an integral that may appear.)

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