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

Multi-transonic accretion for a spinning black hole has been compared amongdifferent disc geometries within post Newtonian pseudo potential framework. Thevariation of stationary shock characteristics with black hole spin has beenstudied in details for all the disc models and compared for adiabatic as wellas for isothermal scenario. The variations of surface gravity with spin for allthese cases have also been investigated.

Model dependence of the multi-transonic behavior, stability properties and corresponding acoustic geometry for accretion onto a spinning black hole