Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-27T13:08:37.264Z Has data issue: false hasContentIssue false

Astronomy with Radioactivities

Published online by Cambridge University Press:  02 January 2013

Roland Diehl*
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, D-85741 Garching, Germany
Maria Lugaro
Affiliation:
Monash Centre for Astrophysics, School of Mathematical Sciences, Monash University, Melbourne, Vic. 3800, Australia
*
CCorresponding author. Email: [email protected]
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Cosmic radioactivity represents a cross-disciplinary theme and an interesting alternate viewpoint on cosmic nuclear astrophysics. Radioactive isotopes and their decay provide unique messages from sites of cosmic nucleosynthesis, as the decay is mediated by weak interaction physics and independent of environmental conditions. The radioactive clock of various isotopes traces stellar mixing processes and the process of solidification of bodies when the solar system was formed. Isotopic abundances directly reflect the conditions of their formation in the nucleosynthesis site, which is unobservable otherwise. Measurements range from meteorites and their included stardust grain compositions through to cosmic rays and electromagnetic radiation from infrared to gamma ray wavelengths. Thus, various astronomical disciplines with their different messengers of cosmic nucleosynthesis as seen through unstable, decaying isotopes are linked to the physics of nuclear reactions, and to theories and models of the variety of cosmic nucleosynthesis sites and of cosmic isotopic evolution.

Type
Research Front: Astronomy with Radioactivities
Copyright
Copyright © Astronomical Society of Australia 2012

References

Feige, J., Wallner, A., Winkler, S. R., Merchel, S., Fifield, L. K., Korschinek, G., Rugel, G. & Breitschwerdt, D., 2012, PASA, 29, 109CrossRefGoogle Scholar
Ott, U., Besmehn, A., Farouqi, K., Hallmann, O., Hoppe, P., Kratz, K.-L., Melber, K. & Wallner, A., 2012, PASA, 29, 90CrossRefGoogle Scholar
Tetzlaff, N., Schmidt, J. G., Hohle, M. M. & Neuhäuser, R., 2012, PASA, 29, 98CrossRefGoogle Scholar
Wallner, A., et al. , 2012, PASA, 29, 115CrossRefGoogle Scholar