Emergence of Classicality in Stern-Gerlach Experiment via Self-Gravity
arXiv:2211.08363 · doi:10.1002/andp.202200627
Abstract
Emergence of classicality from quantum mechanics, a hotly debated topic, has had no satisfactory resolution so far. Various approaches including decoherence and gravitational interactions have been suggested. In the present work, the Schrödinger-Newton model is used to study the role of semi-classical self-gravity in the evolution of massive spin-1/2 particles in a Stern-Gerlach experiment. For small mass, evolution of the initial wavepacket in a spin superposition shows a splitting in the magnetic field gradient into two trajectories as in the standard Stern-Gerlach experiment. For larger mass, the deviations from the central path are less than in the standard Stern-Gerlach case, while for high enough mass, the wavepacket does not split, and instead follows the classical trajectory for a magnetic moment in inhomogeneous magnetic field. This indicates the emergence of classicality due to self-gravitational interaction when the mass is increased. In contrast, decoherence which is a strong contender for emergence of classicality, leads to a \emph{mixed state} of two trajectories corresponding to the spin-up and spin-down states, and not the classically expected path. The classically expected path of the particle probably cannot be explained even in the many-worlds interpretation of quantum mechanics. Stern-Gerlach experiments in the macroscopic domain are needed to settle this question.
arXiv commentTo appear in Annalen der Physik
References in corpus (13)
- Models of Wave-function Collapse, Underlying Theories, and Experimental Tests
- A Spin Entanglement Witness for Quantum Gravity
- Testing the limits of quantum mechanical superpositions
- Gravitation and quantummechanical localization of macroobjects
- The Schrödinger-Newton equation and its foundations
- The Schrödinger-Newton equation as non-relativistic limit of self-gravitating Klein-Gordon and Dirac fields
- Macroscopic Quantum Mechanics in a Classical Spacetime
- Problems with the Newton-Schrödinger Equations
- Schrödinger-Newton "collapse" of the wave function
- Effects of Newtonian gravitational self-interaction in harmonically trapped quantum systems
- Approximations for the free evolution of self-gravitating quantum particles
- Nanoscale magnetism probed in a matter-wave interferometer
- Testing Gravitational Self-interaction via Matter-Wave Interferometry