A fully mirrored Standard Model can explain dark matter as mirror electrons while predicting dark radiation and gravitational wave signals tied to measured particle masses.
WIMP isocurvature perturbation and small scale structure
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
The adiabatic perturbation of dark matter is damped during the kinetic decoupling due to the collision with relativistic component on sub-horizon scales. However the isocurvature part is free from damping and could be large enough to make a substantial contribution to the formation of small scale structure. We explicitly study the weakly interacting massive particles as dark matter with an early mater dominated period before radiation domination and show that the isocurvature perturbation is generated during the phase transition and leaves imprint in the observable signatures for small scale structure.
fields
hep-ph 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Dark Matter, Dark Radiation and Gravitational Waves from Mirror Higgs Parity
A fully mirrored Standard Model can explain dark matter as mirror electrons while predicting dark radiation and gravitational wave signals tied to measured particle masses.