Nambu Spinor Notation in Kitaev spinless p-wave model

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SUMMARY

The discussion focuses on rewriting a Hamiltonian in Bogoliubov-de Gennes (BdG) form using Nambu spinors within the Kitaev spinless p-wave model. The Hamiltonian is expressed as a tridiagonal matrix involving Pauli matrices, specifically with terms defined as D and T. Participants clarify the process of identifying when a Hamiltonian can be simplified using Nambu spinors and discuss matrix transformations to achieve this representation. The conversation emphasizes the importance of understanding the structure of the Hamiltonian to facilitate its conversion into Nambu spinor form.

PREREQUISITES
  • Understanding of Bogoliubov-de Gennes formalism
  • Familiarity with Nambu spinors and their applications
  • Knowledge of matrix representations in quantum mechanics
  • Proficiency in manipulating Hamiltonians in condensed matter physics
NEXT STEPS
  • Study the derivation of the Bogoliubov-de Gennes equations
  • Learn about tridiagonal matrix forms in quantum mechanics
  • Explore the role of Pauli matrices in quantum systems
  • Investigate matrix transformations relevant to Hamiltonian simplifications
USEFUL FOR

Physicists, particularly those specializing in condensed matter physics, quantum mechanics students, and researchers working with superconductivity and topological phases will benefit from this discussion.

DeathbyGreen
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Hey all! Thanks for reading. I'm currently following along in some reading and had some trouble with re-writing a Hamiltonian in Bogluibov-de Gennes form using Nambu notation (Nambu spinors). Here is the low down:

Say we have a Hamiltonian:
\frac{1}{2} \sum_{i=1}^{N} c_{i}^{\dagger} D c_{i} + \frac{1}{2}\sum_{i=1}^{N-1}c^{\dagger}_{i+1}Tc_{i} + c^{\dagger}_{i}T^{\dagger}c_{i+1}<br />

where we have
D = (\frac{\hbar^2}{ma^2} - \mu)\tau_{z}

and
T = (-\frac{\hbar^2}{2ma^2}\tau_{z} - \frac{i\Delta}{2a}\tau_{x})

The tau are Pauli matrices. We are to be able to write the Hamiltonian as a 2Nx2N matrix (N being the number of particles), by defining Nambu spinors

\tilde{c} = (c_{1}, c_{2},...,c_{N})^T

which is of length 2N since each c_{i} is a 2 spinor. Finally, we can simplify the Hamiltonian to
H = \frac{1}{2} \tilde{c^{\dagger}}H\tilde{c}

Where H is a tridiagonal matrix consisting of T's and D's. I understand how the two are equivalent, but how could I just look at a Hamiltonian and tell if I could simplify it using Nambu spinors? When using the Bogluibov quasiparticles we see the same type of thing to get a BdG Hamiltonian. I can check the equivalence by working backwards, but how could I start with the original H in my statement and rearrange it to ultimately get the Nambu form? Hopefully I'm being clear enough :P
 
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When you say "We are to be able to write the Hamiltonian as a 2Nx2N matrix (N being the number of particles), by defining Nambu spinors" you are simply forming a vector out of Nambu spinors, not defining them. Your starting Hamiltonian seems to be already defined in terms of Nambu spinors. I fear I don't quite get your point.
 
Yes sorry, I was worried my question wouldn't be clear. I think it is a pretty simple procedure, but I just don't see how I can look at the first Hamiltonian and know that I can re-write it as a vector of Nambu spinors. It is already written in terms of them, but I don't know how the tridiagonal matrix form is so apparent. Is there some kind of matrix transformation that is commonly used that I'm just not aware of?
 
I think I just figured it out...I just re-wrote each individual term in matrix notation and added them, then got the tridiagonal thing. :D Thanks!
 

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