TY - JOUR
T1 - AMS measurements of 41Ca and 55Fe at VERA - two radionuclides of astrophysical interest
AU - Wallner, Anton
AU - Bichler, Max
AU - Dillmann, Iris
AU - Golser, Robin
AU - Käppeler, Franz
AU - Kutschera, Walter
AU - Paul, Michael
AU - Priller, Alfred
AU - Steier, Peter
AU - Vockenhuber, Christof
PY - 2007/6
Y1 - 2007/6
N2 - The potential for measuring the radionuclides 41Ca and 55Fe was investigated with the 3 MV tandem accelerator at VERA. Interestingly, up to now, no applications have been published for 55Fe using the technique of AMS. This is in strong contrast to 41Ca, which is routinely measured by medium and large tandem accelerators in various applications. Using CaF2 samples the quantification of 41Ca down to levels of a few 10-13 for the isotope ratio 41Ca/Ca has become possible with the use of the ΔTOF technique. Both nuclides, 41Ca and 55Fe were found to be of interest in nuclear astrophysics. A first application of 41Ca detection at VERA is the measurement of the 40Ca(n, γ)41Ca cross section at stellar temperatures. Similarly, of astrophysical interest is the production of 55Fe via neutron capture on 54Fe. To this end, different Ca and Fe blank and standard samples were investigated with the goal to establish an AMS method for 41Ca and 55Fe measurements. Indeed, low background levels for both radionuclides, 41Ca and 55Fe, were observed in these studies. The full separation power of VERA results in a very low detection limit, while still providing a high overall transmission.
AB - The potential for measuring the radionuclides 41Ca and 55Fe was investigated with the 3 MV tandem accelerator at VERA. Interestingly, up to now, no applications have been published for 55Fe using the technique of AMS. This is in strong contrast to 41Ca, which is routinely measured by medium and large tandem accelerators in various applications. Using CaF2 samples the quantification of 41Ca down to levels of a few 10-13 for the isotope ratio 41Ca/Ca has become possible with the use of the ΔTOF technique. Both nuclides, 41Ca and 55Fe were found to be of interest in nuclear astrophysics. A first application of 41Ca detection at VERA is the measurement of the 40Ca(n, γ)41Ca cross section at stellar temperatures. Similarly, of astrophysical interest is the production of 55Fe via neutron capture on 54Fe. To this end, different Ca and Fe blank and standard samples were investigated with the goal to establish an AMS method for 41Ca and 55Fe measurements. Indeed, low background levels for both radionuclides, 41Ca and 55Fe, were observed in these studies. The full separation power of VERA results in a very low detection limit, while still providing a high overall transmission.
KW - AMS
KW - Ca
KW - Fe
KW - Nuclear astrophysics
KW - ΔTOF
UR - http://www.scopus.com/inward/record.url?scp=34248156846&partnerID=8YFLogxK
U2 - 10.1016/j.nimb.2007.01.207
DO - 10.1016/j.nimb.2007.01.207
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AN - SCOPUS:34248156846
SN - 0168-583X
VL - 259
SP - 677
EP - 682
JO - Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms
JF - Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms
IS - 1
ER -