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The curvature perturbation in a box

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arxiv 0707.0361 v2 pith:544AILGP submitted 2007-07-03 astro-ph gr-qchep-phhep-th

David H. Lyth This is my paper · ORCID
classification astro-phgr-qchep-phhep-th
keywords curvatureperturbationarisingbestcosmologicaldefineddiscussexpansion
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The stochastic properties of cosmological perturbations are best defined through the Fourier expansion in a finite box. I discuss the reasons for that with reference the curvature perturbation, and explore some issues arising from it.

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Cited by 1 Pith paper

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  1. Curvaton distribution from stochastic inflation

    astro-ph.CO 2024-11 conditional novelty 5.0 of 10

    Closed-form probability distributions for the curvature perturbation are derived for four exactly solvable curvaton potentials, and the mass-decay-rate parameter space is split into regions by the probability of produ...

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