pith. sign in

arxiv: 0904.0400 · v2 · pith:2OHY5NY7new · submitted 2009-04-02 · ✦ hep-th

Noncommutative Quantum Mechanics and Quantum Cosmology

classification ✦ hep-th
keywords noncommutativequantumcosmologyequationmechanicsmomentanoncommutativityobtain
0
0 comments X p. Extension
pith:2OHY5NY7 Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{2OHY5NY7}

Prints a linked pith:2OHY5NY7 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We present a phase-space noncommutative version of quantum mechanics and apply this extension to Quantum Cosmology. We motivate this type of noncommutative algebra through the gravitational quantum well (GQW) where the noncommutativity between momenta is shown to be relevant. We also discuss some qualitative features of the GQW such as the Berry phase. In the context of quantum cosmology we consider a Kantowski-Sachs cosmological model and obtain the Wheeler-DeWitt (WDW) equation for the noncommutative system through the ADM formalism and a suitable Seiberg-Witten (SW) map. The WDW equation is explicitly dependent on the noncommutative parameters, $\theta$ and $\eta$. We obtain numerical solutions of the noncommutative WDW equation for different values of the noncommutative parameters. We conclude that the noncommutativity in the momenta sector leads to a damped wave function implying that this type of noncommmutativity can be relevant for a selection of possible initial states for the universe.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.