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

Following the basic prescriptions of the Tsallis’ nonextensive thermodynamics, we study the relativistic nuclear equation of state in the hadronic and in the quark plasma phase. We show that small deviations from the standard extensive statistics, due to long-range and memory interactions between particles inside astrophysical plasma, imply remarkable effects into the shape of the equation of state and, as a consequence, in many high-energy astrophysical problems such as the evolution of a newly-born proton-neutron star after a supernova explosion.

Nonextensive statistical effects on the nuclear equation of state and on nuclear astrophysical problems