tidy3d.Lorentz#
- class Lorentz[source]#
Bases:
DispersiveMedium
A dispersive medium described by the Lorentz model.
- Parameters:
name (Attribute:
name
) βType
Optional[str]
Default
= None
Description
Optional unique name for medium.
frequency_range (Attribute:
frequency_range
) βType
Optional[Tuple[float, float]]
Default
= None
Units
(Hz, Hz)
Description
Optional range of validity for the medium.
allow_gain (Attribute:
allow_gain
) βType
bool
Default
= False
Description
Allow 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
) βType
Union[NonlinearSpec, NonlinearSusceptibility]
Default
= None
Description
Nonlinear spec applied on top of the base medium properties.
modulation_spec (Attribute:
modulation_spec
) βType
Optional[ModulationSpec]
Default
= None
Description
Modulation spec applied on top of the base medium properties.
heat_spec (Attribute:
heat_spec
) βType
Union[FluidSpec, SolidSpec, NoneType]
Default
= None
Description
Specification of the medium heat properties. They are used for solving the heat equation via the
HeatSimulation
interface. 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 usingHeatSimulation
object,Simulation.perturbed_mediums_copy()
can be used to convert mediums with perturbation models defined into spatially dependent custom mediums. Otherwise, theheat_spec
does not directly affect the running of an opticalSimulation
.eps_inf (Attribute:
eps_inf
) βType
PositiveFloat
Default
= 1.0
Units
None (relative permittivity)
Description
Relative permittivity at infinite frequency (\(\epsilon_\infty\)).
coeffs (Attribute:
coeffs
) βType
Tuple[Tuple[float, float, pydantic.v1.types.NonNegativeFloat], β¦]
Default
Units
(None (relative permittivity), Hz, Hz)
Description
List 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
n
andk
values at frequencyfreq
to a single-pole Lorentz medium.- eps_inf#
- coeffs#
- classmethod from_nk(n, k, freq, **kwargs)[source]#
Convert
n
andk
values at frequencyfreq
to 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.