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

It has been recently argued \cite{Barvinsky:2017lfl} that the de Sitter phasein cosmology might be naturally generated as a result of dynamics of thetopologically nontrivial sectors in a strongly coupled QCD-like gauge theory inexpanding universe. It is known that the de Sitter phase is realized in thehistory of our Universe twice: the first occurrence is coined as the inflation,while the second time (which is occurring now) is dubbed as the dark energy(DE). The crucial element of the proposal \cite{Barvinsky:2017lfl} is thepresence of a nontrivial gauge holonomy which is the source of the vacuumenergy leading to the de Sitter behaviour. It has been also argued that theanomalous coupling of the system with the Standard Model (SM) particles leadsto the reheating epoch in case of the {\it inflationary} phase. A similaranomalous coupling of the system with the Maxwell $E\&M$ field during the {\itDE epoch} generates the cosmological magnetic field. The intensity of the fieldis estimated on the level of $10^{-10}$G while the corresponding correlationlength reaches the scale of the visible Universe.

Cosmological Magnetic Field and Dark Energy as two sides of the same coin