A numerical study of the Schrödinger-Newton equations
The Schrödinger-Newton (S-N) equations were proposed by Penrose [18] as a model for gravitational collapse of the wave-function. The potential in the Schrödinger equation is the gravity due to the density of $|\psi|^2$, where $\psi$ is the wave-function. As with normal Quantum Mechanics the probabil...
| Հիմնական հեղինակ: | |
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| Ձևաչափ: | Թեզիս |
| Հրապարակվել է: |
University of Oxford;Mathematical Institute
2001
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