Numerical Methods in Quantum Mechanics - Dipartimento di Fisica
Numerical Methods in Quantum Mechanics - Dipartimento di Fisica
Numerical Methods in Quantum Mechanics - Dipartimento di Fisica
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For Z = 2 the correction is equal to 2.5 Ry and yields E = −8 + 2.5 = −5.5 Ry.<br />
The experimental value is −5.8074 Ry. The perturbative approximation is not<br />
accurate but provides a reasonable estimate of the correction, even if the “perturbation”,<br />
i.e. the Coulomb repulsion between electrons, is of the same order<br />
of magnitude of all other <strong>in</strong>teractions. Moreover, he ground state assumed <strong>in</strong><br />
perturbation theory is usually qualitatively correct: the exact wave function for<br />
He will be close to a product of two 1s functions.<br />
D.2 Variational treatment for Helium atom<br />
The Helium atom provides a simple example of application of the variational<br />
method. The <strong>in</strong>dependent-electron solution, Eq.(D.10), is miss<strong>in</strong>g the phenomenon<br />
of screen<strong>in</strong>g: each electron will ”feel” a nucleus with partially screened<br />
charge, due to the presence of the other electron. In order to account for this<br />
phenomenon, we may take as our trial wave function an expression like the<br />
one of Eq.(D.10), with the true charge of the nucleus Z replaced by an “effective<br />
charge” Z e , presumably smaller than Z. Let us f<strong>in</strong>d the optimal Z e<br />
variationally, i.e. by m<strong>in</strong>imiz<strong>in</strong>g the energy. We assume<br />
ψ(r 1 , r 2 ; Z e ) = Z3 e<br />
π e−Ze(r 1+r 2 )<br />
and we re-write the Hamiltonian as:<br />
[<br />
H = −¯h2 ∇ 2 1<br />
− Zq2 e<br />
− ¯h2 ∇ 2 ]<br />
2<br />
− Zq2 e<br />
+<br />
2m e r 1 2m e r 2<br />
[<br />
− (Z − Z e)q 2 e<br />
r 1<br />
− (Z − Z e)q 2 e<br />
r 2<br />
We now calculate<br />
∫<br />
E(Z e ) = ψ ∗ (r 1 , r 2 ; Z e )Hψ(r 1 , r 2 ; Z e ) d 3 r 1 d 3 r 2<br />
(D.15)<br />
]<br />
+ q2 e<br />
r 12<br />
(D.16)<br />
(D.17)<br />
The contribution to the energy due to the first square bracket <strong>in</strong> Eq.(D.16) is<br />
−2Ze 2 a.u.: this is <strong>in</strong> fact a Hydrogen-like problem for a nucleus with charge Z e ,<br />
for two non-<strong>in</strong>teract<strong>in</strong>g electrons. By expand<strong>in</strong>g the rema<strong>in</strong><strong>in</strong>g <strong>in</strong>tegrals and<br />
us<strong>in</strong>g symmetry we f<strong>in</strong>d<br />
∫<br />
E(Z e ) = −2Ze 2 −<br />
(<strong>in</strong> a.u.) with<br />
|ψ| 2 4(Z − Z ∫<br />
e)<br />
d 3 r 1 d 3 r 2 +<br />
r 1<br />
|ψ| 2 = Z6 e<br />
π 2 e−2Ze(r 1+r 2 )<br />
Integrals can be easily calculated and the result is<br />
|ψ| 2 2<br />
r 12<br />
d 3 r 1 d 3 r 2<br />
(D.18)<br />
(D.19)<br />
E(Z e ) = −2Z 2 e − 4(Z − Z e )Z e + 2 5 8 Z e = 2Z 2 e − 27<br />
4 Z e (D.20)<br />
where we explicitly set Z = 2.<br />
imme<strong>di</strong>ately leads to<br />
M<strong>in</strong>imization of E(Z e ) with respect to Z e<br />
Z e = 27 = 1.6875 (D.21)<br />
16<br />
92