Published August 12, 2010 | Version v1
Journal article

High-resolution study of 56Fe→56Mn Gamow-Teller transition by the combined analysis of 56Fe(3He, t)56Co and 56Fe(P, p')56Fe reactions

  • 1. Graduate School of Science and Technology, Niigata University, Nishi-ku, Niigata 950-2181 (Japan)
  • 2. Department of Physics, Osaka University, Toyonaka, Osaka 560-0043 (Japan)
  • 3. Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047 (Japan)
  • 4. iThemba LABS, PO Box 722, Somerset West 7129 (South Africa)
  • 5. Physics Department, Istanbul University, TR-34459 Istanbul (Turkey)

Description

The Gamow-Teller (GT) transitions in the β+(electron capture) direction from the ground state of 56Fe to the excited states of 56Mn play an important role in the core collapse of presupernova. Assuming that isospin analogous transitions in isobars have corresponding strengths, we deduced these GT strengths by combining the results of the 56Fe(p, p')56Fe experiment performed at 200 MeV and 0 deg. and the 56Fe(3He, t)56Co experiment in the ββ direction at 140 MeV/u and 0 deg. The ground state of 56Fe has the isospin value of T = 2, while the GT states in 56Mn have T = 3. In order to identify the analogous T = 2→3, GT transitions in the 56Fe(p, p')56Fe and the 56Fe(3He, t)56Co measurements, we used the fact that the isospin Clebsch-Gordan (CG) coefficients for these T = 2→3 transitions are different in these measurements. Then the GT transition strengths B(GT) in the β+ direction can be deduced from the B(GT) values of the corresponding transitions well determined in the 56Fe(3He, t)56Co measurement assuming the isospin symmetry and correcting the difference of CG coefficients.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1269
Journal Issue
1
Journal Page Range
p. 427-429
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
10. international symposium on origin of matter and evolution of galaxies
Acronym
OMEG-2010
Dates
8-10 Mar 2010
Place
Osaka (Japan)

Optional Information

Notes
(c) 2010 American Institute of Physics