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

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

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5.4. LOW TEMPERATURE LIMIT 53At first we look at the first order contribution:H t,1 = H 0 = ∑ (ij)σt σ (1 − ¯n j−σ− ¯n i−σ+ 2¯n i−σ¯n j−σ)d † iσ d jσ, (5.50)where the notation (ij) signifies that i and j are nearest neighbors, so that in the sum over(ij) each bond occurs twice. Because each site is singly occupied, the first order contributionvanishes: Either (<strong>for</strong> fixed i,j) both spins are parallel, and then hopping is <strong>for</strong>bidden becauseof the Pauli exclusion principle, or they are antiparallel, and then the hopping is suppressedby the (1 − ¯n j−σ− ¯n i−σ+ 2¯n i−σ¯n j−σ) term, since hopping would cause an increase of thedouble occupancies. Every term of the sum is there<strong>for</strong>e equal to 0.Also most of the second order contributions vanish, because they have combinations ofoperators, which are only able to create or annihilate doubly occupied sites:- H t2,1 = 0 because of the occurrence of ¯n i+α,−σd † i+α,σ- H t2,3 = 0 because of the occurrence of d † i,σ d† i,−σ- H t2,4 = 0 because of the occurrence of d i,σd i,−σ- H t2,5 = 0 because of the occurrence of ¯n i+β,σd † i+β,−σ.Hence the only second order contributions arise from H t2,2 and H t2,6 . These terms can bedrastically simplified, since each site is assumed to be singly occupied. Terms with α ≠ βare nonzero only if double occupancies exist. Additionally using that in our subspace eachsite is singly occupied with one fermion we have the identity:¯n iσ= 1 − ¯n i−σ. (5.51)With the help of (5.51) we can simplify the remaining contributions as:H t2,2 = − ∑ iασt 2 σ¯n i,−σ¯n i+α,σ(5.52)and (by again using the single occupancy of each site):∑H t2,6 = −t ↑ t ↓ d † i+α,σ d i,σ d† i,−σ d i+α,−σ. (5.53)iασThus H t2,2 describes a nearest neighbor spin interaction, while H t2,6 describes nearest neighborspin exchange.We will now show that the second order contribution can be rewritten as an effectiveanisotropic Heisenberg Hamiltonian. Because the number operators ¯n i,σcommute, we canrewrite H t2,2 by symmetrizing the sum as:H t2,2 = − 1 2 (t2 ↑ + t2 ↓ )∑ iασ¯n i,−σ¯n i+α,σ. (5.54)We introduce:( d† )d † i = i↑d † i↓; d i =( di↑d i↓)(5.55)

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