tidy3d.Lorentz#
- class Lorentz[source]#
Bases:
DispersiveMediumA dispersive medium described by the Lorentz model.
- Parameters:
name (Attribute:
name) βTypeOptional[str]
Default= None
DescriptionOptional unique name for medium.
frequency_range (Attribute:
frequency_range) βTypeOptional[Tuple[float, float]]
Default= None
Units(Hz, Hz)
DescriptionOptional range of validity for the medium.
allow_gain (Attribute:
allow_gain) βTypebool
Default= False
DescriptionAllow the medium to be active. Caution: simulations with a gain medium are unstable, and are likely to diverge.Simulations where βallow_gainβ is set to βTrueβ will still be charged even if diverged. Monitor data up to the divergence point will still be returned and can be useful in some cases.
nonlinear_spec (Attribute:
nonlinear_spec) βTypeUnion[NonlinearSpec, NonlinearSusceptibility]
Default= None
DescriptionNonlinear spec applied on top of the base medium properties.
modulation_spec (Attribute:
modulation_spec) βTypeOptional[ModulationSpec]
Default= None
DescriptionModulation spec applied on top of the base medium properties.
heat_spec (Attribute:
heat_spec) βTypeUnion[FluidSpec, SolidSpec, NoneType]
Default= None
DescriptionSpecification of the medium heat properties. They are used for solving the heat equation via the
HeatSimulationinterface. Such simulations can be used for investigating the influence of heat propagation on the properties of optical systems. Once the temperature distribution in the system is found usingHeatSimulationobject,Simulation.perturbed_mediums_copy()can be used to convert mediums with perturbation models defined into spatially dependent custom mediums. Otherwise, theheat_specdoes not directly affect the running of an opticalSimulation.eps_inf (Attribute:
eps_inf) βTypePositiveFloat
Default= 1.0
UnitsNone (relative permittivity)
DescriptionRelative permittivity at infinite frequency (\(\epsilon_\infty\)).
coeffs (Attribute:
coeffs) βTypeTuple[Tuple[float, float, pydantic.v1.types.NonNegativeFloat], β¦]
DefaultUnits(None (relative permittivity), Hz, Hz)
DescriptionList of (\(\Delta\epsilon_i, f_i, \delta_i\)) values for model.
Notes
The frequency-dependence of the complex-valued permittivity is described by:
\[\epsilon(f) = \epsilon_\infty + \sum_i \frac{\Delta\epsilon_i f_i^2}{f_i^2 - 2jf\delta_i - f^2}\]Example
>>> lorentz_medium = Lorentz(eps_inf=2.0, coeffs=[(1,2,3), (4,5,6)]) >>> eps = lorentz_medium.eps_model(200e12)
See also
- Notebooks
- Lectures
Attributes
Methods
eps_model(frequency)Complex-valued permittivity as a function of frequency.
from_nk(n,Β k,Β freq,Β **kwargs)Convert
nandkvalues at frequencyfreqto a single-pole Lorentz medium.- eps_inf#
- coeffs#
- classmethod from_nk(n, k, freq, **kwargs)[source]#
Convert
nandkvalues at frequencyfreqto a single-pole Lorentz medium.- Parameters:
n (float) β Real part of refractive index.
k (float = 0) β Imaginary part of refrative index.
freq (float) β Frequency to evaluate permittivity at (Hz).
- Returns:
Lorentz medium having refractive index n+ik at frequency
freq.- Return type:
- __hash__()#
Hash method.