2002
DOI: 10.1016/s0550-3213(02)00338-3
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Type II theories compactified on Calabi–Yau threefolds in the presence of background fluxes

Abstract: Compactifications of type II theories on Calabi-Yau threefolds including electric and magnetic background fluxes are discussed. We derive the bosonic part of the four-dimensional low energy effective action and show that it is a non-canonical N = 2 supergravity which includes a massive two-form. The symplectic invariance of the theory is maintained as long as the flux parameters transform as a symplectic vector and a massive two-form which couples to both electric and magnetic field strengths is present. The m… Show more

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Cited by 230 publications
(514 citation statements)
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“…An interesting issue which arises for these solutions is the stabilization of the overall size modulus. In all the known examples of IIB compactifications the resulting effective four-dimensional models were of no-scale type [8,19,23,25,31,35,38] and the overall size modulus remained free even after the introduction of fluxes. This cannot happen in the heterotic compactifications because of the modified Bianchi identity for the three-form [55,46].…”
Section: The Superpotential and The Torsional Constraintsmentioning
confidence: 99%
“…An interesting issue which arises for these solutions is the stabilization of the overall size modulus. In all the known examples of IIB compactifications the resulting effective four-dimensional models were of no-scale type [8,19,23,25,31,35,38] and the overall size modulus remained free even after the introduction of fluxes. This cannot happen in the heterotic compactifications because of the modified Bianchi identity for the three-form [55,46].…”
Section: The Superpotential and The Torsional Constraintsmentioning
confidence: 99%
“…These are the theories that describe the compactifications of eleven-dimensional supergravity on Calabi-Yau fourfolds with background fluxes. We introduce the following split of scalar fields 9) and define the real components ϕ A = ℜφ A ,φ A = ℑφ A . We now assume that the Kähler potential does not depend on theφ A…”
Section: Redualizingmentioning
confidence: 99%
“…9 The starting point is the eleven-dimensional supergravity with (bosonic) Lagrangian [26] e −1 L (11) = 1 2…”
Section: Compactification Without Fluxmentioning
confidence: 99%
“…The negative definite matrix M is defined as in [30]. Note that when the flux H 3 is turned on, the effective theory in four dimensions does not correspond to the usual N = 2 supergravity but to the gauged N = 2 supergravity, see for instance [31].…”
Section: Conditions To Preserve N = 2 In 4dmentioning
confidence: 99%
“…The presence of the NS-NS flux H 3 in the internal manifold induces a change in the effective action. The resulting action of the gauged N = 2 supergravity in four dimensions is given in [30], where the N = 2 supersymmetry is maintained by the presence of a positive definite scalar potential. To summarize, both fluxes, RR and NS-NS, must be turned on and moreover, they must be supported on the same cycle Π 3 .…”
Section: Conditions To Preserve N = 2 In 4dmentioning
confidence: 99%