Prof. Paddy Regan Department of Physics



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tarix28.07.2018
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Nuclear Spectroscopy: From Natural Radioactivity to Studies of the Most Exotic Isotopes.


Outline of talk

  • Elements, Isotopes and Isotones

  • Alpha, beta and gamma decay

  • Primordial radionuclides…..why so long ?

  • Internal structures, gamma rays and shells.

  • How big is the nuclear chart ?

  • What could this tell us about nucleosynthesis?





















Some current nuclear physics questions

  • 286 combinations of protons and neutrons are either stable or have decay half-lives of more than 500 million years.

    • What are the limits of nuclear existence…i.e. how many different nuclear species can exist?
  • N/Z ratio changes for stable nuclei from ~1:1 for light nuclei (e.g., 16O, 40Ca) to ~1.5 for 208Pb (126/82 ~ 1.5)

    • How does nuclear structure change when the N/Z ratio differs from stable nuclear matter?


Accelerator facility at GSI-Darmstadt



An Efficient Way to Make Exotic Nuclei: Projectile Fragmentation Reaction Process









A few physics examples….

























Evidence for nuclear shell structure….. energy of 1st excited state in even-even nuclei….E(2+).





Summary

  • Radionuclides (e.g. 235U, 238U, 232Th, 40K) are everywhere.

  • Radioactive decays arise from energy conservation and other (quantum) conservation laws.

  • Characteristic gamma ray energies tell us structural info.

  • The limits for proton-richness in nuclei has been reached.

  • Neutron-rich nuclei are harder to make at the extremes, but we are starting to be able to reach r-process radionuclides.

    • Does the nuclear shell model remain valid for nuclei with ‘diffuse neutron skins’ ?
  • FAIR will increase dramatically our reach of nuclear species for experimental study



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