scholarly journals Fano collective resonance as complex mode in a two-dimensional planar metasurface of plasmonic nanoparticles

2014 ◽  
Vol 105 (19) ◽  
pp. 191107 ◽  
Author(s):  
Salvatore Campione ◽  
Domenico de Ceglia ◽  
Caner Guclu ◽  
Maria A. Vincenti ◽  
Michael Scalora ◽  
...  
2016 ◽  
Vol 4 (3) ◽  
pp. 1020-1027 ◽  
Author(s):  
M. Sygletou ◽  
P. Tzourmpakis ◽  
C. Petridis ◽  
D. Konios ◽  
C. Fotakis ◽  
...  

A novel top-down and universal optical technique for the effective decoration of two-dimensional (2D) nanosheets (NS), graphene oxide (GO), boron nitride (BN) and tungsten disulfide (WS2), with noble metallic nanoparticles (NPs) is reported.


2019 ◽  
Vol 7 (12) ◽  
pp. 3675-3687 ◽  
Author(s):  
Chinedu Obiakara ◽  
Mahmoud A. Mahmoud

The electromagnetic field of the plasmonic nanoparticles altered the spin–orbital coupling in the MoS2 2D-material thus changed its optical properties.


1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.


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