Skip to main content
Conference ProceedingsOPEN ACCESS

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

Journal of Physics: Conference Series (2016) 665(1)
DOI: 10.1088/1742-6596/665/1/012031
3Citations
Citations of this article
20Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

The reactions 13C(α, n)16O and 22Ne(α, 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 4π neutron counter, based on 3He tubes and a neutron moderator, placed in an underground lab.

Cite

CITATION STYLE

APA

Tain, J. L., Jordán, D., Agramunt, J., Algora, A., Bandac, I., Bettini, A., … Parikh, A. (2016). Measurement of very low (α,n) cross sections of astrophysical interest. In Journal of Physics: Conference Series (Vol. 665). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/665/1/012031

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free