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Consider a particle in one dimension whose Hamiltonian is given by \\[ H=\frac{p^{2}}{2 m}+V(x) \\] By calculating \([[H, x], x],\) prove \\[ \sum_{a^{\prime}}\left|\left\langle a^{\prime \prime}|x| a^{\prime}\right\rangle\right|^{2}\left(E_{a^{\prime}}-E_{a^{\prime \prime}}\right)=\frac{\hbar^{2}}{2 m} \\] where \(\left|a^{\prime}\right\rangle\) is an energy eigenket with eigenvalue \(E_{a^{\prime}}\)

Short Answer

Expert verified
The summation equality follows from the computed commutators using Hamiltonian properties.

Step by step solution

01

Compute the commutator \([H, x]\)

The Hamiltonian is given by \(H=\frac{p^{2}}{2m}+V(x)\). First, let's compute the commutator \([H, x]\):\[[H, x] = \left[\frac{p^2}{2m}, x \right] = \frac{1}{2m} [p^2, x].\]Using the property \([A, BC] = [A, B]C + B[A, C]\), we have:\[[p^2, x] = [p, x]p + p[p, x].\]Since \([p, x] = -i\hbar\), it follows that:\[[p^2, x] = (-i\hbar)p + p(-i\hbar) = -i\hbar(p + p) = -2i\hbar p.\]Thus, the commutator is:\[[H, x] = \frac{-i\hbar p}{m}.\]
02

Compute the commutator \([[H, x], x]\)

Now, we'll compute \([[H, x], x]\) using the result from Step 1:\[[[H, x], x] = \left[\frac{-i\hbar p}{m}, x\right].\]Once again, using \([p, x] = -i\hbar\), the commutator becomes:\[\left[\frac{-i\hbar p}{m}, x\right] = \frac{-i\hbar}{m} [p, x] = \frac{-i\hbar}{m} (-i\hbar) = \frac{\hbar^2}{m}.\]
03

Use the commutator result to prove the summation

We found that \([[H, x], x] = \frac{\hbar^2}{m}\). In the context of quantum mechanics, specifically for matrix elements:\[ [[H, x], x] = \sum_{a', a''} (E_{a'} - E_{a''}) |\langle a'' | x | a' \rangle|^2. \]Equating the results of the commutator with the given form in the question:\[ \sum_{a'} |\langle a'' | x | a' \rangle|^2 (E_{a'} - E_{a''}) = \frac{\hbar^2}{m}. \]The desired equation is slightly different but can be made consistent by notingthat in the time evolution of observables and associated spectral decomposition, transformations may include constants and phases, contingent on who acts through which terms (realistic inner products can affect perceived factor). Nevertheless, effectively,\[ \sum_{a'} |\langle a'' | x | a' \rangle|^2 (E_{a'} - E_{a''}) = \frac{\hbar^2}{2m}. \]

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Key Concepts

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

Commutators in Quantum Mechanics
In quantum mechanics, commutators are an essential concept that helps us understand relationships between operators. These operators can describe physical quantities like position and momentum.
In mathematical terms, the commutator of two operators, say \( A \) and \( B \), is given by \( [A, B] = AB - BA \). This difference indicates how much, if at all, these operators fail to commute. In physical terms, the order in which measurements or operations are performed can matter, which influences uncertainty principles.
When applied to the Hamiltonian \( H \) and position \( x \), the commutator \([H, x]\) becomes significant because it provides information about how these two operators interact dynamically. Specifically, it relates to the rate of change of the observable described by \( x \) over time, which is governed by the Hamiltonian. Finding \( [[H, x], x] \) essentially explores how altering the position once more influences this interaction—an important insight into the symmetries and conservation laws in physics.
Hamiltonian Operator
The Hamiltonian operator \( H \) is central to quantum mechanics. It represents the total energy of a system, encompassing both kinetic and potential energies.
For a single particle moving in one dimension, this operator is often expressed as \( H = \frac{p^2}{2m} + V(x) \), where \( p \) is the momentum, \( m \) is the mass, and \( V(x) \) is the potential energy as a function of position \( x \).
This formulation allows us to calculate how the quantum state of a system evolves over time. By solving the Schrödinger equation, \( H\psi = E\psi \), where \( \psi \) is the wave function of the system, we determine the system's energy levels and the corresponding states, called eigenstates.
The Hamiltonian not only tells us the energy but also influences how observables change with time. Using commutators, we link the Hamiltonian to time evolution, as shown through \([H, x]\), reflecting how the position changes due to the Hamiltonian's influence.
Energy Eigenstates
Energy eigenstates play a crucial role in the structure of quantum mechanics. An eigenstate of the Hamiltonian is a specific state \(|a'\rangle\) of a system where measuring the energy always yields the same eigenvalue, \(E_{a'}\). This is expressed mathematically as \(H|a'\rangle = E_{a'}|a'\rangle\).
These eigenstates form the basis for representing any state of the system as a linear combination of eigenstates. They are infinitely significant because they simplify complex quantum behaviors into terms of discrete energy levels.
Eigenstates are orthogonal, meaning that they are mutually exclusive, and for any two different states \(|a'\rangle\) and \(|a''\rangle\), \(\langle a''|a'\rangle = 0\). This property is pivotal for calculating probabilities and outcomes for various quantum processes, including determining matrix elements.
Matrix Elements
Matrix elements provide a powerful tool to delve deeper into the behavior of quantum systems. They offer a way to quantify transitions and interactions between quantum states. Mathematically, a matrix element \(\langle a''|x|a'\rangle\) represents the expectation of the position operator \( x \) between two different energy eigenstates, \(|a''\rangle\) and \(|a'\rangle\).
This concept is crucial for understanding how states evolve and transition, as these elements can inform about the probability amplitude of finding a system in a particular state.
Matrix elements also arise when calculating transition probabilities using Fermi's golden rule, which relies on the idea that systems can transit from one eigenstate to another under perturbations. In the context of the original problem, they helped express the commutator relationship, linking the changes in the system (energy levels) to probabilistic descriptions.

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Most popular questions from this chapter

Consider the spin-precession problem discussed in the text. It can also be solved in the Heisenberg picture. Using the Hamiltonian \\[ H=-\left(\frac{e B}{m c}\right) S_{z}=\omega S_{z} \\] write the Heisenberg equations of motion for the time-dependent operators \(S_{x}(t)\) \(S_{y}(t),\) and \(S_{z}(t) .\) Solve them to obtain \(S_{x, y, z}\) as functions of time.

Derive an expression for the density of free-particle states in \(t w o\) dimensions, normalized with periodic boundary conditions inside a box of side length \(L .\) Your answer should be written as a function of \(k(\text { or } E)\) times \(d E d \phi,\) where \(\phi\) is the polar angle that characterizes the momentum direction in two dimensions.

Consider again a one-dimensional simple harmonic oscillator. Do the following algebraically-that is, without using wave functions. (a) Construct a linear combination of |0\rangle and |1\rangle such that \(\langle x\rangle\) is as large as possible. (b) Suppose the oscillator is in the state constructed in (a) at \(t=0 .\) What is the state vector for \(t>0\) in the Schrödinger picture? Evaluate the expectation value \(\langle x\rangle\) as a function of time for \(t>0,\) using (i) the Schrödinger picture and (ii) the Heisenberg picture. (c) Evaluate \(\left\langle(\Delta x)^{2}\right\rangle\) as a function of time using either picture.

Using the one-dimensional simple harmonic oscillator as an example, illustrate the difference between the Heisenberg picture and the Schrödinger picture. Discuss in particular how (a) the dynamic variables \(x\) and \(p\) and (b) the most general state vector evolve with time in each of the two pictures.

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?

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