Camelback-shaped band reconciles heavy-electron behavior with weak electronic Coulomb correlations in superconducting TlNi$_{2}$Se$_{2}$
ORAL
Abstract
Combining photoemission spectroscopy, Raman spectroscopy, and first-principles calculations, we characterize superconducting TlNi$_{2}$Se$_{2}$ as a material with weak electronic Coulomb correlations leading to a bandwidth renormalization of 1.4. We identify a camelback-shaped band, whose energetic position strongly depends on the selenium height. While this feature is universal in transition metal pnictides, in TlNi$_2$Se$_2$ it lies in the immediate vicinity of the Fermi level, giving rise to a pronounced van Hove singularity (VHS). The resulting heavy band mass resolves the apparent puzzle of a large normal-state Sommerfeld coefficient in this weakly correlated compound. The correlation effect evolution in pnictides upon d-shell filling in the presence of significant Hund's exchange coupling will also be discussed.
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Authors
Christian Matt
Swiss Light Source, Paul Scherrer Insitut, CH-5232 Villigen PSI, Switzerland
Nan Xu
Swiss Light Source, Paul Scherrer Insitut, CH-5232 Villigen PSI, Switzerland
A. van Roekeghem
Ecole Polytechnique, CNRS-UMR7644, 91128 Palaiseau, France
S. Biermann
Ecole Polytechnique, CNRS-UMR7644, 91128 Palaiseau, France
P. Richard
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
X. Shi
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
S.-F. Wu
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
H. W. Liu
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
D. Chen
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
T. Qian
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
H. Ding
Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
H. Wang
Department of Physics, Zhejiang University, Hangzhou 310027, China
Q. Mao
Department of Physics, Zhejiang University, Hangzhou 310027, China
J. Du
Department of Physics, Zhejiang University, Hangzhou 310027, China
M. Fang
Department of Physics, Zhejiang University, Hangzhou 310027, China
N. Plumb
Swiss Light Source, Paul Scherrer Insitut, CH-5232 Villigen PSI, Switzerland
M. Radovic
Swiss Light Source, Paul Scherrer Insitut, CH-5232 Villigen PSI, Switzerland
J. Mesot
Swiss Light Source, Paul Scherrer Insitut, CH-5232 Villigen PSI, Switzerland
M. Shi
Swiss Light Source, Paul Scherrer Insitut, CH-5232 Villigen PSI, Switzerland