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2021

The Early Dark Sector, the Hubble Tension, and the Swampland

McDonough, Evan, Lin, Meng-Xiang, Hill, J. Colin et al.

Understand

We consider the interplay of the Early Dark Energy (EDE) model, the Swampland Distance Conjecture (SDC), and cosmological parameter tensions.

EDE is a proposed resolution of the Hubble tension relying upon a near-Planckian scalar field excursion, while the SDC predicts an exponential sensitivity of masses of other fields to such an excursion, $m\propto e^{-c|\Delta \phi|/M_{\rm pl}}$ with $c\sim{\cal O}(1)$.
Meanwhile, EDE is in tension with large-scale structure (LSS) data, due to shifts in the standard $\Lambda$CDM parameters necessary to fit the cosmic microwave background (CMB).
One might hope that a proper treatment of the model, e.g., accounting for the SDC, may ameliorate the tension with LSS.