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I have seen in some papers that the energy levels in some arbitrary potential are specified. How can one find the energy levels in such arbitrary potentials. For example, $V(x)=\sin^2(x/2)$ with $x\in[−3\pi,3\pi]$.

I understand that in a triple well potential, there will be 3 bands comprising of three energy levels. But how do we find the exact value of these energy levels. I would like to know about the numerical methods used for this. It 'd be nice if you prefer Fortran or C, since I am not good in Python.

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  • $\begingroup$ Welcome to SciComp.SE. What are the boundary conditions for the example that you propose? $\endgroup$
    – nicoguaro
    Commented May 18, 2015 at 19:31
  • $\begingroup$ @nicoguaro infinite boundary conditions at [−3π,3π] $\endgroup$ Commented May 18, 2015 at 19:36
  • $\begingroup$ Do you mean zero boundary conditions, i.e., that the probability is zero ($\psi(x)=0$) for $x\geq|3\pi|$? $\endgroup$
    – nicoguaro
    Commented May 18, 2015 at 19:37
  • $\begingroup$ @nicoguaro exactly $\endgroup$ Commented May 18, 2015 at 19:37

1 Answer 1

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Finding the eigenvalues for the Schrödinger equation is really similar to finding the eigenvalues for the wave equation. You start with your differential equation

$$\left[-\frac{1}{2}\nabla'^2 + V(r)\right]\psi(\mathbf{r}) = E' \psi(\mathbf{r})$$

where we did the change of variable $(x,y,z) \rightarrow (a_0 x, a_0 y, a_0 z)$, with $a_0 \equiv 1$ Bohr, $E'= E/E_0$, $E_0 \equiv \frac{\hbar^2}{m_e a_0^2}$. The equation is written in a system of units that is more suitable for numerics ($m_e=1, \hbar=1, e=1$).

The more straightforward approach is to discretize the operator with finite differences and find the eigenvalues. An example for the particle in a box, written in Python is here:

from __future__ import division, print_function
import numpy as np
from scipy.sparse import diags
from scipy.sparse.linalg import eigsh

L = 2
N = 1000
dx = L/(N-1)

H = diags([-2., 1., 1.], [0,-1, 1], shape=(N, N))/dx**2

vals, vecs = eigsh(-0.5*H, which='SA')

print(np.round(vals, 6))
print(np.round([(n*np.pi/L)**2/2 for n in range(1,6)], 6))

Where the results are

[  1.228775   4.915086  11.058899  19.660151  30.71876   44.234615]
[  1.233701   4.934802  11.103305  19.739209  30.842514  44.41322 ]

The analytic solution for this normalized case is $E' = \frac{n^2 \pi^2}{2L^2}$. That is printed in the second line, the agreement is "adequate", and if we discretize more, the error is smaller.

In the case of an "arbitrary" potential, we can do the same, just adding the potential energy

from __future__ import division, print_function
import numpy as np
from scipy.sparse import diags
from scipy.sparse.linalg import eigsh
import matplotlib.pyplot as plt

L = 2*np.pi
N = 501
x = np.linspace(0, L, N)
dx = x[1] - x[0]

T = -0.5*diags([-2., 1., 1.], [0,-1, 1], shape=(N, N))/dx**2
U_vec = np.sin(x)**2
U = diags([U_vec], [0])

H = T + U

vals, vecs = eigsh(H, which='SM')

print(np.round(vals, 6))

for k in range(4):
    vec = vecs[:, k]
    mag = np.sqrt(np.dot(vecs[:, k],vecs[:, k]))
    vec = vec/mag
    plt.plot(x, vec, label=r"$n=%i$"%k)

plt.xlabel(r"$x$")
plt.ylabel(r"$\psi(x)$")
plt.savefig("eigenvectors.png", dpi=600)
plt.legend()    
plt.show()

with results

[ 0.545762  1.227567  1.657063  2.470791  3.610032  4.970446]

That I have no idea if are good or not. The eigenvectors make sense, though

enter image description here

Comparing to the Ritz method (with 10 sine functions)

[0.4111, 0.8299, 1.6696, 2.83472, 4.3342, 6.16726]

it makes sense

Another option is to base your formulation on a variational approach. In this case, you start from the variational formulation of the problem, i.e.

$$ \Pi[u] = \int_\Omega\left[\frac{1}{2}\nabla u^*(\mathbf{r}) \cdot\nabla u(\mathbf{r}) + u^*(\mathbf{r})(V(\mathbf{r})-E)u(\mathbf{r})\right] d\Omega$$

That has as components, the Hamiltonian

$$H[u] = \int_\Omega\left[\frac{1}{2}\nabla u^*(\mathbf{r}) \cdot\nabla u(\mathbf{r}) + u^*(\mathbf{r})V(\mathbf{r})u(\mathbf{r})\right] d\Omega$$

and the overlap operator $$S[u] = \int_\Omega\left[u^*(\mathbf{r})u(\mathbf{r})\right] d\Omega \enspace .$$

The solution for this system is at a stationary point of the functional. For an approximate solution of the form $\hat{u} = \sum_i^N c_i f_i(x)$, we obtain an approximation of the functionals. And we can form the eigenvalue problem

$$[\hat{H}]\lbrace c\rbrace = E [\hat{S}]\lbrace c\rbrace$$

with $\hat{H}_{ij} = \frac{H}{\partial c_i \partial c_j}$ and $\hat{S}_{ij}=\frac{S}{\partial c_i \partial c_j} \enspace.$ This approach is a Ritz method and it is similar to the one used in Hartree-Fock Methods and Density Functional Theory (DFT), and also to Finite Element Methods.

I solved for a potential $V(x) = x(2\pi - x)$ analytically using Sympy here, with eigenvalues

[  5.72324464,   9.04413044,  11.55005606,  14.95945642,  19.85359933]

Using 20 functions I found these values (not in Sympy though)

 [5.717086647332907,9.033168327518542,11.52268082000659,14.84436075114633,19.25485456061611]

that are really close.

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  • $\begingroup$ Your replies with code is interesting and I did them all in my pc. I am also interested to know how you used Ritz method with 20 functions for that potential problem. Can you share the code for that ? Thanks in advance, Nicoguaro Anand $\endgroup$
    – Anandaram
    Commented Jan 13, 2020 at 3:43
  • $\begingroup$ @Anandaram, you can check this blog post: nicoguaro.github.io/posts/hermite_ritz_qm $\endgroup$
    – nicoguaro
    Commented Jan 13, 2020 at 4:45

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