Distributed Radioactivities

  • Roland DiehlEmail author
  • Dieter H. Hartmann
  • Nikos Prantzos
Part of the Astrophysics and Space Science Library book series (ASSL, volume 453)


Radioactive nuclei freshly produced in compact sources of cosmic nucleosynthesis are ejected into the source surroundings. Then, their decay may be directly observable through characteristic gamma-ray lines, or they may be transported directly to a terrestrial detector. Also, condensation into dust and solids may occur, and then freeze the composition of gas at the dust formation site, which can be inferred from such stardust as found in meteorites. The intrinsic clocks provided by the radioactive decay of each isotope then provide a tool to investigate the characteristics of transport away from the sources, and through interstellar medium, and in the solidification and planet formation phase of our solar system around its earliest history. In this Chapter we discuss what radioactive isotopes such as26Al, 60Fe, 129I, 59Ni, but also very heavy element isotopes such as 244Pu, or positrons from β+ decay can teach us about sources and transport of radioactive nuclei.


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Copyright information

© The Author(s) 2018

Authors and Affiliations

  • Roland Diehl
    • 1
    Email author
  • Dieter H. Hartmann
    • 2
  • Nikos Prantzos
    • 3
  1. 1.Max Planck Institut für extraterrestrische PhysikGarchingGermany
  2. 2.Clemson UniversityClemsonUSA
  3. 3.Institut d’AstrophysiqueParisFrance

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