Time dependent Schrödinger equation
We want to describe an electron wavefunction by a wavepacket that is a function of position and time . We assume that the electron is initially localized around , and model this by a Gaussian multiplying a plane wave:
This wave function does not correspond to an electron with a well defined momentum. However, if the width of the Gaussian is made very large, the electron gets spread over a sufficiently large region of space and can be considered as a plane wave with momentum with a slowly varying amplitude.
The behavior of this wave packet as a function of time is described by the time-dependent Schröedinger equation (here in 1d):
is the Hamiltonian operator:
where is a time independent potential. The Hamiltonian is chosen to be real. we have picked teh energy units such that , and from now on, we will pick mass units such that to make equations simpler.
Scrhödinger’s equation is obviously a PDE, and we can use generalizations of the techniques learned in previous sections to solve it. The main observation is that this time we have to deal with complex numbers, and the function has real and imaginary parts: However, is this section we will present an alternative method that makes the quantum mechanical nature of this problem more transparent.
The time-evolution operator
The Scrödinger equation ([time]) can be integrated in a formal sense to obtain:
From here we deduce that the wave function can be evolved forward in time by applying the time-evolution operator : Likewise, the inverse of the time-evolution operator moves the wave function back in time: where we have use the property Although it would be nice to have an algorithm based on the direct application of , it has been shown that this is not stable. Hence, we apply the following relation: Now, the derivatives with recpect to can be approximated by
The time evolution operator is approximated by: Replacing the expression ([hami]) for , we obtain:
with . The probability of finding an electron at is given by . This equations do no conserve this probability exactly, but the error is of the order of . The convergence can be determined by using smaller steps.
We can write this expression explicitly for the real and imaginary parts, becoming:
Notice the symmetry between these equations a: while the calculation of the imaginary part of the wave function at the later time involves a weighted average of the real part of the wave function at di erent positions from the earlier time, the calculation of the real part involves a weighted average of the imaginary part for di erent positions at the earlier time. This intermixing of the real and imaginary parts of the wave function may seem a bit strange, but remember that this situation is a direct result of our breaking up the wave function into its real and imaginary parts in the first place.
Exercise 8.1: Harmonic Potential
Simulate a Gaussian wave-packet moving along the axis in a harmonic potential
Exercise 8.2: Potential barrier
Simulate a Gaussian wave-packet moving along the x axis passing through a potential barrier
Exercise 8.2: Single-slit diffraction
Young’s single-slit experiment consists of a wave passing though a small slit, which causes the emerging wavelets to intefere with eachother forming a diffraction pattern. In quantum mechanics, where particles are represented by probabilities, and probabilities by wave packets, it means that the same phenomenon should occur when a particle (electron, neutron) passes though a small slit. Consider a wave packet of initial width 3 incident on a slit of width 5, and plot the probability density as the packet crosses the slit. Generalize the time-evolution equation ([time_diff]) for 2 dimensions. Model the slit with a potential wall: