Charged Nariai black holes on the dark bubble

Abstract

In this paper, we realise the charged Nariai black hole on a braneworld from a nucleated bubble in AdS${}_5$, known as the dark bubble model. Geometrically, the black hole takes the form of a cylindrical spacetime pulling on the dark bubble. This is realised by a brane embedding in an AdS${}_5$ black string background. Identifying the brane with a D3-brane in string theory allows us to determine a relation between the fine structure constant and the string coupling, ${\alpha }_{\text{EM}}=\frac{3}{2}{g}_s$, which was previously obtained for a microscopic black hole. We also speculate on the consequences for the Festina Lente bound and neutrino masses.

arXiv comment23 pages + appendices, 2 figures; v2: Minor changes and clarifications, improved discussion at the end of section 5, accepted version in Classical and Quantum Gravity

References in corpus (40)

• Black Strings and p-Branes are Unstable
• Distance and de Sitter Conjectures on the Swampland
• De Sitter Space and the Swampland
• Supersymmetric, cold and lukewarm black holes in cosmological Einstein-Maxwell theory
• What if string theory has no de Sitter vacua?
• The evolution of unstable black holes in anti-de Sitter space
• Trans-Planckian Censorship and the Swampland
• Duality between Electric and Magnetic Black Holes
• Pair Creation of Black Holes During Inflation
• Born-Infeld Black Holes in (A)dS Spaces
• Instabilities of Black Strings and Branes
• Emergent de Sitter Cosmology from Decaying AdS
• Festina Lente: EFT Constraints from Charged Black Hole Evaporation in de Sitter
• Supersymmetry of Black Strings in D=5 Gauged Supergravities
• Charged Nariai Black Holes With a Dilaton
• Black string solutions with negative cosmological constant
• Magnetic Strings In Five Dimensional Gauged Supergravity Theories
• de Sitter in non-supersymmetric string theories: no-go theorems and brane-worlds
• Quintessence and the Swampland: The parametrically controlled regime of moduli space
• Counter-examples to the correlated stability conjecture
• de Sitter Cosmology on an expanding bubble
• Asymptotic Scalar Field Cosmology in String Theory
• The $F$-term Problem and other Challenges of Stringy Quintessence
• On the stability of AdS black strings
• Quintessence and the Swampland: The numerically controlled regime of moduli space
• Black strings in AdS_5
• (Quasi-) de Sitter solutions across dimensions and the TCC bound
• Dark bubbles: decorating the wall
• Supersymmetry Breaking and Stability in String Vacua: brane dynamics, bubbles and the swampland
• On de Sitter Spacetime and String Theory
• From black strings to black holes: nuttier and squashed AdS${}_5$ solutions
• A stringy realization of a small and positive cosmological constant in dark bubble cosmology
• Correlated stability conjecture revisited
• Dark bubbles and black holes
• Catalytic Creation of Baby Bubble Universe with Small Positive Cosmological Constant
• Features of a dark energy model in string theory
• Can the correlated stability conjecture be saved?
• dS${}_4$ universe emergent from Kerr-AdS${}_5$ spacetime: bubble nucleation catalyzed by a black hole
• Over-extremal brane shells from string theory?
• Shedding light on dark bubble cosmology

Cited by in corpus (3)

• Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
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