a) At the first step of "\\beta"-emission, the "^{90}Sr" goes to produce "^{90}Y" and releases an electron and some amount of energy
"^{90}Sr \\rightarrow ^{90}Y + \\bar{e} + \\bar{\\nu}_e"
At the second step of "\\beta"-emission, "^{90}Y" as a not stable isotope decay to a stable "^{90}Zr"
"^{90}Y \\rightarrow ^{90}Zr + \\bar{e} + \\bar{\\nu}_e"
The overall decay then will look like
"^{90}Sr \\rightarrow ^{90}Zr + 2\\bar{e} +2 \\bar{\\nu}_e"
b) The difference in atomic mass (a.u.) can be found by taking a table values of atomic masses of each isotopes by neglecting a mass of electron:
"M_A(^{90}Sr) = 89.907738 a.u\\\\\nM_A(^{90}Zr) = 89.904703 a.u"
"\\Delta M_A = M_A(^{90}Zr)-M_A(^{90}Sr) = \\\\=89.904703 - 89.907738= -0.003035 a.u"
By looking at the decay equation from a), the number of moles is equivalent, so one mole of "^{90}Sr" produces one mole of "^{90}Zr". So, to calculate the mass difference, the atomic units have to be converted to kilograms. The conversion factor is:
"1a.u = 0.0166054 \\times 10^{-25} kg\\\\\n\\Delta m = -0.003035 \\times 0.0166054 \\times 10^{-25} = 0.504 \\times 10^{-29} kg"
c) The energy which is given off by the decay is:
"E=(\\Delta m)c^2"
The 6.5 mg have to be converted to a.u first.
"\\Delta m=6.5 mg = 3.91492 \\times 10^{21} a.u"
Using "1 a.u = 931.5MeV\/c^2" , we obtain the simpler way of the energy calculation:
"E= (3.91492 \\times 10^{21} a.u)(931.5MeV\/c^)c^2 = 3.64675 \\times 10^{24} MeV"
Converting to kJ:
"E=3.64675 \\times 10^{24} MeV \\times 1.60218\\times 10^{-16} = 584.27373 \\times 10^{6} kJ"
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