I want the answers for both the questions, please!
I want the answers for both the questions, please! u points PREVIOUS Aswers USCIPRU16 31.0.WAUST.Tutoriai A...
In the plot of binding energy per nucleon versus mass number, you will note that the plot peaks around A 60. Nuclei below and above this value have a smaller binding energy. To prove this point determine the binding energy (in MeV) of 28 Ni, 626Fe with an A number of one less than 628Ni, and 639Cu with an A number of one greater than 638 Ni. (Let the mass of a proton be 1.0078 u, the mass of a...
Activity 27-3. Nuclear binding energy [Accompanies
Section 27-3]
The energy that would be required to separate a nucleus
into its individual nucleons is called the binding energy EB. The
graph shows the binding energy per nucleon EB/A versus mass number
A.
For each of the following processes in which nuclei are
combined to make a larger one, state whether the process releases
energy or requires an input of energy, and explain your
reasoning.
(i) 4He + 4He + 4He →...
Hi I need help with both questions for an upcoming test. Please
help! Thanks for the help!
2. Rutherford Scattering Protons are shot into a copper foil with d-12 μm. what is the proton energy if the central collisions minbecome equal to the nuclear radius r copper atoms? The derivation of the impact parameter with respect to deflection angle is obtained by assuming a Coulomb potential of the form F x 1/r2 (equation 4.12 in Haken-Wolf textbook). Derive the impact...
Please fill in the empty shells in excel and include how you
calculated each of the cell values in excel.
Mass of atomic constituents (MeV Mass Defect [MeV Mass Number Atomic Mass Mass of neutrons Mass of protons & electrons [Mev Mass defect per proton+neutron, aka Binding Energy per Nucleon [MeV Nuclide Atomic Mass |MeV] [amu [MeV) H-1 1 H-2 2 H-3 3 Не3 1.007825 938.79100 2,014101 3.016049 1 2 1876.12300 2809.43173 2 1 3.016029 2809.41292 He-4 2 7 4.002603...
Please use the formulate sheet and show all steps to make sure
the question is worth any points
a) The initial ratio of deuterium (D) to hydrogen (H) in a planet's atmosphere was 175000; however, the present ratio is 1/1500 and the initial and final abundances of D are 5 x 10° atoms per m3 and 9 x 106 atoms per m2, respectively. What fraction of deuterium has been lost, and what fraction of hydrogen has been lost in this...