Numerical Solution to Schrodinger Equation w/ Coulomb Potential

In summary, the numerical solution to the Schrödinger equation with Coulomb potential involves employing computational methods to analyze the behavior of quantum systems influenced by an electrostatic potential. This approach typically includes discretization techniques, such as finite difference or finite element methods, to transform the continuous equation into a solvable matrix form. The resulting eigenvalue problem allows for the determination of energy levels and wave functions of particles, such as electrons in the field of a nucleus, providing insights into atomic and molecular structures. Such numerical techniques are essential for solving complex systems where analytical solutions are not feasible.
  • #1
Tertius
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Homework Statement
I am trying to numerically solve the time-independent Schrödinger equation for the tunneling problem encountered in fusion processes (with a Coulomb barrier), specifically avoiding the use of the WKB approximation.
Relevant Equations
Schrodinger Equation
Coulomb Potential
I am doing this to have my own solution for customization and understanding. I also want to manually check the WKB approximation accuracy at various energies against this static solution.

I've split the problem into 3 regions and am solving it in 1D, but am having problems with how to define the initial boundary of Region 1.
$$r_{ctp}$$ is the classical turning point where incoming kinetic energy E equals coulomb potential V.
$$r_{nuc}$$ is the point where the nuclear strong force takes over at approximately the nuclear radius.

Region 1:
$$-\infty < x <= r_{ctp}$$
Region 1 has some of V(x) before reaching ##r_{ctp}##.
Equation:
$$-\frac{\hbar^{2}}{2m} \frac{d^{2}}{dx^{2}} \psi_I(x) +V(x)\psi_I(x)=E\psi_I(x)$$
BCs:
$$\psi_I(-100) = 0$$
$$\psi_I'(-100) = 0.0001$$ (this is nonsense, and it propagates through the solutions).
If it is set to 0, then the solution is trivially 0. But the wave function should approach 0 going to ##-\infty##.

Region 2:
$$r_{ctp} < x <= r_{nuc}$$
Region 2 has negative kinetic energy because E < V.
Equation:
$$-\frac{\hbar^{2}}{2m} \frac{d^{2}}{dx^{2}} \psi_{II}(x) +V(x)\psi_{II}(x)=E\psi_{II}(x)$$
BCs:
$$\psi_I(r_{ctp}) = \psi_{II}(r_{ctp})$$
$$\psi_I'(r_{ctp}) = \psi_{II}'(r_{ctp})$$

Region 3:
$$r_{nuc} < x <= 0$$
Region 3 is 'freely propagating' where ##V(x)=0##
Equation:
$$-\frac{\hbar^{2}}{2m} \frac{d^{2}}{dx^{2}} \psi_{III}(x) =E\psi_{III}(x)$$
BCs:
$$\psi_{II}(r_{nuc}) = \psi_{III}(r_{nuc})$$

$$\psi_{II}'(r_{nuc}) = \psi_{III}'(r_{nuc})$$

This setup is producing the attached graph using NDSolve in Mathematica.

The two questions i have are:
1) what are the appropriate BCs for Region 1?
2) why is the Region 2 solution oscillatory when it should be exponential? Usually that's a minus sign problem but wondering if there is something else going on.

Thanks
 

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  • #2
I figured out where my approach was wrong. The boundary conditions for this are a little tricky because it is not a bound system.
So I discretized it manually and just solved $$H\psi = E\psi$$, where E is the kinetic energy of the incoming particle. E in this case is just a single eigenvalue because it is not a bound system, so it is possible to solve it as a simplified linear system as $$(H-EI)\psi = 0$$. This made it fast and give the same answer. But I did need to give the LinearSolver a small non-zero initial wave function value so it didn't give the trivial answer. Hope this helps someone.
 
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FAQ: Numerical Solution to Schrodinger Equation w/ Coulomb Potential

What is the Schrödinger equation, and why is it important?

The Schrödinger equation is a fundamental equation in quantum mechanics that describes how the quantum state of a physical system changes over time. It is important because it provides a mathematical framework for understanding the behavior of particles at the quantum level, allowing scientists to predict the properties of atoms, molecules, and other quantum systems.

What is the Coulomb potential, and how does it relate to the Schrödinger equation?

The Coulomb potential describes the interaction between charged particles, such as electrons and protons, and is given by the formula \( V(r) = -\frac{k e^2}{r} \) in three-dimensional space, where \( k \) is a constant, \( e \) is the charge, and \( r \) is the distance between the charges. In the context of the Schrödinger equation, the Coulomb potential is used to model systems like the hydrogen atom, where the electron is influenced by the attractive force of the proton.

What are the common numerical methods used to solve the Schrödinger equation with Coulomb potential?

Common numerical methods include the Finite Difference Method (FDM), the Variational Method, the Rayleigh-Ritz method, and the spectral method. Each of these methods has its own advantages and is chosen based on the specific requirements of the problem being solved, such as the desired accuracy and computational efficiency.

What challenges arise when numerically solving the Schrödinger equation with a Coulomb potential?

Challenges include dealing with singularities at the origin (where the potential becomes infinite), ensuring stability and convergence of the numerical solution, and handling boundary conditions effectively. Additionally, accurately representing the wave function in regions where it may change rapidly can be difficult, requiring careful discretization and mesh refinement.

How can one validate the numerical solutions obtained for the Schrödinger equation with Coulomb potential?

Validation can be achieved by comparing numerical results with analytical solutions for simpler cases, checking the conservation of probability, and testing the results against known physical properties such as energy levels and wave functions. Additionally, conducting convergence tests by refining the numerical grid and observing the stability of results can help ensure the reliability of the solutions.

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