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Nucleosynthesis in neutrino-driven winds: Influence of the nuclear physics input

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
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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