Undergrad Numerical solution to the Schrodinger eqn. using Finite Difference Method

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SUMMARY

The discussion focuses on using the finite difference method to numerically solve the Schrödinger equation, particularly in the context of a finite square well. Participants emphasize the need to determine energy eigenvalues, which are not directly obtainable from the numerical solution. A recommended approach involves selecting an energy value, solving the equation, and checking the behavior of the wave function at infinity to identify valid eigenvalues. Additionally, boundary conditions at the origin are crucial for accurate solutions.

PREREQUISITES
  • Finite Difference Method for numerical analysis
  • Schrödinger Equation fundamentals
  • Understanding of energy eigenvalues in quantum mechanics
  • Boundary conditions in differential equations
NEXT STEPS
  • Explore numerical methods for solving the Schrödinger equation
  • Research techniques for determining energy eigenvalues in quantum systems
  • Learn about boundary condition applications in quantum mechanics
  • Investigate separation of variables in three-dimensional quantum problems
USEFUL FOR

Quantum physicists, computational physicists, and students working on numerical methods for solving differential equations in quantum mechanics.

patrykh18
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As part of my project I was asked to use the finite difference method to solve Schrödinger equation. I see how you can turn it into a matrix equation, but I don't know how to solve it if the energy eigenvalues are unknown. Are there any recommended methods I can use to determine those eigenvalues. Maybe for simplicity assume we are dealing with a finite square well and assume that for some reason you can't determine the energies in advance.
 
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patrykh18 said:
As part of my project I was asked to use the finite difference method to solve Schrödinger equation. I see how you can turn it into a matrix equation, but I don't know how to solve it if the energy eigenvalues are unknown. Are there any recommended methods I can use to determine those eigenvalues. Maybe for simplicity assume we are dealing with a finite square well and assume that for some reason you can't determine the energies in advance.

Do you mean to numerically solve the Schrödinger equation? That does not directly lead to eigenvalues.

What you can do, although this is a lot of work, is to pick an energy, numerically solve the Schrödinger equation for the energy, and then look to see if the wave function blows up as ##x \rightarrow \infty##. If so, try a slightly different energy. You've found an energy eigenvalue if the numerical solution of Schrödinger's equation leads to a wave function that is well-behaved at both ##x=0## and ##x \rightarrow \infty##.

Actually, to solve Schrödinger's equation numerically, you need more than just the energy. You also need boundary conditions at ##x=0##.

(The above is about the one-dimensional Schrödinger equation. In three-dimensions, you can often reduce the problem to a one-dimensional case if you have a spherically symmetric potential by using separation of variables.)
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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