Source code for openmc.deplete.cram

"""Chebyshev Rational Approximation Method module

Implements two different forms of CRAM for use in openmc.deplete.
"""

from functools import partial
import numbers

import numpy as np
from scipy.sparse.linalg import spsolve, splu

from openmc.checkvalue import check_type, check_length, check_greater_than
from .abc import DepSystemSolver
from .._sparse_compat import csc_array, eye_array

__all__ = ["CRAM16", "CRAM48", "Cram16Solver", "Cram48Solver", "IPFCramSolver"]


[docs] class IPFCramSolver(DepSystemSolver): r"""CRAM depletion solver that uses incomplete partial factorization Provides a :meth:`__call__` that utilizes an incomplete partial factorization (IPF) for the Chebyshev Rational Approximation Method (CRAM), as described in the following paper: M. Pusa, "`Higher-Order Chebyshev Rational Approximation Method and Application to Burnup Equations <https://doi.org/10.13182/NSE15-26>`_," Nucl. Sci. Eng., 182:3, 297-318. When `substeps` > 1, the time interval is split into `substeps` identical sub-intervals and LU factorizations are reused across them, as described in: A. Isotalo and M. Pusa, "`Improving the Accuracy of the Chebyshev Rational Approximation Method Using Substeps <https://doi.org/10.13182/NSE15-67>`_," Nucl. Sci. Eng., 183:1, 65-77. Parameters ---------- alpha : numpy.ndarray Complex residues of poles used in the factorization. Must be a vector with even number of items. theta : numpy.ndarray Complex poles. Must have an equal size as ``alpha``. alpha0 : float Limit of the approximation at infinity Attributes ---------- alpha : numpy.ndarray Complex residues of poles :attr:`theta` in the incomplete partial factorization. Denoted as :math:`\tilde{\alpha}` theta : numpy.ndarray Complex poles :math:`\theta` of the rational approximation alpha0 : float Limit of the approximation at infinity """ def __init__(self, alpha, theta, alpha0): check_type("alpha", alpha, np.ndarray, numbers.Complex) check_type("theta", theta, np.ndarray, numbers.Complex) check_length("theta", theta, alpha.size) check_type("alpha0", alpha0, numbers.Real) self.alpha = alpha self.theta = theta self.alpha0 = alpha0
[docs] def __call__(self, A, n0, dt, substeps=1): """Solve depletion equations using IPF CRAM Parameters ---------- A : scipy.sparse.csc_array Sparse transmutation matrix ``A[j, i]`` desribing rates at which isotope ``i`` transmutes to isotope ``j`` n0 : numpy.ndarray Initial compositions, typically given in number of atoms in some material or an atom density dt : float Time [s] of the specific interval to be solved substeps : int, optional Number of substeps per depletion interval. Returns ------- numpy.ndarray Final compositions after ``dt`` """ check_type("substeps", substeps, numbers.Integral) check_greater_than("substeps", substeps, 0) step_dt = dt if substeps == 1 else dt / substeps A = step_dt * csc_array(A, dtype=np.float64) ident = eye_array(A.shape[0], format='csc') if substeps == 1: solvers = [partial(spsolve, A - theta * ident) for theta in self.theta] else: # Pre-compute LU factorizations and reuse them across substeps. solvers = [splu(A - theta * ident).solve for theta in self.theta] y = n0.copy() for _ in range(substeps): for alpha, solve in zip(self.alpha, solvers): y += 2 * np.real(alpha * solve(y)) y *= self.alpha0 return y
# Coefficients for IPF Cram 16 c16_alpha = np.array([ +5.464930576870210e+3 - 3.797983575308356e+4j, +9.045112476907548e+1 - 1.115537522430261e+3j, +2.344818070467641e+2 - 4.228020157070496e+2j, +9.453304067358312e+1 - 2.951294291446048e+2j, +7.283792954673409e+2 - 1.205646080220011e+5j, +3.648229059594851e+1 - 1.155509621409682e+2j, +2.547321630156819e+1 - 2.639500283021502e+1j, +2.394538338734709e+1 - 5.650522971778156e+0j], dtype=np.complex128) c16_theta = np.array([ +3.509103608414918 + 8.436198985884374j, +5.948152268951177 + 3.587457362018322j, -5.264971343442647 + 16.22022147316793j, +1.419375897185666 + 10.92536348449672j, +6.416177699099435 + 1.194122393370139j, +4.993174737717997 + 5.996881713603942j, -1.413928462488886 + 13.49772569889275j, -10.84391707869699 + 19.27744616718165j], dtype=np.complex128) c16_alpha0 = 2.124853710495224e-16 Cram16Solver = IPFCramSolver(c16_alpha, c16_theta, c16_alpha0) CRAM16 = Cram16Solver.__call__ del c16_alpha, c16_alpha0, c16_theta # Coefficients for 48th order IPF Cram theta_r = np.array([ -4.465731934165702e+1, -5.284616241568964e+0, -8.867715667624458e+0, +3.493013124279215e+0, +1.564102508858634e+1, +1.742097597385893e+1, -2.834466755180654e+1, +1.661569367939544e+1, +8.011836167974721e+0, -2.056267541998229e+0, +1.449208170441839e+1, +1.853807176907916e+1, +9.932562704505182e+0, -2.244223871767187e+1, +8.590014121680897e-1, -1.286192925744479e+1, +1.164596909542055e+1, +1.806076684783089e+1, +5.870672154659249e+0, -3.542938819659747e+1, +1.901323489060250e+1, +1.885508331552577e+1, -1.734689708174982e+1, +1.316284237125190e+1]) theta_i = np.array([ +6.233225190695437e+1, +4.057499381311059e+1, +4.325515754166724e+1, +3.281615453173585e+1, +1.558061616372237e+1, +1.076629305714420e+1, +5.492841024648724e+1, +1.316994930024688e+1, +2.780232111309410e+1, +3.794824788914354e+1, +1.799988210051809e+1, +5.974332563100539e+0, +2.532823409972962e+1, +5.179633600312162e+1, +3.536456194294350e+1, +4.600304902833652e+1, +2.287153304140217e+1, +8.368200580099821e+0, +3.029700159040121e+1, +5.834381701800013e+1, +1.194282058271408e+0, +3.583428564427879e+0, +4.883941101108207e+1, +2.042951874827759e+1]) c48_theta = np.array(theta_r + theta_i * 1j, dtype=np.complex128) alpha_r = np.array([ +6.387380733878774e+2, +1.909896179065730e+2, +4.236195226571914e+2, +4.645770595258726e+2, +7.765163276752433e+2, +1.907115136768522e+3, +2.909892685603256e+3, +1.944772206620450e+2, +1.382799786972332e+5, +5.628442079602433e+3, +2.151681283794220e+2, +1.324720240514420e+3, +1.617548476343347e+4, +1.112729040439685e+2, +1.074624783191125e+2, +8.835727765158191e+1, +9.354078136054179e+1, +9.418142823531573e+1, +1.040012390717851e+2, +6.861882624343235e+1, +8.766654491283722e+1, +1.056007619389650e+2, +7.738987569039419e+1, +1.041366366475571e+2]) alpha_i = np.array([ -6.743912502859256e+2, -3.973203432721332e+2, -2.041233768918671e+3, -1.652917287299683e+3, -1.783617639907328e+4, -5.887068595142284e+4, -9.953255345514560e+3, -1.427131226068449e+3, -3.256885197214938e+6, -2.924284515884309e+4, -1.121774011188224e+3, -6.370088443140973e+4, -1.008798413156542e+6, -8.837109731680418e+1, -1.457246116408180e+2, -6.388286188419360e+1, -2.195424319460237e+2, -6.719055740098035e+2, -1.693747595553868e+2, -1.177598523430493e+1, -4.596464999363902e+3, -1.738294585524067e+3, -4.311715386228984e+1, -2.777743732451969e+2]) c48_alpha = np.array(alpha_r + alpha_i * 1j, dtype=np.complex128) c48_alpha0 = 2.258038182743983e-47 Cram48Solver = IPFCramSolver(c48_alpha, c48_theta, c48_alpha0) del c48_alpha, c48_alpha0, c48_theta, alpha_r, alpha_i, theta_r, theta_i CRAM48 = Cram48Solver.__call__