Remarks on the Cosmological Constant and the $λΦ^4$ Phase Transition

Details Remarks on the Cosmological Constant and the $λΦ^4$ Phase Transition Remarks on the Cosmological Constant and the $λΦ^4$ Phase Transition

1995-05-17

arxiv.org/abs/hep-ph/9505323v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

11 pages, RevTeX

Scientific paper

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 $<\Phi>=0$.

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