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New Detector at the Tandem Laboratory of INPP for astrophysics studies Axiotis Michail. Outline. Heavy elements nucleosynthesis p-nuclei abundances Measurement techniques 4 π γ summing method Experimental results Our new detector. Heavy elements nucleosynthesis. β -. s-nuclei.
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New Detector at the Tandem Laboratory of INPP for astrophysics studies AxiotisMichail
Outline • Heavy elements nucleosynthesis • p-nuclei abundances • Measurement techniques • 4πγ summing method • Experimental results • Our new detector
Heavy elements nucleosynthesis β- s-nuclei (n,γ) r-nuclei s/r-nuclei p unstable p Z p p r-process 1 sec 1020 n/cm3 s-process 100 yr 108n/cm3 N
p-nuclei abundances C. Iliadis, Nuclear Physics of Stars (2008) Differences between observed and calculated by Hauser-Fesbach abundances of p-nuclei in the solar system Need to measure cross-sections to improve the “ingredients” of HF calculations
Measurement techniques 4πγ-summing method γ angular distribution measurements
pos. a pos. c pos. b 4πγ summing method Spyrou et al. Phys. Rev. C 76,015802 (2007)
Experimental results DTL-Bochum: 12 inch x12 inch NaI crystal Demokritos-Bochum Demokritos-Bochum Demokritos-Bochum
Our new detector 14 inch x 14 inch NaI crystal segmented in two – Up/Down