/*! 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 29 (a) An electron with initial kin... [FREE SOLUTION] | 91Ó°ÊÓ

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(a) An electron with initial kinetic energy \(32 \mathrm{eV}\) encounters a square barrier with height \(41 \mathrm{eV}\) and width \(0.25 \mathrm{nm}\). What is the probability that the electron will tunnel through the barrier? (b) A proton with the same kinetic energy encounters the same barrier. What is the probability that the proton will tunnel through the barrier?

Short Answer

Expert verified
The calculation yields that the electron has a significantly higher probability to tunnel through the barrier compared to the proton, due to its smaller mass. This disparity between the two particles is a consequence of the particle's mass being inversely proportional to the tunneling probability.

Step by step solution

01

Calculate the Energy Difference and Velocity

Calculate the energy difference between the barrier and the kinetic energy of the particle, \( \Delta E = E_{barrier}-E_{particle} = 41eV-32eV = 9eV \). Also, calculate the velocity, \( v = \sqrt{(2E_{particle})/m} \), for both particles using their respective masses (electron: \( m_e = 9.10938356 \times 10^{-31} kg \), proton: \( m_p = 1.67262192 \times 10^{-27} kg \)).
02

Calculate the Tunneling Probability

Use the formula for tunneling, \(T = e^{-2 \sqrt{(2m_a \Delta E)}w/h}\), where \(T\) is the tunneling probability, \(w\) is the width of the barrier, \( \Delta E \) is the energy difference, and \( h \) is the reduced Planck's constant. Compute \(T\) for both electron and proton.
03

Convert Units

Ensure all units are in the International System (SI) before performing the computation. For example, convert electric volt (eV) into Joules (J), express the width of the barrier in meters (m), and use the reduced Planck's constant in J.s.

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Key Concepts

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

Kinetic Energy
Kinetic energy is the energy that an object possesses due to its motion. In this context, we're looking at the kinetic energy of particles such as electrons and protons. The kinetic energy of a particle is given by the formula \( KE = \frac{1}{2}mv^2 \), where \( m \) is the mass of the particle and \( v \) is its velocity.
This property is crucial when discussing quantum tunneling because it helps determine the potential for a particle to overcome a barrier. For instance, in our exercise, the kinetic energy of each particle (electron and proton) is \(32 \mathrm{eV}\).
This initial energy partially dictates the probability of the particle being able to tunnel through a barrier that has a higher potential energy threshold.
Square Barrier
A square barrier refers to a potential energy barrier that has a constant height for a certain width. This means the particle will encounter the same amount of resistance across the barrier that it must "tunnel" through.
The square barrier in this problem has a height of \(41 \mathrm{eV}\) and a width of \(0.25 \mathrm{nm}\). These values set up the potential challenge an electron or proton would face when encountering the barrier.
Although the kinetic energy of the particles is less than the barrier height, quantum mechanics provides a mathematical framework to explore the possibility of tunneling through.
Tunneling Probability
Tunneling probability is the likelihood that a quantum particle will pass through a potential barrier that it classically would not be able to surpass due to its kinetic energy being lower than the barrier height.
We calculate this probability using the formula \( T = e^{-2 \sqrt{(2m \Delta E)}w/\hbar} \), where \( \Delta E \) is the energy difference between the barrier height and particle's kinetic energy, \( m \) is the particle's mass, \( w \) is the width of the barrier, and \( \hbar \) is the reduced Planck's constant.
This probability is exponentially dependent on the mass and energy difference, meaning lighter particles like electrons have a higher chance of tunneling than heavier particles like protons.
Differential Equations
Differential equations are a type of mathematical equation that involve functions and their derivatives. In quantum mechanics, these equations describe how quantum states change over time.
The Schrödinger equation is a fundamental differential equation used in quantum mechanics to determine the wave function of a quantum system.
For quantum tunneling, solving this equation under the potential barrier gives us the exponential decay form that leads to the tunneling probability. It provides insights into the behavior and characteristics of particles interacting with potential barriers, such as wave-like properties and probabilities.
Planck's Constant
Planck's constant \( h \) is a fundamental constant in physics that describes the quantization of physical properties. The reduced version, denoted as \( \hbar = \frac{h}{2\pi} \), frequently appears in quantum mechanics equations.
This constant is pivotal in determining the scale at which quantum effects become significant. In the exercise, it's used to calculate the tunneling probability of particles traveling through a barrier.
Planck's constant helps link the energy of particles to the frequency of their associated wave, thus, playing a critical role in understanding and calculating the quantum tunneling phenomena.

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Most popular questions from this chapter

An electron is in a one-dimensional box. When the electron is in its ground state, the longest-wavelength photon it can absorb is \(420 \mathrm{nm} .\) What is the next longest-wavelength photon it can absorb, again starting in the ground state?

Dots that are the same size but made from different materials are compared. In the same transition, a dot of material 1 emits a photon of longer wavelength than the dot of material 2 does. Based on this model, what is a possible explanation? (a) The mass of the confined particle in material 1 is greater. (b) The mass of the confined particle in material 2 is greater. (c) The confined particles make more transitions per second in material 1 . (d) The confined particles make more transitions per second in material 2 .

A particle with mass \(m\) is in a one-dimensional box with width \(L\). If the energy of the particle is \(9 \pi^{2} \hbar^{2} / 2 m L^{2},\) (a) what is the linear momentum of the particle and (b) what is the ratio of the width of the box to the de Broglie wavelength \(\lambda\) of the particle?

When low-energy electrons pass through an ionized gas, electrons of certain energies pass through the gas as if the gas atoms weren't there and thus have transmission coefficients (tunneling probabilities) \(T\) equal to unity. The gas ions can be modeled approximately as a rectangular barrier. The value of \(T=1\) occurs when an integral or half-integral number of de Broglie wavelengths of the electron as it passes over the barrier equal the width \(L\) of the barrier. You are planning an experiment to measure this effect. To assist you in designing the necessary apparatus, you estimate the electron energies \(E\) that will result in \(T=1\). You assume a barrier height of \(10 \mathrm{eV}\) and a width of \(1.8 \times 10^{-10} \mathrm{~m} .\) Calculate the three lowest values of \(E\) for which \(T=1\)

One advantage of the quantum dot is that, compared to many other fluorescent materials, excited states have relatively long lifetimes (10 ns). What does this mean for the spread in the energy of the photons emitted by quantum dots? (a) Quantum dots emit photons of more well-defined energies than do other fluorescent materials. (b) Quantum dots emit photons of less well-defined energies than do other fluorescent materials. (c) The spread in the energy is affected by the size of the dot, not by the lifetime. (d) There is no spread in the energy of the emitted photons, regardless of the lifetime.

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