On the weak gravity conjecture in string theory with broken supersymmetry
- 1. CPHT, CNRS, Ecole polytechnique, IP Paris, F-91128 Palaiseau (France)
- 2. Institut de Physique Théorique, Université Paris Saclay, CEA, CNRS, Orme des Merisiers, 91191 Gif-sur-Yvette Cedex (France)
Description
We use type I string models with supersymmetry broken by compactification (à la Scherk-Schwarz) in order to test the weak gravity conjecture in the presence of runaway potentials in a perturbative string theory setting. For a finite value of the supersymmetry breaking radius there is a runaway potential, which is the only possibility if one accepts the non-existence of de Sitter vacua. Although the weak gravity conjecture is valid in the decompactification limit, for fixed values of the radius we show that there are short-ranged attractive D1 brane-brane interactions. We argue however that at one-loop level the effective tension of the branes decreases and becomes smaller than the effective charge such that there is a long-ranged repulsive force and the weak gravity conjecture is respected. Moreover, for very small we expect a large number of stable bound states to be present.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nuclphysb.2019.114738Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysb.2019.114738;
- arXiv
- arXiv:1811.11199v3;
- PII
- S055032131930224X;
Publishing Information
- Journal Title
- Nuclear Physics. B
- Journal Volume
- 947
- Journal Page Range
- p. 114738
- ISSN
- 0550-3213
- CODEN
- NUPBBO
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51048502
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BOUND STATE; DE SITTER GROUP; DE SITTER SPACE; EFFECTIVE CHARGE; GRAVITATION; STRING MODELS; STRING THEORY; SUPERSYMMETRY; SYMMETRY BREAKING
- Descriptors DEC
- COMPOSITE MODELS; EXTENDED PARTICLE MODEL; LIE GROUPS; MATHEMATICAL MODELS; MATHEMATICAL SPACE; M-THEORY; PARTICLE MODELS; QUARK MODEL; SPACE; SYMMETRY; SYMMETRY GROUPS
Optional Information
- Notes
- © 2019 The Authors. Published by Elsevier B.V.