2005
DOI: 10.1002/prop.200510250
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Heterotic strings on homogeneous spaces

Abstract: We construct heterotic string backgrounds corresponding to families of homogeneous spaces as exact conformal field theories. They contain left cosets of compact groups by their maximal tori supported by NS-NS 2-forms and gauge field fluxes. We give the general formalism and modular-invariant partition functions, then we consider some examples such as SU(2)/U(1) ~ S^2 (already described in a previous paper) and the SU(3)/U(1)^2 flag space. As an application we construct new supersymmetric string vacua with magn… Show more

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Cited by 47 publications
(66 citation statements)
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“…4 Now we explain how one can obtain the same masses from the asymptotic AdS 4 × S 7 gravity solution in the large N limit. Contrary to the simple case with single M2-branes, which is described by a free quantum field theory, the masses that we calculate below with the large N gravity solution is the bare mass, or the UV mass, of the field theory.…”
Section: Mass Deformation Of the Uv Cftmentioning
confidence: 98%
“…4 Now we explain how one can obtain the same masses from the asymptotic AdS 4 × S 7 gravity solution in the large N limit. Contrary to the simple case with single M2-branes, which is described by a free quantum field theory, the masses that we calculate below with the large N gravity solution is the bare mass, or the UV mass, of the field theory.…”
Section: Mass Deformation Of the Uv Cftmentioning
confidence: 98%
“…For instance, WAdS spaces provide gravity duals for condensed matter systems with Schrödinger symmetry [12,13], they are closely related to the geometry of rotating black holes [14,15], and they also appear in relation to many other interesting subjects [16][17][18]. Asymptotically WAdS 3 spaces turn out to be exact solutions of String Theory [19][20][21][22][23] as well as of other models of threedimensional gravity, including Higher-Spin Gravity [24], Topologically Massive Gravity (TMG) [25,26], and New Massive Gravity (NMG) [27]. Here, we will be concerned with the latter: We will consider asymptotically WAdS 3 black holes in NMG.…”
Section: Introductionmentioning
confidence: 99%
“…It is worth mentioning that a set of asymmetric deformations, very similar to our δS λ , δSλ above, has been considered also in the past in the context of heterotic SU (2) and SL(2) WZW models [15,16]. There it was argued that an appropriate asymmetric deformation gives rise to a line of exact conformal field theories interpolating between the SU (2) (or SL (2)) WZW model and the CFT that describes string propagation on the geometric coset S 2 (or AdS 2 ).…”
Section: Introductionmentioning
confidence: 73%