Stable matter of 4th generation: hidden in the Universe and close to detection?

Abstract

Stable neutrino and U quark of 4th generation are excluded neither by experimental data, nor by astrophysical constraints. Moreover, excess of stable $\bar{U}$ quarks in the Universe can lead to an exciting composite nuclear-interacting form of dark matter, which can even dominate in large scale structure formation.

Submitted to the proceedings of the 12th Lomonosov Conference on Elementary Particle Physics, Moscow, 25-31 August, 2005

Cited by in corpus (22)

• Constraints on the Dark Matter Particle Mass from the Number of Milky Way Satellites
• Strong Interactive Massive Particles from a Strong Coupled Theory
• Physics of Dark Matter in the Light of Dark Atoms
• The Dark Side of Strongly Coupled Theories
• Composite dark matter from stable charged constituents
• High Energy Positrons and Gamma Radiation from Decaying Constituents of a two-component Dark Atom Model
• Proceedings to the 12th Workshop 'What Comes Beyond the Standard Models', Bled, July 14. - 24., 2009, Slovenia
• Composite Dark Matter and its Charged Constituents
• Stable quarks of the 4th family?
• ${}^3$He experimentum crucis for Dark Matter puzzles
• Dark photon dark matter and fast radio bursts
• Dark matter from stable charged particles?
• Low energy binding of composite dark matter with nuclei as a solution for the puzzles of dark matter searches
• The dark atoms of dark matter
• Dark Atoms and their decaying constituents
• Charge asymmetry of new stable quarks in baryon asymmetrical Universe
• Dark Atoms of the Universe: towards OHe nuclear physics
• Primordial heavy elements in composite dark matter models
• Accelerator probes for new stable quarks
• Probes for 4th generation constituents of dark atoms in Higgs boson studies at the LHC
• Test of the 4-th quark generation from the Cabibbo-Kobayashi-Maskawa matrix
• Balancing Asymmetric Dark Matter with Baryon Asymmetry by Sphaleron Transitions