Abstract

We analytically construct asymptotically AdS5 black string solutions starting from the four-dimensional domain wall black hole of [1]. It is shown that its uplift gives a black string in d = 5 minimal gauged supergravity, with momentum along the string. Applying instead the residual symmetries of N = 2, d = 4 Fayet-Iliopoulos-gauged super-gravity discovered in [2] to the domain wall seed leads, after uplifting, to a dyonic black string that interpolates between AdS5 and AdS3 × H2 at the horizon. A Kaluza-Klein reduction of the latter along an angular Killing direction ϕ followed by a duality transformation yields, after going back to five dimensions, a black string with both momentum along the string and rotation along ϕ. This is the first instance of using solution-generating techniques in gauged supergravity to add rotation to a given seed. These solutions all have constant scalar fields. As was shown in [3], the construction of supersymmetric static magnetic black strings in the FI-gauged stu model amounts to solving the SO(2, 1) spinning top equations, which descend from an inhomogeneous version of the Nahm equations. We are able to solve these in a particular case, which leads to a generalization of the Maldacena-Nuñez solution.

Highlights

  • Well, which essentially involves the stabilization of the symplectic vector of gauge couplings (FI parameters) under the action of the U-duality symmetry of the ungauged theory

  • As was shown in [3], the construction of supersymmetric static magnetic black strings in the FI-gauged stu model amounts to solving the SO(2, 1) spinning top equations, which descend from an inhomogeneous version of the Nahm equations

  • We used the residual symmetries of N = 2, d = 4 Fayet-Iliopoulos-gauged supergravity discovered in [2] to add an electric charge density and rotation to fivedimensional black strings that asymptote to AdS5

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Summary

Dyonic black string with momentum

The results of [2] can be used to generate a new configuration from the seed solution (2.15) and the respective fluxes and scalars (2.17). Looking at (4.2) one may think that the graviphoton can be set to zero by choosing properly the parameters a1, a2. This is not the case, as can be seen from the field strengths in presence of axions, that read. Note that the metric remains untouched by the duality rotation This solution describes again a flow between magnetic AdS5 and AdS3×H2, and preserves the same amount of supersymmetry as before, as can be seen by using the Killing spinor equations following from (A.1)

Dyonic black string with both momentum and rotation
Solutions with running scalars
Inclusion of hypermultiplets
Conclusions
A Supersymmetry variations
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