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Hubbard Model for Asymmetric Ultracold Fermionic ... - KOMET 337

Hubbard Model for Asymmetric Ultracold Fermionic ... - KOMET 337

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4.4. NUMERICAL RESULTS FOR THE GROUND STATE 41Thus the algorithm is very similar to the algorithm presented in Figure 3.11, where we presentthe way of solving (3.3) and (3.4) at fixed µ and ∆. Since µ appears only implicitly in theself-consistency equations, we decouple the Equations (3.3) and (3.4) at fixed n and use abisection method to solve (3.3) at fixed m and a successive iteration as in Figure 3.11 to solve(3.4). Afterwards we check if both equations are solved within the desired accurancy ǫ n andǫ m .The algorithm <strong>for</strong> solving the self-consistency equations uses scheme 4.4 and is presentedhere:Find µ and m at ∆ = 0Scan <strong>for</strong> sign changes in Res(∆)Sign change found?noTake ∆ = 0 as solutionyesUse combination of secant and bisection methodin order to solve (3.5) (as in algorithm 3.11)Compare Helmholtz free energy of the solutionsOutput of µ, m and ∆Figure 4.5: Solution algorithm <strong>for</strong> the self-consistency equations (3.3)-(3.5). algorithm 4.4 isused implicitly to obtain µ and m.With this procedure we are able to find the ground state of our spin-dependent hoppingHamiltonian at fixed occupation number n. We will now present results obtained with theuse of this method.4.4 Numerical results <strong>for</strong> the ground stateWe will now present the results of numerical calculations done according to algorithm 4.5.As hopping amplitude we have chosen t ↑ = 1 and t ↓ = 0.5. We calculate the parameters µ,m and ∆ as a function of U <strong>for</strong> different occupation numbers n.

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