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Dark Energy and the Symbiosis Between Micro-physics and Cosmology (Naturally)

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arxiv 2509.00688 v1 pith:R77L5KU2 submitted 2025-08-31 hep-th astro-ph.COgr-qchep-ph

Dark Energy and the Symbiosis Between Micro-physics and Cosmology (Naturally)

classification hep-th astro-ph.COgr-qchep-ph
keywords darkenergyapproacheslecturesnaturalnessphysicssymbiosistheories
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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These lectures aim to highlight the remarkable symbiosis that currently exists between the physics of the very small and the physics of the very large, using the unsolved puzzle of the nature of Dark Energy as a vehicle for so doing. The lectures first summarize what we know observationally about the properties of Dark Energy (and the Dark sector more broadly) and then discuss several approaches to explain them. Along the way this involves determining the types of interactions that would on general grounds be expected to be present in the low-energy limit of fundamental theories involving the many hierarchy of scales we see around us. This includes (but is not limited to) a discussion of technical naturalness (and `t Hooft naturalness) as well as the arguments for their use as a criterion for distinguishing amongst candidate theories. Some recent approaches I find promising are briefly summarized at the end.

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Cited by 3 Pith papers

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    A Weyl-invariant SM+mirror-dark-matter+gravity model is developed via algebraic renormalization; its conformal cohomology is claimed trivial, and the required counterterms could — the author concedes not conclusively ...

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  3. Anomaly footprints in SM+Gravity

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