Publication : t19/135

Holomorphic Wave Superstrata

Heidmann P. (CEA, IPhT (Institut de Physique Théorique), F-91191 Gif-sur-Yvette, France)
mayerson, d. r. (CEA, IPhT (Institut de Physique Théorique), F-91191 Gif-sur-Yvette, France)
Walker, Robert (CEA, IPhT (Institut de Physique Théorique), F-91191 Gif-sur-Yvette, France)
Warner N.P. (CEA, IPhT (Institut de Physique Théorique), F-91191 Gif-sur-Yvette, France)
Abstract:
We obtain the largest families constructed to date of $coeff{1}{8}$-BPS solutions of type IIB supergravity. They have the same charges and mass as supersymmetric D1-D5-P black holes, but they cap off smoothly with no horizon. Their construction relies on the structure of superstratum states, but it allows the momentum wave to have an arbitrary shape. Each family is based on an arbitrary holomorphic function of one variable. More broadly, we show that the most general solution is described by two arbitrary holomorphic functions of three variables. After exhibiting several new families of such ``holomorphic superstrata,'' we reformulate the BPS backgrounds and equations in holomorphic form and show how this simplifies their structure. The holomorphic formulation is thus both a fundamental part of superstrata as well as an effective tool for their construction. We also find new families of solutions in which the momentum waves of the superstrata are highly localized at infinity but diffuse and spread into the infra-red limit in the core of the superstratum. Our work also leads to some holographic predictions that can be tested within the CFT.
Année de publication : 2019
Langue : Anglais

 

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