Positivity in the Sky: Constraining dark energy and modified gravity from the UV

Positivity bounds-the consequences of requiring a unitary, causal, local UV completion-place strong restrictions on theories of dark energy and/or modified gravity. We derive and investigate such bounds for Horndeski scalar-tensor theories and for the first time pair these bounds with a cosmological...

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Bibliographic Details
Published in:Physical review. D 2020-01, Vol.101 (2), p.1, Article 021502
Main Authors: Melville, S., Noller, J.
Format: Article
Language:English
Subjects:
Constraining
Dark energy
Gravitation
Gravitational waves
Parameter estimation
Parameter modification
Red shift
Tensors
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Summary:Positivity bounds-the consequences of requiring a unitary, causal, local UV completion-place strong restrictions on theories of dark energy and/or modified gravity. We derive and investigate such bounds for Horndeski scalar-tensor theories and for the first time pair these bounds with a cosmological parameter estimation analysis, using CMB, redshift space distortion, matter power spectrum, and baryon acoustic oscillation measurements from the Planck, SDSS/BOSS, and 6dF surveys. Using positivity bounds as theoretical priors, we show that their inclusion in the parameter estimation significantly improves the constraints on dark energy/modified gravity parameters. Considering as an example a specific class of models, which are particularly well-suited to illustrate the constraining power of positivity bounds, we find that these bounds eliminate over 60% of the previously allowed parameter space. We also discuss how combining positivity requirements with additional theoretical priors has the potential to further tighten these constraints: for instance, also requiring a subluminal speed of gravitational waves eliminates all but ≲1% of the previously allowed parameter space.
ISSN:2470-0010
2470-0029
DOI:10.1103/PhysRevD.101.021502