@article{
 title = {Entanglement entropy and entanglement spectrum of triplet topological superconductors},
 type = {article},
 year = {2014},
 identifiers = {[object Object]},
 pages = {425702},
 volume = {26},
 websites = {http://arxiv.org/abs/1312.7782,http://stacks.iop.org/0953-8984/26/i=42/a=425702?key=crossref.b60e9b41fae67c7407dcab8d95dc095c},
 month = {10},
 day = {22},
 id = {9ea2e78d-11fe-3ceb-b0db-ecb17b5bb236},
 created = {2015-06-13T14:59:11.000Z},
 file_attached = {true},
 profile_id = {29e45dc8-9183-33d2-9a32-ee061689aa68},
 last_modified = {2017-04-26T09:35:48.611Z},
 read = {false},
 starred = {false},
 authored = {true},
 confirmed = {true},
 hidden = {false},
 citation_key = {Oliveira2013},
 folder_uuids = {382d62f0-05e5-4a13-9a8f-8b4aa97ce1ae},
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 abstract = {We analyse the entanglement entropy properties of a two-dimensional p-wave superconductor with Rashba spin-orbit coupling, which displays a rich phase-space that supports non-trivial topological phases, as the chemical potential and the Zeeman term are varied. We show that the entanglement entropy and its derivatives clearly signal the topological transitions and provides a sensible signature of each topological phase. We separately analyse the contributions to the entanglement entropy that are proportional to or independent of the perimeter of the system, as a function of the Hamiltonian coupling constants and the geometry of the subsystem. We conclude that both contributions are generically non-universal depending on the specific Hamiltonian parameters and on the particular geometry. Nevertheless, contributions to the entanglement entropy due to different kinds of boundaries or edges simply add up. We also observe a relationship between a topological contribution to the entanglement entropy in a half- cylinder geometry and the number of edge states, and that the entanglement spectrum has robust modes associated with each edge state.},
 bibtype = {article},
 author = {Oliveira, T P and Ribeiro, P and Sacramento, P D},
 journal = {Journal of Physics: Condensed Matter},
 number = {42}
}

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