We present angle-resolved photoemission spectroscopy data taken from the structurally simplest representative of iron-based superconductors, FeSe, in a wide temperature range. Apart from the variations related to the nematic transition, we detect very pronounced shifts of the dispersions on the scale of hundreds of degrees Kelvin. Remarkably, upon warming up the sample, the band structure has a tendency to relax to the one predicted by conventional band structure calculations, directly opposite to what is intuitively expected. Our findings shed light on the origin of the dominant interaction shaping the electronic states responsible for high-temperature superconductivity in iron-based materials
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
In this thesis, the results of analyzing the electronic structure of two iron-based superconductors:...
Abstract Iron-chalcogenide superconductors display rich phenomena caused by orbital-dependent band s...
FeSe is a fascinating superconducting material at the frontier of research in condensed matter physi...
FeSe is a fascinating superconducting material at the frontier of research in condensed matter physi...
We present a comprehensive study of the evolution of the nematic electronic structure of FeSe using ...
Superconductivity emerges in proximity to a nematic phase in most iron-based superconductors. It is ...
Electronically driven nematic order is often considered as an essential ingredient of high-temperatu...
Superconductivity emerges in proximity to a nematic phase in most iron-based superconductors. It is ...
Electronically driven nematic order is often considered as an essential ingredient of high-temperatu...
Electronically driven nematic order is often considered as an essential ingredient of high-temperatu...
The lifting of $d_{xz}$-$d_{yz}$ orbital degeneracy is often considered a hallmark of the nematic ph...
Our valence band photoelectron spectroscopic studies show a temperature dependent spectral weight tr...
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
In this thesis, the results of analyzing the electronic structure of two iron-based superconductors:...
Abstract Iron-chalcogenide superconductors display rich phenomena caused by orbital-dependent band s...
FeSe is a fascinating superconducting material at the frontier of research in condensed matter physi...
FeSe is a fascinating superconducting material at the frontier of research in condensed matter physi...
We present a comprehensive study of the evolution of the nematic electronic structure of FeSe using ...
Superconductivity emerges in proximity to a nematic phase in most iron-based superconductors. It is ...
Electronically driven nematic order is often considered as an essential ingredient of high-temperatu...
Superconductivity emerges in proximity to a nematic phase in most iron-based superconductors. It is ...
Electronically driven nematic order is often considered as an essential ingredient of high-temperatu...
Electronically driven nematic order is often considered as an essential ingredient of high-temperatu...
The lifting of $d_{xz}$-$d_{yz}$ orbital degeneracy is often considered a hallmark of the nematic ph...
Our valence band photoelectron spectroscopic studies show a temperature dependent spectral weight tr...
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
The presence of dxz−dyz orbital ordering is often considered a hallmark of the nematic phase of Fe-b...
In this thesis, the results of analyzing the electronic structure of two iron-based superconductors:...
Abstract Iron-chalcogenide superconductors display rich phenomena caused by orbital-dependent band s...