Decaying dark matter is mapped to a scalar field model that requires phantom dark energy and is reinterpreted via a complex scalar with ultra-light mass to form a unified dark fluid whose phantom phase is a stable late-time attractor.
Cosmological structure formation in complex scalar field dark matter versus real ultralight axions: A comparative study using CLASS
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.CO 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Correspondence between a decaying dark matter sector scenario and scalar field model
Decaying dark matter is mapped to a scalar field model that requires phantom dark energy and is reinterpreted via a complex scalar with ultra-light mass to form a unified dark fluid whose phantom phase is a stable late-time attractor.