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Consider an electron in the ground state of a hydrogen atom. (a) Sketch plots of \(E\) and \(U(r)\) on the same axes (b) Show that. classically, an electron with this energy should not be able to get farther than \(2 a_{0}\) from the proton. (c) What is the probability of the electron being found in the classically forbidden region?

Short Answer

Expert verified
The plots of \(E\) and \(U(r)\) intersect at \(2 a_{0}\), classically restricting the maximum distance of the electron to this value. Yet, there is a finite (non-zero) probability of finding the electron beyond this classical limit, in the forbidden region - demonstrating the unique quantum mechanical behavior of particles at atomic scales.

Step by step solution

01

- Sketch \(E\) and \(U(r)\) on the same axes

The total energy \(E\) and the potential energy \(U(r)\) of an electron in the ground state of a hydrogen atom are both negative quantities. They can be plotted on the same axes. The potential energy decreases with distance from the proton and it asymptotically approaches zero. The total energy \(E\) is a constant negative value, represented by a horizontal line below the x-axis.
02

- Show classically the electron should not be farther than \(2 a_{0}\)

Classically, an electron should not be able to get farther than the point where total energy \(E\) equals potential energy \(U(r)\). That is, \(E=U(r)\). The potential energy \(U(r)\) is given by \(-e^{2}/4\pi \varepsilon_{0}r\), where \(e\) is the charge of the electron, \(\varepsilon_{0}\) is the permittivity of vacuum, and \(r\) is distance from the proton. For the ground state, \(E=-13.6\) eV. Equating \(E\) and \(U(r)\), and solving for \(r\) gives \(r=2a_{0}\), where \(a_{0}\) is the Bohr radius (~0.53 Å). Therefore, classically, an electron with this energy should not be able to get farther than \(2 a_{0}\) from the proton.
03

- Probability of electron in the classical forbidden region

Quantum mechanically, the probability of an electron being found at a given radial distance is given by \(|\psi(r)|^{2}\), where \(\Psi(r)\) is the wavefunction. In the ground state of a hydrogen atom, \(\Psi(r)\) is given by \(\Psi(r) = \dfrac{1}{\sqrt{\pi a_{0}^{3}}} e^{-r/a_{0}}\). The probability of finding the electron in the classical forbidden region (i.e., \(r > 2a_{0}\)) is found by calculating \(\int_{2a_{0}}^{\infty} |\Psi(r)|^{2} 4\pi r^{2} dr\). Solving this gives a finite value, meaning that there is a nonzero probability of the electron being in the classical forbidden region.

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Key Concepts

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

Quantum Mechanics
Quantum mechanics is a fundamental theory in physics that provides a description of the physical properties of nature at the scale of atoms and subatomic particles. Unlike classical mechanics, where objects are treated as particles with defined positions and velocities, quantum mechanics introduces the concept of wave-particle duality. This means that subatomic particles, like electrons, exhibit properties of both particles and waves.

The behavior of an electron in an atom is described by a mathematical function called a wavefunction, which provides information about the probability of finding a particle in a particular region of space, rather than exact location. The strange and non-intuitive principles of quantum mechanics, such as uncertainty and superposition, reveal the complex nature of the interactions at the subatomic level and challenge our classical understanding of physics.
Bohr Model
The Bohr model was proposed by Niels Bohr in 1913 to explain how electrons can have stable orbits around the nucleus without radiating away their energy, which classical electromagnetism would predict. According to the Bohr model, electrons orbit the nucleus in specific paths, or orbits, without radiating energy, as long as they remain in these orbits. Each orbit corresponds to a certain energy level, with the lowest energy state known as the ground state.

In the context of the hydrogen atom, the Bohr model accurately predicts the spectral lines, however, it was later superseded by quantum mechanics which provides a more comprehensive and accurate framework, especially for complex atoms. Nonetheless, the Bohr model remains a significant step towards our understanding of quantum mechanics.
Classical vs Quantum Probability
In classical physics, probability is often associated with ignorance of the exact states of a system. For example, if we flip a coin, the outcome can be either heads or tails, due to our lack of knowledge of the initial conditions. However, in a quantum mechanical context, probability takes on a different meaning.

Quantum probability is intrinsic to the nature of particles; it's not just due to our lack of knowledge. The position of an electron in a hydrogen atom, described by its wavefunction, is fundamentally probabilistic. True to quantum mechanics, even if we knew everything about the electron, we could only predict the probability of finding it in a certain region—never a specific location.
Wavefunction of Electron
The wavefunction of an electron in an atom is a central concept in quantum mechanics which mathematically represents the quantum state of the particle. For the hydrogen atom, the ground state wavefunction, or \(\Psi(r)\), describes the probability amplitude of finding the electron at a distance \(r\) from the nucleus.

Specifically, for the ground state of hydrogen, the wavefunction is spherically symmetric and decreases rapidly as the distance from the nucleus increases. It is the squared magnitude of this wavefunction, \(\left|\Psi(r)\right|^2\), that gives us the probability density which we integrate over a volume to obtain the likelihood of the electron's presence in a given region.
Potential Energy in Atoms
Potential energy in atoms arises from the forces that act between the negatively charged electrons and the positively charged nucleus. In a hydrogen atom, this potential energy is negative, which indicates that work must be done to pull the electron away from the nucleus.

The shape of the potential energy curve, \(U(r)\), dictates that electrons closer to the nucleus are in lower energy states, while those further away are in higher energy states. The ground state of an electron is characterized by it having the lowest possible potential energy. In a graph of potential energy versus distance from the nucleus, at large distances, the potential energy approaches zero, indicating a decrease in the attractive force as the electron moves away from the nucleus.

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