2021
DOI: 10.1016/j.optmat.2021.110831
|View full text |Cite
|
Sign up to set email alerts
|

Temperature-dependent transverse-field magneto-plasmons properties in InSb

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
1
0

Year Published

2021
2021
2024
2024

Publication Types

Select...
5
1

Relationship

1
5

Authors

Journals

citations
Cited by 8 publications
(1 citation statement)
references
References 27 publications
0
1
0
Order By: Relevance
“…Dispersion bands and associated Chern numbers of (a) nontrivial bulk modes and (b) trivial modes using the local Drude and nonlocal hydrodynamic Drude models; k p = ω p /c 0 , where c 0 is the speed of light in free space. The magnetized plasma region is modeled by (4), using the parameters n e = 3.6 × 10 21 (m −3 ), ε ∞ = 15.68, m * = 0.0175m 0 , B 0 = 0.6T, µ = ∞, corresponding to ω * p = 2π(1.03THz), ω c /ω p = 0.23 and γ = 0, related to the InSb crystal at low temperature[29], and the nonlocality parameter of β = 0.77 × 10 6 m/s.…”
mentioning
confidence: 99%
“…Dispersion bands and associated Chern numbers of (a) nontrivial bulk modes and (b) trivial modes using the local Drude and nonlocal hydrodynamic Drude models; k p = ω p /c 0 , where c 0 is the speed of light in free space. The magnetized plasma region is modeled by (4), using the parameters n e = 3.6 × 10 21 (m −3 ), ε ∞ = 15.68, m * = 0.0175m 0 , B 0 = 0.6T, µ = ∞, corresponding to ω * p = 2π(1.03THz), ω c /ω p = 0.23 and γ = 0, related to the InSb crystal at low temperature[29], and the nonlocality parameter of β = 0.77 × 10 6 m/s.…”
mentioning
confidence: 99%