Source code for burnman.eos.reciprocal_kprime

from __future__ import absolute_import

# This file is part of BurnMan - a thermoelastic and thermodynamic toolkit for the Earth and Planetary Sciences
# Copyright (C) 2012 - 2017 by the BurnMan team, released under the GNU
# GPL v2 or later.


import scipy.optimize as opt
from scipy.special import gamma, gammainc
from . import equation_of_state as eos
from ..utils.math import bracket
import warnings
import numpy as np

# Try to import the jit from numba.  If it is
# not available, just go with the standard
# python interpreter
try:
    from numba import jit
except ImportError:

    def jit(fn):
        return fn


@jit(nopython=True)
def _delta_PoverK_from_P(PoverK, pressure, K_0, Kprime_0, Kprime_inf):
    return PoverK - (pressure / K_0) * np.power(
        (1.0 - Kprime_inf * PoverK), Kprime_0 / Kprime_inf
    )  # eq. 58


@jit(nopython=True)
def _delta_PoverK_from_V(PoverK, V, V_0, K_0, Kprime_0, Kprime_inf):
    Kprime_ratio = Kprime_0 / Kprime_inf
    return (
        np.log(V_0 / V)
        + Kprime_ratio / Kprime_inf * np.log(1.0 - Kprime_inf * PoverK)
        + (Kprime_ratio - 1.0) * PoverK
    )  # eq. 61


def _upper_incomplete_gamma(z, a):
    """
    An implementation of the non-regularised upper incomplete gamma
    function. Computed using the relationship with the regularised
    lower incomplete gamma function (scipy.special.gammainc).
    Uses the recurrence relation wherever z<0.
    """
    n = int(-np.floor(z))
    if n > 0:
        z = z + n
        u_gamma = (1.0 - gammainc(z, a)) * gamma(z)

        for i in range(n):
            z = z - 1.0
            u_gamma = (u_gamma - np.power(a, z) * np.exp(-a)) / z
        return u_gamma
    else:
        return (1.0 - gammainc(z, a)) * gamma(z)


def _PoverK_from_P(pressure, params):
    """
    Calculates the pressure:bulk modulus ratio
    from a given pressure using brentq optimization
    """
    args = (
        (pressure - params["P_0"]),
        params["K_0"],
        params["Kprime_0"],
        params["Kprime_inf"],
    )
    return opt.brentq(
        _delta_PoverK_from_P,
        1.0 / (params["Kprime_inf"] - params["Kprime_0"]) + np.finfo(float).eps,
        1.0 / params["Kprime_inf"] - np.finfo(float).eps,
        args=args,
    )


def _PoverK_from_V(volume, params):
    """
    Calculates the pressure:bulk modulus ratio
    from a given volume using brentq optimization
    """
    args = (
        volume,
        params["V_0"],
        params["K_0"],
        params["Kprime_0"],
        params["Kprime_inf"],
    )
    return opt.brentq(
        _delta_PoverK_from_V,
        1.0 / (params["Kprime_inf"] - params["Kprime_0"]) + np.finfo(float).eps,
        1.0 / params["Kprime_inf"] - np.finfo(float).eps,
        args=args,
    )


def bulk_modulus(pressure, params):
    """
    Returns the bulk modulus at a given pressure
    """
    PoverK = _PoverK_from_P(pressure, params)
    K = params["K_0"] * np.power(
        (1.0 - params["Kprime_inf"] * PoverK),
        -params["Kprime_0"] / params["Kprime_inf"],
    )
    return K


def shear_modulus(pressure, params):
    """
    Returns the shear modulus at a given pressure
    """
    G = (
        params["G_0"] / params["K_0"] * bulk_modulus(pressure, params)
        - (params["G_0"] / params["K_0"] * params["Kprime_inf"] - params["Gprime_inf"])
        * pressure
    )
    return G  # eq. 78


[docs]class RKprime(eos.EquationOfState): """ Class for the isothermal reciprocal K-prime equation of state detailed in :cite:`StaceyDavis2004`. This equation of state is a development of work by :cite:`Keane1954` and :cite:`Stacey2000`, making use of the fact that :math:`K'` typically varies smoothly as a function of :math:`P/K`, and is thermodynamically required to exceed 5/3 at infinite pressure. It is worth noting that this equation of state rapidly becomes unstable at negative pressures, so should not be trusted to provide a good *HT-LP* equation of state using a thermal pressure formulation. The negative root of :math:`dP/dK` can be found at :math:`K/P = K'_{\infty} - K'_0`, which corresponds to a bulk modulus of :math:`K = K_0 ( 1 - K'_{\infty}/K'_0 )^{K'_0/K'_{\infty}}` and a volume of :math:`V = V_0 ( K'_0 / (K'_0 - K'_{\infty}) )^{K'_0/{K'}^2_{\infty}} \exp{(-1/K'_{\infty})}`. This equation of state has no temperature dependence. """
[docs] def volume(self, pressure, temperature, params): """ Returns volume :math:`[m^3]` as a function of pressure :math:`[Pa]`. """ Kprime_ratio = params["Kprime_0"] / params["Kprime_inf"] PoverK = _PoverK_from_P(pressure, params) V = params["V_0"] * np.exp( Kprime_ratio / params["Kprime_inf"] * np.log(1.0 - params["Kprime_inf"] * PoverK) + (Kprime_ratio - 1.0) * PoverK ) # Eq. 61 return V
[docs] def pressure(self, temperature, volume, params): """ Returns pressure :math:`[Pa]` as a function of volume :math:`[m^3]`. """ PoverK = _PoverK_from_V(volume, params) return params["P_0"] + ( params["K_0"] * PoverK * np.power( 1.0 - params["Kprime_inf"] * PoverK, -params["Kprime_0"] / params["Kprime_inf"], ) )
[docs] def isothermal_bulk_modulus(self, pressure, temperature, volume, params): """ Returns isothermal bulk modulus :math:`K_T` :math:`[Pa]` as a function of pressure :math:`[Pa]`, temperature :math:`[K]` and volume :math:`[m^3]`. """ return bulk_modulus(pressure, params)
[docs] def adiabatic_bulk_modulus(self, pressure, temperature, volume, params): """ Returns adiabatic bulk modulus :math:`K_s` of the mineral. :math:`[Pa]`. """ return bulk_modulus(pressure, params)
[docs] def shear_modulus(self, pressure, temperature, volume, params): """ Returns shear modulus :math:`G` of the mineral. :math:`[Pa]` """ return shear_modulus(pressure, params)
[docs] def entropy(self, pressure, temperature, volume, params): """ Returns the molar entropy :math:`\mathcal{S}` of the mineral. :math:`[J/K/mol]` """ return 0.0
def _intVdP(self, xi, params): a = params["Kprime_inf"] b = ( params["Kprime_0"] / params["Kprime_inf"] / params["Kprime_inf"] - params["Kprime_0"] / params["Kprime_inf"] - 1.0 ) c = params["Kprime_0"] - params["Kprime_inf"] f = params["Kprime_0"] / params["Kprime_inf"] - 1.0 i1 = float( params["V_0"] * params["K_0"] * np.exp(f / a) * np.power(a, b - 1.0) / np.power(f, b + 2.0) * ( f * params["Kprime_0"] * _upper_incomplete_gamma(b + 1.0, f * (1.0 / a - xi)) - a * c * _upper_incomplete_gamma(b + 2.0, f * (1.0 / a - xi)) ) ) return i1
[docs] def gibbs_free_energy(self, pressure, temperature, volume, params): """ Returns the Gibbs free energy :math:`\mathcal{G}` of the mineral. :math:`[J/mol]` """ # G = E0 + int VdP (when S = 0) K = self.isothermal_bulk_modulus(pressure, temperature, volume, params) return ( params["E_0"] + params["P_0"] * params["V_0"] + self._intVdP((pressure - params["P_0"]) / K, params) - self._intVdP(0.0, params) )
[docs] def molar_internal_energy(self, pressure, temperature, volume, params): """ Returns the internal energy :math:`\mathcal{E}` of the mineral. :math:`[J/mol]` """ # E = G - PV (+ TS) return ( self.gibbs_free_energy(pressure, temperature, volume, params) - pressure * volume )
[docs] def molar_heat_capacity_v(self, pressure, temperature, volume, params): """ Since this equation of state does not contain temperature effects, simply return a very large number. :math:`[J/K/mol]` """ return 1.0e99
[docs] def molar_heat_capacity_p(self, pressure, temperature, volume, params): """ Since this equation of state does not contain temperature effects, simply return a very large number. :math:`[J/K/mol]` """ return 1.0e99
[docs] def thermal_expansivity(self, pressure, temperature, volume, params): """ Since this equation of state does not contain temperature effects, simply return zero. :math:`[1/K]` """ return 0.0
[docs] def grueneisen_parameter(self, pressure, temperature, volume, params): """ Since this equation of state does not contain temperature effects, simply return zero. :math:`[unitless]` """ return 0.0
[docs] def validate_parameters(self, params): """ Check for existence and validity of the parameters. The value for :math:`K'_{\infty}` is thermodynamically bounded between 5/3 and :math:`K'_0` :cite:`StaceyDavis2004`. """ if "E_0" not in params: params["E_0"] = 0.0 if "P_0" not in params: params["P_0"] = 0.0 # If G and Gprime_inf are not included this is presumably deliberate, # as we can model density and bulk modulus just fine without them, # so just add them to the dictionary as nans if "G_0" not in params: params["G_0"] = float("nan") if "Gprime_inf" not in params: params["Gprime_inf"] = float("nan") # Check that all the required keys are in the dictionary expected_keys = ["V_0", "K_0", "Kprime_0", "Kprime_inf", "G_0", "Gprime_inf"] for k in expected_keys: if k not in params: raise KeyError("params object missing parameter : " + k) # Finally, check that the values are reasonable. if params["P_0"] < 0.0: warnings.warn("Unusual value for P_0", stacklevel=2) if params["V_0"] < 1.0e-7 or params["V_0"] > 1.0e-3: warnings.warn("Unusual value for V_0", stacklevel=2) if params["K_0"] < 1.0e9 or params["K_0"] > 1.0e13: warnings.warn("Unusual value for K_0", stacklevel=2) if params["Kprime_0"] < 0.0 or params["Kprime_0"] > 10.0: warnings.warn("Unusual value for Kprime_0", stacklevel=2) if ( params["Kprime_inf"] < 5.0 / 3.0 or params["Kprime_inf"] > params["Kprime_0"] ): warnings.warn("Unusual value for Kprime_inf", stacklevel=2) # eq. 17 if params["G_0"] < 0.0 or params["G_0"] > 1.0e13: warnings.warn("Unusual value for G_0", stacklevel=2) if params["Gprime_inf"] < -5.0 or params["Gprime_inf"] > 10.0: warnings.warn("Unusual value for Gprime_inf", stacklevel=2)