Direct Measurement of 12C+4He --> 16O + γ Reaction at Stellar Energy

Details Direct Measurement of 12C+4He --> 16O + γ Reaction at Stellar Energy Direct Measurement of 12C+4He --> 16O + γ Reaction at Stellar Energy

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..865..225s&link_type=abstract

NUCLEAR PHYSICS TRENDS: 6th China-Japan Joint Nuclear Physics Symposium. AIP Conference Proceedings, Volume 865, pp. 225-230 (2

Physics

Nuclear Physics

1

Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments

Scientific paper

Preparation for direct measurement of 12C+4He-->16O+γ reaction at stellar energy has been made in Kyushu University tandem laboratory (KUTL) since 1914. We plan to measure the reaction at Ecm = 2.4-0.7 MeV where the cross section is estimated to be 60 nbarn-1pbarn. Many instrumental developments have been made for a 12C beam, a windowless helium gas target, 16O detection, background reduction. We started the measurement in 2006.

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