Sharpening the Weak Gravity Conjecture with Dimensional Reduction
TL;DR: In this paper, the weak gravity conjecture was investigated under toroidal compactification and RG flows, finding evidence that WGC bounds for single photons become weaker in the infrared and a superextremal particle should exist for every charge in the charge lattice.
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Abstract: We investigate the behavior of the Weak Gravity Conjecture (WGC) under toroidal compactification and RG flows, finding evidence that WGC bounds for single photons become weaker in the infrared. By contrast, we find that a photon satisfying the WGC will not necessarily satisfy it after toroidal compactification when black holes charged under the Kaluza-Klein photons are considered. Doing so either requires an infinite number of states of different charges to satisfy the WGC in the original theory or a restriction on allowed compactification radii. These subtleties suggest that if the Weak Gravity Conjecture is true, we must seek a stronger form of the conjecture that is robust under compactification. We propose a "Lattice Weak Gravity Conjecture" that meets this requirement: a superextremal particle should exist for every charge in the charge lattice. The perturbative heterotic string satisfies this conjecture. We also use compactification to explore the extent to which the WGC applies to axions. We argue that gravitational instanton solutions in theories of axions coupled to dilaton-like fields are analogous to extremal black holes, motivating a WGC for axions. This is further supported by a match between the instanton action and that of wrapped black branes in a higher-dimensional UV completion.
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CMB-S4 Science Book, First Edition
Kevork N. Abazajian,Peter Adshead,Zeeshan Ahmed,Steven W. Allen,David Alonso,Kam Arnold,Carlo Baccigalupi,James G. Bartlett,Nicholas Battaglia,Bradford Benson,Colin A. Bischoff,Julian Borrill,Victor Buza,Erminia Calabrese,Robert R. Caldwell,John E. Carlstrom,C. L. Chang,T. M. Crawford,Francis-Yan Cyr-Racine,Francesco De Bernardis,Tijmen de Haan,Sperello di Serego Alighieri,Joanna Dunkley,Cora Dvorkin,Josquin Errard,Giulio Fabbian,Stephen M. Feeney,Simone Ferraro,Jeffrey P. Filippini,Raphael Flauger,George M. Fuller,Vera Gluscevic,Daniel Green,Daniel Grin,Evan Grohs,Jason W. Henning,J. Colin Hill,Renée Hlozek,Gilbert Holder,W. L. Holzapfel,Wayne Hu,Kevin M. Huffenberger,Reijo Keskitalo,Lloyd Knox,Arthur Kosowsky,John M Kovac,Ely D. Kovetz,Chao-Lin Kuo,Akito Kusaka,Maude Le Jeune,Adrian T. Lee,M. Lilley,Marilena LoVerde,Mathew S. Madhavacheril,Adam Mantz,David J. E. Marsh,Jeff McMahon,P. D. Meerburg,Joel Meyers,Amber Miller,Julian B. Muñoz,Ho Nam Nguyen,Michael D. Niemack,Marco Peloso,J. Peloton,Levon Pogosian,C. Pryke,Marco Raveri,Christian L. Reichardt,Graca Rocha,Aditya Rotti,Emmanuel Schaan,Marcel Schmittfull,Douglas Scott,Neelima Sehgal,Sarah Shandera,Blake D. Sherwin,Tristan L. Smith,Lorenzo Sorbo,Glenn D. Starkman,K. T. Story,Alexander van Engelen,Joaquin Vieira,Scott Watson,Nathan Whitehorn,W. L. Kimmy Wu +85 more
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TL;DR: The CMB-S4 project as discussed by the authors is a ground-based cosmic microwave background (CMB) experiment with superconducting cameras, which will be used for the search for the B-mode polarization signature of primordial gravitational waves and the determination of the number and masses of neutrinos.
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TL;DR: The Swampland program aims to distinguish effective theories which can be completed into quantum gravity in the ultraviolet from those which cannot as mentioned in this paper, assuming only a knowledge of quantum field theory and general relativity.
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TL;DR: In this article, the authors sharpen the weak gravity conjecture by the statement that, except for BPS states in a supersymmetric theory, the gravitational force is strictly weaker than any electric force.
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TL;DR: In this paper, it was shown that any global symmetry, discrete or continuous, in a bulk quantum gravity theory with a CFT dual would lead to an inconsistency in that CFT, and thus that there are no bulk global symmetries in AdS/CFT.
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TL;DR: In this article, a brief overview of the string landscape and techniques used to construct string compactifications is given, and a number of conjectures that attempt to characterize theories in the swampland are reviewed.
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