Abstract

In this paper we consider aspects of the holographic interpretation of Taub-NUT-${\mathrm{AdS}}_{4}$. We review our earlier results which show that ${\mathrm{TNAdS}}_{4}$ gives rise to a holographic three-dimensional conformal fluid having constant vorticity. We then study the holographic relevance of the Misner string by considering bulk scalar fluctuations. The scalar fluctuations organize naturally into representations of the $SU(2)\ifmmode\times\else\texttimes\fi{}\mathbb{R}$ isometry algebra. If we require the string's invisibility we obtain a Dirac-like quantization relating the frequency of the scalar field modes to the NUT charge. As the latter quantity determines the total vorticity flux of the boundary fluid, we argue that such an assumption allows for a holographic interpretation of ${\mathrm{TNAdS}}_{4}$ as a nondissipative superfluid whose excitations are quantized vortices. Alternatively, if we regard the Misner string as a physical object, as has recently been advocated for thermodynamically, the aforementioned quantization conditions are removed, and we find that ${\mathrm{TNAdS}}_{4}$ corresponds to a holographic fluid whose dissipative properties are probed as usual by the complex quasinormal modes of the bulk fluctuations. We show that such quasinormal modes are, perhaps surprisingly, organized into infinite-dimensional nonunitary representations of the isometry algebra.

Highlights

  • There is a considerable amount of evidence that asymptotically locally AdS4 spacetimes are related to threedimensional conformal fluids in local thermal equilibrium [1]

  • We show that under these circumstances, TNAdS4 gives rise to a holographic fluid whose dissipative properties are probed by the usual quasinormal modes of the scalar fluctuations

  • Single vortices appear regularly in superfluid flows [35] where their stability is guaranteed by topological considerations. With this in mind we suggest that there are two complementary ways to make sense of the boundary TNAdS4 fluid: (i) If we require that the fluid lives on a compact spatial surface at the boundary, we may tolerate having a singular velocity field such as (8) since the homogeneity of the TNAdS4 spacetime can be used to argue that there is no physical meaning to the boundary point where the velocity diverges

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Summary

INTRODUCTION

There is a considerable amount of evidence that asymptotically locally AdS4 spacetimes are related to threedimensional conformal fluids in local thermal equilibrium [1]. If we consider the Misner string as a physical object, we should excise a point on the fluid’s surface This follows from the fact that the angular equation for the scalar field fluctuations has a complete set of eigenfunctions only under such circumstances. We show that under these circumstances, TNAdS4 gives rise to a holographic fluid whose dissipative properties are probed by the usual quasinormal modes of the scalar fluctuations In this case, we will show that scalar modes satisfying infalling boundary conditions at the black hole horizon are quasinormal modes with complex frequencies, and that these modes fall into infinite-dimensional highest- and lowestweight representations of the SUð2Þ × R isometry algebra, in keeping with the fact that in these circumstances no quantization condition can be consistently imposed.

General analysis
The total vorticity flux at the boundary
Making sense of the TNAdS4 fluid
SCALAR FIELD FLUCTUATIONS IN TNAdS4
The angular equation and SUð2Þ modules
The radial equation
The Schrödinger Problem
Physical Misner string
DISCUSSION AND OUTLOOK
Full Text
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