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QMsolve: A module for solving and visualizing the Schrödinger equation

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QMsolve seeks to provide a solid and easy to use solver, capable of solving the Schrödinger equation for one and two particles, and creating descriptive and stunning visualizations of its solutions both in 1D, 2D, and 3D.


pip install qmsolve

3D plotting requires to have installed Mayavi. To install Mayavi directly along with QMsolve, you can type:

pip install qmsolve[with_mayavi]


The way this simulator works is by discretizing the Hamiltonian with an arbitrary potential, that you can specify as a function of the particle observables. This is achieved with the Hamiltonian constructor.

For example:

#define the interaction potential
def harmonic_oscillator(particle):
    k = 100. * eV / Å**2
    return 0.5 * k * particle.x**2

#define the Hamiltonian
H = Hamiltonian(particles = SingleParticle(), 
                potential = harmonic_oscillator, 
                spatial_ndim = 1, N = 512, extent = 20*Å)

Then, the method Hamiltonian.solve can be used to efficiently diagonalize the Hamiltonian and output the energies and the eigenstates of the system:

eigenstates = H.solve(max_states = 30)
print(eigenstates.energies) # The printed energies are in eV.

Finally, the eigenstates can be plotted with the use of the visualization class.

The visualization.superpositions method features the possibility of interactively visualizing a superposition of the computed eigenstates and studying the time dependence of the resulting wavefunction.

For efficiently solving the time dependent Schrödinger equation, TimeSimulation class must be used. It takes as an argument the Hamiltonian you have previously defined, and the method you desire to use.

For a quick start, take a look to the examples found in the examples subdirectory.

Eigenstate Solver Examples

To perform the example simulations, just run from the corresponding Python example scripts on the command prompt.

python python
Link to the example Link to the example

This is the simplest example and one of the most well-studied Hamiltonians. The first script, serves as an example of how to use the interface of the Eigenstate solver. This script returns the energies and a visualization of the eigenstates of the harmonic oscillator with an interactive slider. The second script, uses exactly the same Hamiltonian, but this time returns a simulation of a superposition of the computed eigenstates, whose coefficients can be interactively modified using the circular widgets presented below the animation.

python python
Link to the example Link to the example

These two examples show two fermions confined in 1D harmonic oscillator. The top-left plot represents the configuration space of the system.

Because we have two 1D particles, we need a two-dimensional space to represent it. Notice that because the particles are fermions, the wavefunction satisfies the antisymmetric condition: 𝜓(x1, x2) = - 𝜓(x2, x1)

An interesting characteristic that can be observed in these examples is how in the non interactive case the energy levels are equally spaced and degenerated, while in the interactive case the degeneracy is broken. As a starting point we suggest you to modify the confinement and the interaction potential to see what happens!

The time dependent version of this example can be found in

Link to the example

This example serves to illustrate how to use the 3D solver. The results for other number of Gaussian wells are presented in this video. Gaussian wells are preferred as didactic examples because the absence of a singularities in its potential makes the computations easier. For realistic atomic examples, you can take a look at and which use Coulomb potential.

Furthermore, in the hydrogen atom example you can turn on an electric field to visualize the Stark effect, or a magnetic field in to visualize the Zeeman effect.

The default numerical method used for diagonalizing the Hamiltonian is ARPACK implementation of Implicitly Restarted Lanczos Method, which is called with scipy via eigsh method. For 3D examples, LOBPCG is preferred since its convergence is faster for high-dimensional matrices.

3D examples are also considerably faster when using a GPU. GPU acceleration requires having CuPy and CUDA installed in your computer.

To use GPU acceleration in your 3D simulations, add the argument method ='lobpcg-cupy' in the Hamiltonian solve method. For example:

eigenstates = H.solve( max_states = 50, method ='lobpcg-cupy')

Time Dependent Examples

These examples use the TimeSimulation class. This class takes as arguments the Hamiltonian you have previously defined, and the method you desire to use. Currently, there are two methods implemented: Split-Step Fourier and Cayley-Crank-Nicolson. To specify the method you want to use, use the arguments method ='split-step' and method ='crank-nicolson' respectively.

Once the TimeSimulation is set up, you need to use method to perform the simulation. It takes the following arguments:

  • initial_wavefunction: State of the system at t=0, specified as a function of the particle observables.
  • dt: size of simulation time step.
  • total_time: amount of time to evolve the wavefunction.
  • store_steps: number of time steps to save in the array denoted by TimeSimulation.Ψ to later visualize or analyze. total_time/store_steps must be larger or equal to dt.

By default in the examples, initial_wavefunction initializes a Gaussian wave-packet with a spatial standard deviation equal to σ and initial momentum p_x0 and p_y0.

Link to the example

This is a famous example, which was used to demonstrate the wave-like behavior of matter. In this script, the user can vary the slits separation, width, and depth to study their effect on the diffracted wavefunction.

Link to the example

This script shows an example where Crank Nicolson method is required. It presents a charged particle under a strong and uniform magnetic field, being confined in a quantum mechanical cyclotron orbit. The period and the radius of the orbit are compared with the classical values. Unlike other confinement potentials like the harmonic oscillator, the initial wavepacket is greatly dispersed over time.

Generally, the Split Step method is preferred over Crank Nicolson both because of the computational cost of the time step and its associated error. Split Step has a time step error of cubic order O(Δt^3) while Crank Nicolson time step error is quadratic O(Δt^2). Thus Crank Nicolson requires more time steps to achieve the Split Step accuracy. However, Split Step can only be used for potentials of the form V(x,y,z) and Crank Nicolson use is necessary when the potential is also dependent of the particles momentum, like in the cyclotron orbit example.

Both methods are also implemented to be GPU-accelerated with cupy. Specifically, the speed boost of the cupy split-step is tested to be one and two orders of magnitudes faster than the CPU implementation, depending of the GPU and the grid size used. To use GPU acceleration in your simulations, use the arguments method ='split-step-cupy' and method ='crank-nicolson-cupy' in the TimeSimulation constructor.

The interface uses Hartree atomic units for input. In the file there is a list of common conversion factors from other units, that can be imported and used to build your potential.

Main developers


  • Hudson Smith (shift-invert trick for eigsh solver, lobpcg prototype, support for the project and multiple suggestions)
  • Andrew Knyazev (lobpcg algorithm and AMG preconditioner)