Band splitting and signatures of Fermi-arcs in the magnetic Weyl candidate CeBi
ORAL
Abstract
Weyl semimetals are characterized by topologically protected Weyl nodes in the bulk and Fermi-arcs states with momentum-locked spin or chirality on the surface. Among various Weyl semimetals, magnetic Weyl semimetals are particularly attractive because they have fewer, more widely separated Weyl nodes. Additionally, their Weyl nodes can potentially be manipulated by external magnetic field or changes in the local moment ordering. Here we present a scanning tunneling microscopy and quasiparticle interference (QPI) study of the magnetic Weyl semimetal candidate CeBi. In particular, we resolve splitting of the Bi p and Ce d bands of CeBi with 9T external magnetic field, which is the necessary precondition for Weyl nodes. We also observe signatures of Fermi-arcs in the QPI pattern. The QPI-derived band structure of CeBi in different magnetic phases is also studied.
*This work was supported by DOE EFRC, CATS Swiss National Science foundation Grant P400P2_183890 Gordon and Betty Moore Foundation Grant GBMF4536 and Grant GBMF4411 U.S. DOE, BES, DMSE under Contract No. DE-AC02-07CH11358
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Presenters
Yu Liu
Harvard University
Department of Physics, Harvard University
Physics, Harvard University
Authors
Yu Liu
Harvard University
Department of Physics, Harvard University
Physics, Harvard University
Christian Matt
Harvard University
Department of Physics, Harvard University
Harris Pirie
Harvard University
Department of Physics, Harvard University
Nathan Drucker
Department of Applied Physics, Harvard University
Robert-Jan Slager
Harvard University
Department of Physics, Harvard University
Harvard
Na Hyun Jo
Iowa State University
Ames Laboratory, Iowa State University
Department of Physics & Astronomy, Iowa State University/Ames Laboratory
Department of Physics and Astronomy, Iowa State University/Ames Laboratory
Iowa State University/Ames Laboratory
Brinda Kuthanazhi
Ames Laboratory, Iowa State University
Iowa State University
Department of Physics & Astronomy, Iowa State University/Ames Laboratory
Department of Physics and Astronomy, Ames Laboratory/Iowa State Univeristy
Iowa State University/Ames Laboratory
Sergey L. Bud'ko
Iowa State University
Ames Laboratory and Iowa State University
Ames Lab
Ames laboratory, Ames, IA
Department of Physics & Astronomy, Iowa State University/Ames Laboratory
Ames Laboratory
Department of Physics and Astronomy, Iowa State University/Ames Laboratory
Iowa State University and Ames Laboratory
Iowa State University, Ames Laboratory
Division of Materials Sciences & Engineering, Ames Lab and Iowa State University
Iowa State University/Ames Laboratory
Paul C Canfield
Iowa State University
Ames Laboratory and Iowa State University
Ames Lab
Ames Laboratory and Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA
Ames laboratory, Ames, IA
Ames Laboratory, Iowa State University
Department of Physics & Astronomy, Iowa State University/Ames Laboratory
Department of Physics and Astronomy, Iowa State University/Ames Laboratory
Iowa State University and Ames Laboratory
Iowa State University, Ames Laboratory
Department of Physics and Astronomy, Iowa State University
Division of Materials Sciences & Engineering, Ames Lab and Iowa State University
Department of Physics and Astronomy, Ames Laboratory/Iowa State Univeristy