Finite-temperature-calculations.md

@@ -5,11 +5,11 @@ Finite temperature effects are introduced by adding quasiparticle occupation pro
 ```math
 f_{\beta}(E_n)=\dfrac{1}{\exp(\beta E_n)+1}
 ```
-to definition of densities (see [here](https://gitlab.fizyka.pw.edu.pl/gabrielw/wslda/-/wikis/Physical%20quantities#densities) from explicit formulas). Here $`\beta=1/T`$  is inverse of temperature. In zero temperature limit this function reduced to step function. Quasiparticle energies $`E_n`$ are taken from solution of Bogoliubov-de Gennes type equations
+to definition of densities (see [here](https://gitlab.fizyka.pw.edu.pl/wtools/wslda/-/wikis/Physical%20quantities#densities) from explicit formulas). Here $`\beta=1/T`$  is inverse of temperature. In zero temperature limit this function reduced to step function. Quasiparticle energies $`E_n`$ are taken from solution of Bogoliubov-de Gennes type equations
 ```math
 H_{\textrm{BdG}} \begin{pmatrix}u_{n\uparrow}(r) \\ v_{n\downarrow}(r)\end{pmatrix}= E_n\begin{pmatrix}u_{n\uparrow}(r) \\ v_{n\downarrow}(r)\end{pmatrix}
 ```   
-See [here](https://gitlab.fizyka.pw.edu.pl/gabrielw/wslda/-/wikis/Physical%20quantities#potentials) from explicit form of $`H_{\textrm{BdG}}`$.  
+See [here](https://gitlab.fizyka.pw.edu.pl/wtools/wslda/-/wikis/Physical%20quantities#potentials) from explicit form of $`H_{\textrm{BdG}}`$.  
 
 Presently, **definition of densities is the only place where temperature enters into calculation process**. In general finite temperature DFT allows energy density functional $`\mathcal{E}_{\textrm{edf}}`$ to be temperature dependent, which is not the case neither (A)SLDA or BdG functionals.