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- W2009054627 abstract "We apply the many-particle Schr{o}dinger-Newton equation, which describes the co-evolution of an many-particle quantum wave function and a classical space-time geometry, to macroscopic mechanical objects. By averaging over motions of the objects' internal degrees of freedom, we obtain an effective Schrodinger-Newton equation for their centers of mass, which are degrees of freedom that can be monitored and manipulated at the quantum mechanical levels by state-of-the-art optoemchanics experiments. For a single macroscopic object moving quantum mechanically within a harmonic potential well, we found that its quantum uncertainty evolves in a different frequency from its classical eigenfrequency --- with a difference that depends on the internal structure of the object, and can be observable using current technology. For several objects, the Schrodinger-Newton equation predicts semiclassical motions just like Newtonian physics, yet they do not allow quantum uncertainty to be transferred from one object to another through gravity." @default.
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- W2009054627 date "2013-04-22" @default.
- W2009054627 modified "2023-10-12" @default.
- W2009054627 title "Macroscopic Quantum Mechanics in a Classical Spacetime" @default.
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- W2009054627 doi "https://doi.org/10.1103/physrevlett.110.170401" @default.
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