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

It has been suggested that whether a star explodes or not, and what kind ofexplosion properties it shows, is strongly dependent on the progenitor's corestructure. We present the results from 101 axisymmetric core-collapse supernovasimulations performed with progenitors spanning initial masses in the rangefrom 10.8 to 75 solar masses, and focus on their connections to the compactnessof the progenitor's core. Our simulations confirm a correlation between theneutrinos emitted during the accretion phase and the progenitor's compactness.We suggest that the ratio of observed neutrino events during the first hundredsof milliseconds can be used to infer the progenitor's inner mass densitystructure.

Diagnosing the Structure of Massive Stars with Galactic Supernova Neutrinos