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 analyze the data of Kamiokande-II, IMB, Baksan using a parameterizeddescription of the antineutrino emission, that includes an initial phase ofintense luminosity. The luminosity curve, the average energy of $\bar\nu_e$ andthe astrophysical parameters of the model, derived by fitting the observedevents (energies, times and angles) are in reasonable agreement with thegeneric expectations of the delayed scenario for the explosion.

How much can we learn from SN1987A events? Or: An analysis with a two-Component model for the antineutrino signal