Quantum mechanics before the big bang in heterotic-M-theory
Andrea Zanzi

TL;DR
This paper explores quantum mechanics' role before the big bang in heterotic-M-theory, revealing how quantum interference patterns localize particles and define branes, potentially avoiding cosmological singularities.
Contribution
It introduces a novel approach linking quantum interference to brane localization and stability in heterotic-M-theory, with a modified Schrödinger equation and implications for early universe cosmology.
Findings
Particles localize around black holes via quantum interference
Casimir potential acts as a gravitational effective potential
Quantum interference helps define and stabilize branes
Abstract
In this letter we investigate the role played by quantum mechanics before the big-bang in heterotic-M-theory assuming an orbifold compactification of time. As we will see particles are localized around a black hole but only in regions where a constructive quantum interference takes place. We infer that the creation of this interference pattern is interesting for many reasons: (A) it is a mechanism to localize particles on branes; (B) the Casimir potential for the dilaton can be interpreted as a gravitational effective potential for a two-body problem; (C) the quantum interference is a new way to define the branes in heterotic-M-theory. Remarkably, a modified Schroedinger equation is obtained. The stabilization of the branes' position is related to the absence of a cosmological singularity.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
