Localized gravity, de Sitter, and the Horizon Criterion

Realizing de Sitter-like solutions in string theory remains challenging, prompting speculation about which specific feature might be responsible for their inconsistency in quantum gravity. In this work, we focus on the ‘Horizon Criterion’, which identifies spacetimes as problematic if they exhibit c...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Friedrich, Bjoern (VerfasserIn) , Hebecker, Arthur (VerfasserIn) , Schiller, Daniel (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 16 October 2025
In: Journal of high energy physics
Year: 2025, Heft: 10, Pages: 1-38
ISSN:1029-8479
DOI:10.1007/JHEP10(2025)151
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1007/JHEP10(2025)151
Verlag, kostenfrei, Volltext: https://link.springer.com/article/10.1007/JHEP10(2025)151
Volltext
Verfasserangaben:Bjoern Friedrich, Arthur Hebecker and Daniel Schiller
Beschreibung
Zusammenfassung:Realizing de Sitter-like solutions in string theory remains challenging, prompting speculation about which specific feature might be responsible for their inconsistency in quantum gravity. In this work, we focus on the ‘Horizon Criterion’, which identifies spacetimes as problematic if they exhibit cosmological horizons. In particular, we study the implications for spacetimes with dynamical boundaries. We argue that requiring inertial observers localized on an end-of-the-world (ETW) brane to be in causal contact with every other observer is too restrictive as there exist string-theoretic solutions without this property. Hence, if one does not want to abandon the idea of cosmological horizons being the fundamental issue with de Sitter, a refined condition is needed. The requirement that inertial, boundary-localized observers should be in causal contact with all other observers on the same ETW brane is such an appropriate refinement. We explore the consequences of this criterion for ETW branes whose energy density is governed by a scalar field, considering two cases: First, with a scalar field confined to the ETW brane, and second, with a bulk modulus subject to a brane-localized potential.
Beschreibung:Gesehen am 20.01.2026
Beschreibung:Online Resource
ISSN:1029-8479
DOI:10.1007/JHEP10(2025)151