I try to understand the concept of topological invariants in condensed matter specially in the case of the Z2 invariante and graphene.
From Fradkins book I know that the Z2 invariante can be written as
(−1)ν=∏iδi=∏i√det(w(→Qi))pf(w(→Qi))
where wmn(→k)=⟨um(−→k)|Θ|un(→k)⟩, Θ the time-reversal Operator, un(→k) are the Bloch eigenfunctions and →Qi are the time-reversal invariant points in the Brillouin zone →Qi=−→Qi+→G, usually →Qi∈{(0,0),(π,0),(0,π),(π,π)}.
My question is now what happens in the case of graphene (i.e. the Kane and Mele model) with the Definition of →Qi? In the book by Bernevig the pfaffian is calculated at the Dirac points K and K′ (as long as the C3 is unbroken). Therefore, in the Z2 invariant should have the following form for graphene:
(−1)ν=√det(w(K))pf(w(K))⋅√det(w(K′))pf(w(K′)).
Intuitively, it is clear to me why, because at these points the energy gap is closing. However, I also want to understand from a mathematical point of view why we can write the topological invariant as a pfaffian at specific points in the Brillouin zone.
This post imported from StackExchange Physics at 2016-08-24 17:06 (UTC), posted by SE-user Lars Milz