English

Holography of Linear Dilaton Spacetimes from the Bottom Up

High Energy Physics - Theory 2024-05-20 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

The linear dilaton background is the keystone of a string-derived holographic correspondence beyond AdSd+1_{d+1}/CFTd_d. This motivates an exploration of the (d+1)(d+1)-dimensional linear dilaton spacetime (LDd+1_{d+1}) and its holographic properties from the low-energy viewpoint. We first notice that the LDd+1_{d+1} space has simple conformal symmetries, that we use to shape an effective field theory (EFT) on the LD background. We then place a brane in the background to study holography at the level of quantum fields and gravity. We find that the holographic correlators from the EFT feature a pattern of singularities at certain kinematic thresholds. We argue that such singularities can be used to bootstrap the putative dd-dimensional dual theory using techniques analogous to those of the Cosmological Bootstrap program. Turning on finite temperature, we study the holographic fluid emerging on the brane in the presence of a bulk black hole. We find that the holographic fluid is pressureless for any dd due to a cancellation between Weyl curvature and dilaton stress tensor, and verify consistency with the time evolution of the theory. From the fluid thermodynamics, we find a universal temperature and Hagedorn behavior for any dd. This matches the properties of a CFT2_2 with large TTT\overline T deformation, and of little string theory for d=6d=6. Both the fluid equation of state and the spectrum of quantum fluctuations suggest that the dd-dimensional dual theory arising from LDd+1_{d+1} is generically gapped.

Keywords

Cite

@article{arxiv.2309.02489,
  title  = {Holography of Linear Dilaton Spacetimes from the Bottom Up},
  author = {Sylvain Fichet and Eugenio Megias and Mariano Quiros},
  journal= {arXiv preprint arXiv:2309.02489},
  year   = {2024}
}

Comments

40+11 pages, 3 figures