Difference between revisions of "User:Finlay Nelson"

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== '''Inverse Mie and Numerical Modelling''' ==
 
 
Based on a Drude interpretation of electrical conduction, the effects of charge on the optical properties of plasmonic nanostructures are confined, through electrostatic screening effects, to only their very peripheries. Within the so-called Thomas-Fermi screening length, metals exhibit drastically different permittivities than found in the bulk, but penetrating typically less than a single Angstrom into the metal its effects on the structure as a whole are usually negligible. However, when considering plasmonic nanostructures, who’s dimensions are no more than a few hundreds of nanometres, these charge-dependent effects become far more significant. It is extremely useful, therefore, to be armed with prior knowledge of the optical properties of a proposed nanostructure morphology. This task, while usually allocated to numerical simulation using finite element models, becomes exceedingly problematic in the case of charged nanostructures owing to the dimensions of the Thomas-Fermi screening length. One facet of this work is therefore to develop an alternative approach to modelling the optical response of charged nanostructures based on effective medium theory.
 
 
This branch of material science is concerned with describing complex composite materials with heterogeneous properties as homogeneous equivalents. In this particular application we therefore replace the material within the Thomas-Fermi domain and a portion of the adjacent bulk, with a larger artificial domain of uniform permittivity that accurately reflects the behaviour of the original system. Charge-dependent effects are thus preserved within this new description, but importantly by virtue of its increased thickness such a domain can be easily described in finite element models. While there already exist effective medium approximations for will dispersed mixtures, the applicability of these to charged nanostructures remains in question and so a more robust method is being investigated. This begins with an inverse approach to Mie theory.
 
Traditionally Mie theory is used to ascertain the optical properties (scattering, absorption, etc.) of particles, specifically spheres, whose diameter is in the order of the wavelength of incident light. It is important to note that Mie theory can be applied to both homogeneous spheres and spheres consisting of core and shell domains, much like our previous description of charged particles (a core with bulk permittivity and a shell with permittivity described by the Thomas-Fermi screening length). The inverse method therefore follows 2 steps:
 
 
# Geometry 1:
 
#*Compute the forward model for a charged nanosphere to obtain its scattering and absorption cross-sections. These serve as the reference against which to compare all other solutions; an accurate equivalent system will have scattering and absorption cross-sections that match these originals.
 
# Geometry 2:
 
#* Define a second geometry with shell of desired thickness but whose total diameter remains the same as in the first instance.
 
#* Define a search space in both n and k (the real and imaginary components of refractive index) over which to search for a solution. Having iteratively computed the forward model over this range of n and k, the instance in which the values of scattering and absorption cross-sections both match their counterparts from geometry 1 constitute the desired solution.
 
#* Repeat for the desired range of wavelengths, re-defining the search space on each iteration to retain high resolution solutions.
 
 
[[File:Inverse_intersection_example.png]]
 
 
Finite element models describing the optical response of charged nanoparticles can then be computed using this set of effective refractive indices. If the indices were computed correctly there should be strong agreement between the numerical simulations and Mie theory results. Extending this to more complex geometries remains a challenge of considerable interest.
 

Latest revision as of 23:26, 21 January 2024