Remarks on the Cosmological Constant and the $\lambda {\Phi }^4$ Phase Transition

Abstract

We reanalyze the problem of the cosmological constant associated with the phase transition in a self-interacting scalar theory. It is pointed out that the generally accepted ``triviality'' of $(\lambda {\Phi }^4{)}_4$ implies a first-order phase transition. As a consequence, Spontaneous Symmetry Breaking can be consistent with zero cosmological constant if one assumes that it vanishes in the symmetric phase $<\Phi >=0$.

Comments: 11 pages, RevTeX