Shell model studies for nuclear astrophysics

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Item Type:	Article
Type of entry:	Secondary publication
Title:	Shell model studies for nuclear astrophysics
Language:	English
Date:	21 November 2023
Place of Publication:	Darmstadt
Year of primary publication:	2015
Place of primary publication:	Bristol
Publisher:	IOP Publishing
Journal or Publication Title:	Journal of Physics: Conference Series
Volume of the journal:	580
Issue Number:	1
Collation:	6 Seiten
DOI:	10.26083/tuprints-00020843
Corresponding Links:	Publisher-DOI
Origin:	Secondary publication DeepGreen
Abstract:	Shell model studies have contributed in recent years significantly to improve nuclear input required in simulations of the dynamics of astrophysical objects and their associated nucleosynthesis. This manuscript highlights a few examples like electron capture rates of importance for the evolution of core-collapse supernovae and the nucleosynthesis in thermonuclear supernovae, neutrino-nucleus cross sections with relevance to the supernova neutrino spectra and finally half lives of neutron-rich nuclei with magic neutron numbers which serve as waiting points in the mass flow of the astrophysical r-process.
Status:	Publisher's Version
URN:	urn:nbn:de:tuda-tuprints-208430
Additional Information:	Ischia14
Classification DDC:	500 Science and mathematics > 530 Physics
Divisions:	05 Department of Physics > Institute of Nuclear Physics
Date Deposited:	21 Nov 2023 10:17
Last Modified:	08 Jan 2024 08:41
SWORD Depositor:	Deep Green
URI:	https://tuprints.ulb.tu-darmstadt.de/id/eprint/20843
PPN:	514484578
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