Phys. Rev. C
77,
024307
(2008)
[10 pages]
Gamow-Teller strength for the analog transitions to the first T=1/2,Jπ=3/2- states in 13C and 13N and the implications for type Ia supernovae
R. G. Zegers et al.
Show All Authors/Affiliations
Hide All Authors/Affiliations
R. G. T. Zegers1,2,3,*, E. F. Brown1,2,3, H. Akimune4, Sam M. Austin1,3, A. M. van den Berg5, B. A. Brown1,2,3, D. A. Chamulak2,3, Y. Fujita6, M. Fujiwara7,8, S. Galès9, M. N. Harakeh5, H. Hashimoto8, R. Hayami10, G. W. Hitt1,2,3, M. Itoh11, T. Kawabata12, K. Kawase8, M. Kinoshita4, K. Nakanishi8, S. Nakayama10, S. Okumura8, Y. Shimbara1,3, M. Uchida13, H. Ueno14, T. Yamagata4, and M. Yosoi8
1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321, USA 2Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA 3Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA 4Department of Physics, Konan University, Kobe, Hyogo, 658-8501, Japan 5Kernfysisch Versneller Instituut, University of Groningen, Zernikelaan 25, 9747 AA Groningen, The Netherlands 6Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan 7Kansai Photon Science Institute, Japan Atomic Energy Agency, Kizu, Kyoto 619-0215, Japan 8Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047, Japan 9Institut de Physique Nucléaire, IN2P3-CNRS, Orsay, France 10Department of Physics, University of Tokushima, Tokushima 770-8502, Japan 11Cyclotron and Radioisotope Center, Tohoku University, Sendai, Miyagi 980-8578, Japan 12Center for Nuclear Study, University of Tokyo, RIKEN Campus, Wako, Saitama 351-0198, Japan 13Tokyo Institute of Technology, 2-12-1 O-Okayama, Tokyo 152-8550, Japan 14Applied Nuclear Physics Laboratory, RIKEN, Wako, Saitama 351-0198, Japan
Received 12 October 2007; published 21 February 2008
The Gamow-Teller strength for the transition from the ground state of 13C to the T=1/2,Jπ=3/2- excited state at 3.51 MeV in 13N is extracted via the 13C(3He,t) reaction at 420 MeV. In contrast to results from earlier (p,n) studies on 13C, 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 13N(e-,νe)13C reaction, which plays a role in the pre-explosion convective phase of type Ia supernovae. Although the differences between the results from the (3He,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.
© 2008 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevC.77.024307
DOI:
10.1103/PhysRevC.77.024307
PACS:
21.60.Cs, 24.50.+g, 25.40.Kv, 25.55.-e
|
|