1997
DOI: 10.1016/s0393-0440(97)80004-6
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On nearly parallel G2-structures

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Cited by 169 publications
(189 citation statements)
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“…Since the other spinors ǫ A are not Killing for the deformed metric, the resulting space carries a strict nearly parallel G 2 -structure [32]. See below for the deformation.…”
Section: -Sasakianmentioning
confidence: 99%
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“…Since the other spinors ǫ A are not Killing for the deformed metric, the resulting space carries a strict nearly parallel G 2 -structure [32]. See below for the deformation.…”
Section: -Sasakianmentioning
confidence: 99%
“…Two other special h-values are h = 0 and exp(2h) = 2m + 3; both metrics are Einstein, but only the first is 3-Sasakian. In dimension 7 the metric with exp(2h) = 5 is nearly parallel G 2 [32].…”
Section: -Sasakianmentioning
confidence: 99%
“…We set d = 3, and the spacetime SUSY requires the condition 15) where U(1) 3/2 denotes a c = 1 CFT whose conformal blocks are described by characters Θ * ,3/2 (τ )/η(τ ). Precisely this relation means that the conformal blocks of the M-sector are expanded in terms of characters Θ * ,3/2 (τ )/η(τ ) and the branching coefficients are not hit by the GSO projection.…”
Section: General Set Up and Aspects Of Spacetime Susymentioning
confidence: 99%
“…Einstein metric that provides a weak G 2 holonomy [13,15] (see also [8,12]). A way to present the squashing procedure is to replace the original tri-Sasakian coset G/H…”
Section: G/h = (Su(2) × Su(2))/su(2)mentioning
confidence: 99%
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