Analytic evaluation of Kane fermion magneto-optics in two and three dimensions
Source abstract
Abstract
We calculate and present an analytic form of the magneto-optical conductivity for the gapped low-energy Kane model in two and three dimensions separately. The two-dimensional case maps onto the $\ensuremath{\alpha}\text{\ensuremath{-}}{\mathcal{T}}3$ model at a particular value of $\ensuremath{\alpha}=1/\sqrt{3}$. In two dimensions, two chiral sectors exist, between which there are no optically activated transitions. In three dimensions, the extra dimension of dispersion mixes the two sectors so that intra- and intersector transitions can occur. The latter type of transition can be separated out via circular polarizations of light, and it shows a distinct signature in the transverse conductivity.
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Research context
OpenAlex topics: Quantum and electron transport phenomena · Topological Materials and Phenomena · Physics of Superconductivity and Magnetism
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References (20)
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1. 10.1016/0022-3697(57)90013-610.1016/0022-3697(57)90013-6 ↗
2. 10.1103/PhysRevLett.107.12720510.1103/PhysRevLett.107.127205 ↗
3. 10.1209/0295-5075/97/6700410.1209/0295-5075/97/67004 ↗
4. 10.1103/PhysRevB.92.03511810.1103/PhysRevB.92.035118 ↗
5. 10.1103/PhysRevLett.112.02640210.1103/PhysRevLett.112.026402 ↗
6. 10.1103/PhysRevB.90.04531010.1103/PhysRevB.90.045310 ↗
7. 10.1088/1742-6596/603/1/01200110.1088/1742-6596/603/1/012001 ↗
8. 10.1103/PhysRevB.92.15511610.1103/PhysRevB.92.155116 ↗
9. 10.1103/PhysRevB.92.24541010.1103/PhysRevB.92.245410 ↗
10. 10.1103/PhysRevB.94.12543510.1103/PhysRevB.94.125435 ↗
11. 10.1088/0953-8984/28/49/49530210.1088/0953-8984/28/49/495302 ↗
12. 10.1038/nphys285710.1038/nphys2857 ↗
13. 10.1038/ncomms1257610.1038/ncomms12576 ↗
14. 10.1103/PhysRevLett.117.13640110.1103/PhysRevLett.117.136401 ↗
15. 10.1103/PhysRevB.90.03540510.1103/PhysRevB.90.035405 ↗
16. M. E. Peskin · 1995
17. G. D. Mahan · 2013
18. 10.1103/PhysRevB.87.23512110.1103/PhysRevB.87.235121 ↗
19. 10.1103/PhysRevB.87.24513110.1103/PhysRevB.87.245131 ↗
20. 10.1103/PhysRevLett.115.17640410.1103/PhysRevLett.115.176404 ↗