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Lecture 7: Operators, Free Particles and the Quantum Superposition Principle

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    38872
  • Overview of Lecture 6:

    The equation that substitutes for Newton's equations of motion in classical mechanics (trajectories) is the Schrödinger Equation, which is a wave-equation discussed last week and solutions of which are called wavefunctions. There are two "flavors" of the Schrödinger Equation, the time dependent and the time independent.

    \[\hat{H} \psi (x,t) = i \hbar \dfrac{\partial}{\partial t} \psi(x,t) \nonumber\]

    The time-dependent Schrödinger Equation results time-dependent wavefunctions with both spatial aspect and a temporal aspects,

    \[\hat{H}\psi (x)=E \psi (x) \nonumber\]

    The time-independent Schrödinger Equation results in time-independent wavefunctions with only a spatial aspect (the temporal aspects). Which one we use depends on if there is an explicit time-dependence in the Hamiltonian \(\hat{H}\), which is an operator that represents the total energy (e.g., kinetic and potential) of the system. All the topics in Chem 110A, require the use of time-independent Schrödinger Equation, but it is important to recognize that the true wavefunction ALWAYS has a temporal part (we are just ignoring it).

    Via the Correspondence Principle, all measurements are eigen-value problems with different operators representing different observables. The observables are typically quantized and are the eigenvalues of the operator. If we are talking the Hamiltonian operation, then the eigenvalues are energies and the eigenvectors of the the wavefunctions (often called eigenvectors)

    Conceptually, applying operator \(\hat{A}\) to an eigenfunction such as \(\psi (x)\) gives an eigenvalue \(a\) back, multiplied by the same eigenfunction. Mathematically, this looks like

    \[\hat{A}\psi (x) = a\psi (x) \nonumber\]

    Example of operators:

    \[ \hat {\vec{p}} = -i \hbar \nabla \tag{linear momentum} \]

    \[ \hat {\vec{L}} = -i \hbar ( \vec{r} \times \nabla) \tag{angular momentum} \]

    \[ \hat {KE}_{quantum}= -\dfrac{\hbar^2}{2m} \nabla^2 \tag{kinetic energy} \]

    \[\hat{H}=-\dfrac{\hbar^2}{2m}\nabla^2+V(\vec{r}) \tag{total energy}\]

    Eigenstates and Eigenvectors and Eigenvalues

    Classical mechanic quantities are evaluated by operators in quantum mechanics. A wavefunction fully describes a system via operators. Conceptually, applying operator \(\hat{A}\) to an eigenfunction such as \(\psi (x)\) gives an eigenvalue \(a\) back, multiplied by the same eigenfunction. Mathematically, this looks like

    \[\hat{A}\psi (x) = a\psi (x)\]

    Applying this concept to the Schrödinger equation is similar. The Schrödinger equation is an eigenvalue problem where the operator in one dimension is

    \[\dfrac {-\hbar^2}{2m} \dfrac{d^2}{d x^2}\]

    This is commonly referred to as the Hamiltonian with the operator symbol \(\hat{H}\). Rewriting the equation to

    \[\hat{H} \psi (x) = E\psi (x)\]

    gives a clearer picture - the energy of the wave function is found when applying the Hamiltonian to the wave function.

    Eigenstate, Eigenvalues, Wavefunctions, and Measurables

    Often in discussions of quantum mechanics, the terms eigenstate and wavefunction are used interchangeably. The term eigenvalue is used to designate the value of measurable quantity associated with the wavefunction. For example, when discussing the eigenstates of the Hamiltonian (\(\hat{H}\)), the associated eigenvalues represent energies and within the context of the momentum operators, the associated eigenstate refer to the momentum of the particle.

    Commonly Used Operators

    Although we could theoretically come up with an infinite number of operators, in practice there are a few which are much more important than any others.

    • Linear Momentum:

    The linear momentum operator of a particle moving in one dimension (the \(x\)-direction) is

    \[\hat p_x = -i \hbar \dfrac{\partial}{\partial x} \label{3.3.7}\]

    and can be generalized in three dimensions:

    \[ \hat {\vec{p}} = -i \hbar \nabla \label{3.3.8}\]
    • Kinetic Energy

    Classically, the kinetic energy of a particle moving in one dimension (the \(x\)-direction), in terms of momentum, is

    \[KE_{classical}= \dfrac{p_x^2}{2m} \label{3.3.9}\]

    Quantum mechanically, the corresponding kinetic energy operator is

    \[ \hat {KE}_{quantum}= -\dfrac{\hbar^2}{2m} \dfrac{\partial^2}{\partial x^2}\label{3.3.10}\]

    and can be generalized in three dimensions:

    \[ \hat {KE}_{quantum}= -\dfrac{\hbar^2}{2m} \nabla^2 \label{3.3.11}\]

    • Angular Momentum:

    Angular momentum requires a more complex discussion, but is the cross product of the position operator \(\hat{\vec{r}}\) and the momentum operator \(\hat p\)

    \[ \hat {\vec{L}} = -i \hbar ( \vec{r} \times \nabla) \label{3.3.12}\]

    • Hamiltonian:

    The Hamiltonian operator corresponds to the total energy of the system

    \[\hat {H} = - \dfrac{\hbar^2}{2m} \dfrac{{\partial}^2}{{\partial x}^2} + V(x) \label{3.3.13}\]

    and it represents the total energy of the particle of mass \(m\) in the potential \(V(x)\). The Hamiltonian in three dimensions is

    \[\hat{H}=-\dfrac{\hbar^2}{2m}\nabla^2+V(\vec{r}) \label{3.3.5a}\]

    • Energy:

    The energy operator from the time-dependent Schrödinger equation

    \[ i \hbar \dfrac{\partial}{\partial t} \Psi(x,t)= \hat {H}\Psi(x,t) \label{3.3.14}\]

    The right hand side of Equation \(\ref{3.3.14}\) is the Hamiltonian Operator.

    Wavefunctions Have a Probabilistic Interpretation

    The Born interpretation therefore calls the wavefunction the probability amplitude, the absolute square of the wavefunction is called the probability density, and the probability density times a volume element in three-dimensional space (\(d\tau\)) is the probability \(P\)

    \[ P(\vec{r},t)= \Psi^*(r,t) \Psi(r,t) = {|\Psi(r,t)|}^2 \]

    The probability that a single quantum particle moving in one spatial dimension will be found in a region \(x\in[a,b]\) if a measurement of its location is performed is

    \[P(x\in[a,b])=\int_{a}^{b}|\psi (x)|^2 dx \label{3.4.2}\]

    In three dimensions, Equation \(\ref{3.4.2}\) is represented differently

    \[P(x \in[a,b])=\int_{a}^{b}|\psi (\vec{\tau})|^2 d\tau \label{3.4.3}\]

    The Quantum Mechanical Free Particle

    The simplest system in quantum mechanics has the potential energy \(V=0\) everywhere. This is called a free particle since it has no forces acting on it. We consider the one-dimensional case, with motion only in the \(x\)-direction, giving the time-independent Schrödinger equation

    \[- \dfrac{\hbar^{2}}{2m}\dfrac{d^{2}\psi (x)}{dx^2}= E\psi (x)\label{1}\]

    or more simply

    \[ \hat{H} \psi (x)= E\psi (x)\label{H1}\]

    with

    \[ \hat{H} = - \dfrac{\hbar^{2}}{2m}\dfrac{d^{2} }{dx^2} \label{H2}\]

    Total derivatives can be used since there is one independent variable. The equation simplifies to

    \[\psi'' (x)+k^{2}\psi (x)=0\label{2}\]

    with the definition

    \[k^2 \equiv \dfrac{2mE}{\hbar^2}\label{3}\]

    Possible solutions of Equation \ref{2} are

    \[\psi (x)= const\begin{Bmatrix}
    \sin(kx)\\
    \cos(kx)\\
    e^{\pm ikx}\end{Bmatrix}\label{4}\]

    There is no restriction on the value of \(k\). Thus a free particle, even in quantum mechanics, can have any non-negative value of the energy

    \[E=\dfrac{\hbar^2k^2}{2m}\geq 0\label{5}\]

    The energy levels in this case are not quantized and correspond to the same continuum of kinetic energy shown by a classical particle.

    Example \(\PageIndex{1}\): Eigenstates of the Hamiltonian of a free particle

    Consider for a free particle (i.e., \(V(x)=0\)) moving in one dimension.

    1. Demonstrate that \(\sin (kx)\) is an eigenfunction of \(\hat{H}\).
    2. What are their corresponding eigenstates?
    3. Why are the energies not quantized?
    Approach

    To demonstrate that a function is indeed a specific eigenfunction \(f(x)\) of an operator \(\hat{O}\), we have to ask if this Eigenvalue equation is correct, i.e., \[ \hat{O} f(x) = \lambda f(x) \label{Eigen1}\] where \(\lambda\) is the eigenvalue associated with that eigenfunction associated with the operator. Change the operator and the eigenfunctions and eigenvalues will change. Change the eigenfunction and the eigenvalue will change. They are all connected like the Mufasa's "Circle of Life."

    Solution A

    Let's take the \(\sin (kx)\) function and the Hamiltonian operator (Equation \ref{H2}) and insert it into Equation \ref{Eigen1} and is if the equality is ensured. Keep in mind that any value of \(lambda\) will work as long as it is a constant.

    \[ - \dfrac{\hbar^{2}}{2m}\dfrac{d^{2}}{dx^2} \sin (kx) \overset{?}{=} \lambda \sin (kx) \label{Eigen1A}\]

    first step in evaluating the 2nd derivative

    \[ - \dfrac{\hbar^{2}}{2m} k \dfrac{d }{dx} (\cos (kx)) \overset{?}{=} \lambda \sin (kx) \label{Eigen1B}\]

    and second step

    \[ + \dfrac{\hbar^{2}}{2m} k^2 (\sin (kx)) \overset{?}{=} \lambda \sin (kx) \label{Eigen1C}\]

    This equation is confirmed when

    \[\lambda = + \dfrac{\hbar^{2} k^2}{2m} \]

    Which makes sense when compared to Equation \ref{5} since the Hamiltonian gives the total energy \(E\).

    Solution B

    As shown in the Solution A, the Eigenvalue equation is confirm to be correct for all \(\sin (kx)\) functions (so they are eigenfunctions of the Hamiltonian) and the eigenvalues are \[\lambda = + \dfrac{\hbar^{2} k^2}{2m} .\] Eigenvalues can be positive, negative, real, imaginary and complex and all of the above.

    Solution C

    Since any value of \(k\) is allowed in the \(\sin (kx)\) eigenfunctions (i.e., the Eigenvalue equation holds for all values of \(k\)), then there is no quantization. We need boundary conditions to force the quantization like with the Bohr hydrogen atom.

    A free particle, even in quantum mechanics, can have any non-negative value of the energy

    It is of interest also to consider the x-component of linear momentum for the free-particle solutions (Equation \ref{4}). The eigenvalue equation for momentum is

    \[\hat{p}_{x}\psi (x)=-i\hbar\dfrac{d\psi (x)}{dx}=p\psi (x)\label{6}\]

    where we have denoted the momentum eigenvalue as \(p\).

    2000px-Propagation_of_a_de_broglie_plane_wave.svg.png

    Figure \(\PageIndex{1}\): Propagation of quantum free particle (i.e. de Broglie waves) in 1D space. The real part of the complex amplitude is blue and imaginary part is green. The probability (shown as the yellow opacity) of finding the particle at a given point \(x\) is spread out evenly over space, there is no definite position of the particle. Image used with permission (Public Domain; Maschen).

    Back to the Superposition Principle

    The functions \(\sin kx\) and \(\cos kx\) are not eigenfunctions of \(\hat{p}_{x}\), but are each superpositions of the two eigenfunctions \(e^{\pm ikx}\), by virtue of the trigonometric identities

    \[\cos (kx)=\dfrac{1}{2}(e^{ikx} +e^{-ikx})\]

    and

    \[\sin(kx)= \dfrac{1}{2i}(e^{ikx} -e^{-ikx})\label{7}\]

    The eigenfunction \(e^{ikx}\) for \( k > 0\) represents the particle moving from left to right on the x-axis (blue curve in Figure \(\PageIndex{2}\)) with momentum \(p > 0\). Correspondingly, \(e^{-ikx}\) represents motion from right to left with \(p < 0\) (red curve in Figure \(\PageIndex{2}\)).

    Standing_wave_2.gif

    Two waves traveling in opposite directions across the same medium combine linearly. In this animation, both waves have the same wavelength and the sum of amplitudes results in a standing wave. Image used with permission (Public Domain; LucasVB)

    Wavepackets - The Superposition Principle in Action

    If we add together two sine waves with frequencies close together, we get "beats." This pattern can be viewed as a string of wavepackets. For example, consider adding two sine waves together with spatial and temporal frequencies of \((k \pm \Delta k\)) and (\( \omega \pm \Delta \omega\)), respectively.

    \[\sin \left[(k - \Delta k) x - (\omega - \Delta \omega) t \right] + \sin \left[ (k + \Delta k) x - ( \omega + \Delta \omega )t \right]) \label{WP1}\]

    If we we use the trigonometric addition formula, the sum in Equation \ref{WP1} can be simplified to

    \[ 2 \sin (kx - \omega t ) \cos \left[ (\Delta k) x - (\Delta \omega)t \right] \label{beats}\]

    Sine waves extend to infinity in both spatial directions, so they cannot represent a particle whose wavefunction is nonzero in a limited region of space. Physically, that it must have a wavefunction that goes to zero far away in either direction. A localized wavefunction of this type is called a “wavepacket”. A wavepacket can be constructed by adding plane waves together.

    Sequential_superposition_of_plane_waves.gif

    Figure \(\PageIndex{3}\): The superposition of several plane waves to form a wave packet. This wave packet becomes increasingly localized with the addition of many waves. The Fourier transform is a mathematical operation that separates a wave packet into its individual plane waves. Note that the waves shown here are real for illustrative purposes only, whereas in quantum mechanics the wavefunction is generally complex. Image used with permission (Public Domain; Teply).

    This wavepacket perspective of a free particle is shown in Figure \(\PageIndex{4}\), where the wavefunction amplitude (both real and imaginary) is localized and tapers off on either side (constrast this image with Figure \(\PageIndex{1}\) that exhibits uniform amplide over all space since it is a oscillatory eigenfunction.

    Wavepacket 2.png

    Figure \(\PageIndex{4}\): Propagation of quantum free particle wavepacket in 1D space. The real part of the complex amplitude is blue and imaginary part is green. The probability (shown as the yellow opacity) of finding the particle at a given point \(x\) is localize with a specific "position" (technically range thereof) of the particle. Image used with permission (Public Domain; Maschen).

    What do you want to master for any specific quantum problem?

    1. The appropriate Hamiltonian (\(\hat{H}\)) for the system
    2. The specific functional form for the solutions of the Eigenvalue problem with this operator.
    3. The specific functional form of the eigenvalues associated with the eigenfunctions (i. e., solutions)
    4. Identify the relevant quantum number(s) for the solution
    5. Identify the relevant range of the quantum numbers.

    Once you get these basics down, then you can start to do some fun quantuming.