Quaternionic Kähler Detour Complexes and Supersymmetric Black Holes

We study a class of supersymmetric spinning particle models derived from the radial quantization of stationary, spherically symmetric black holes of four dimensional supergravities. By virtue of the c -map, these spinning particles move in quaternionic Kähler manifolds. Their spinning degrees of fre...

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Bibliographic Details
Published inCommunications in mathematical physics Vol. 302; no. 3; pp. 843 - 873
Main Authors Cherney, D., Latini, E., Waldron, A.
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer-Verlag 2011
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Summary:We study a class of supersymmetric spinning particle models derived from the radial quantization of stationary, spherically symmetric black holes of four dimensional supergravities. By virtue of the c -map, these spinning particles move in quaternionic Kähler manifolds. Their spinning degrees of freedom describe mini-superspace-reduced supergravity fermions. We quantize these models using BRST detour complex technology. The construction of a nilpotent BRST charge is achieved by using local (worldline) supersymmetry ghosts to generate special holonomy transformations. (An interesting byproduct of the construction is a novel Dirac operator on the superghost extended Hilbert space.) The resulting quantized models are gauge invariant field theories with fields equaling sections of special quaternionic vector bundles. They underly and generalize the quaternionic version of Dolbeault cohomology discovered by Baston. In fact, Baston’s complex is related to the BPS sector of the models we write down. Our results rely on a calculus of operators on quaternionic Kähler manifolds that follows from BRST machinery, and although directly motivated by black hole physics, can be broadly applied to any model relying on quaternionic geometry.
ISSN:0010-3616
1432-0916
DOI:10.1007/s00220-010-1169-6