Published December 19, 2013 | Version v1
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AMS measurements of cosmogenic and supernova-ejected radionuclides in deep-sea sediment cores

  • 1. University of Vienna, Faculty of Physics, VERA Laboratory, Waehringerstrasse 17, 1090 Vienna (Austria)
  • 2. Department of Nuclear Physics Australian National University, Canberra, ACT 0200 (Australia)
  • 3. Physics Department, TU Munich, James-Franck-Strasse, 85748 Garching (Germany)
  • 4. Helmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstrasse 400, 01328 Dresden (Germany)

Description

Samples of two deep-sea sediment cores from the Indian Ocean are analyzed with accelerator mass spectrometry (AMS) to search for traces of recent supernova activity ∼2 Myr ago. Here, long-lived radionuclides, which are synthesized in massive stars and ejected in supernova explosions, namely 26Al, 53Mn and 60Fe, are extracted from the sediment samples. The cosmogenic isotope 10Be, which is mainly produced in the Earth's atmosphere, is analyzed for dating purposes of the marine sediment cores. The first AMS measurement results for 10Be and 26Al are presented, which represent for the first time a detailed study in the time period of 1.7-3.1 Myr with high time resolution. Our first results do not support a significant extraterrestrial signal of 26Al above terrestrial background. However, there is evidence that, like 10Be, 26Al might be a valuable isotope for dating of deep-sea sediment cores for the past few million years. (authors)

Availability note (English)

Available from doi: http://dx.doi.org/10.1051/epjconf/20136303003

Additional details

Identifiers

Publishing Information

Publisher
EDP Sciences
Imprint Place
Les Ulis (France)
Imprint Pagination
(v.63) 5 p.

Conference

Title
Heavy Ion Accelerator Symposium 2013
Dates
8-12 Apr 2013
Place
Canberra (Australia)

Optional Information

Notes
36 refs