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On the limitations of non-geometric fluxes to realize dS vacua

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arxiv 2402.13899 v2 pith:MWN7X6RL submitted 2024-02-21 hep-th

classification hep-th
keywords fluxesconfigurationsno-goconditionsfindfluxformscalar
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abstract

In this paper, we perform a systematic and analytical exploration of de Sitter conditions in type IIA compactifications with (non-)geometric fluxes along with the standard NS-NS and RR $p$-form fluxes. Exploiting the fact that the F-term scalar potential can be written as a bilinear form, we start by studying the most generic case. We find four conditions that the scalar fields and fluxes must satisfy to achieve de Sitter vacua. Particularizing to different configurations, we recover and extend previous results in the literature. We then impose an Ansatz in which the F-terms are proportional to the respective K\"ahler derivatives. In this set-up we are able to derive additional constraints and to classify the possible dS no-go scenarios in terms of eight axionic fluxes. Individually considering that any of these fluxes can be vanishing or non-vanishing leads to a total of 256 flux configurations. We find that 227 of these 256 possibilities result in a dS no-go scenario. The remaining 29 flux configurations, a priori, do not lead to dS no-go cases and would deserve further investigation.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Towards a String Realization of the Dark Dimension via T-folds

    hep-th 2024-11 conditional novelty 6.0 of 10

    A Scherk-Schwarz T-fold compactification is engineered so that, along a selected runaway trajectory, the scalar potential scales as V proportional to m_KK^4, as required by the Dark Dimension Scenario.

  2. An effective description of the instability of coherent states of gravitons in string theory

    hep-th 2024-11 reject novelty 5.0 of 10

    Using SEAQT dynamics, the authors argue that a coherent graviton state in type II string theory decoheres into a mixed state of NS-NS and RR fields, and that near equilibrium the quantum break time exceeds the classic...

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