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We use the Hamiltonian Eq. (IV.2.1),
The energy functional now depends on the
wave functions
,
,
![$\displaystyle F[\Psi]= F[\psi_{\nu_1},...,\psi_{\nu_N}]=F[\{\psi_{\nu_i}\}].$](img665.png) |
|
|
(3.14) |
The definition of the functional derivative is not more complicated than in the one-component case,
![$\displaystyle \frac{\delta F[\Psi]}{\delta \Psi}\equiv
\lim_{\varepsilon\to 0} ...
..._{\nu_i}+\varepsilon \cdot \delta \psi_i\}] -F[\{\psi_{\nu_i}\}]}{\varepsilon},$](img666.png) |
|
|
(3.15) |
where we now have
independent `deviations'
from the functions
. We furthermore want to ensure that all single particle states
are normalised. Therefore, we introduce our functional
with
Lagrange multipliers
,
![$\displaystyle F[\Psi] \equiv \langle \nu_N,...,\nu_1 \vert\hat{H}\vert\nu_1,...,\nu_N\rangle_A
+ \sum_{i=1}^N \lambda_i[ \langle \nu_i\vert\nu_i\rangle -1 ].$](img670.png) |
|
|
(3.16) |
We have calculated the energy expectation values already in Eq. (IV.2.5) and Eq. (IV.2.9),
The individual terms are simply calculated:
The term from the interaction
yields
We can use the symmetry property (Exercise: proof!)
 |
|
|
(3.20) |
to simplify things by using, e.g.,
and changing the summation indices
,
such
that
where again in the `
' term we have swapped indices, and
means that there are two terms which
are the hermitian conjugates of the two others.
Next: `Direct' and `Exchange' Operators
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Tobias Brandes
2005-04-26