Appendix 5: Comparison of intensity and velocity modulation

Keyword(s):  
Nanomaterials ◽  
2021 ◽  
Vol 11 (7) ◽  
pp. 1808
Author(s):  
Liqiang Zhuo ◽  
Huiru He ◽  
Ruimin Huang ◽  
Shaojian Su ◽  
Zhili Lin ◽  
...  

The valley degree of freedom, like the spin degree of freedom in spintronics, is regarded as a new information carrier, promoting the emerging valley photonics. Although there exist topologically protected valley edge states which are immune to optical backscattering caused by defects and sharp edges at the inverse valley Hall phase interfaces composed of ordinary optical dielectric materials, the dispersion and the frequency range of the edge states cannot be tuned once the geometrical parameters of the materials are determined. In this paper, we propose a chirped valley graphene plasmonic metamaterial waveguide composed of the valley graphene plasmonic metamaterials (VGPMs) with regularly varying chemical potentials while keeping the geometrical parameters constant. Due to the excellent tunability of graphene, the proposed waveguide supports group velocity modulation and zero group velocity of the edge states, where the light field of different frequencies focuses at different specific locations. The proposed structures may find significant applications in the fields of slow light, micro–nano-optics, topological plasmonics, and on-chip light manipulation.


1991 ◽  
Vol 63 (23) ◽  
pp. 2795-2797 ◽  
Author(s):  
Tshenge. Demana ◽  
Maureen. Lanan ◽  
Michael D. Morris

1989 ◽  
Vol 66 (6) ◽  
pp. 1193-1202 ◽  
Author(s):  
Mark Polak ◽  
Martin Gruebele ◽  
Bruce W. DeKock ◽  
Richard J. Saykally

2004 ◽  
Vol 92 (4) ◽  
Author(s):  
Takuma Gohda ◽  
Seiji Ishiguro ◽  
Satoru Iizuka ◽  
Noriyoshi Sato
Keyword(s):  
Ion Beam ◽  

1934 ◽  
Vol 46 (4) ◽  
pp. 512-514 ◽  
Author(s):  
E E Wright
Keyword(s):  

2014 ◽  
Vol 11 (S308) ◽  
pp. 475-476
Author(s):  
Jaan Vennik

AbstractWe studied the variation of stellar mass and various star-formation characteristics of satellite galaxies in a volume limited sample of nearby groups as a function of their group-centric distance and of their relative line-of-sight velocity in the group rest frame. We found clear radial dependencies, e.g. massive, red and passive satellites being distributed predominantly near the center of composite group. We also found some evidence of velocity modulation of star-forming properties of satellite galaxies near the group virial radius. We conclude that using kinematical data, it should be feasible to separate dynamical classes of bound, in-falling and 'backsplash' satellite galaxies.


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