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• W1980158039 abstract "Certain remnants of a quantum spacetime foam can be modeled by a distribution of defects embedded in a flat classical spacetime. The presence of such spacetime defects affects the propagation of elementary particles. In this article, we show explicitly that both topology and differential structure of the defects are important for the particle motion. Specifically, we consider three types of spacetime defects which are described by the same topological manifold documentclass[12pt]{minimal}begin{document}$mathbb {R}times big (mathbb {R}P^3-lbrace text{point}rbrace big )$end{document}R×RP3−{point} but which are not diffeomorphic to each other. We investigate the propagation of a massless scalar field over the three different manifolds and find different solutions of the Klein–Gordon equation." @default.
• W1980158039 created "2016-06-24" @default.
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• W1980158039 date "2014-11-01" @default.
• W1980158039 modified "2023-09-23" @default.
• W1980158039 title "Comparison of spacetime defects which are homeomorphic but not diffeomorphic" @default.
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• W1980158039 doi "https://doi.org/10.1063/1.4900883" @default.
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