Saved in:
Bibliographic Details
Main Authors: Ferko, Christian, Sethi, Savdeep
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2506.20765
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866908426643177472
author Ferko, Christian
Sethi, Savdeep
author_facet Ferko, Christian
Sethi, Savdeep
contents One of the key issues in holography is going beyond $\mathrm{AdS}$ and defining quantum gravity in spacetimes with a null boundary. Recent examples of this type involve linear dilaton asymptotics and are related to the $T \overline{T}$ deformation. We present a holographic correspondence derived from string theory, which is an example of a kind of celestial holography. The holographic definition is a spacetime non-commutative open string theory supported on D1-D5 branes together with fundamental strings. The gravity solutions interpolate between $\mathrm{AdS}_3$ metrics and six-dimensional metrics. Radiation can escape to null infinity, which makes both the encoding of quantum information in the boundary and the dynamics of black holes quite different from $\mathrm{AdS}$ spacetimes.
format Preprint
id arxiv_https___arxiv_org_abs_2506_20765
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Holography with Null Boundaries
Ferko, Christian
Sethi, Savdeep
High Energy Physics - Theory
General Relativity and Quantum Cosmology
One of the key issues in holography is going beyond $\mathrm{AdS}$ and defining quantum gravity in spacetimes with a null boundary. Recent examples of this type involve linear dilaton asymptotics and are related to the $T \overline{T}$ deformation. We present a holographic correspondence derived from string theory, which is an example of a kind of celestial holography. The holographic definition is a spacetime non-commutative open string theory supported on D1-D5 branes together with fundamental strings. The gravity solutions interpolate between $\mathrm{AdS}_3$ metrics and six-dimensional metrics. Radiation can escape to null infinity, which makes both the encoding of quantum information in the boundary and the dynamics of black holes quite different from $\mathrm{AdS}$ spacetimes.
title Holography with Null Boundaries
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2506.20765