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arxiv: 1105.4539 · v2 · pith:QJBEGVP3new · submitted 2011-05-23 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph· nucl-th

Effective potential for quantum scalar fields on a de Sitter geometry

classification ✦ hep-th astro-ph.COgr-qchep-phnucl-th
keywords fieldpotentialsittereffectivegeometryquantumscalaracquires
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We study the quantum theory of an O(N) scalar field on de Sitter geometry at leading order in a nonperturbative 1/N-expansion. This resums the infinite series of so-called superdaisy loop diagrams. We obtain the de Sitter symmetric solutions of the corresponding, properly renormalized, dynamical field equations and compute the complete effective potential. Because of its self-interactions, the field acquires a strictly positive square mass which screens potential infrared divergences. Moreover, strongly enhanced ultralong-wavelength fluctuations prevent the existence of a spontaneously broken symmetry state in any dimension.

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  1. Scalar field effective potentials in de Sitter spacetime

    hep-th 2025-11 unverdicted novelty 5.0

    Explicit one-loop computation shows the constraint effective potential for scalars in de Sitter is free of infrared problems and supports its use in stochastic Starobinsky-Yokoyama inflation.