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S. Lee, W. Lerche and T. Weigand, Modular Fluxes, Elliptic Genera, and Weak Gravity Conjectures in Four Dimensions , JHEP 08
Original
1901
Earlier work this paper cites.
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Original
1903
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Original
1903
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S. Shirai and M. Yamazaki, Is Gravity the Weakest Force? , [arXiv:1904.10577 [hep-th]]
Original
1904
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N. Craig, I. Garcia Garcia and S. Koren, The Weak Scale from Weak Gravity , JHEP 09
Original
1904
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Original
1904
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1904
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Similar

I. Zlatev, L. Wang and P. J. Steinhardt, Quintessence, cosmic coincidence, and the cosmological constant , Phys. Rev. Lett. 82
1999
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T. Barreiro, E. J. Copeland and N. Nunes, Quintessence arising from exponential potentials , Phys. Rev. D 61
2000
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G. Dall’Agata and M. Morittu, Covariant formulation of BPS black holes and the scalar weak gravity conjecture , JHEP 03
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2001
Cited alongside, same era.
T. Daus, A. Hebecker, S. Leonhardt and J. March-Russell, Towards a Swampland Global Symmetry Conjecture using Weak Gravity , [arXiv:2002.02456 [hep-th]]
Original
2002
Cited alongside, same era.
D. Andriot, N. Cribiori and D. Erkinger, The web of swampland conjectures and the TCC bound , [arXiv:2004.00030 [hep-th]]
Original

Then

L. E. Ibanez, M. Montero, A. Uranga and I. Valenzuela, Relaxion Monodromy and the Weak Gravity Conjecture , JHEP 04
Original
2016
Later among the works it cites.
A. Hebecker, F. Rompineve and A. Westphal, Axion Monodromy and the Weak Gravity Conjecture , JHEP 04
Original
2016
Later among the works it cites.
T.D. Brennan, F. Carta, and C. Vafa, The String Landscape, The Swampland, and the Missing Corner , PoS TASI2017 (2017) 015 [arXiv: 1711.00864v3 [hep-th]]
2017
Later among the works it cites.
E. Palti, The Weak Gravity Conjecture and Scalar Fields , JHEP 1708
Original
2017
Later among the works it cites.
D. Klaewer and E. Palti, Super-Planckian Spatial Field Variations and Quantum Gravity , JHEP 01
Original

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2020

Revisiting the Scalar Weak Gravity Conjecture

Benakli, Karim, Branchina, Carlo, Lafforgue-Marmet, Gaëtan

Understand

We revisit the Scalar Weak Gravity Conjecture and investigate the possibility to impose that scalar interactions dominate over gravitational ones.

More precisely, we look for consequences of assuming that, for leading scalar interactions, the corresponding gravitational contribution is sub-dominant in the non-relativistic limit.
For a single massive scalar particle, this leads us to compare four-point self-interactions in different type of potentials.
For axion-like particles, we retrieve the result of the Axion Weak Gravity Conjecture: the decay constant $f$ is bounded by the Planck mass, $f < {M_{Pl}}$.