Vernardos, G.Goriely, S.Lalazissis, G.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.application/pdf10.12681/hnps.2582https://eproceedings.epublishing.ekt.gr/index.php/hnps/article/view/2582engHellenic Nuclear Physics Society (HNPS)Πνευματική ιδιοκτησία (c) 2019 G. Vernardos, S. Goriely, G. LalazissisAnnual Symposium of the Hellenic Nuclear Physics Society2654-00882654-007XAnnual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 16 (2008): HNPS2008; 67-74HNPS Advances in Nuclear Physics; Vol. 16 (2008): HNPS2008; 67-74Nucleosynthesis by accelerated particles in a bipolar Supernova explosioninfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion2020-01-01Πυρηνική φυσικήNuclear Physicsisi - Physics, Nuclear includes resources on the study of nuclear structure, decay, radioactivity, reactions, and scattering. Resources in this category focus on low-energy physics. High-energy physics is covered in the PHYSICS, PARTICLES & FIELDS category.Άρθρο συνεδρίουConference articleΕπιστημονικό άρθροScientific articleHellenic Nuclear Physics SocietyGreek Aggregator OpenArchives.gr | National Documentation Centre (EKT)other