Direct measurement of 12C+4He → 16O + γ reaction at stellar energy

K. Sagara, H. Oba, K. Nishida, M. Kouzuma, S. Kamibeppu, T. Maeda, S. Tanimoto, T. Kawada, T. Teranishi, K. Tamura, N. Ikeda

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

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.

Original languageEnglish
Title of host publicationNUCLEAR PHYSICS TRENDS
Subtitle of host publication6th China-Japan Joint Nuclear Physics Symposium
Pages225-230
Number of pages6
DOIs
Publication statusPublished - 2006
EventNUCLEAR PHYSICS TRENDS: 6th China-Japan Joint Nuclear Physics Symposium - Shanghai, China
Duration: May 16 2006May 20 2006

Publication series

NameAIP Conference Proceedings
Volume865
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherNUCLEAR PHYSICS TRENDS: 6th China-Japan Joint Nuclear Physics Symposium
Country/TerritoryChina
CityShanghai
Period5/16/065/20/06

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Fingerprint

Dive into the research topics of 'Direct measurement of <sup>12</sup>C+<sup>4</sup>He → <sup>16</sup>O + γ reaction at stellar energy'. Together they form a unique fingerprint.

Cite this