TU Darmstadt / ULB / TUprints

Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds

Bliss, Julia ; Arcones, Almudena (2024)
Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds.
In: Journal of Physics: Conference Series, 2018, 940 (1)
doi: 10.26083/tuprints-00020917
Article, Secondary publication, Publisher's Version

[img] Text
Copyright Information: CC BY 3.0 Unported - Creative Commons, Attribution.

Download (651kB)
Item Type: Article
Type of entry: Secondary publication
Title: Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds
Language: English
Date: 14 May 2024
Place of Publication: Darmstadt
Year of primary publication: 2018
Place of primary 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: 10.26083/tuprints-00020917
Corresponding Links:
Origin: Secondary publication DeepGreen

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
Status: Publisher's Version
URN: urn:nbn:de:tuda-tuprints-209177
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 > Institute of Nuclear Physics
Date Deposited: 14 May 2024 09:38
Last Modified: 14 May 2024 09:39
SWORD Depositor: Deep Green
URI: https://tuprints.ulb.tu-darmstadt.de/id/eprint/20917
Actions (login required)
View Item View Item