1. Home page
  2. Search

Nucleosynthesis by accelerated particles in a bipolar Supernova explosion

This item is provided by the institution :
Hellenic Nuclear Physics Society   

Repository :
Annual Symposium of the Hellenic Nuclear Physics Society  | ΕΚΤ eProceedings   

see the original item page
in the repository's web site and access all digital files if the item*



Nucleosynthesis by accelerated particles in a bipolar Supernova explosion (EN)
Vernardos, G.
Goriely, S.
Lalazissis, G.
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
2020-01-01
The most spectacular final phase of an evolved star, is the supernova explosion. It has been suggested by observations that such an event might not be spherically symmetric. This asphericity could be explained by the formation of jets of accel- erated particles by the explosion, which could interact with the stellar matter and give rise to a possible nucleosynthesis. Such a nucleosynthesis is studied. The fi- nal abundance pattern is shown to depend on the values of the model parameters adopted, especially the energy spectrum of the accelerated particles. (EN)
Annual Symposium of the Hellenic Nuclear Physics Society
English
Hellenic Nuclear Physics Society (HNPS) (EN)
2654-0088
2654-007X
Annual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 16 (2008): HNPS2008; 67-74 (EL)
HNPS Advances in Nuclear Physics; Vol. 16 (2008): HNPS2008; 67-74 (EN)
Πνευματική ιδιοκτησία (c) 2019 G. Vernardos, S. Goriely, G. Lalazissis (EL)
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



*Institutions are responsible for keeping their URLs functional (digital file, item page in repository site)