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

We propose a relativistic model of hybrid star admitting conformal symmetryconsidering quark matter and baryonic matter as two different fluids. We defineinteraction equations between the normal baryonic matter and the quark matterand study the physical situations for repulsive, attractive and zerointeraction between the constituent matters. From the interaction equations wefind out the value of the equation of state (EOS) parameter for normal baryonicmatter which is found to be consistent with the value obtained from the Waleckamodel for nucleonic matter at high density. The measured value of the Bagconstant is used to explore the space time geometry inside the star. Thetheoretical mass-radius values are compared with the available observationaldata of the compact objects. From the nature of the match with theobservational data, we predict the nature of interaction that must be presentinside the hybrid stars

A new relativistic model of hybrid star with interactive quark matter and dense baryonic matter