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牛顿引力自相互作用对简谐囚禁量子系统的影响。

Effects of Newtonian gravitational self-interaction in harmonically trapped quantum systems.

作者信息

Großardt André, Bateman James, Ulbricht Hendrik, Bassi Angelo

机构信息

Department of Physics, University of Trieste, 34151 Miramare-Trieste, Italy.

Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Via Valerio 2, 34127 Trieste, Italy.

出版信息

Sci Rep. 2016 Aug 4;6:30840. doi: 10.1038/srep30840.

DOI:10.1038/srep30840
PMID:27488656
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC4973281/
Abstract

The Schrödinger-Newton equation has gained attention in the recent past as a nonlinear modification of the Schrödinger equation due to a gravitational self-interaction. Such a modification is expected from a fundamentally semi-classical theory of gravity and can, therefore, be considered a test case for the necessity of the quantisation of the gravitational field. Here we provide a thorough study of the effects of the Schrödinger-Newton equation for a micron-sized sphere trapped in a harmonic oscillator potential. We discuss both the effect on the energy eigenstates and the dynamical behaviour of squeezed states, covering the experimentally relevant parameter regimes.

摘要

薛定谔-牛顿方程作为因引力自相互作用对薛定谔方程的非线性修正,在最近受到了关注。这种修正源于一种基本的半经典引力理论,因此可被视为引力场量子化必要性的一个测试案例。在此,我们对处于谐振子势阱中的微米级球体的薛定谔-牛顿方程的效应进行了全面研究。我们讨论了其对能量本征态的影响以及压缩态的动力学行为,涵盖了实验相关的参数范围。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/70ef86283400/srep30840-f6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/0584b4302b49/srep30840-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/40b5f3419f40/srep30840-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/47e3879e3fde/srep30840-f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/5002765cfd5b/srep30840-f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/9edbc5f5ac0f/srep30840-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/70ef86283400/srep30840-f6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/0584b4302b49/srep30840-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/40b5f3419f40/srep30840-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/47e3879e3fde/srep30840-f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/5002765cfd5b/srep30840-f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/9edbc5f5ac0f/srep30840-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abf1/4973281/70ef86283400/srep30840-f6.jpg

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本文引用的文献

1
Macroscopic quantum mechanics in a classical spacetime.经典时空中的宏观量子力学。
Phys Rev Lett. 2013 Apr 26;110(17):170401. doi: 10.1103/PhysRevLett.110.170401. Epub 2013 Apr 22.
2
Parameterization of the temperature dependence of the Debye-Waller factors.德拜-瓦勒因子温度依赖性的参数化
Acta Crystallogr A. 1999 Sep 1;55(Pt 5):926-932. doi: 10.1107/s0108767399005176.