Consider the Deuterium-Tritium fusion reaction ²H +³H → ˆHe+n How much is the energy released per nucleon?
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Q: Use the following data to calculate the binding energy per nucleon in MeV of the Rhodium-103 nuclide…
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- Use the following data to calculate the binding energy per nucleon in MeV of the Rhodium-103 nuclide Mass of atom = 102.905503 u Mass of proton = 1.007276 u Mass of n Use the following data to calculate the binding energy per nucleon in MeV of the Rhodium-103 nuclide Mass of atom = 102.905503 u Mass of proton = 1.007276 u Mass of neutron = 1.008664 u Mass of electron = 0.00054858 u 1 u = 931.494 MeV eutron = 1.008664 u Mass of electron = 0.00054858 u 1 u = 931.494 MeVUsing the graph given, estimate how much energy is released when a nucleus of mass number 200 fissions into two nuclei each of mass number 100.Calculate the energy released in the following nuclear fission reaction: 239Pu+n→98Tc+138Sb+4n239Pu+n→98Tc+138Sb+4n Recall that the atomic masses are 239 Pu239 Pu = 239.052157 u u, 98 Tc 98Tc = 97.907215 uu, 138 Sb 138Sb = 137.940793u
- Another series of nuclear reactions that can produce energy in the interior of stars is the cycle described below. This cycle is most efficient when the central temperature in a star is above 1.6 × 107 K. Because the temperature at the center of the Sun is only 1.5 × 107 K, the following cycle produces less than 10% of the Sun’s energy. (a) A high-energy proton is absorbed by 12 C. Another nucleus, A , is produced in the reaction, along with a gamma ray. Identify nucleus A decays through positron emission to form nucleus B. (c) Nucleus B absorbs a proton to produce nucleus C and a gamma ray. Identify nucleus C absorbs a proton to produce nucleus D and a gamma ray. Identify nucleus D. (e) Nucleus D decays through positron emission to produce nucleus E. Identify nucleus E. (f) Nucleus E absorbs a proton to produce nucleus F plus an alpha particle. What is nucleus F ? Note: If nucleus F is not 12C—that is, the nucleus you started with—you have made an error and should review the sequence…The uranium decay series from U-238 to stable lead (Pb-206) is: U → Th → *Pa → U → 0Th → Ra → Rn → 18Th → Pb → Bi 238U 234TH 226 → Po 92 92 210Pb → 210 Bi → 210P0 → 206Pb 83 84 Of the 15 nuclei from U-238 to Pb-206, list those radionuclides that are alpha-particle emitters, and those that are beta-particle emitters. State your reasons.One of the fusion reactions that takes place as a star ages is called the triple alpha process. 3 42He → 126C Calculate the mass defect (in u) and the energy produced (in MeV) each time the reaction takes place.
- Two nuclei having the same mass number are called isobars. Calculate the difference in binding energy per nucleon for the isobars 2311Na and 2312Mg. How do you account for the difference?Question 4 Use the following data to calculate the binding energy per nucleon in MeV of the Rhodium-103 nuclide Mass of Rh atom = 102.905503 u 103 45 %3D Mass of proton = 1.007276 u Mass of neutron = 1.008664 u %3D Mass of electron = 0.00054858 u %3D 1u = 931.494 MeV [2.2] Question 5