PlasmaPhase.h

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/**
 * @file PlasmaPhase.h
 * Header file for class PlasmaPhase.
 */
 
// This file is part of Cantera. See License.txt in the top-level directory or
// at https://cantera.org/license.txt for license and copyright information.
 
#ifndef CT_PLASMAPHASE_H
#define CT_PLASMAPHASE_H
 
#include "cantera/thermo/IdealGasPhase.h"
#include "cantera/numerics/eigen_sparse.h"
 
namespace Cantera
{
 
class Reaction;
class ElectronCollisionPlasmaRate;
 
//! Base class for handling plasma properties, specifically focusing on the
//! electron energy distribution.
/*!
 * This class provides functionality to manage the the electron energy distribution
 * using two primary methods for defining the electron distribution and electron
 * temperature.
 *
 * The first method utilizes setElectronTemperature(), which sets the electron
 * temperature and calculates the electron energy distribution assuming an
 * isotropic-velocity model. Note that all units in PlasmaPhase are in SI, except
 * for electron energy, which is measured in volts.
 *
 * The generalized electron energy distribution for an isotropic-velocity
 * distribution (as described by Gudmundsson @cite gudmundsson2001 and Khalilpour
 * and Foroutan @cite khalilpour2020)
 * is given by:
 *   @f[
 *          f(\epsilon) = c_1 \frac{\sqrt{\epsilon}}{\epsilon_m^{3/2}}
 *          \exp \left(-c_2 \left(\frac{\epsilon}{\epsilon_m}\right)^x \right),
 *   @f]
 * where @f$ x = 1 @f$ corresponds to a Maxwellian distribution and
 * @f$ x = 2 @f$ corresponds to a Druyvesteyn distribution (which is the
 * default). Here, @f$ \epsilon_m = \frac{3}{2} T_e @f$ [V] represents the
 * mean electron energy.
 *
 * The total probability distribution integrates to one:
 *   @f[
 *           \int_0^{\infty} f(\epsilon) d\epsilon = 1.
 *   @f]
 * According to Hagelaar and Pitchford @cite hagelaar2005, the electron energy
 * probability function can be defined as
 * @f$ F(\epsilon) = \frac{f(\epsilon)}{\sqrt{\epsilon}} @f$ with units of
 * [V@f$^{-3/2}@f$]. The generalized form of the electron energy probability
 * function for isotropic-velocity distributions is:
 *   @f[
 *          F(\epsilon) = c_1 \frac{1}{\epsilon_m^{3/2}}
 *          \exp\left(-c_2 \left(\frac{\epsilon}{\epsilon_m}\right)^x\right),
 *   @f]
 * and this form is used to model the isotropic electron energy distribution
 * in PlasmaPhase.
 *
 * The second method allows for manual definition of the electron energy
 * distribution using setDiscretizedElectronEnergyDist(). In this approach,
 * the electron temperature is derived from the mean electron energy,
 * @f$ \epsilon_m @f$, which can be calculated as follows @cite hagelaar2005 :
 *   @f[
 *          \epsilon_m = \int_0^{\infty} \epsilon^{3/2} F(\epsilon) d\epsilon.
 *   @f]
 * This integral can be approximated using the trapezoidal rule,
 *   @f[
 *          \epsilon_m = \sum_i \left(\epsilon_{i+1}^{5/2} - \epsilon_i^{5/2}\right)
 *                       \frac{F(\epsilon_{i+1}) + F(\epsilon_i)}{2},
 *   @f]
 * where @f$ i @f$ is the index of discrete energy levels, or Simpson's rule.
 *
 * @warning  This class is an experimental part of %Cantera and may be
 *           changed or removed without notice.
 * @todo Implement electron Boltzmann equation solver to solve EEDF.
 *       https://github.com/Cantera/enhancements/issues/127
 * @ingroup thermoprops
 */
class PlasmaPhase: public IdealGasPhase
{
public:
    //! Construct and initialize a PlasmaPhase object
    //! directly from an input file. The constructor initializes the electron
    //! energy distribution to be Druyvesteyn distribution (m_x = 2.0). The initial
    //! electron energy grid is set to a linear space which starts at 0.01 eV and ends
    //! at 1 eV with 1000 points.
    /*!
     * @param  inputFile Name of the input file containing the phase definition
     *                   to set up the object. If blank, an empty phase will be
     *                   created.
     * @param  id        ID of the phase in the input file. Defaults to the
     *                   empty string.
     */
    explicit PlasmaPhase(const string& inputFile="", const string& id="");
 
    ~PlasmaPhase();
 
    string type() const override {
        return "plasma";
    }
 
    void initThermo() override;
 
    //! Set electron energy levels.
    //! @param  levels The vector of electron energy levels (eV).
    //!                Length: #m_nPoints.
    //! @param  length The length of the @c levels.
    //! @param  updateEnergyDist update electron energy distribution
    void setElectronEnergyLevels(const double* levels, size_t length,
                                 bool updateEnergyDist=true);
 
    //! Get electron energy levels.
    //! @param  levels The vector of electron energy levels (eV). Length: #m_nPoints
    void getElectronEnergyLevels(double* levels) const {
        Eigen::Map<Eigen::ArrayXd>(levels, m_nPoints) = m_electronEnergyLevels;
    }
 
    //! Set discretized electron energy distribution.
    //! @param  levels The vector of electron energy levels (eV).
    //!                Length: #m_nPoints.
    //! @param  distrb The vector of electron energy distribution.
    //!                Length: #m_nPoints.
    //! @param  length The length of the vectors, which equals #m_nPoints.
    void setDiscretizedElectronEnergyDist(const double* levels,
                                          const double* distrb,
                                          size_t length);
 
    //! Get electron energy distribution.
    //! @param  distrb The vector of electron energy distribution.
    //!                Length: #m_nPoints.
    void getElectronEnergyDistribution(double* distrb) const {
        Eigen::Map<Eigen::ArrayXd>(distrb, m_nPoints) = m_electronEnergyDist;
    }
 
    //! Set the shape factor of isotropic electron energy distribution.
    //! Note that @f$ x = 1 @f$ and @f$ x = 2 @f$ correspond to the
    //! Maxwellian and Druyvesteyn distribution, respectively.
    //! @param  x The shape factor
    void setIsotropicShapeFactor(double x);
 
    //! The shape factor of isotropic electron energy distribution
    double isotropicShapeFactor() const {
        return m_isotropicShapeFactor;
    }
 
    //! Set the internally stored electron temperature of the phase (K).
    //! @param  Te Electron temperature in Kelvin
    void setElectronTemperature(double Te) override;
 
    //! Set mean electron energy [eV]. This method also sets electron temperature
    //! accordingly.
    void setMeanElectronEnergy(double energy);
 
    //! Get electron energy distribution type
    string electronEnergyDistributionType() const {
        return m_distributionType;
    }
 
    //! Set electron energy distribution type
    void setElectronEnergyDistributionType(const string& type);
 
    //! Numerical quadrature method. Method: #m_quadratureMethod
    string quadratureMethod() const {
        return m_quadratureMethod;
    }
 
    //! Set numerical quadrature method for integrating electron
    //! energy distribution function. Method: #m_quadratureMethod
    void setQuadratureMethod(const string& method) {
        m_quadratureMethod = method;
    }
 
    //! Mean electron energy [eV]
    double meanElectronEnergy() const {
        return 3.0 / 2.0 * electronTemperature() * Boltzmann / ElectronCharge;
    }
 
    //! Set flag of automatically normalize electron energy distribution
    //! Flag: #m_do_normalizeElectronEnergyDist
    void enableNormalizeElectronEnergyDist(bool enable) {
        m_do_normalizeElectronEnergyDist = enable;
    }
 
    //! Flag of automatically normalize electron energy distribution.
    //! Flag: #m_do_normalizeElectronEnergyDist
    bool normalizeElectronEnergyDistEnabled() const {
        return m_do_normalizeElectronEnergyDist;
    }
 
    bool addSpecies(shared_ptr<Species> spec) override;
 
    //! Electron Temperature (K)
    //!     @return The electron temperature of the phase
    double electronTemperature() const override {
        return m_electronTemp;
    }
 
    //! Return the Gas Constant multiplied by the current electron temperature
    /*!
     *  The units are Joules kmol-1
     */
    double RTe() const {
        return electronTemperature() * GasConstant;
    }
 
    /**
     * Electron pressure. Units: Pa.
     * @f[P = n_{k_e} R T_e @f]
     */
    virtual double electronPressure() const {
        return GasConstant * concentration(m_electronSpeciesIndex) *
               electronTemperature();
    }
 
    //! Number of electron levels
    size_t nElectronEnergyLevels() const {
        return m_nPoints;
    }
 
    //! Number of collisions
    size_t nCollisions() const {
        return m_collisions.size();
    }
 
    //! Electron Species Index
    size_t electronSpeciesIndex() const {
        return m_electronSpeciesIndex;
    }
 
    //! Return the Molar enthalpy. Units: J/kmol.
    /*!
     * For an ideal gas mixture with additional electron,
     * @f[
     * \hat h(T) = \sum_{k \neq k_e} X_k \hat h^0_k(T) + X_{k_e} \hat h^0_{k_e}(T_e),
     * @f]
     * and is a function only of temperature. The standard-state pure-species
     * enthalpies @f$ \hat h^0_k(T) @f$ are computed by the species
     * thermodynamic property manager.
     *
     * @see MultiSpeciesThermo
     */
    double enthalpy_mole() const override;
 
    double cp_mole() const override {
        throw NotImplementedError("PlasmaPhase::cp_mole");
    }
 
    double entropy_mole() const override {
        throw NotImplementedError("PlasmaPhase::entropy_mole");
    }
 
    double gibbs_mole() const override {
        throw NotImplementedError("PlasmaPhase::gibbs_mole");
    }
 
    double intEnergy_mole() const override {
        throw NotImplementedError("PlasmaPhase::intEnergy_mole");
    }
 
    void getEntropy_R(double* sr) const override;
 
    void getGibbs_RT(double* grt) const override;
 
    void getGibbs_ref(double* g) const override;
 
    void getStandardVolumes_ref(double* vol) const override;
 
    void getChemPotentials(double* mu) const override;
 
    void getStandardChemPotentials(double* muStar) const override;
 
    void getPartialMolarEnthalpies(double* hbar) const override;
 
    void getPartialMolarEntropies(double* sbar) const override;
 
    void getPartialMolarIntEnergies(double* ubar) const override;
 
    void getParameters(AnyMap& phaseNode) const override;
 
    void setParameters(const AnyMap& phaseNode,
                       const AnyMap& rootNode=AnyMap()) override;
 
    //! Electron species name
    string electronSpeciesName() const {
        return speciesName(m_electronSpeciesIndex);
    }
 
    //! Return the distribution Number #m_distNum
    int distributionNumber() const {
        return m_distNum;
    }
 
    //! Return the electron energy level Number #m_levelNum
    int levelNumber() const {
        return m_levelNum;
    }
 
    virtual void setSolution(std::weak_ptr<Solution> soln) override;
 
    /**
     * The elastic power loss (J/s/m³)
     *   @f[
     *     P_k = N_A N_A C_e e \sum_k C_k K_k,
     *   @f]
     * where @f$ C_k @f$ and @f$ C_e @f$ are the concentration (kmol/m³) of the
     * target species and electrons, respectively. @f$ K_k @f$ is the elastic
     * electron energy loss coefficient (eV-m³/s).
     */
    double elasticPowerLoss();
 
protected:
    void updateThermo() const override;
 
    //! When electron energy distribution changed, plasma properties such as
    //! electron-collision reaction rates need to be re-evaluated.
    void electronEnergyDistributionChanged();
 
    //! When electron energy level changed, plasma properties such as
    //! electron-collision reaction rates need to be re-evaluate.
    //! In addition, the cross-sections need to be interpolated at
    //! the new level.
    void electronEnergyLevelChanged();
 
    //! Check the electron energy levels
    /*!
     *  The values of electron energy levels need to be positive and
     *  monotonically increasing.
     */
    void checkElectronEnergyLevels() const;
 
    //! Check the electron energy distribution
    /*!
     *  This method check the electron energy distribution for the criteria
     *  below.
     *
     *  1. The values of electron energy distribution cannot be negative.
     *
     *  2. If the last value of electron energy distribution is larger
     *  than 0.01, it will raise a warning to suggest using a higher electron
     *  energy levels.
     */
    void checkElectronEnergyDistribution() const;
 
    //! Update electron energy distribution.
    void updateElectronEnergyDistribution();
 
    //! Set isotropic electron energy distribution
    void setIsotropicElectronEnergyDistribution();
 
    //! Update electron temperature (K) From energy distribution.
    //! #m_electronTemp
    void updateElectronTemperatureFromEnergyDist();
 
    //! Electron energy distribution norm
    void normalizeElectronEnergyDistribution();
 
    //! Update interpolated cross section of a collision
    bool updateInterpolatedCrossSection(size_t k);
 
    //! Update electron energy distribution difference
    void updateElectronEnergyDistDifference();
 
    // Electron energy order in the exponential term
    double m_isotropicShapeFactor = 2.0;
 
    //! Number of points of electron energy levels
    size_t m_nPoints = 1001;
 
    //! electron energy levels [ev]. Length: #m_nPoints
    Eigen::ArrayXd m_electronEnergyLevels;
 
    //! Normalized electron energy distribution vector [-]
    //! Length: #m_nPoints
    Eigen::ArrayXd m_electronEnergyDist;
 
    //! Index of electron species
    size_t m_electronSpeciesIndex = npos;
 
    //! Electron temperature [K]
    double m_electronTemp;
 
    //! Electron energy distribution type
    string m_distributionType = "isotropic";
 
    //! Numerical quadrature method for electron energy distribution
    string m_quadratureMethod = "simpson";
 
    //! Flag of normalizing electron energy distribution
    bool m_do_normalizeElectronEnergyDist = true;
 
    //! Data for initiate reaction
    AnyMap m_root;
 
    //! Electron energy distribution Difference dF/dε (V^-5/2)
    Eigen::ArrayXd m_electronEnergyDistDiff;
 
    //! Elastic electron energy loss coefficients (eV m3/s)
    /*! The elastic electron energy loss coefficient for species k is,
     *   @f[
     *     K_k = \frac{2 m_e}{m_k} \sqrt{\frac{2 e}{m_e}} \int_0^{\infty} \sigma_k
     *           \epsilon^2 \left( F_0 + \frac{k_B T}{e}
     *           \frac{\partial F_0}{\partial \epsilon} \right) d \epsilon,
     *   @f]
     * where @f$ m_e @f$ [kg] is the electron mass, @f$ \epsilon @f$ [V] is the
     * electron energy, @f$ \sigma_k @f$ [m2] is the reaction collision cross section,
     * @f$ F_0 @f$ [V^(-3/2)] is the normalized electron energy distribution function.
     */
    vector<double> m_elasticElectronEnergyLossCoefficients;
 
    //! Updates the elastic electron energy loss coefficient for collision index i
    /*! Calculates the elastic energy loss coefficient using the current electron
        energy distribution and cross sections.
    */
    void updateElasticElectronEnergyLossCoefficient(size_t i);
 
    //! Update elastic electron energy loss coefficients
    /*! Used by elasticPowerLoss() and other plasma property calculations that
        depends on #m_elasticElectronEnergyLossCoefficients. This function calls
        updateInterpolatedCrossSection() before calling
        updateElasticElectronEnergyLossCoefficient()
    */
    void updateElasticElectronEnergyLossCoefficients();
 
private:
    //! Electron energy distribution change variable. Whenever
    //! #m_electronEnergyDist changes, this int is incremented.
    int m_distNum = -1;
 
    //! Electron energy level change variable. Whenever
    //! #m_electronEnergyLevels changes, this int is incremented.
    int m_levelNum = -1;
 
    //! The list of shared pointers of plasma collision reactions
    vector<shared_ptr<Reaction>> m_collisions;
 
    //! The list of shared pointers of collision rates
    vector<shared_ptr<ElectronCollisionPlasmaRate>> m_collisionRates;
 
    //! The collision-target species indices of #m_collisions
    vector<size_t> m_targetSpeciesIndices;
 
    //! Interpolated cross sections. This is used for storing
    //! interpolated cross sections temporarily.
    vector<double> m_interp_cs;
 
    //! The list of whether the interpolated cross sections is ready
    vector<bool> m_interp_cs_ready;
 
    //! Set collisions. This function sets the list of collisions and
    //! the list of target species using #addCollision.
    void setCollisions();
 
    //! Add a collision and record the target species
    void addCollision(std::shared_ptr<Reaction> collision);
 
};
 
}
 
#endif