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Gamow-Teller strength for the analog transitions to the first T=1/2,Jπ=3/2- states in C13 and N13 and the implications for type Ia supernovae

  • R. G.T. Zegers
  • , E. F. Brown
  • , H. Akimune
  • , Sam M. Austin
  • , A. M. Van Den Berg
  • , B. A. Brown
  • , D. A. Chamulak
  • , Y. Fujita
  • , M. Fujiwara
  • , S. Galès
  • , M. N. Harakeh
  • , H. Hashimoto
  • , R. Hayami
  • , G. W. Hitt
  • , M. Itoh
  • , T. Kawabata
  • , K. Kawase
  • , M. Kinoshita
  • , K. Nakanishi
  • , S. Nakayama
  • S. Okumura, Y. Shimbara, M. Uchida, H. Ueno, T. Yamagata, M. Yosoi

Research output: Contribution to journalArticlepeer-review

24 Scopus citations

Abstract

The Gamow-Teller strength for the transition from the ground state of C13 to the T=1/2,Jπ=3/2- excited state at 3.51 MeV in N13 is extracted via the C13(He3,t) reaction at 420 MeV. In contrast to results from earlier (p,n) studies on C13, a good agreement with shell-model calculations and the empirical unit cross-section systematics from other nuclei is found. The results are used to study the analog N13(e-,νe)C13 reaction, which plays a role in the pre-explosion convective phase of type Ia supernovae. Although the differences between the results from the (He3,t) and (p,n) data significantly affect the deduced electron-capture rate and the net heat deposition in the star resulting from this transition, the overall effect on the pre-explosive evolution is small.

Original languageEnglish
Article number024307
JournalPhysical Review C - Nuclear Physics
Volume77
Issue number2
DOIs
StatePublished - 21 Feb 2008
Externally publishedYes

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