Abstract

In this paper, we study the 6d Little String Theory (LST) (the decoupled theory on the worldvolume of N NS5-branes) on curved manifolds, by using its holographic duality to Type II string theory in asymptotically linear dilaton backgrounds. We focus on backgrounds with a large number of Killing vectors (namely, products of maximally symmetric spaces), without requiring supersymmetry (we do not turn on any background fields except the metric). LST is non-local so it is not obvious which spaces it can be defined on; we show that holography implies that the theory cannot be put on negatively curved spaces, but only on spaces with zero or positive curvature. For example, one cannot put LST on a product of an anti-de Sitter space times another space, without turning on extra background fields. On spaces with positive curvature, such as S6, ℝ2× S4, S3× S3, etc., we typically find (for large N) dual holographic backgrounds which are weakly coupled and weakly curved everywhere, so that they can be well-described by Type II supergravity. In some cases more than one smooth solution exists for LST on the same space, and they all contribute to the partition function. We also study the thermodynamical properties of LST compactified on spheres, finding the leading correction to the Hagedorn behavior of the spectrum, which is different on curved space than on flat space. We discuss the holographic renormalization procedure, which must be implemented in order to get a finite free energy for the LST; we do not know how to implement it for general spaces, but we can (and we do) implement it for the theory compactified on S4.

Highlights

  • Little String Theory (LST) in flat space doesn’t have any dimensionless parameters, which could have been used for a perturbative expansion

  • In this paper, we study the 6d Little String Theory (LST) on curved manifolds, by using its holographic duality to Type II string theory in asymptotically linear dilaton backgrounds

  • We focus on backgrounds with a large number of Killing vectors, without requiring supersymmetry

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Summary

The holographic setup

We will be using the holographic correspondence to study LST, and we will be working in the low-energy supergravity approximation to Type II string theory, without turning on any Ramond-Ramond fields. We will assume for simplicity that the S3 factor in the string frame metric remains intact; it is clear from the worldsheet that this always gives a consistent solution, since it is a decoupled CFT (though it may not be the most general solution). The function c2(r) can be fixed to any desired value by a diffeomorphism of r, so its equation of motion gives a constraint C[ci(r)] of first order in derivatives rather than a second order equation. From the worldsheet point of view, (2.11) captures the fact that while flat spaces (κk = 0) give CFTs, curved spaces have a non-vanishing beta function on the worldsheet for their curvature, which has to be canceled in the context of our solution by having their size depend on the radial direction r (and modifying the linear dilaton solution)

Solving the equations of motion
Asymptotic limit
Series solution
Numerical solution
The free energy and thermodynamics
Corrections to the Hagedorn spectrum
Instability
Oscillations near singular solutions
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