2012
DOI: 10.1007/jhep04(2012)114
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Nearly Kähler heterotic compactifications with fermion condensates

Abstract: We revisit AdS4 heterotic compactifications on nearly Kähler manifolds in the presence of H-flux and certain fermion condensates. Unlike previous studies, we do not assume the vanishing of the supersymmetry variations. Instead we determine the full equations of motion originating from the ten-dimensional action, and subsequently we provide explicit solutions to them on nearly Kähler manifolds at first order in α ′ . The Bianchi identity is also taken into account in order to guarantee the absence of all anomal… Show more

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Cited by 27 publications
(31 citation statements)
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References 35 publications
(77 reference statements)
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“…14 Then a well-known no-go theorem [21] states that at zeroth order in α warping, dilaton and H-flux vanish and the internal geometry must be Calabi-Yau. We denote the CY 14 Compact solutions with condensates and non trivial AdS 4 parameter have been found before in the literature, see e.g. [12][13][14][15].…”
Section: C)mentioning
confidence: 99%
“…14 Then a well-known no-go theorem [21] states that at zeroth order in α warping, dilaton and H-flux vanish and the internal geometry must be Calabi-Yau. We denote the CY 14 Compact solutions with condensates and non trivial AdS 4 parameter have been found before in the literature, see e.g. [12][13][14][15].…”
Section: C)mentioning
confidence: 99%
“…This was demonstrated to work by a "proof of principle" in [27]. See also [28][29][30][31][32][33][34][35] for related work in this direction.…”
Section: Jhep03(2016)177mentioning
confidence: 89%
“…[22,24,25,27]. Furthermore, in order to study the phenomenology of these solutions, they have to be lifted to maximally symmetric vacua by means of non-perturbative effects such as gaugino condensates [27,33], or one can look for non-supersymmetric perturbative vacua as was done in [57]. Work in this direction is in progress.…”
Section: Discussion and Outlookmentioning
confidence: 99%
“…The gaugino equation (1.1c) is already solved by the instanton solutions above. The remaining equations should be solvable in a manner similar to [22,23,32,33], which may look as follows:…”
Section: Discussionmentioning
confidence: 99%
“…γ(F A ) = γ(R) = 0. Therefore, in the spirit of [22,23,32,33], we study the instanton equation (1.1c) for non-integrable SU(3)-structures in order to provide an important ingredient for full heterotic supergravity solutions. 2 The construction of metric cones and sine-cones over manifolds M d with a G-structure provides a tool to generate and link different G -structures on (d+1)-dimensional manifolds.…”
Section: Jhep01(2015)030mentioning
confidence: 99%