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/

Zendy Plus

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

Zendy Tools

Zendy Open

Interaction of very low-frequency primordial(relic) gravitational waves(GWs)to cosmic microwave background(CMB) can generate B-mode polarization. Here, forthe first time we point out that the electromagnetic(EM) response tohigh-frequency GWs(HFGWs) would produce quasi-B-mode distribution of theperturbative photon fluxes, and study the duality and high complementaritybetween such two B-modes. Based on this quasi-B-mode in HFGWs, it is shown thatthe distinguishing and observing of HFGWs from the braneworld would be quitepossible due to their large amplitude, higher frequency and very differentphysical behaviors between the perturbative photon fluxes and backgroundphotons, and the measurement of relic HFGWs may also be possible though face toenormous challenge.

Quasi-B-mode generated by high-frequency gravitational waves and corresponding perturbative photon fluxes