PaperPanorama

arXiv:2106.03549·v3·High Energy Physics — Phenomenology

QCD surprises: strong CP problem, neutrino mass, Dark Matter and Dark Energy

Andrea Addazi🇨🇳 · Antonino Marciano🇨🇳 · Roman Pasechnik🇸🇪 · Kaiqiang Alan Zeng🇨🇳

PDFarXivINSPIREDOI

Abstract

An unexpected explanation for neutrino mass, Dark Matter (DM) and Dark Energy (DE) from genuine Quantum Chromodynamics (QCD) of the Standard Model (SM) is proposed here, while the strong CP problem is resolved without any need to account for fundamental axions. We suggest that the neutrino sector can be in a double phase in the Universe: i) relativistic neutrinos, belonging to the SM; ii) non-relativistic condensate of Majorana neutrinos. The condensate of neutrinos can provide an attractive alternative candidate for the DM, being in a cold coherent state. We will explain how neutrinos, combining into Cooper pairs, can form collective low-energy degrees of freedom, hence providing a strongly motivated candidate for the QCD (composite) axion.

Comments: 6 pages, 2 figures; a typo fixed; acknowledgments added; conclusions unchanged

Citation historyopen in Citation History ↗