Weak Gravity Conjecture in de Sitter Space‐Time

Antoniadis, Ignatios; Benakli, Karim (2020). Weak Gravity Conjecture in de Sitter Space‐Time. Fortschritte der Physik / Progress of physics, 68(9), p. 2000054. Wiley-VCH 10.1002/prop.202000054

[img] Text
prop.202000054.pdf - Published Version
Restricted to registered users only
Available under License Publisher holds Copyright.

Download (408kB)

We propose a generalisation of the Weak Gravity Conjecture in de Sitter spaceby studying charged black-holes and comparing the gravitational and anabelian gauge forces. Using the same condition as in flat space, namely theabsence of black-hole remnants, one finds that for a given mass m thereshould be a state with a charge q bigger than a minimal value qmin(m, l),depending on the mass and the de Sitter radius l , in Planck units. In the largeradius flat space limit (large l), qmin->m leading to the known result q > m / ..2, while in the highly curved case (small l) qmin behaves as ..ml.Wealso discuss the example of the gauged R-symmetry in N = 1 supergravity.

Item Type:

Journal Article (Original Article)

Division/Institute:

10 Strategic Research Centers > Albert Einstein Center for Fundamental Physics (AEC)
08 Faculty of Science > Institute of Theoretical Physics

UniBE Contributor:

Antoniadis, Ignatios

Subjects:

500 Science > 530 Physics

ISSN:

0015-8208

Publisher:

Wiley-VCH

Language:

English

Submitter:

Esther Fiechter

Date Deposited:

16 Nov 2020 14:40

Last Modified:

05 Dec 2022 15:41

Publisher DOI:

10.1002/prop.202000054

ArXiv ID:

2006.12512

BORIS DOI:

10.7892/boris.147905

URI:

https://boris.unibe.ch/id/eprint/147905

Actions (login required)

Edit item Edit item
Provide Feedback