Ionization of hydrogen atom by sinusoidal electric field

Click For Summary
SUMMARY

The discussion focuses on calculating the rate of transitions from the ground state of a hydrogen atom to the continuum when subjected to an oscillating electric field described by ##\mathcal{E}_0 \cos(\omega t) \mathbf{\hat{z}}##, with the condition that ##\hbar \omega \gg -13.6\text{eV}##. The transition rate is given by the formula ##R = \frac{\pi}{2\hbar} |H_{fi}'|^2 \rho (E_f)##, where ##H_{fi}'## is the matrix element and ##\rho(E)## represents the density of states. The density of states for an infinite cuboidal well is defined as ##\rho(E) = \frac{V}{2\pi^2} (\frac{2m}{\hbar^2})^{\frac{3}{2}}\sqrt{E}##. The discussion highlights challenges in determining the density of states in the continuum limit and calculating the matrix element ##H_{fi}'## using both Cartesian and spherical coordinates.

PREREQUISITES
  • Quantum mechanics fundamentals, specifically the hydrogen atom model
  • Understanding of time-dependent perturbation theory
  • Familiarity with matrix elements in quantum mechanics
  • Knowledge of density of states in quantum systems
NEXT STEPS
  • Study time-dependent perturbation theory in quantum mechanics
  • Learn about calculating matrix elements for quantum transitions
  • Research the implications of density of states in continuum limits
  • Explore the behavior of hydrogen atoms in external electric fields
USEFUL FOR

Students and researchers in quantum mechanics, particularly those studying atomic transitions and perturbation theory, as well as physicists interested in the effects of external electric fields on atomic systems.

pixatlazaki
Messages
9
Reaction score
1

Homework Statement


"Suppose that a hydrogen atom, initially in its ground state, is placed in an oscillating electric field ##\mathcal{E}_0 \cos(\omega t) \mathbf{\hat{z}}##, with ##\hbar \omega \gg -13.6\text{eV}##. Calculate the rate of transitions to the continuum."

Homework Equations


##R = \frac{\pi}{2\hbar} |H_{fi}'|^2 \rho (E_f)##, where ##R## is the rate of transitions to the state with final energy ##E_f##, ##H_{fi}' = \langle \psi_f | H' | \psi_i \rangle ##, and ##\rho(E)## is the density of states at an energy ##E##. (Derived in course, though similar to equations in Griffiths.)

Density of states for an infinite cuboidal well of volume ##V##:
##\rho(E) = \frac{V}{2\pi^2} (\frac{2m}{\hbar^2})^{\frac{3}{2}}\sqrt{E}##

The Attempt at a Solution


I am unclear on two points in the solution of this problem.

Firstly, for the density of states for the continuum, I would think that we may just take the limit ##V \to \infty##, but that clearly will blow up (at least if done at the beginning).

Secondly, what is the most sensible way to approach determining the matrix element ##H_{fi}'##? Our final state will be that of a free particle, i.e. ##\psi_f(\mathbf{r},t) = A e^{\mathbf{k}\cdot\mathbf{r} - \omega_0 t} (\omega_0 \equiv \frac{E_f - E_i}{\hbar})## (which is really only reasonable to manipulate in Cartesian coordinates), while our initial state will be the bound state ##\psi_i(\mathbf{r},t) = \frac{1}{\sqrt{\pi} a_0^{3/2}} e^{\frac{r}{2a_0}}##, which only involves ##r##, not ##r^2##, making it suited for spherical coordinates.
 
Later in the week, we were allowed to assume that ##\mathbf{k} = k\mathbf{\hat{z}}##, which simplified the problem a great deal. I ended up performing the integral for ##H'_{fi}## in spherical coordinates. I will post the solution in a week or two.
 
  • Like
Likes   Reactions: BvU

Similar threads

Replies
3
Views
2K
  • · Replies 0 ·
Replies
0
Views
2K
Replies
5
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K
Replies
19
Views
3K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
Replies
2
Views
2K
Replies
2
Views
2K