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Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds

Bliss, Julia ; Arcones, Almudena (2018)
Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds.
In: Journal of Physics: Conference Series, 940 (1)
doi: 10.1088/1742-6596/940/1/012030
Article, Bibliographie

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Abstract

The solar system origin of the p-isotopes ⁹²,⁹⁴Mo and ⁹⁶,⁹⁸Ru is a long-lasting mystery. Several astrophysical scenarios failed to explain their formation. Moreover, SiC X grains show a different abundance ratio of ⁹⁵,⁹⁷Mo than in the solar system. We have investigated if neutrino-driven winds can offer a solution to those problems.

Item Type: Article
Erschienen: 2018
Creators: Bliss, Julia ; Arcones, Almudena
Type of entry: Bibliographie
Title: Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds
Language: English
Date: 2018
Place of Publication: Bristol
Publisher: IOP Publishing
Journal or Publication Title: Journal of Physics: Conference Series
Volume of the journal: 940
Issue Number: 1
Collation: 3 Seiten
DOI: 10.1088/1742-6596/940/1/012030
Corresponding Links:
Abstract:

The solar system origin of the p-isotopes ⁹²,⁹⁴Mo and ⁹⁶,⁹⁸Ru is a long-lasting mystery. Several astrophysical scenarios failed to explain their formation. Moreover, SiC X grains show a different abundance ratio of ⁹⁵,⁹⁷Mo than in the solar system. We have investigated if neutrino-driven winds can offer a solution to those problems.

Identification Number: Artikel-ID: 012030
Additional Information:

Nuclear Physics in Astrophysics Conference (NPA VII) 18–22 May 2015, York, UK

Classification DDC: 500 Science and mathematics > 530 Physics
Divisions: 05 Department of Physics
05 Department of Physics > Institute of Nuclear Physics
Date Deposited: 16 May 2024 15:34
Last Modified: 16 May 2024 15:34
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