2021
DOI: 10.1007/jhep08(2021)099
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Systematics of the α′ expansion in F-theory

Abstract: Extracting reliable low-energy information from string compactifications notoriously requires a detailed understanding of the UV sensitivity of the corresponding effective field theories. Despite past efforts in computing perturbative string corrections to the tree-level action, neither a systematic approach nor a unified framework has emerged yet. We make progress in this direction, focusing on the moduli dependence of perturbative corrections to the 4D scalar potential of type IIB Calabi-Yau orientifold comp… Show more

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Cited by 31 publications
(46 citation statements)
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“…We will not attempt to be complete but rather discuss a selection of corrections that are potentially relevant for our purpose. See also [15] for a recent survey of perturbative corrections in IIB/F-theory compactifications. It is well known that the Kähler potential in toroidal orientifold compactifications receives string-loop corrections at order α ′2 due to an exchange of Kaluza-Klein modes between D7/D3 branes or O7/O3 planes [29][30][31][32] (see also [33]).…”
Section: Correctionsmentioning
confidence: 99%
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“…We will not attempt to be complete but rather discuss a selection of corrections that are potentially relevant for our purpose. See also [15] for a recent survey of perturbative corrections in IIB/F-theory compactifications. It is well known that the Kähler potential in toroidal orientifold compactifications receives string-loop corrections at order α ′2 due to an exchange of Kaluza-Klein modes between D7/D3 branes or O7/O3 planes [29][30][31][32] (see also [33]).…”
Section: Correctionsmentioning
confidence: 99%
“…The problem is rather that the 4D EFT describing this highly stringy regime is unknown and might look very different from the naive EFT derived from a dimensional reduction of 10D supergravity. 15 It follows from [28,66] that a necessary condition to avoid the singular-bulk problem is…”
Section: Curvature/warping Corrections From Conifold-flux Backreactionmentioning
confidence: 99%
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“…For example, comparing terms O(α 3 g 2 s ) and O(α 2 g 3 s ) can be hard. A very important part of ongoing supergravity research is to systematically analyse these corrections at all orders and ensure that Kähler moduli stabilisation is not spoiled in the bulk of moduli space (see for example [11][12][13][14][15]). Furthermore, since we lack a complete picture of non-perturbative supergravity, it is difficult to define frameworks where computations can be carried out under complete control.…”
Section: Introductionmentioning
confidence: 99%
“…By comparison, the recent analysis of [20] used these conditions together with a number of conditions related to further corrections (see e.g. [26][27][28][29][30][31][32][33][34][35][36][37][38][39][40]) to collectively constrain the LVS. These analytical constraints were then applied to a specific Calabi-Yau orientifold.…”
Section: Introductionmentioning
confidence: 99%