Boosted dark matter from a phantom fluid
James M. Cline, Matteo Puel, Takashi Toma

TL;DR
The paper proposes that vacuum decay in phantom dark energy models can produce boosted dark matter or radiation, which could be detected directly, and uses experimental data to constrain these models and explain recent excess events.
Contribution
It introduces a novel mechanism where vacuum decay in phantom dark energy models generates boosted dark matter or radiation, linking cosmological theory with direct detection experiments.
Findings
Constraints on vacuum decay models from XENONnT data
Explanation of DAMIC excess events as dark radiation from vacuum decay
Potential new detection channel for dark matter related to phantom energy
Abstract
It is known that theories of phantom dark energy, considered as quantum fields, predict a continuous production of positive- plus negative-energy particles, from spontaneous decay of the vacuum. We show that this can be a new source of boosted dark matter or radiation, with consequences for direct detection. We set constraints on such models using data from the XENONnT experiment, and we show that recent excess events reported by the DAMIC experiment can be consistently described as coming from dark radiation, produced by vacuum decay, interacting with electrons.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
