A new spin on the Weak Gravity Conjecture
Abstract
The mild form of the Weak Gravity Conjecture states that quantum or higher-derivative corrections should decrease the mass of large extremal charged black holes at fixed charge. This allows extremal black holes to decay, unless protected by a symmetry (such as supersymmetry). We reformulate this conjecture as an integrated condition on the effective stress tensor capturing the effect of quantum or higher-derivative corrections. In addition to charged black holes, we also consider rotating BTZ black holes and show that this condition is satisfied as a consequence of the $$\textit{c}$$-theorem, proving a spinning version of the Weak Gravity Conjecture. We also apply our results to a five-dimensional boosted black string with higher-derivative corrections. The boosted black string has a BTZ×$S^2$ near-horizon geometry and, after Kaluza-Klein reduction, describes a four-dimensional charged black hole. Combining the spinning and charged Weak Gravity Conjecture we obtain positivity bounds on the five-dimensional Wilson coefficients that are stronger than those obtained from charged black holes alone.
- Authors:
-
- Univ. of Wisconsin, Madison, WI (United States). Dept. of Physics
- Univ. of Amsterdam (Netherlands). Inst. of Physics, GRAPPA and ITFA
- Publication Date:
- Research Org.:
- Univ. of Wisconsin, Madison, WI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); National Science Foundation (NSF)
- OSTI Identifier:
- 1852385
- Grant/Contract Number:
- SC0017647; NSF PHY-1748958
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of High Energy Physics (Online)
- Additional Journal Information:
- Journal Name: Journal of High Energy Physics (Online); Journal Volume: 2021; Journal Issue: 3; Journal ID: ISSN 1029-8479
- Publisher:
- Springer Nature
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Physics; Black Holes in String Theory; Models of Quantum Gravity; AdS-CFT Correspondence
Citation Formats
Aalsma, Lars, Cole, Alex, Loges, Gregory J., and Shiu, Gary. A new spin on the Weak Gravity Conjecture. United States: N. p., 2021.
Web. doi:10.1007/jhep03(2021)085.
Aalsma, Lars, Cole, Alex, Loges, Gregory J., & Shiu, Gary. A new spin on the Weak Gravity Conjecture. United States. https://doi.org/10.1007/jhep03(2021)085
Aalsma, Lars, Cole, Alex, Loges, Gregory J., and Shiu, Gary. Mon .
"A new spin on the Weak Gravity Conjecture". United States. https://doi.org/10.1007/jhep03(2021)085. https://www.osti.gov/servlets/purl/1852385.
@article{osti_1852385,
title = {A new spin on the Weak Gravity Conjecture},
author = {Aalsma, Lars and Cole, Alex and Loges, Gregory J. and Shiu, Gary},
abstractNote = {The mild form of the Weak Gravity Conjecture states that quantum or higher-derivative corrections should decrease the mass of large extremal charged black holes at fixed charge. This allows extremal black holes to decay, unless protected by a symmetry (such as supersymmetry). We reformulate this conjecture as an integrated condition on the effective stress tensor capturing the effect of quantum or higher-derivative corrections. In addition to charged black holes, we also consider rotating BTZ black holes and show that this condition is satisfied as a consequence of the $\textit{c}$-theorem, proving a spinning version of the Weak Gravity Conjecture. We also apply our results to a five-dimensional boosted black string with higher-derivative corrections. The boosted black string has a BTZ×$S^2$ near-horizon geometry and, after Kaluza-Klein reduction, describes a four-dimensional charged black hole. Combining the spinning and charged Weak Gravity Conjecture we obtain positivity bounds on the five-dimensional Wilson coefficients that are stronger than those obtained from charged black holes alone.},
doi = {10.1007/jhep03(2021)085},
journal = {Journal of High Energy Physics (Online)},
number = 3,
volume = 2021,
place = {United States},
year = {Mon Mar 08 00:00:00 EST 2021},
month = {Mon Mar 08 00:00:00 EST 2021}
}
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