Self-consistent Hartree-Fock approach to Phase Transitions: Difference between revisions
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Define <math>G_{\sigma}(\vec{r}-\vec{r}^{\prime})= <\Phi_{0}|\psi_{\sigma}^{\dagger}(\vec{r})\psi_{\sigma}(\vec{r}^{\prime})|\Phi_{0}></math> | Define <math>G_{\sigma}(\vec{r}-\vec{r}^{\prime})= <\Phi_{0}|\psi_{\sigma}^{\dagger}(\vec{r})\psi_{\sigma}(\vec{r}^{\prime})|\Phi_{0}></math> | ||
Then, we find that | |||
<math>E^{(1)} = \frac{1}{2}\int d^{3}r d^{3}r^{\prime} v(\vec{r}-\vec{r}^{ \prime})[n^{2}-\sum_{\sigma}G_{\sigma}(\vec{r}-\vec{r}^{\prime})^{2}] |
Revision as of 18:52, 30 November 2012
Hartree-Fock approach to Phase Transitions
Hartree-Fock in second quantized form
The interaction energy operator for a two body system with pairwise interactions is given by
In the above operator, it is important to note the order of the operators. Including the kinetic energy term we can write the Hamiltonian for particles of mass m with pairwise interactions in second quantized formalism as
The first-order correction to the energy induced by the interaction is
Define
Then, we find that
<math>E^{(1)} = \frac{1}{2}\int d^{3}r d^{3}r^{\prime} v(\vec{r}-\vec{r}^{ \prime})[n^{2}-\sum_{\sigma}G_{\sigma}(\vec{r}-\vec{r}^{\prime})^{2}]