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Write out the total wave function \(\Psi(x, t)\) for an electron in the \(n=3\) state of a \(10 \mathrm{nm}\) wide infinite well. Other than the symbols \(x\) and \(t,\) the function should include only numerical values.

Short Answer

Expert verified
\(\Psi(x,t) = \sqrt{\frac{2}{10^{-9}}}\sin \left(\frac{3\pi x} {10^{-9}} \right) \cdot e^{(-i \frac{9 \pi^2 (1.0545718 \times 10^{-34}) t}{2 * (9.10938356\times10^{-31}) * (10^{-9})^2})} \)

Step by step solution

01

Get Spatial Component

Substitute the values into the spatial function as follows: \(\psi(x)=\sqrt{\frac{2}{10^{-9}}}\sin \left(\frac{3\pi x} {10^{-9}} \right)\)
02

Get Temporal Component

Now, substitute the values into the temporal function. Remember that \(\hbar = 1.0545718 \times 10^{-34} \mathrm{m}^2 \mathrm{kg} / \mathrm{s}\) and the mass of an electron \(m = 9.10938356\times10^{-31}\):\(\phi(t) = e^{(-i \frac{(3)^2 \pi^2 (1.0545718 \times 10^{-34}) t}{2 * (9.10938356\times10^{-31}) * (10^{-9})^2})}\)
03

Form Total Wave Function

Combine both spatial and temporal parts to form the complete wave function: \(\Psi(x,t) = \psi(x) \cdot \phi(t)\)

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Key Concepts

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

Quantum Mechanics
The intriguing world of quantum mechanics diverges from classical physics, particularly at the atomic and subatomic scales. This realm is governed by principles that confound our everyday experiences, operating under rules that allow particles, like electrons, to exhibit wave-like properties, and vice versa. This dual nature is captured elegantly in the concept of the wave function, a mathematical expression that summarizes all that can be known about a quantum system.

The exercise provided explores quantum mechanics by asking students to calculate the wave function for an electron in a specific quantum state within an infinite potential well. To understand this, it's vital to grasp that unlike the orbits of planets, the position and momentum of an electron cannot be pinpointed simultaneously with absolute certainty. Instead, quantum mechanics describes probable locations and momenta through complex mathematical constructs called wave functions, denoted by \( \Psi(x, t) \). These wave functions evolve over time, encapsulating the probabilistic nature of quantum systems.
Electron Probability Amplitude
A critical concept within quantum mechanics is the probability amplitude for an electron's position. This concept emphasizes that the wave function represents more than just the wave nature of particles; it also provides a way to calculate the probability of finding an electron at a specific position. The square of an electron's wave function, \( |\psi(x)|^2 \), indicates the probability density – the likelihood of locating an electron in a particular region of space.

The amplitude itself, represented by \( \psi(x) \), provides the spatial component of an electron's wave function in the step-by-step solution. When this spatial wave function is combined with its temporal counterpart, \( \phi(t) \), it defines the state of the electron over time. By following these steps, students can uncover the beautifully complex dance of probabilities that dictates where an electron might be at any given moment.
Infinite Potential Well
An infinite potential well is a quintessential concept in quantum mechanics, serving as a fundamental model for understanding the quantization of energy levels in a confined space. Imagine a particle, like an electron, trapped inside a well with perfectly rigid walls that it cannot escape. This well is a hypothetical construct used to simplify the complex reality of particle confinement.

Within this well, the particle's energy levels are discrete, meaning the electron can only occupy certain states, each corresponding to a distinct quantum number \( n \). The solution provided showcases the calculation for the \( n=3 \) state, indicating the third allowable energy state for the electron in the well. For students, visualizing these energy states can be as simple as picturing a musical instrument's strings, where each vibration mode corresponds to a different note – except in quantum mechanics, each 'note' represents a possible energy level for the particle.

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Most popular questions from this chapter

The quantized energy levels in the infinite well get farther apart as \(n\) increases, but in the harmonic oscillator they are equally spaced. (a) Explain the difference by considering the distance "between the walls" in each case and how it depends on the particle's energy. (b) A very important bound system, the hydrogen atom, has energy levels that actually get closer together as \(n\) increases. How do you think the separation between the potential energy "walls" in this system varies relative to the other two? Explain.

Determine the expectation value of the position of a harmonic oscillator in its ground state.

A particle is described by the wave function $$ \psi(x)=\frac{\sqrt{2 / \pi}}{x^{2}-x+1.25} $$ (a) Show that the normalization constant \(\sqrt{2 / \pi}\) is correct. (b) A measurement of the position of the particle is to be made. At what location is it most probable that the particle would be found? (c) What is the probability per unit length of finding the particle at this location?

Consider a particle of mass \(m\) and energy \(E\) in a region where the potential energy is a constant \(U_{0}\). greaterthan E. and the region extends to \(x=+\infty\). (a) Guess a physically acceptable solution of the Schrödinger equation in this region and demonstrate that it is a solution. (b) The region noted in part (a) extends from \(x=+1 \mathrm{~nm}\) to \(+\infty\). To the left of \(x=1 \mathrm{~nm}\), the particle's wave function is \(D \cos \left(10^{9} \mathrm{~m}^{-1} x\right)\). Is \(U(x)\) also greater than \(E\) here? (c) The particle's mass \(m\) is \(10^{-30} \mathrm{~kg}\). By how much (in \(\mathrm{eV}\) ) does \(U_{0}\), the potential energy prevailing from \(x=1 \mathrm{~nm}\) to \(+\infty\), exceed the particle's energy?

In Section \(5.5\). it was shown that the infinite well coergis follow simply from \(\Lambda=h / p\), the fornulafor kinelic encrgy. \(p^{2} / 2 m\); and a famous standing-wave condition \(\lambda=2 U_{n} .\) The arguments are perfectly valid when the potential energy is 0 (inside the well) and \(L\) is strictly conskant, but they can also be useful in other cases. The length \(L\) allowed the wave should be roughly the distance between the classical tuming points, where there is no kinetic eneigy left. Apply these arguments to the oscillator potential energy, \(U(x)=\frac{1}{2} \kappa x^{2}\). Find the location \(x\) of the classical tuming point in terms of \(E\); use nwice this distance for L: then insert this into the infinite well eneigy fonnula so that \(E\) appears on both sides. Thus far, the procedure Ieally only deals with kinctic energy. Assume, as is tue for a classical oscillator, that there is as much potential eneigy, on average, as kinetic energy. What do you obtain for the quantized energies?

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