Martin, Dirk ; Perego, Albino ; Arcones, Almudena ; Thielemann, Friedrich-Karl ; Korobkin, Oleg ; Rosswog, Stephan (2018)
Synthesis of Heavy Elements in the Ejecta of Neutron Star Mergers.
In: Journal of Physics: Conference Series, 940 (1)
doi: 10.1088/1742-6596/940/1/012047
Article, Bibliographie
This is the latest version of this item.
Abstract
We present a nucleosynthesis study on the neutrino-driven wind after neutron star merger. Post-processing tracers from a hydrodynamical simulation, we determine nucleosynthesis yields that depend on both life time of the massive neutron star and polar angle. In comparison with the dynamic ejecta we find a complementary nucleosynthesis, which can explain the r-process pattern beyond the first r-process peak. Additionally, we predict possible forms of light curves for the detection of a kilonova.
Item Type: | Article |
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Erschienen: | 2018 |
Creators: | Martin, Dirk ; Perego, Albino ; Arcones, Almudena ; Thielemann, Friedrich-Karl ; Korobkin, Oleg ; Rosswog, Stephan |
Type of entry: | Bibliographie |
Title: | Synthesis of Heavy Elements in the Ejecta of Neutron Star Mergers |
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: | 10.1088/1742-6596/940/1/012047 |
Corresponding Links: | |
Abstract: | We present a nucleosynthesis study on the neutrino-driven wind after neutron star merger. Post-processing tracers from a hydrodynamical simulation, we determine nucleosynthesis yields that depend on both life time of the massive neutron star and polar angle. In comparison with the dynamic ejecta we find a complementary nucleosynthesis, which can explain the r-process pattern beyond the first r-process peak. Additionally, we predict possible forms of light curves for the detection of a kilonova. |
Identification Number: | Artikel-ID: 012047 |
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: | 17 May 2024 11:01 |
Last Modified: | 17 May 2024 11:01 |
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Synthesis of Heavy Elements in the Ejecta of Neutron Star Mergers. (deposited 14 May 2024 09:43)
- Synthesis of Heavy Elements in the Ejecta of Neutron Star Mergers. (deposited 17 May 2024 11:01) [Currently Displayed]
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