2024
DOI: 10.1007/jhep01(2024)157
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Flux vacua of the mirror octic

Erik Plauschinn,
Lorenz Schlechter

Abstract: We determine all flux vacua with flux numbers Nflux ≤ 10 for a type IIB orientifold-compactification on the mirror-octic three-fold. To achieve this, we develop and apply techniques for performing a complete scan of flux vacua for the whole moduli space — we do not randomly sample fluxes nor do we consider only boundary regions of the moduli space. We compare our findings to results in the literature.

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Cited by 4 publications
(2 citation statements)
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“…This observation was called the 'tadpole problem' in [16], where it was conjectured that there is, at least asymptotically, a linear relationship between the number of stabilized moduli and the tadpole contribution. The tadpole conjecture has been subsequently investigated in [17][18][19][20][21][22][23][24][25][26][27][28] and a sizable amount of evidence for its validity has been collected.…”
Section: Jhep06(2024)046mentioning
confidence: 99%
“…This observation was called the 'tadpole problem' in [16], where it was conjectured that there is, at least asymptotically, a linear relationship between the number of stabilized moduli and the tadpole contribution. The tadpole conjecture has been subsequently investigated in [17][18][19][20][21][22][23][24][25][26][27][28] and a sizable amount of evidence for its validity has been collected.…”
Section: Jhep06(2024)046mentioning
confidence: 99%
“…In the context of string Landscape, there have been many studies on the statistics that count flux vacua to discuss the naturalness. Considering only the Ramond-Ramond (R-R) and Neveu Schwarz-Neveu Schwarz (NS-NS) fluxes, 3 the number of "physical" vacua with a certain bound on fluxes is shown to be finite by the density method which treats fluxes as continuous variables and is reliable in large flux region [19], and many concrete examples with no approximation can be found in [20][21][22][23][24] for instance. Furthermore, the number of SUSY vacua is proved to be finite with the D3 brane charge of fluxes bounded [25].…”
Section: Introductionmentioning
confidence: 99%