TY - JOUR
T1 - AMS - A powerful tool for probing nucleosynthesis via long-lived radionuclides
AU - Wallner, Anton
AU - Golser, Robin
AU - Kutschera, Walter
AU - Priller, Alfred
AU - Steier, Peter
AU - Vockenhuber, Christof
N1 - 19.06.2008: Datenanforderung 2324 (kein Statusverlauf, kein Scopus)
PY - 2006
Y1 - 2006
N2 - Well-established data on production-rates of long-lived radionuclides are important for the understanding and calculation of varions nucleosynthesis processes. However, lack of information exists for a list of nuclides as pointed out by nuclear-data requests. In addition, the search for supernova (SN)-produced radionuclides will give an improved insight into explosive scenarios. Accelerator mass spectrometry (AMS) represents a technique, which is capable to quantify such long-lived radionuclides using mass spectrometric methods. The potential of AMS is presented here as a powerful tool for probing nucleosynthesis. Applications of AMS are exemplified for a few specific cases: the detection of extraterrestrial radioactivity on Earth in terrestrial archives as a signature of nearby SN explosions, and the measurement of cross-sections, as an important ingredient for stellar as well as nuclear model calculations.
AB - Well-established data on production-rates of long-lived radionuclides are important for the understanding and calculation of varions nucleosynthesis processes. However, lack of information exists for a list of nuclides as pointed out by nuclear-data requests. In addition, the search for supernova (SN)-produced radionuclides will give an improved insight into explosive scenarios. Accelerator mass spectrometry (AMS) represents a technique, which is capable to quantify such long-lived radionuclides using mass spectrometric methods. The potential of AMS is presented here as a powerful tool for probing nucleosynthesis. Applications of AMS are exemplified for a few specific cases: the detection of extraterrestrial radioactivity on Earth in terrestrial archives as a signature of nearby SN explosions, and the measurement of cross-sections, as an important ingredient for stellar as well as nuclear model calculations.
U2 - 10.1140/epja/i2006-08-052-3
DO - 10.1140/epja/i2006-08-052-3
M3 - Meeting abstract/Conference paper
VL - 27
SP - 337
EP - 342
JO - European Physical Journal A
JF - European Physical Journal A
SN - 1434-6001
IS - 1 Suppl.
ER -