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Exploring the astrophysical conditions for the creation of the first r-process peak, and the impact of nuclear physics uncertainties

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Hellenic Nuclear Physics Society   

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Exploring the astrophysical conditions for the creation of the first r-process peak, and the impact of nuclear physics uncertainties (EN)
Sieverding, A.
Wu, M. R.
Reiter, M. P.
Martínez-Pinedo, G.
Nikas, Stylianos
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Theoretical (EN)
2020-04-17
We present a study of nucleosynthesis for conditions of high Ye outflows from NeutronStar Mergers (NSMs). We investigate the effect of new beta-decay rates measurements and uncertaintiesin nuclear masses of the newly measured 84,85 Ga to the r-process nucleosynthesis calculations. The impactof these quantities to the production of the elements of the r-process abundance pattern for A < 100 isquantified and presented. (EN)
nuclear astrophysics (EN)
nucleosynthesis (EN)
r-process (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. 27 (2019): HNPS2019; 175-179 (EL)
HNPS Advances in Nuclear Physics; Vol. 27 (2019): HNPS2019; 175-179 (EN)
Πνευματική ιδιοκτησία (c) 2020 Stylianos Nikas (EL)
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



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