Abstract
Abstract
If Euclidean wormholes contribute meaningfully to the path integral of quantum gravity they can have important implications for particle physics and cosmology. The dominant effects arise from wormholes whose sizes are comparable to the cut-off scale of effective field theory, for which ultraviolet corrections become relevant. We study corrections to classical axion wormhole solutions in string motivated scenarios in which the dilaton partner of the axion becomes massive. We find corrections near the neck region which are consistent with a recent version of the weak gravity conjecture for axions.
Funder
Israel Science Foundation
DOE
KU Leuven C1 Grant
German Research Foundation
Institute for Basic Science
Subject
Physics and Astronomy (miscellaneous)
Cited by
10 articles.
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