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

The influence of cosmological constant type dark energy in the early universeis investigated. This is accommodated by a new dispersion relation in de Sitterspacetime. We perform a global fitting to explore the cosmological parametersspace by using the CosmoMC package with the recently released Planck TT andWMAP Polarization datasets. Using the results from global fitting, we compute anew CMB temperature-temperature spectrum. The obtained TT spectrum has lowerpower compared with the one based on $\Lambda$CDM model at large scales.

Inflation in de Sitter spacetime and CMB large scales anomaly