Photo-induced depopulation of the 180Tam isomer via low-lying intermediate states:: Structure and astrophysical implications -: art. no. 035801

被引:102
作者
Belic, D
Arlandini, C
Besserer, J
de Boer, J
Carroll, JJ
Enders, J
Hartmann, T
Käppeler, F
Kaiser, H
Kneissl, U
Kolbe, E
Lnaganke, K
Loewe, M
Maier, HJ
Maser, H
Mohr, P
von Neumann-Cosel, P
Nord, A
Pitz, HH
Richer, A
Schumann, M
Thielemann, FK
Volz, S
Zilges, A
机构
[1] Univ Stuttgart, Inst Strahlenphys, D-70569 Stuttgart, Germany
[2] Forschungszentrum Karlsruhe, Inst Kernphys, D-76021 Karlsruhe, Germany
[3] Univ Munich, Sekt Phys, D-85748 Garching, Germany
[4] Youngstown State Univ, Dept Phys & Astron, Youngstown, OH 44555 USA
[5] Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany
[6] Univ Basel, Inst Phys, CH-4056 Basel, Switzerland
[7] Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus, Denmark
关键词
D O I
10.1103/PhysRevC.65.035801
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The photo-induced depopulation of the quasistable isomer (t(1/2) greater than or equal to1.2 x10(15) yr) in Ta-180 with angular momentum and parity J(pi) = 9(-) at an excitation energy E-x = 75 keV was studied at the new bremsstrahlung irradiation facility installed at the Stuttgart 4.3 MV DYNAMITRON accelerator in the energy range of bremsstrahlung end point energies between E-0 = 0.8-3.1 MeV. The onset of the isomer depopulation could be observed starting at an end point energy of E-0 approximate to1 MeV, i. e., at an intermediate state of Ta-180 at or below that energy. Higher-lying intermediate states were found at 1.22, 1.43, 1.55, 1.85, 2.16, 2.40, 2.64, and 2.80 MeV. The extracted integrated cross sections show a remarkably strong depopulation of the Ta-180(m) isomer by photoexcitation. The results are compared with previous experiments and recent quasiparticle-phonon model calculations. Implications of the results for a possible nucleosynthesis of Ta-180 in the s process and the neutrino process are discussed.
引用
收藏
页码:358011 / 3580113
页数:13
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