The impact of n_TOF data on s-process modelling
- We show examples of the impact of the Maxwellian averaged capture cross sections determined at n_TOF over the past 20 years on AGB stellar nucleosynthesis models. In particular, we developed an automated procedure to derive MACSs from evaluated data libraries, which are subsequently used as input to stellar models computed by means of the FuNS code. In this contribution, we present a number of s-process abundances obtained using different data libraries as input to stellar models, with a focus on the role of n_TOF data.
Author: | Samuele Lanzi, Sergio CristalloORCiD, Francesco GiacominiORCiD, Cristian MassimiORCiD, Alberto MengoniORCiD, Diego VescoviORCiD |
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URN: | urn:nbn:de:hebis:30:3-659392 |
DOI: | https://doi.org/10.1051/epjconf/202327906003 |
ISSN: | 2100-014X |
Parent Title (German): | EPJ Web of Conferences |
Publisher: | EDP Sciences |
Place of publication: | Les Ulis |
Document Type: | Conference Proceeding |
Language: | English |
Date of Publication (online): | 2023/03/22 |
Date of first Publication: | 2023/03/22 |
Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
Contributing Corporation: | Nuclear Physics in Astrophysics (Veranstaltung (10. : 2022 : Genf; Online) |
Release Date: | 2024/02/28 |
Volume: | 279 |
Issue: | 06003 |
Article Number: | 06003 |
Page Number: | 5 |
HeBIS-PPN: | 516206222 |
Institutes: | Physik |
Dewey Decimal Classification: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
Sammlungen: | Universitätspublikationen |
Licence (German): | Creative Commons - Namensnennung 4.0 |