CHEM1901 Lecture Notes - Lecture 1: Triple-Alpha Process, Nucleosynthesis, Hydrogen Atom

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19 Jul 2018
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Isotope: nuclei with same atomic number but different mass numbers. Stellar nucleogenesis: all atoms are formed from hydrogen 1. Synthesis of carbon: as a star exhausts it"s hydrogen, begins helium burning to fuse heavier nuclei to form increasingly larger atoms. 11h+11h 12h+10e11h+11h 12h+10e12h+11h 23he+g23he+23he 24he+211p411h 24he+210e+2g224he 48be : heavier carbon nuclei are produced by larger stars eg red giants, supergiants and supernovae. Natural radioactivity: nucleogenesis: produces nuclides that can be stable or unstable, unstable nuclei decay through a range of mechanisms radioactivity. Xray: more common when there are more protons in nucleas nucleas is pulling electrons in more tightly. Thus u-238 generates a family of daughter isotopes. 10e+ + -10e- g712n 612c+10e+2655fe+-10e- 2555mn92238u 90234th+24a90234th 91234pa+-10bn(t)=n0exp(-lt)o n0 number of nuclei present at beginning. The decay constant: formula for half life, therefore, decay, t1/2 number of half lives, nuclear decay is a stochastic process.

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