Dark Phoenix: dark matter relic from its own decay
Abstract
We propose a novel mechanism for generating correct relic of dark matter (DM) which otherwise gets thermally overproduced from the conventional freeze-out mechanism. The mechanism, dubbed as {\it Dark Phoenix}, relies on a transient decay window for DM after its freeze-out which brings its relic within observed limits. Due to finite-temperature effects on masses, DM becomes heavier than its dark sector partner in this window allowing it to decay. The decay of DM then stops after gets a sudden jump in its mass from a first-order phase transition (FOPT) driven by another scalar . The dark sector partner , assumed to be a charged scalar, undergoes sufficient pair annihilation during this epoch such that its late decay into DM does not overproduce the latter again. While direct-detection rates of DM remains suppressed due to small couplings, the charged scalar can have interesting signatures like long-lived charged track at colliders. The associated FOPT can also lead to observable gravitational waves at future experiments like LISA.
Keywords
Cite
@article{arxiv.2607.08838,
title = {Dark Phoenix: dark matter relic from its own decay},
author = {Debasish Borah and Satyabrata Mahapatra and Indrajit Saha and Narendra Sahu and Vicky Singh Thounaojam},
journal= {arXiv preprint arXiv:2607.08838},
year = {2026}
}
Comments
11 pages, 8 captioned figures