
Most interacting nuclei are isotopes of hydrogen (Z=1) for 2 reasons:
According to the plot B/A they will release the maximum energy
That minimises the Coulomb repulsive force
We can see that reactions leading to production of a particle (particularly stable) produce a large amount of energy.
Note: one reaction is missing -p+p. While it is omitted here, it is the primary astrophysical reaction. We will come back to this one later.
Calculate the barrier height of all reactions in slide number 3 ?
We know that, the barrier height (VB) can be calculated using the eqaution,
VB = (Z1 * Z2 * e / R), where Z1 and Z2 are the atomic numbers of the isotope and e is the charge of the proton, which is 1.6 *19-19 C. R is the nulcear radius = R0(A11/3 + A21/3), where R0 = 1.3 *10-15m
I will find the barrier height for each of the reactions and is uploaded below.



Most interacting nuclei are isotopes of hydrogen (Z=1) for 2 reasons:
Read the articles provided (Riggio, 2008) and Javidan &
Walker (2012). Perform a self-assessment of the global mindset
competencies. What competencies do you feel are your strengths?
Your areas for improvement? What next learning steps could you take
to address your areas for improvement?
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