AMS measurements of cosmogenic and supernova-ejected radionuclides in deep-sea sediment cores

J. Feige (Korresp. Autor*in), A. Wallner, L. K. Fifield, G. Korschinek, S. Merchel, G. Rugel, P. Steier, S. R. Winkler, R. Golser

Veröffentlichungen: Beitrag in BuchBeitrag in Konferenzband

Abstract

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.
OriginalspracheEnglisch
TitelHeavy Ion Accelerator Symposium 2013
Redakteure*innenC Simenel, M Evers, T Kibedi, DH Luong, M Reed, M Srncik, A Wallner
Herausgeber (Verlag)E D P Sciences
Seitenumfang5
DOIs
PublikationsstatusVeröffentlicht - 2013
VeranstaltungSymposium on Heavy Ion Accelerator - Canberra, Australien
Dauer: 8 Apr. 201312 Apr. 2013

Publikationsreihe

ReiheEPJ Web of Conferences
Band63
ISSN2100-014X

Konferenz

KonferenzSymposium on Heavy Ion Accelerator
Land/GebietAustralien
OrtCanberra
Zeitraum8/04/1312/04/13

ÖFOS 2012

  • 103005 Atomphysik

Zitationsweisen