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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We present a multi‐polytrope approach to describe high‐mass twins fulfilling chiral effective field theory estimations of the neutron star equation of state and test it against the appearance of mixed phases at the hadron–quark interface. In addition, we discuss astrophysical applications of this method and the expected future measurements that will further constrain neutron star matter and the understanding of the quantum chromodynamics phase diagram.

Mixed phase within the multi‐polytrope approach to high‐mass twins