** *
The Shell Model**:

The
*Schrodinger Equation* is then set up for this
potential, e.g.

**d ^{2}**

**u**

_{I}**/dr**

^{2}+ 2m’/**ħ**

^{2 }**[E + V**

_{o}] u_{I}= 0And solved. Where: m’= m _{n} m _{p}/ (m _{n} + m _{p})

The solution yields stationary quantum states, somewhat like the states which are associated with electrons in the outer shells of the atom.

Like the electrons occupying atomic shells, the nucleons are fermions, i.e. particles each with spin ½ and therefore obeying the Pauli Exclusion Principle so that no more than two nucleons of the same type can occupy the same energy level (e.g. one with spin +½, the other with spin -½.). This leads to particles pairing up in the nucleus: spin up (+ ½) protons with spin down (-½) protons, and spin up neutrons with spin down neutrons.

The form or expression for the energy of a nucleus is very closely approximated by the energy associated with a “square well” potential. The Fermi energy in more explicit form (which we will not elaborate upon too much beyond this) is:

*E*_{F}
= 3 ^{2/3} p ^{4/3} ħ^{2}
r ^{2/3}/ 2M

Where
M is the nucleon mass, and ħ = h/2p* is the adjusted Planck constant (h divided
by *2p) and r is the nucleon density.
Performing the operation with known or estimated values, the result is E

_{F}= 30 MeV

**.**

If we assume a spherical nucleus then the radius is just:

R
= r _{o} A ^{1/3}

**^{ }**This
is also the dimension on either side of the central symmetry line of Fig. 6. The
evidence for the shell model includes the following:

i)Particularly stable nuclei are borne out by “closed shells”, based on our observations.

ii) The model predicts (correctly) that the even N (or A – Z) nuclei will be most stable and the odd Z, odd N nuclei the least stable. Experiments bear this out: there are 160 stable nuclides (with even Z, N) and only 4 with odd Z, N.

iii) The model predicts that for even N, Z nuclides the total angular momentum J = 0, and that for odd nuclides it is half-integral. (Borne out by measurements of nuclear magnetic moments.)*Example Problem*: Find the diameter of the
oxygen (O ^{16}) nucleus.

__Solution:__

We
apply: R = r _{o} A ^{1/3}

Where: r _{o} = 1.2
x 10 ^{-15} m

Is
the Bohr radius, and A (atomic mass) = 16. Then:

R**
= **(1.2
x 10 ^{-15} m) (16) ^{1/3 }= 3.0238 x 10 ^{-15}
m

And
the diameter D = 2R = 2(3.0238 x 10 ^{-15} m)

D
= 6.05 x 10 ^{-15} m

The preceding result can also be generalized to a situation in which the ratio of radii (between two nuclei) is sought. In this case, we can write:

R1/
R2 **= ** [r _{o} A1 ^{1/3}] **/** [r _{o } A2 ^{1/3}]

Or:

R1/
R2 = (A1/ A2) ^{1/3}

^{ }

*Example (2)*: How much larger is a
copper nucleus than an oxygen nucleus?

Let R1 denote the radius of the copper nucleus, and R2, oxygen’s.

Then: A1 = 64, and A2 = 16. So:

R1/
R2 = (64/16)** ^{1/3 }= **4/
2.51 = 1.587

Thus,
the copper nucleus is about 1.587 times the size of the oxygen nucleus*.*

1(a)Find the ratio of the helium nucleus to the uranium 238 nucleus.

(b) Estimate, using any technique you can think of, the ratio of the nuclear densities for part (a).

2) An element has mass number A = 202 and atomic number Z = 80.

a) Find the diameter of the nucleus and how many times it is greater than that of hydrogen.

b)
Find the mass defect D
M for this nucleus.

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