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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In this work, we have illustrated the difference between both Tsallis andKaniadakis entropies through cosmological models obtained from the formalismproposed by Padmanabhan, which is called holographic equipartition law.Similarly to the formalism proposed by Komatsu, we have obtained an extradriving constant term in the Friedmann equation if we deform the Tsallisentropy by Kaniadakis' formalism. We have considered initially Tsallis entropyas the Black Hole (BH) area entropy. This constant term may lead the universeto be in an accelerated mode. On the other hand, if we start with theKaniadakis entropy as the BH area entropy and then by modifying the Kappaexpression by Tsallis' formalism, the same constant, which shows that theuniverse have an acceleration is obtained. In an opposite limit, no drivinginflation term of the early universe was derived from both deformations.

Tsallis and Kaniadakis statistics from a point of view of the holographic equipartition law