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Quantum mechanical simulation of the cyclotron motion of an electron confined under a magnetic field
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Quantum mechanical simulation of the cyclotron motion of an electron confined under a strong, uniform magnetic field, made by solving the Schrödinger equation. As time passes, the wavepacket spatial distribution disperses until it finally reaches a stationary state with a fixed radial length.
In the visualization, the color hue shows the phase of the wave function of the electron ψ(x,y, t), while the opacity shows the amplitude.
In the example, the magnetic field is uniform over the entire plane and points downwards. If the magnetic field points upwards, the electron would orbit counterclockwise. Notice that we needed a magnetic field of the order of thousands of Teslas to confine the electron in such a small orbit (of the order of Angstroms), but a similar result can be obtained with a weaker magnetic field and therefore larger cyclotron radius.
The resulting wavefunction is just a superposition of these eigenstates. Because the eigenstates decay in the center, the time-dependent version would also. It's also interesting to notice that the energy spectrum presents regions where the density of the states is higher. These regions are equally spaced and are called Landau levels, which represent the quantization of the cyclotron orbits of charged particles.
These examples are made qmsolve, an open-source python open-source package we made for visualizing and solving the Schrödinger equation, with which we recently added an efficient time-dependent solver!
You can find the simulator used here:
This particular example was solved using the Crank-Nicolson method with a Cayley expansion, parallelized on GPU with cupy.
#SchrödingerEquation #QuantumPhysics #QMsolve
In the visualization, the color hue shows the phase of the wave function of the electron ψ(x,y, t), while the opacity shows the amplitude.
In the example, the magnetic field is uniform over the entire plane and points downwards. If the magnetic field points upwards, the electron would orbit counterclockwise. Notice that we needed a magnetic field of the order of thousands of Teslas to confine the electron in such a small orbit (of the order of Angstroms), but a similar result can be obtained with a weaker magnetic field and therefore larger cyclotron radius.
The resulting wavefunction is just a superposition of these eigenstates. Because the eigenstates decay in the center, the time-dependent version would also. It's also interesting to notice that the energy spectrum presents regions where the density of the states is higher. These regions are equally spaced and are called Landau levels, which represent the quantization of the cyclotron orbits of charged particles.
These examples are made qmsolve, an open-source python open-source package we made for visualizing and solving the Schrödinger equation, with which we recently added an efficient time-dependent solver!
You can find the simulator used here:
This particular example was solved using the Crank-Nicolson method with a Cayley expansion, parallelized on GPU with cupy.
#SchrödingerEquation #QuantumPhysics #QMsolve
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