Measurement of very low (alpha,n) cross sections of astrophysical interest

The reactions 13C( ; n)16O and 22Ne( ; n)25Mg are the primary sources of neutrons for the astrophysical s-process. The feasibility of cross section measurements within the respective Gamow windows is discussed in quantitative terms for a 4 neutron counter, based on 3He tubes and a neutron moderator, placed in an underground lab.

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Article

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English

Subjects and keywords

Àrees temàtiques de la UPC::Física; Àrees temàtiques de la UPC::Física::Astronomia i astrofísica; Àrees temàtiques de la UPC::Energies::Energia nuclear; Astrophysics; Neutrons; Astrofísica; Neutrons

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Institute of Physics (IOP)

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http://iopscience.iop.org/article/10.1088/1742-6596/665/1/012031/meta

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DIDL MARC MARC_CCUC METS OAI_DC ORE QDC RDF

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http://creativecommons.org/licenses/by-nc-nd/3.0/es/

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E-prints [73060]

Measurement of very low (alpha,n) cross sections of astrophysical interest

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