Cosmological constant from degenerate vacua

Phys Rev Lett. 2002 Apr 15;88(15):151302. doi: 10.1103/PhysRevLett.88.151302. Epub 2002 Mar 28.

Abstract

Under the hypothesis that the cosmological constant vanishes in the true ground state with lowest possible energy density, we argue that the observed small but finite vacuumlike energy density can be explained if we consider a theory with two or more degenerate perturbative vacua, which are unstable due to quantum tunneling, and if we still live in one of such states. An example is given making use of the topological vacua in non-Abelian gauge theories.