Please use this identifier to cite or link to this item: https://doi.org/10.1103/PhysRevB.102.035138
Title: Enhanced higher harmonic generation from nodal topology
Authors: Lee, Ching Hua
Yap, Han Hoe
Tai, Tommy
Xu, Gang
Zhang, Xiao
Gong, Jiangbin 
Keywords: Science & Technology
Technology
Physical Sciences
Materials Science, Multidisciplinary
Physics, Applied
Physics, Condensed Matter
Materials Science
Physics
STATE
ALLOYS
PHASE
Issue Date: 21-Jul-2020
Publisher: AMER PHYSICAL SOC
Citation: Lee, Ching Hua, Yap, Han Hoe, Tai, Tommy, Xu, Gang, Zhang, Xiao, Gong, Jiangbin (2020-07-21). Enhanced higher harmonic generation from nodal topology. PHYSICAL REVIEW B 102 (3). ScholarBank@NUS Repository. https://doi.org/10.1103/PhysRevB.102.035138
Abstract: Among topological materials, nodal loop semimetals are arguably the most topologically sophisticated, with their valence and conduction bands intersecting along arbitrarily intertwined nodes. But unlike the well-known topological band insulators with quantized edge conductivities, nodal loop materials possess topologically nontrivial Fermi surfaces, not bands. Hence an important question arises: Are there also directly measurable or even technologically useful physical properties characterizing nontrivial nodal loop topology? In this paper, we provide an affirmative answer by showing that nodal linkages protect the higher harmonic generation (HHG) of electromagnetic signals. Specifically, nodal linkages enforce nonmonotonicity in the intraband semiclassical response of nodal materials, which will be robust against perturbations preserving the nodal topology. These nonlinearities distort incident radiation and produce higher frequency peaks in the teraHertz (THz) regime, as we quantitatively demonstrate for a few known nodal materials. Since THz sources are not yet ubiquitous, our new mechanism for HHG will greatly aid applications like material characterization and nonionizing imaging of object interiors.
Source Title: PHYSICAL REVIEW B
URI: https://scholarbank.nus.edu.sg/handle/10635/200720
ISSN: 24699950
24699969
DOI: 10.1103/PhysRevB.102.035138
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