Abstract

In this note, we calculate the one-loop determinant for a massive scalar (with conformal dimension $\Delta$) in even-dimensional AdS$_{d+1}$ space, using the quasinormal mode method developed in arXiv:0908.2657 by Denef, Hartnoll, and Sachdev. Working first in two dimensions on the related Euclidean hyperbolic plane $H_2$, we find a series of zero modes for negative real values of $\Delta$ whose presence indicates a series of poles in the one-loop partition function $Z(\Delta)$ in the $\Delta$ complex plane; these poles contribute temperature-independent terms to the thermal AdS partition function computed in arXiv:0908.2657. Our results match those in a series of papers by Camporesi and Higuchi, as well as Gopakumar et al. in arXiv:1103.3627 and Banerjee et al. in arXiv:1005.3044. We additionally examine the meaning of these zero modes, finding that they Wick-rotate to quasinormal modes of the AdS$_2$ black hole. They are also interpretable as matrix elements of the discrete series representations of $SO(2,1)$ in the space of smooth functions on $S^1$. We generalize our results to general even dimensional AdS$_{2n}$, again finding a series of zero modes which are related to discrete series representations of $SO(2n,1)$, the motion group of $H_{2n}$.

Highlights

  • Several known ways to calculate the heat kernel

  • Working first in two dimensions on the related Euclidean hyperbolic plane H2, we find a series of zero modes for negative real values of ∆ whose presence indicates a series of poles in the one-loop partition function Z(∆) in the ∆ complex plane; these poles contribute temperature-independent terms to the thermal AdS partition function computed in [1]

  • In the case of AdS2, these zero modes are the Wick rotation of quasinormal modes for the AdS2 black hole

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Summary

Applying the zero-mode method to AdS2

We use the zero-mode method to calculate the 1-loop partition function for a complex scalar φ with mass m in Euclidean AdS2 with AdS length L. We find the poles in Z(∆) by searching for values of ∆ where det −∇2 + m2 becomes zero These ∆⋆ occur whenever there exists a φ⋆ solving. Where φ⋆ is smooth in the interior of the (Euclidean) AdS, and satisfies the boundary condition (2.3). That is, at these (generally complex) ∆⋆, φ⋆ is a zero mode. As we will show for AdS2, even a noncompact space may have a discrete set of poles, when we choose the appropriate boundary condition. Find the polynomial Pol(∆) by matching the zeta-function regularization at large ∆ to the local heat kernel curvature expansion expression for log Z(∆)

Finding the zero modes
Summing the contributions of the zero modes
Comparison with full eigenfunction heat kernel method
Two interesting properties of AdS2 zero modes
Zero modes Wick rotate to quasinormal modes
Zero modes as discrete series representations
The thermal partition function on AdS2
Extension of story to all even dimensions
Discussions and conclusions
Full Text
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