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2021

Direct detection of dark energy: the XENON1T excess and future prospects

Vagnozzi, Sunny, Visinelli, Luca, Brax, Philippe et al.

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We explore the prospects for direct detection of dark energy by current and upcoming terrestrial dark matter direct detection experiments.

If dark energy is driven by a new light degree of freedom coupled to matter and photons then dark energy quanta are predicted to be produced in the Sun.
These quanta free-stream towards Earth where they can interact with Standard Model particles in the detection chambers of direct detection experiments, presenting the possibility that these experiments could be used to test dark energy.
Screening mechanisms, which suppress fifth forces associated with new light particles, and are a necessary feature of many dark energy models, prevent production processes from occurring in the core of the Sun, and similarly, in the cores of red giant, horizontal branch, and white dwarf stars.

Direct detection of dark energy: the XENON1T excess and future prospects · Around

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