Four isotopes on the s-process path are given idealised neutron-capture cross…

PHYSICS · Multi-part · Fermi University Physics · Nuclear Physics · Nuclear astrophysics and applications · Nuclear astrophysics and applications

Stars from the Inside, Ch Thermonuclear energy generation: reaction rates, burning stages and the elements they make

Problem

Four isotopes on the s-process path are given idealised neutron-capture cross sections σ\sigma (in millibarn, at the relevant thermal energy) and relative abundances NN (arbitrary units). The values are round illustrative numbers, not measurements. Data (isotope, neutron number, σ\sigma, NN): 88Sr{}^{88}\mathrm{Sr}, 5050, 5 mb5\,\mathrm{mb}, 200200; 96Zr{}^{96}\mathrm{Zr}, 5656, 50 mb50\,\mathrm{mb}, 2020; 140Ce{}^{140}\mathrm{Ce}, 8282, 20 mb20\,\mathrm{mb}, 5050; 150Sm{}^{150}\mathrm{Sm}, 8888, 100 mb100\,\mathrm{mb}, 1010. ((a)) Check that these four isotopes obey the steady-flow rule σANA≈constant\sigma_A N_A \approx \text{constant}, and state the value of that constant. ((b)) 208Pb{}^{208}\mathrm{Pb} (Nneutrons=126N_{\rm neutrons}=126) is given, on the same illustrative scale, a cross section σ=2 mb\sigma = 2\,\mathrm{mb}. Using the same constant, predict its relative abundance, and say why this isotope, together with 88Sr{}^{88}\mathrm{Sr}, sits at an abundance peak.

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