Light axiodilatons: matter couplings, weak-scale completions and long-distance tests of gravity

We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in 2110.10352 . We address the two main problems concerning the light axiodilaton that appears in the low-energy limit, namely that the axion has a very...

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Published inJournal of cosmology and astroparticle physics Vol. 2023; no. 8; pp. 11 - 51
Main Authors Brax, Philippe, Burgess, C.P., Quevedo, F.
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 01.08.2023
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Abstract We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in 2110.10352 . We address the two main problems concerning the light axiodilaton that appears in the low-energy limit, namely that the axion has a very low decay constant f a ∼ eV (as read from its kinetic term) and that the dilaton is subject to bounds that are relevant to tests of GR once ρ vac ≲ 10 -80   M p 4 . We show that eV scale axion decay constants need not be a problem by showing how supersymmetric extra dimensions provide a sample unitarization for axion physics above eV scales for which non-anomalous matter/axiodilaton couplings can really have gravitational strength, showing how naive EFT reasoning can mistakenly overestimates axion interactions at eV. When axions really do couple strongly at eV scales we identify the dimensionless interaction in the UV completion that is also O(1), and how axion energy-loss bounds map onto known extra-dimensional constraints. We find a broad new class of exact exterior solutions to the vacuum axiodilaton equations and knowledge of axiodilaton-matter couplings also allows us to numerically search for interior solutions that match to known exterior solutions that can evade solar-system tests. We find no examples that do so, but also identify potential new candidate mechanisms for reducing the effective dilaton-matter coupling to gravitating objects without also undermining the underlying suppression of ρ vac .
AbstractList We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in 2110.10352 . We address the two main problems concerning the light axiodilaton that appears in the low-energy limit, namely that the axion has a very low decay constant f a ∼ eV (as read from its kinetic term) and that the dilaton is subject to bounds that are relevant to tests of GR once ρ vac ≲ 10 -80   M p 4 . We show that eV scale axion decay constants need not be a problem by showing how supersymmetric extra dimensions provide a sample unitarization for axion physics above eV scales for which non-anomalous matter/axiodilaton couplings can really have gravitational strength, showing how naive EFT reasoning can mistakenly overestimates axion interactions at eV. When axions really do couple strongly at eV scales we identify the dimensionless interaction in the UV completion that is also O(1), and how axion energy-loss bounds map onto known extra-dimensional constraints. We find a broad new class of exact exterior solutions to the vacuum axiodilaton equations and knowledge of axiodilaton-matter couplings also allows us to numerically search for interior solutions that match to known exterior solutions that can evade solar-system tests. We find no examples that do so, but also identify potential new candidate mechanisms for reducing the effective dilaton-matter coupling to gravitating objects without also undermining the underlying suppression of ρ vac .
We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in arXiv:2110.10352. We address the two main problems concerning the light axiodilaton that appears in the low-energy limit, namely that the axion has a very low decay constant $f_a \sim $ eV (as read from its kinetic term) and that the dilaton is subject to bounds that are relevant to tests of GR once $\rho_{\rm vac} \leq 10^{-80} M_p^4$. We show that eV scale axion decay constants need not be a problem by showing how supersymmetric extra dimensions provide a sample unitarization for axion physics above eV scales for which non-anomalous matter/axiodilaton couplings can really have gravitational strength, showing how naive EFT reasoning can mistakenly overestimates axion interactions at eV. When axions really do couple strongly at eV scales we identify the dimensionless interaction in the UV completion that is also O(1), and how axion energy-loss bounds map onto known extra-dimensional constraints. We find a broad new class of exact exterior solutions to the vacuum axiodilaton equations and knowledge of axiodilaton-matter couplings also allows us to numerically search for interior solutions that match to known exterior solutions that can evade solar-system tests. We find no examples that do so, but also identify potential new candidate mechanisms for reducing the effective dilaton-matter coupling to gravitating objects without also undermining the underlying suppression of $\rho_{\rm vac}$.
We consider the physical implications of very light axiodilatons motivated by a novelmechanism to substantially reduce the vacuum energy proposed in 2110.10352. We addressthe two main problems concerning the light axiodilaton that appears in the low-energy limit,namely that the axion has a very low decay constant fa ∼ eV (as read from its kinetic term)and that the dilaton is subject to bounds that are relevant to tests of GR once ρvac ≲ 10-80 Mp4. We show that eV scale axion decay constants need not be a problem byshowing how supersymmetric extra dimensions provide a sample unitarization for axion physics aboveeV scales for which non-anomalous matter/axiodilaton couplings can really have gravitationalstrength, showing how naive EFT reasoning can mistakenly overestimates axion interactions ateV. When axions really do couple strongly at eV scales we identify the dimensionless interactionin the UV completion that is also O(1), and how axion energy-loss bounds map onto knownextra-dimensional constraints. We find a broad new class of exact exterior solutions to the vacuumaxiodilaton equations and knowledge of axiodilaton-matter couplings also allows us to numericallysearch for interior solutions that match to known exterior solutions that can evade solar-systemtests. We find no examples that do so, but also identify potential new candidate mechanisms forreducing the effective dilaton-matter coupling to gravitating objects without also undermining theunderlying suppression of ρvac.
Author Quevedo, F.
Burgess, C.P.
Brax, Philippe
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  givenname: F.
  surname: Quevedo
  fullname: Quevedo, F.
  organization: DAMTP, University of Cambridge, Wilberforce Road, Cambridge, CB3 0WA, U.K
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Issue 8
Keywords supersymmetry
dilaton
solar system
vacuum state
scale
decay
matter
unitarity
effective field theory
coupling
decay constant
gravitation
interaction
suppression
energy loss
kinetic
axion
electroweak interaction
energy
higher-dimensional
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Snippet We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in...
We consider the physical implications of very light axiodilatons motivated by a novelmechanism to substantially reduce the vacuum energy proposed in...
We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in...
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StartPage 11
SubjectTerms axions
cosmology with extra dimensions
Couplings
dark energy theory
Decay
Decay rate
Dilatons
High Energy Physics - Phenomenology
High Energy Physics - Theory
Physics
Title Light axiodilatons: matter couplings, weak-scale completions and long-distance tests of gravity
URI https://iopscience.iop.org/article/10.1088/1475-7516/2023/08/011
https://www.proquest.com/docview/2849007646
https://hal.science/hal-03936161
Volume 2023
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