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Spherically-symmetric solutions of the Schrödinger-Newton equations

Classical and Quantum Gravity · 1998 · Vol. 15(9) · pp. 2733–2742
Irene M. MorozRoger PenrosePaul Tod

Abstract

As part of a programme in which quantum state reduction is understood as a gravitational phenomenon, we consider the Schrödinger-Newton equations. For a single particle, this is a coupled system consisting of the Schrödinger equation for the particle moving in its own gravitational field, where this is generated by its own probability density via the Poisson equation. Restricting to the spherically-symmetric case, we find numerical evidence for a discrete family of solutions, everywhere regular, and with normalizable wavefunctions. The solutions are labelled by the non-negative integers, the nth solution having n zeros in the wavefunction. Furthermore, these are the only globally defined solutions. Analytical support is provided for some of the features found numerically.

Quantum Mechanics and ApplicationsQuantum Information and CryptographyCosmology and Gravitation TheoriesPhysicsWave functionSchrödinger equationMathematical physicsGravitational fieldClassical mechanicsField (mathematics)State (computer science)GravitationSchrödinger's cat

Funding

  • National Science Foundation
Citations
443
FWCI
2.07
field-weighted impact
References
18
Percentile
86%
vs. same field & year
Citations per year
References
<i>Quantum Theory and Measurement</i>
American Journal of Physics · 1984 · 1,452 citations
Models for universal reduction of macroscopic quantum fluctuations
Physical review. A, General physics · 1989 · 973 citations
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