Can all the infrared secular growth really be understood as increase of classical statistical variance?
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Publication:5023696
DOI10.1088/1475-7516/2018/11/022OpenAlexW2806393583WikidataQ128921419 ScholiaQ128921419MaRDI QIDQ5023696
Takahiro Tanaka, Junsei Tokuda
Publication date: 24 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1806.03262
Related Items (11)
Statistics of coarse-grained cosmological fields in stochastic inflation ⋮ Stochastic collapse ⋮ Scalar correlation functions for a double-well potential in de Sitter space ⋮ Feynman rules for stochastic inflationary correlators ⋮ Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation ⋮ Squeezed bispectrum and one-loop corrections in transient constant-roll inflation ⋮ Higgs vacuum (in)stability during inflation. The dangerous relevance of De Sitter departure and Planck-suppressed operators ⋮ Inflationary stochastic anomalies ⋮ Renormalisation group improvement in the stochastic formalism ⋮ A manifestly covariant theory of multifield stochastic inflation in phase space: solving the discretisation ambiguity in stochastic inflation ⋮ Anisotropic separate universe and Weinberg's adiabatic mode
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