Orbital mixing at the onset of high-temperature superconductivity in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msub><mml:mi>FeSe</mml:mi><mml:mrow><mml:mn>1</mml:mn><mml:mo>−</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mi>Te</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>CaF</mml:mi><mml:mn>2</mml:mn></mml:msub></mml:mrow></mml:math>
K. Nakayama, Ryuji Tsubono, G. N. Phan, Fuyuki Nabeshima, Naoki Shikama, T. Ishikawa, Yuki Sakishita, S. Ideta, Kiyohisa Tanaka, Atsutaka Maeda, T. Takahashi, T. Sato
Abstract
The authors use angle-resolved photoemission spectroscopy to show distinct electronic structures with different orbital characters between pristine FeSe and high-$T$${}_{c}$ FeSe${}_{1\ensuremath{-}x}$Te${}_{x}$ superconductors.
Topics & Concepts
Mixing (physics)PhysicsAlgorithmComputer scienceQuantum mechanicsIron-based superconductors researchCorporate Taxation and AvoidanceRare-earth and actinide compounds