Exciton motion in CrSBr is driven by incoherent magnon currents, producing enhanced isotropic transport near the Neel temperature and superdiffusive spreading in bilayers.
Param- agnetic electronic structure of CrSBr: Comparison between ab initio GW theory and angle-resolved photoemission spectroscopy
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Exciton transport driven by spin excitations in an antiferromagnet
Exciton motion in CrSBr is driven by incoherent magnon currents, producing enhanced isotropic transport near the Neel temperature and superdiffusive spreading in bilayers.