Thin-shell approximation of Mie theory for a thin anisotropic layer spaced away from a spherical core: Application to dye-coated nanostructures

2021 ◽  
Vol 104 (3) ◽  
Author(s):  
Chhayly Tang ◽  
Baptiste Auguié ◽  
Eric C. Le Ru
Keyword(s):  
Thin Shell ◽  
Mie Theory ◽  
Anisotropic Layer ◽  
Spherical Core ◽  
Shell Approximation

Nonlinear Ferromagnetic Shield Modeling by the Thin-Shell Approximation

2006 ◽  
Vol 42 (10) ◽  
pp. 3144-3146 ◽  
Author(s):  
O. Bottauscio ◽  
M. Chiampi ◽  
A. Manzin
Keyword(s):  
Thin Shell ◽  
Shell Approximation

scholarly journals The fragmentation of expanding shells - I. Limitations of the thin-shell approximation

2009 ◽  
Vol 398 (3) ◽  
pp. 1537-1548 ◽  
Author(s):  
James E. Dale ◽  
Richard Wünsch ◽  
Anthony Whitworth ◽  
Jan Palouš
Keyword(s):  
Thin Shell ◽  
Shell Approximation ◽  
Expanding Shells

Generalized Mie theory of light scattering by annular anisotropic layer: anisotropy effects

2001 ◽  
Author(s):  
Alexei D. Kiselev ◽  
Victor Y. Reshetnyak ◽  
Timothy J. Sluckin
Keyword(s):  
Light Scattering ◽  
Mie Theory ◽  
Anisotropic Layer

scholarly journals Dynamics of false vacuum bubbles: beyond the thin shell approximation

2009 ◽  
Vol 2009 (11) ◽  
pp. 016-016 ◽  
Author(s):  
Jakob Hansen ◽  
Dong-il Hwang ◽  
Dong-han Yeom
Keyword(s):  
Thin Shell ◽  
False Vacuum ◽  
Shell Approximation

scholarly journals High spectral field enhancement and tunability in core–double shell metal–dielectric–metal spherical nanoparticles

RSC Advances ◽  
2016 ◽  
Vol 6 (112) ◽  
pp. 110471-110481 ◽  
Author(s):  
Luis J. Mendoza Herrera ◽  
Lucía B. Scaffardi ◽  
Daniel C. Schinca
Keyword(s):  
External Factor ◽  
Mie Theory ◽  
Field Enhancement ◽  
Spherical Nanoparticles ◽  
Optical Extinction ◽  
Plasmon Resonances ◽  
Spherical Core

Full Mie theory for spherical core–double shell NPs has been developed to study plasmon resonances, optical extinction and spectral field enhancement of a generalized metal–dielectric–metal NPs, reaching an external factor of 33 for Al–SiO2–Au.

scholarly journals Mass Spectrum of a Starburst

2004 ◽  
Vol 217 ◽  
pp. 318-323 ◽  
Author(s):  
Jan Palouš ◽  
Richard Wünsch ◽  
Soňa Ehlerová
Keyword(s):  
Mass Spectrum ◽  
Power Law ◽  
Time Scale ◽  
Thin Shell ◽  
Mass Spectra ◽  
Computer Code ◽  
Low Density ◽  
Hydrodynamical Simulations ◽  
Shell Approximation ◽  
Self Gravity

The fragmentation of supershells and filaments driven by a superwind in a starburst region produces clumps with a mass spectrum approximated by a power law. Its spectral index is close to −2.3. We present results of computer simulations using the thin shell approximation, which are compared to 3D hydrodynamical simulations with self-gravity using the ZEUS computer code. In a low density medium the fragmentation time-scale is comparable to the collisional time-scale, and consequently collisions change the mass spectra of fragments to less steep values. In high density environments collisional time-scales are much longer and the mass spectrum results from gravitational fragmentation of expanding sheets and filaments.

Sign in / Sign up

Export Citation Format

Share Document