7–13 Sept 2025
Hermitage Hotel, Isola D'Elba
Europe/Rome timezone

Superheavy Dark Matter, GUT Axions and High Frequency GWs from Structure Formation and X Miracle

Not scheduled
30m
Hermitage Hotel, Isola D'Elba

Hermitage Hotel, Isola D'Elba

57037 Portoferraio Isola d’Elba (Li) Italy
Talk Dark Matter (Its nature: Theory, Observations, Detection, Production at accelerators) Afternoon session

Speaker

Zhijie (Jay) Xu (Pacific Northwest National Lab)

Description

We propose a new framework based on structure formation at the free-streaming scale and a modified "X miracle" beyond the standard WIMP paradigm. Both point to nonthermal, superheavy fermionic dark matter of $10^{12}$GeV. Unlike WIMPs that are light, semi-relativistic, and unaffected by gravity at freeze-out, the X miracle incorporates gravity, introducing a new fundamental scale $r_X=10^{-13}$m$\gg m_X^{-1}$ that breaks the unitarity bound and allows for a large cross section $10^{-21}$m$^3$/s. At this mass, free streaming mass matches the particle mass, enabling the earliest gravitationally bound structures to form at $10^{-6}$s and release binding energy as 100kHz gravitational waves or as GUT-scale axions. Superheavy sterile neutrinos are natural candidates, addressing dark matter, neutrino mass, and baryogenesis. Boltzmann equation suggests a relic abundance from early annihilation, with one in a billion particles surviving. This offers explanations for ultra-high-energy cosmic rays and Hubble tension.

References arXiv:2202.07240

Author

Zhijie (Jay) Xu (Pacific Northwest National Lab)

Presentation materials