Dynamical mechanism for ultra-light scalar Dark Matter

Abstract

Assuming a double-well bare potential for a self-interacting scalar field, with the Higgs vacuum expectation value, it is shown that non-perturbative quantum corrections naturally lead to ultra-light particles of mass $\simeq 10^{-23}$eV, if these non-perturbative effects occur at a time consistent with the Electroweak phase transition. This mechanism could be relevant in the context of Bose Einstein Condensate studies for the description of cold Dark Matter. Given the numerical consistency with the Electroweak transition, an interaction potential for Higgs and Dark Matter fields is proposed, where spontaneous symmetry breaking for the Higgs field leads to the generation of ultra-light particles, in addition to the usual Higgs mechanism. This model also naturally leads to extremely weak interactions between the Higgs and Dark Matter particles.

12 pages, includes the derivation of the effective potential suppressed by the volume

References in corpus (3)

• Axion Cosmology
• Inflation, dark matter and dark energy in the string landscape
• An ultralight pseudoscalar boson

Cited by in corpus (8)

• Phase transitions between dilute and dense axion stars
• Collapse of a self-gravitating Bose-Einstein condensate with attractive self-interaction
• A predictive model of BEC dark matter halos with a solitonic core and an isothermal atmosphere
• Jeans type instability of a complex self-interacting scalar field in general relativity
• Jeans mass-radius relation of self-gravitating Bose-Einstein condensates and typical parameters of the dark matter particle
• Quantum tunneling rate of dilute axion stars close to the maximum mass
• Convexity at finite temperature and non-extensive thermodynamics
• Oscillating scalar field as dark matter through the cosmological epochs