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LUNA: Present status and future prospects

Authors :
A. Caciolli
Source :
EPJ Web of Conferences, Vol 117, p 09002 (2016)
Publication Year :
2016
Publisher :
EDP Sciences, 2016.

Abstract

One of the main ingredients of nuclear astrophysics is the knowledge of the thermonuclear reactions responsible for powering the stellar engine and for the synthesis of the chemical elements. At astrophysical energies the cross section of nuclear processes is extremely reduced by the effect of the Coulomb barrier and often extrapolations are needed. The Laboratory for Underground Nuclear Astrophysics (LUNA) is placed under the Gran Sasso mountain. Thanks to the environmental background reduction provided by its position many reactions involved in hydrogen burning has been measured directly at astrophysical energies. Based on this progress, currently there are efforts in several countries to construct new underground accelerators. The exciting science that can be probed with these new facilities will be highlighted.

Details

Language :
English
Database :
OpenAIRE
Journal :
EPJ Web of Conferences, Vol 117, p 09002 (2016)
Accession number :
edsair.doi.dedup.....96f63148a1db9cdbcd7d62294d002acf