Measurement of 25Mg(p, γ)26Alg resonance strengths via accelerator mass spectrometry

被引:32
作者
Arazi, A.
Faestermann, T.
Niello, J. O. Fernandez
Knie, K.
Korschinek, G.
Poutivtsev, M.
Richter, E.
Rugel, G.
Wallner, A.
机构
[1] Comis Nacl Energia Atom, Lab TANDAR, RA-1429 Buenos Aires, DF, Argentina
[2] Tech Univ Munich, D-85748 Garching, Germany
[3] Rossendorf Inc, Forschungszentrum Rossendorf EV, D-01314 Dresden, Germany
[4] Univ Vienna, Inst Isotopenforsch & Kernphys, Vienna Environm Res Accelerator, A-1090 Vienna, Austria
来源
PHYSICAL REVIEW C | 2006年 / 74卷 / 02期
关键词
D O I
10.1103/PhysRevC.74.025802
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 strengths of resonances located at center-of-mass energies of E-c.m.=189, 304, 374, and 418 keV for the Mg-25(p,gamma) reaction have been measured for the first time with an off-line method: Mg targets were firstly activated with protons at the resonance energies and the produced Al-26(g) nuclei were counted by means of highly sensitive accelerator mass spectrometry (AMS). Thus, the production of Al-26 in its ground state is determined independently from the gamma-decay branching ratio. While the 304, 374, and 418 keV resonances show fair agreement with previous measurements, the 189 keV resonance yield a significantly less strength. In addition, an experimental upper limit for the E-c.m.=92 keV resonance was determined.
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页数:6
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共 24 条
  • [11] High-sensitivity AMS for heavy nuclides at the Munich Tandem accelerator
    Knie, K
    Faestermann, T
    Korschinek, G
    Rugel, G
    Rühm, W
    Wallner, C
    [J]. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS, 2000, 172 : 717 - 720
  • [12] Knödlseder J, 1999, ASTRON ASTROPHYS, V344, P68
  • [13] AL-26 IN EARLY SOLAR-SYSTEM - FOSSIL OR FUEL
    LEE, T
    PAPANASTASSIOU, DA
    WASSERBURG, GJ
    [J]. ASTROPHYSICAL JOURNAL, 1977, 211 (02) : L107 - L110
  • [14] DIFFUSE GALACTIC GAMMA-RAY LINE EMISSION FROM NUCLEOSYNTHETIC FE-60, AL-26, AND NA-22 - PRELIMINARY LIMITS FROM HEAO-3
    MAHONEY, WA
    LING, JC
    JACOBSON, AS
    LINGENFELTER, RE
    [J]. ASTROPHYSICAL JOURNAL, 1982, 262 (02) : 742 - 748
  • [15] Niello JOF, 2003, BRAZ J PHYS, V33, P218, DOI 10.1590/S0103-97332003000200009
  • [16] Low-energy resonance strengths for proton capture on Mg and Al nuclei
    Powell, DC
    Iliadis, C
    Champagne, AE
    Hale, SE
    Hansper, VY
    Surman, RA
    Veal, KD
    [J]. NUCLEAR PHYSICS A, 1998, 644 (04) : 263 - 276
  • [17] Prantzos N, 1996, PHYS REP, V267, P2
  • [18] CURRENT STATUS OF NUCLEAR ASTROPHYSICS
    ROLFS, C
    TRAUTVETTER, HP
    RODNEY, WS
    [J]. REPORTS ON PROGRESS IN PHYSICS, 1987, 50 (03) : 233 - 325
  • [19] SPECTROSCOPIC FACTORS FOR PROTON UNBOUND LEVELS IN AL-26 AND THEIR INFLUENCE ON STELLAR REACTION-RATES
    ROLLEFSON, AA
    WIJEKUMAR, V
    BROWNE, CP
    WIESCHER, M
    HAUSMAN, HJ
    KIM, WY
    SCHMALBROCK, P
    [J]. NUCLEAR PHYSICS A, 1990, 507 (02) : 413 - 425
  • [20] Error analysis for resonant thermonuclear reaction rates
    Thompson, WJ
    Iliadis, C
    [J]. NUCLEAR PHYSICS A, 1999, 647 (3-4) : 259 - 279