A discussion on a possibility to interpret quantum mechanics in terms of general relativity
| dc.creator | Ho, Vu B | |
| dc.date | 1995-07-12 | |
| dc.date.accessioned | 2026-07-07T04:21:18Z | |
| dc.date.available | 2026-07-07T04:21:18Z | |
| dc.description | It is shown that, with some reasonable assumptions, the theory of general relativity can be made compatible with quantum mechanics by using the field equations of general relativity to construct a Robertson-Walker metric for a quantum particle so that the line element of the particle can be transformed entirely to that of the Minkowski spacetime, which is assumed by a quantum observer, and the spacetime dynamics of the particle described by a Minkowski observer takes the form of quantum mechanics. Spacetime structure of a quantum particle may have either positive or negative curvature. However, in order to be describable using the familiar framework of quantum mechanics, the spacetime structure of a quantum particle must be "quantised" by an introduction of the imaginary number $i$. If a particle has a positive curvature then the quantisation is equivalent to turning the pseudo-Riemannian spacetime of the particle into a Riemannian spacetime. This means that it is assumed the particle is capable of measuring its temporal distance like its spatial distances. On the other hand, when a particle has a negative curvature and a negative energy density then quantising the spacetime structure of the particle is equivalent to viewing the particle as if it had a positive curvature and a positive energy density. | |
| dc.description | Latex 6 pages | |
| dc.identifier | https://arxiv.org/abs/hep-th/9507069 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9507069 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/54264 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Quantum Physics | |
| dc.title | A discussion on a possibility to interpret quantum mechanics in terms of general relativity | |
| dc.type | text |