VISCOSITY OF STRONGLY COUPLED GAUGE THEORIES
World Scientific Publishing (2004) 455-463
Asymmetric Sneutrino Dark Matter and the Omega(b)/Omega(DM) Puzzle
ArXiv hep-ph/0410114 (2004)
Abstract:
The inferred values of the cosmological baryon and dark matter densities are strikingly similar, but in most theories of the early universe there is no true explanation of this fact; in particular, the baryon asymmetry and thus density depends upon unknown, and {\it a priori} unknown and possibly small, CP-violating phases which are independent of all parameters determining the dark matter density. We consider models of dark matter possessing a particle-antiparticle asymmetry where this asymmetry determines both the baryon asymmetry and strongly effects the dark matter density, thus naturally linking $\Omega_{\rm{b}}$ and $\Omega_{\rm{dm}}$. We show that sneutrinos can play the role of such dark matter in a previously studied variant of the MSSM in which the light neutrino masses result from higher-dimensional supersymmetry-breaking terms.Asymmetric Sneutrino Dark Matter and the Omega(b)/Omega(DM) Puzzle
(2004)
Stability of branonium
Physical Review D - Particles, Fields, Gravitation and Cosmology 70:8 (2004) 083518-1-083518-7