How to Create Universes with Internal Flux
Jean-Luc Lehners, Rahim Leung, K.S. Stelle

TL;DR
This paper demonstrates that no-boundary cosmological solutions can naturally generate and select quantized internal fluxes in string-inspired models, explaining their origin and distribution in the early universe.
Contribution
It introduces a novel mechanism where the no-boundary proposal explains the emergence and preferred values of fluxes in higher-dimensional string compactifications.
Findings
No-boundary solutions exist with internal fluxes from universe creation.
Fluxes are only present when they lead to positive, flat potentials for accelerated expansion.
The no-boundary wave function favors smaller flux values within the allowed range.
Abstract
String compactifications typically require fluxes, for example in order to stabilise moduli. Such fluxes, when they thread internal dimensions, are topological in nature and take on quantised values. This poses the puzzle as to how they could arise in the early universe, as they cannot be turned on incrementally. Working with string inspired models in and dimensions, we show that there exist no-boundary solutions in which internal fluxes are present from the creation of the universe onwards. The no-boundary proposal can thus explain the origin of fluxes in a Kaluza-Klein context. In fact, it acts as a selection principle since no-boundary solutions are only found to exist when the fluxes have the right magnitude to lead to an effective potential that is positive and flat enough for accelerated expansion. Within the range of selected fluxes, the no-boundary wave function assigns…
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Taxonomy
TopicsComputational Physics and Python Applications · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
