Arcones, Almudena ; Martínez-Pinedo, Gabriel (2024)
Nucleosynthesis in neutrino-driven winds: Influence of the nuclear physics input.
In: Journal of Physics: Conference Series, 2010, 202 (1)
doi: 10.26083/tuprints-00020650
Article, Secondary publication, Publisher's Version
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Item Type: | Article |
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Type of entry: | Secondary publication |
Title: | Nucleosynthesis in neutrino-driven winds: Influence of the nuclear physics input |
Language: | English |
Date: | 12 February 2024 |
Place of Publication: | Darmstadt |
Year of primary publication: | 1 January 2010 |
Place of primary publication: | Bristol |
Publisher: | IOP Publishing |
Journal or Publication Title: | Journal of Physics: Conference Series |
Volume of the journal: | 202 |
Issue Number: | 1 |
Collation: | 4 Seiten |
DOI: | 10.26083/tuprints-00020650 |
Corresponding Links: | |
Origin: | Secondary publication DeepGreen |
Abstract: | We have performed hydrodynamical simulations of the long-time evolution of proto-neutron stars to study the nucleosynthesis using the resulting wind trajectories. Although the conditions found in the present wind models are not favourable for the production of heavy elements, a small enhancement of the entropy results in the production of r-process elements with A ≈ 195. This allows us to explore the sensitivity of their production to the hydrodynamical evolution (wind termination shock) and nuclear physics input used. |
Identification Number: | Artikel-ID: 012007 |
Status: | Publisher's Version |
URN: | urn:nbn:de:tuda-tuprints-206504 |
Additional Information: | Nuclear Physics in Astrophysics IV 8–12 June 2009, Laboratori Nazionali di Frascati, Frascati, Italy |
Classification DDC: | 500 Science and mathematics > 530 Physics |
Divisions: | 05 Department of Physics > Institute of Nuclear Physics |
Date Deposited: | 12 Feb 2024 15:02 |
Last Modified: | 11 Apr 2024 07:42 |
SWORD Depositor: | Deep Green |
URI: | https://tuprints.ulb.tu-darmstadt.de/id/eprint/20650 |
PPN: | 517021676 |
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