tidy3d.PoleResidue

class PoleResidue

Bases: DispersiveMedium

A dispersive medium described by the pole-residue pair model.

Parameters:

• name (Attribute: name) –

  Type	Optional[str]
  Default	= None
  Description	Optional unique name for medium.

• frequency_range (Attribute: frequency_range) –

  Type	Optional[Tuple[float, float]]
  Default	= None
  Units	(Hz, Hz)
  Description	Optional range of validity for the medium.

• allow_gain (Attribute: allow_gain) –

  Type	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 ‘allow_gain’ is set to ‘True’ 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) –

  Type	Union[NonlinearSpec, NonlinearSusceptibility]
  Default	= None
  Description	Nonlinear spec applied on top of the base medium properties.

• modulation_spec (Attribute: modulation_spec) –

  Type	Optional[ModulationSpec]
  Default	= None
  Description	Modulation spec applied on top of the base medium properties.

• heat_spec (Attribute: heat_spec) –

  Type	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 using HeatSimulation object, Simulation.perturbed_mediums_copy() can be used to convert mediums with perturbation models defined into spatially dependent custom mediums. Otherwise, the heat_spec does not directly affect the running of an optical Simulation.

• eps_inf (Attribute: eps_inf) –

  Type	PositiveFloat
  Default	= 1.0
  Units	None (relative permittivity)
  Description	Relative permittivity at infinite frequency (\(\epsilon_\infty\)).

• poles (Attribute: poles) –

  Type	Tuple[Tuple[Union[tidy3d.components.types.tidycomplex, tidy3d.components.types.ComplexNumber], Union[tidy3d.components.types.tidycomplex, tidy3d.components.types.ComplexNumber]], …]
  Default	= ()
  Units	(rad/sec, rad/sec)
  Description	Tuple of complex-valued (\(a_i, c_i\)) poles for the model.

Notes

The frequency-dependence of the complex-valued permittivity is described by:

\[\epsilon(\omega) = \epsilon_\infty - \sum_i \left[\frac{c_i}{j \omega + a_i} + \frac{c_i^*}{j \omega + a_i^*}\right]\]

Example

>>> pole_res = PoleResidue(eps_inf=2.0, poles=[((-1+2j), (3+4j)), ((-5+6j), (7+8j))])
>>> eps = pole_res.eps_model(200e12)

See also

CustomPoleResidue:

A spatially varying dispersive medium described by the pole-residue pair model.

Notebooks

• Fitting dispersive material models

Lectures

• Modeling dispersive material in FDTD

Attributes

loss_upper_bound

Upper bound of Im[eps] in frequency_range

Methods

Hz_to_angular_freq(f_hz)	Convert frequency in unit of Hz to rad/s.
angular_freq_to_Hz(f_rad)	Convert frequency in unit of rad/s to Hz.
angular_freq_to_eV(f_rad)	Convert frequency in unit of rad/s to eV.
eV_to_angular_freq(f_eV)	Convert frequency in unit of eV to rad/s.
eps_model(frequency)	Complex-valued permittivity as a function of frequency.
from_lo_to(poles[, eps_inf])	Construct a pole residue model from the LO-TO form (longitudinal and transverse optical modes).
from_medium(medium)	Convert a Medium to a pole residue model.
imag_ep_extrema(poles)	Extrema of Im[eps] in the same unit as poles.
lo_to_eps_model(poles, eps_inf, frequency)	Complex permittivity as a function of frequency for a given set of LO-TO coefficients.
to_medium()	Convert to a Medium.

eps_inf

poles

eps_model(frequency)

Complex-valued permittivity as a function of frequency.

__str__()

string representation

classmethod from_medium(medium)

Convert a Medium to a pole residue model.

Parameters:

medium (Medium) – The medium with permittivity and conductivity to convert.

Returns:

The pole residue equivalent.

Return type:

PoleResidue

to_medium()

Convert to a Medium. Requires the pole residue model to only have a pole at 0 frequency, corresponding to a constant conductivity term.

Returns:

The non-dispersive equivalent with constant permittivity and conductivity.

Return type:

Medium

static lo_to_eps_model(poles, eps_inf, frequency)

Complex permittivity as a function of frequency for a given set of LO-TO coefficients. See from_lo_to in PoleResidue for the detailed form of the model and a reference paper.

Parameters:

• poles (Tuple[Tuple[float, float, float, float], ...]) – The LO-TO poles, given as list of tuples of the form (omega_LO, gamma_LO, omega_TO, gamma_TO).

• eps_inf (pd.PositiveFloat) – The relative permittivity at infinite frequency.

• frequency (float) – Frequency at which to evaluate the permittivity.

Returns:

The complex permittivity of the given LO-TO model at the given frequency.

Return type:

complex

classmethod from_lo_to(poles, eps_inf=1)

Construct a pole residue model from the LO-TO form (longitudinal and transverse optical modes). The LO-TO form is \(\epsilon_\infty \prod_{i=1}^l \frac{\omega_{LO, i}^2 - \omega^2 - i \omega \gamma_{LO, i}}{\omega_{TO, i}^2 - \omega^2 - i \omega \gamma_{TO, i}}\) as given in the paper:

M. Schubert, T. E. Tiwald, and C. M. Herzinger, “Infrared dielectric anisotropy and phonon modes of sapphire,” Phys. Rev. B 61, 8187 (2000).

Parameters:

• poles (Tuple[Tuple[float, float, float, float], ...]) – The LO-TO poles, given as list of tuples of the form (omega_LO, gamma_LO, omega_TO, gamma_TO).

• eps_inf (pd.PositiveFloat) – The relative permittivity at infinite frequency.

Returns:

The pole residue equivalent of the LO-TO form provided.

Return type:

PoleResidue

static eV_to_angular_freq(f_eV)

Convert frequency in unit of eV to rad/s.

Parameters:

f_eV (float) – Frequency in unit of eV

static angular_freq_to_eV(f_rad)

Convert frequency in unit of rad/s to eV.

Parameters:

f_rad (float) – Frequency in unit of rad/s

static angular_freq_to_Hz(f_rad)

Convert frequency in unit of rad/s to Hz.

Parameters:

f_rad (float) – Frequency in unit of rad/s

static Hz_to_angular_freq(f_hz)

Convert frequency in unit of Hz to rad/s.

Parameters:

f_hz (float) – Frequency in unit of Hz

static imag_ep_extrema(poles)

Extrema of Im[eps] in the same unit as poles.

Parameters:

poles (Tuple[PoleAndResidue, ...]) – Tuple of complex-valued (a_i, c_i) poles for the model.

property loss_upper_bound

Upper bound of Im[eps] in frequency_range

__hash__()

Hash method.