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What is the probability that an electron in the ground state of hydrogen will be found inside the nucleus? (a) First calculate the exact answer, assuming the wave function (Equation 4.80) is correct all the way down to \(r=0 .\) Let \(b\) be the radius of the nucleus. (b) Expand your result as a power series in the small number \(\epsilon \equiv 2 b / a\), and show that the lowest-order term is the cubic: \(P \approx(4 / 3)(b / a)^{3}\). This should be a suitable approximation, provided that \(b \ll a\) (which it \(i s\) ). (c) Alternatively, we might assume that \(\psi(r)\) is essentially constant over the (tiny) volume of the nucleus, so that \(P \approx(4 / 3) \pi b^{3}|\psi(0)|^{2}\). Check that you get the same answer this way. (d) Use \(b \approx 10^{-15} \mathrm{m}\) and \(a \approx 0.5 \times 10^{-10} \mathrm{m}\) to get a numerical estimate for \(P .\) Roughly speaking, this represents the "fraction of its time that the electron spends inside the nucleus."

Short Answer

Expert verified
The probability is approximately \(2.688 \times 10^{-15}\).

Step by step solution

01

Use the wave function for the hydrogen atom

The wave function of a hydrogen atom's electron in its ground state is given by \( \psi(r) = \frac{1}{\sqrt{\pi}} \left( \frac{1}{a} \right)^{3/2} e^{-r/a} \), where \(a\) is the Bohr radius. This will be utilized to find the probability of the electron being inside the nucleus.
02

Calculate the exact probability

To find the probability \(P\) that the electron is inside the nucleus, integrate the probability density \(\psi^2(r)\) from \(r=0\) to \(r=b\): \[ P = \int_0^b \left( \frac{1}{\pi a^3} e^{-2r/a} \right) 4\pi r^2 \, dr \]. Evaluating, \( P = 1 - e^{-2b/a} \left(1 + \frac{2b}{a} + \left(\frac{2b}{a}\right)^2 \right) \).
03

Expand and approximate probability

Assume \( \epsilon = 2b/a\) is small to expand the exponential function for a power series. We have \[ P \approx \frac{4}{3} \left( \frac{b}{a} \right)^3 \] as the lowest order term in \( \epsilon \) for small \(b/a\).
04

Alternative approximation for constant wave function

Assume that \(\psi(r)\) is constant over the nucleus: \(\psi(r) \approx \psi(0)\). Then the probability is \( P \approx \int_0^b |\psi(0)|^2 \, 4\pi r^2 \, dr \). Simplifying, it gives \( P \approx \frac{4}{3} \pi b^3 |\psi(0)|^2 \), matching the form from Step 3.
05

Calculate numerical estimate for P

Using given values, \(b \approx 10^{-15}\,\text{m}\) and \(a \approx 0.5 \times 10^{-10}\,\text{m}\), calculate the numerical probability: \[ P \approx \frac{4}{3} \left( \frac{10^{-15}}{0.5 \times 10^{-10}} \right)^3 \approx 2.688 \times 10^{-15} \]. This indicates the fraction of time an electron spends inside the nucleus.

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Key Concepts

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

Hydrogen Atom
The hydrogen atom is one of the simplest and most extensively studied atomic systems in quantum mechanics. It consists of a single proton as its nucleus and one electron orbiting it. This simplicity makes it an ideal model for introducing and understanding foundational concepts in quantum mechanics.

In quantum terms, the hydrogen atom is often used to explore the idea of quantized energy levels. The electron can only occupy specific energy levels or "orbits," which are determined by the solutions to the Schrödinger equation. These solutions predict the electron's behavior in terms of wave functions rather than classical paths.
  • The atom serves as an excellent model for radial probability distributions, where the radial component describes how electron probability varies with distance from the nucleus.
  • This model helps explain why electrons do not spiral into the nucleus, resolving a major inconsistency in classical physics.
The study of the hydrogen atom paves the way for understanding more complex atoms and the details of atomic structure.
Wave Function
In quantum mechanics, the wave function, denoted as \( \psi \), is a mathematical description of the quantum state of a particle. For the hydrogen atom, the wave function describes the behavior and distribution of the electron around the nucleus.

For the ground state (lowest energy level) of a hydrogen atom, the wave function is spherically symmetric and is given by:\[ \psi(r) = \frac{1}{\sqrt{\pi}} \left( \frac{1}{a} \right)^{3/2} e^{-r/a} \]Here, \( r \) represents the radial distance from the nucleus, and \( a \) is the Bohr radius.
  • Wave functions provide information about the likelihood of finding an electron at a particular point in space by yielding the probability density when squared.
  • They encapsulate both the particle and wave nature of an electron, reflecting the duality inherent in quantum particles.
The concept of a wave function is central in quantum mechanics, as it provides the most complete description available of a quantum system.
Probability Density
The probability density \( \psi^2 \) is derived from the wave function and provides insight into where an electron is most likely to be found at any given moment. In our example of the hydrogen atom, the probability density for the ground state is:\[ \psi^2(r) = \left( \frac{1}{\pi a^3} \right) e^{-2r/a} \]

This function indicates that the electron is more likely to be found closer to the nucleus and less likely as the distance increases.
  • Probability density helps in visualizing the cloud-like electron distribution around the nucleus, often referred to as an "electron cloud."
  • Integrating the probability density over a certain range allows us to compute the actual probability of finding an electron within that region.
In essence, the probability density provides a practical way to map the extent and intensity of electron presence in different regions around the nucleus.
Bohr Radius
The Bohr radius, denoted as \( a \), is a fundamental constant in quantum mechanics. It represents the most probable distance from the nucleus at which the electron in a hydrogen atom's ground state is likely to be found. The Bohr radius serves as a unit of measurement within the atomic scale.

Quantitatively, it is approximately 0.529 Ångströms or \( 0.529 \times 10^{-10} \) meters. This physical constant is crucial for various calculations in quantum mechanics.
  • It provides a scale for understanding the size of orbitals in hydrogen-like atoms.
  • The Bohr radius is utilized for scaling wave functions and probability densities, ensuring that all calculations are consistent with observed physical phenomena.
Recognizing the significance of the Bohr radius helps in appreciating its role in atomic models and its fundamental importance in quantum theory.

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Most popular questions from this chapter

Consider a particle with charge \(q,\) mass \(m,\) and spin \(s,\) in a uniform magnetic field \(\mathbf{B}_{0}\). The vector potential can be chosen as \(\mathbf{A}=-\frac{1}{2} \mathbf{r} \times \mathbf{B}_{0}\). (a) Verify that this vector potential produces a uniform magnetic field \(\mathbf{B}_{0}\). (b) Show that the Hamiltonian can be written \(H=\frac{p^{2}}{2 m}+q \varphi-\mathbf{B}_{0} \cdot\left(\gamma_{o} \mathbf{L}+\gamma \mathbf{S}\right)+\frac{q^{2}}{8 m}\left[r^{2} B_{0}^{2}-\left(\mathbf{r} \cdot \mathbf{B}_{0}\right)^{2}\right]\), where \(\gamma_{o}=q / 2 m\) is the gyromagnetic ratio for orbital motion. Note: The term linear in \(\mathbf{B}_{0}\) makes it energetically favorable for the magnetic moments (orbital and spin) to align with the magnetic field; this is the origin of paramagnetism in materials. The term quadratic in \(\mathbf{B}_{0}\) leads to the opposite effect: diamagnetism.\(^{75}\)

An electron is in the spin state \(\chi=A\left(\begin{array}{c}1-2 i \\\ 2\end{array}\right)\). (a) Determine the constant \(A\) by normalizing \(X\). (b) If you measured \(S_{z}\) on this electron, what values could you get, and what is the probability of each? What is the expectation value of \(S_{z}\) ? (c) If you measured \(S_{x}\) on this electron, what values could you get, and what is the probability of each? What is the expectation value of \(S_{x}\) ? (d) If you measured \(S_{y}\) on this electron, what values could you get, and what is the probability of each? What is the expectation value of \(S_{y}\) ?

A particle of mass \(m\) is placed in a finite spherical well: \(V(r)=\left\\{\begin{array}{ll}-V_{0}, & r \leq a ;\\\ 0, & r>a.\end{array}\right.\) Find the ground state, by solving the radial equation with \(\ell=0 .\) Show that there is no bound state if \(V_{0} a^{2}<\pi^{2} \hbar^{2} / 8 m\).

Starting from the Rodrigues formula, derive the orthonormality condition for Legendre polynomials: \(\int_{-1}^{1} P_{\ell}(x) P_{\ell^{\prime}}(x) d x=\left(\frac{2}{2 \ell+1}\right) \delta_{\ell \ell}\). Hint: Use integration by parts.

(a) At time \(t=0\) a large ensemble of spin-1/2 particles is prepared, all of them in the spin-up state (with respect to the \(z\) axis). 74 They are not subject to any forces or torques. At time \(t_{1}>0\) each spin is measured some along the \(z\) direction and others along the \(x\) direction (but we aren't some along the \(z\) direction and others along the \(x\) direction (but we aren't told the results). At time \(t_{2}>t_{1}\) their spin is measured again, this time along the \(x\) direction, and those with spin up (along \(x\) ) are saved as a subensemble (those with spin down are discarded). Question: Of those remaining (the subensemble), what fraction had spin up (along \(z\) or \(x\), depending on which was measured) in the first measurement? (b) Part (a) was easy-trivial, really, once you see it. Here's a more pithy generalization: At time \(t=0\) an ensemble of spin-1/2 particles is prepared, all in the spin-up state along direction a. At time \(t_{1}>0\) their spins are measured along direction b (but we are not told the results), and at time \(t_{2}>t_{1}\) their spins are measured along direction c. Those with spin up (along \(\mathrm{c}\) ) are saved as a subensemble. Of the particles in this subensemble, what fraction had spin up (along b) in the first measurement? Hint: Use Equation 4.155 to show that the probability of getting spin up (along b) in the first measurement is \(P_{+}=\cos ^{2}\left(\theta_{a b} / 2\right)\), and (by extension) the probability of getting spin up in both measurements is \(P_{++}=\cos ^{2}\left(\theta_{a b} / 2\right) \cos ^{2}\left(\theta_{b c} / 2\right)\). Find the other three probabilities \(\left(P_{+\rightarrow}, P_{-+}, \text {and } P_{--}\right) .\) Beware: If the outcome of the first measurement was spin down, the relevant angle is now the supplement of \(\theta_{b c}\).

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