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Supernova neutrinos and nucleosynthesis

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 21 Feb 2014Embargo end date: 01 Jan 2013Publisher:IOP PublishingJournal:Journal of Physics G: Nuclear and Particle Physics, volume 41, page 44,008 (issn: 0954-3899, eissn: 1361-6471,

Authors: Gabriel Martínez-Pinedo; Tobias Fischer; L. Huther;

doi: 10.1088/0954-3899/41/4/044008 , 10.48550/arxiv.1309.5477

arXiv: http://arxiv.org/abs/1309.5477

Supernova neutrinos and nucleosynthesis

- Summary
- Subjects
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Abstract

Observations of metal-poor stars indicate that at least two different nucleosynthesis sites contribute to the production of r-process elements. One site is responsible for the production of light r-process elements Z

18 pages, 5 figures, submitted to J. Phys. G: Nucl. Part. Phys. (Focus issue "Nucleosynthesis and the role of neutrinos", ed. Baha Balantekin and Cristina Volpe)

Related Organizations

University of Wrocław
Poland
TU Darmstadt
Germany

Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), Nuclear Theory (nucl-th), Nuclear Theory, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	62
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 10%