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A nucleus is composed of protons and neutrons, collectively called nucleons.
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Z is the atomic number (number of protons), and A is the mass number (total number of protons and neutrons). |
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They have the same charge number Z. isotopes of the carbone.
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The radius r of the nucleus is: r = r₀A1/3 |
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Because the mass of electrons is negligible compared to that of the nucleus. |
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Yes, it is approximately the same for all nuclei (~2.3 × 1017 kg/m³). |
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Δm = Z × mp + (A – Z) × mn – mnucleus |
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Because the mass of the nucleus is less than the sum of its components due to the binding energy (mass defect).
Example : Look the figue
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9 |
We use MeV (Mega electron-volt) instead of joules since it suits nuclear scales. |
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10 |
It is the energy required to completely separate all the nucleons in a nucleus. |
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11 |
It is the binding energy per nucleon: Eb / A. It reflects the nucleus’s stability. |
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The binding energy per nucleon. The higher it is, the more stable the nucleus. |
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y is the binding energy per nucleon (E/A), and x is the mass number A.
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To compare nuclear stability and explain fusion and fission processes.
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15 |
Around A ≈ 56 (iron), where the binding energy per nucleon is highest. |
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