English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Suppression of the scalar power spectrum on large scales is one way toreconcile the tension between Planck and BICEP2 data. This suppression canoccur by introducing a phase transition from the fast-roll phase to theslow-roll phase in a single field inflation model. In this paper we consider adeformed single field inflation model in terms of three SO(3) symmetric modulifields. We find that spatially linear solutions for the moduli fields induces aphase transition during the early stage of the inflation and the suppression ofscalar power spectrum at large scale perturbation modes.

Large Scale Suppression of Scalar Power on a Spatial Condensation