Measurement of 21Na(α,p)24Mg stellar reaction using a 21Na RI-beam

D. N. Binh, S. Kubono, H. Yamaguchi, S. Hayakawa, T. Hashimoto, D. Kahl, T. Teranishi, N. Iwasa, S. Kato, L. H. Khiem, N. T. Tho, Y. Wakabayashi

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

Abstract

We performed an experiment of the 21Na(αp)24Mg reaction for the first time by a direct measurement with a thick target method. The studied energy was covered for high temperature conditions in X-ray bursts and core-collapse supernovae. The 21Na(αp)24Mg reaction could make a branch of the extended αp-process and could be important to understand the production of 22Na during the hydrogen explosion at high temperature, like in X-ray bursts, and the 44Ti production from core-collapse supernovae.

Original languageEnglish
Title of host publicationOrigin of Matter and Evolution of Galaxies 2011
Pages25-30
Number of pages6
DOIs
Publication statusPublished - 2012 Dec 1
EventInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan
Duration: 2011 Nov 142011 Nov 17

Publication series

NameAIP Conference Proceedings
Volume1484
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
CountryJapan
CityWako
Period11/11/1411/11/17

Keywords

  • Ne-E problem
  • Stellar reaction of RI beam
  • galactic gamma-ray
  • αp-process

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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