Binding energy, Coulomb energy

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Homework Help Overview

The discussion revolves around calculating the difference in binding energy between the mirror nuclides \(^{15}O\) and \(^{15}N\), as well as determining their radii based on Coulomb energy differences. The problem involves concepts from nuclear physics, particularly binding energy and Coulomb repulsion.

Discussion Character

  • Mixed

Approaches and Questions Raised

  • Participants discuss the calculation of binding energy and the assumptions regarding the Coulomb energy's contribution. There are questions about the value of \(R_0\) used in calculations, with some participants noting discrepancies in their results.

Discussion Status

Several participants are checking calculations and exploring different values for \(R_0\). There is recognition of differing formulas for binding energy, and some participants are attempting to reconcile these differences with their results. Guidance has been offered regarding the interpretation of the Coulomb term in binding energy calculations.

Contextual Notes

Participants note that the question may focus solely on the Coulomb term, which could lead to variations in the calculated values of \(R_0\). There is also mention of classical versus quantum mechanical principles affecting the Coulomb energy calculations.

Incand
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Homework Statement


a) Calculate the difference in binding energy between the mirror nuclide ##^{15}O## and ##^{15}N##.
b) Calculate the radius of both nuclide’s assuming the difference in binding energy exclusively depends on difference in Coulomb energy.

Homework Equations


Mean nuclear radius
##R = R_0A^{1/3}##.
Binding energy
##B = \left[ Zm(^1H)+Nm_n-m(^AX)\right]c^2##.
Binding energy due to Coulomb repulsion between protons
##E_c = -\frac{3}{5}\frac{e^2}{4\pi \epsilon_0 R_0} Z(Z-1)A^{-1/3}##.
Constants:
##m(^1H) = 1.007825u##
##m_n = 1.00866501u##
##m(^{15}O) = 15.003065u##
##m(^{15}N)=15.000109u##
##1 u = 931.502MeV/c^2##
##\frac{e^2}{4\pi \epsilon_0} = 1.439976MeV \cdot fm##.

The Attempt at a Solution


I think I solved part a) but I'm having trouble with part b).
The difference in binding energy should be
##\Delta B = \left[ m_n-m(^1H)+m(^{15}O)-m(^{15}N\right] = (0.00379601u)/c^2 = 3.536MeV##. (The answer says ##3.532## but I guess I worked with more decimals)

The difference in Coulomb energy should be (since ##8\cdot 7 - 7\cdot 6 = 14##)
##\Delta B= 3/5 \frac{e^2}{4\pi \epsilon_0R_0} 14A^{-1/3}##
##R = R_0A^{1/3} = \frac{3\cdot 14 \cdot 1.439976}{5\cdot 3.536}fm = 3.420752fm##
The answer however says ##R = 3.67fm## so I did something wrong (using 3.532 instead doesn't change anything)
 
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check the calculation .
what value of R0 was taken? As i find people taking different values!
 
drvrm said:
check the calculation .
what value of R0 was taken? As i find people taking different values!
As I understand the question I should compute ##R_0## from knowing the binding energy (actually ##R_0A^{(1/3)}##).

The typical value for ##R_0## I've seen is ##R_0 \approx 1.2fm## but from my calculation I have a value of ##R_0 =1.38## (and from the answer I would need an even larger ##R_0##. So perhaps I'm doing something wrong as I understand it ##R_0## should be about the same for a nuclide. I'm not entirely sure I'm using the right formulas either, they were simply the ones that seemed to apply to the question.
 
For a nucleus with A nucleons, including Z protons and N neutrons, a semi-empirical formula for the binding energy (BE) per nucleon is:

ba781d47f57680bfa05cecae128018b0.png

where the coefficients are given by:
6e636a65e044a711bcf2291147e23e47.png
;
ee7848ef02b293553a87dfd086501f3c.png
;
29bb3ddcf2ffcb39e1a79007bb680ffa.png
;
7d4b87252fac76a7c6d5772afe4dfccc.png
;
b32d251d4b0da090a11bfa7ceeb212f2.png
. one can have an estimate by third term of the mass formula - just to check (ref.wiki)
https://en.wikipedia.org/wiki/Nucle...iempirical_formula_for_nuclear_binding_energy
 
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Essentially I'm using the coulomb term out of the that formula. However the version I have is different from the one on wikipedia. My book says
##B = a_vA -a_sA^{(2/3)}-a_cZ(Z-1)A^{(-1/3)}-a_{\text{sym}}\frac{(A-2Z)^2}{A}+\delta.##
Note the difference in the Coulomb term.
If I use ##Z^2## I indeed get the correct result just correcting my earlier value with ##3.42\cdot \frac{15}{14} = 3.67## (since ##8^2-7^2=15##).
Now I'm confused why there's ##Z(Z-1)## in the version In my book. The book argue that the term is proportional to ##Z(Z-1)## since each proton repels each of the other ones.
 
Nucleus Ro (in fermis)

B11 1.28

C13 1.34

N15 1.31

O17 1.26

F19 1.26

Ne21 1.25

Na23 1.22

Mg23 1.23

Al27 1.20

ref.
http://www.bhojvirtualuniversity.com/ss/sim/physics/msc_f_phy_p3u1.doc
The energy discrepancy is because of the use of classical principles instead of quantum mechanical principles in calculating the coulomb energy Ec..
 
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Incand said:
Note the difference in the Coulomb term.
If I use Z2Z2Z^2 I indeed get the correct result just correcting my earlier value with

The difference from wiki is that Wiki Formula is for B/A -binding energy per nucleon - but meanwhile i think its R0 value which changes with nucleids may be responsible for the difference.
 
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Incand said:
Now I'm confused why there's Z(Z−1)Z(Z−1)Z(Z-1) in the version In my book. The book argue that the term is proportional to Z(Z−1)Z(Z−1)Z(Z-1) since each proton repels each of the other ones.

actually its Z(Z-1) but approximated to Z^2 so when you use the former you are very correct. the culprit seems to be R0 value.
 
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Thanks for all the help! I believe the answer was calculated using the ##Z^2## approximation so that should explain everything. As for the ##R_0## value I'm not entirely sure. I don't use the actual value of ##R_0## in my calculations although I could compute it.
I'm guessing the difference in ##R_0##(if I compute it) may be because the question only cares about the Coulomb term which isn't the entire truth.
 

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