Bose–Fermi cancellation of cosmological Coleman–Weinberg potentials

DOI10.1088/1361-6382/AB9881zbMath1478.83258arXiv2003.03752OpenAlexW3098567760MaRDI QIDQ5161857

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Publication date: 1 November 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2003.03752

zbMATH Keywords

cosmologyquantum field theory on curved spaceprimordial inflation

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Geometrodynamics and the holographic principle (83E05) Fermionic systems in quantum theory (81V74) Bosonic systems in quantum theory (81V73)

Related Items (5)

Massless minimal quantum scalar field with an asymmetric self interaction in de Sitter spacetime ⋮ Non-perturbative analysis for a massless minimal quantum scalar with V(ϕ) = λϕ ⁴/4! + βϕ ³/3! in the inflationary de Sitter spacetime ⋮ When tadpoles matter: one-loop corrections for spectator Higgs in inflation ⋮ Non-perturbative \(\langle\phi\rangle\), \(\langle\phi^2\rangle\) and the dynamically generated scalar mass with Yukawa interaction in the inflationary de Sitter spacetime ⋮ Reheating with effective potentials

Cites Work

• Stochastic inflationary scalar electrodynamics

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