Synthesis of Heavy Elements in the Ejecta of Neutron Star Mergers

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Item Type:	Article
Type of entry:	Secondary publication
Title:	Synthesis of Heavy Elements in the Ejecta of Neutron Star Mergers
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-00020920
Corresponding Links:	Publisher-DOI
Origin:	Secondary publication DeepGreen
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
Status:	Publisher's Version
URN:	urn:nbn:de:tuda-tuprints-209201
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 09:43
Last Modified:	14 May 2024 09:43
SWORD Depositor:	Deep Green
URI:	https://tuprints.ulb.tu-darmstadt.de/id/eprint/20920
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