forked from IPKM/nmreval
merge cfunc -> main
This commit is contained in:
commit
7671a56b6f
@ -36,10 +36,10 @@ AppDir:
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include:
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# for /usr/bin/env
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- coreutils
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- dash
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- zsync
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- hicolor-icon-theme
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# - coreutils
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# - dash
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# - zsync
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# - hicolor-icon-theme
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- libatlas3-base
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- python3.9-minimal
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- python3-numpy
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@ -57,17 +57,24 @@ AppDir:
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- libqt5test5
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- libqt5xml5
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- qtbase5-dev-tools
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- qtchooser
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- pyqt5-dev-tools
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- libavahi-client3
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- libavahi-common-data
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- libavahi-common3
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- libwacom2
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- libwacom-common
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after_bundle: |
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echo "MONSTER SED FOLLOWING...(uncomment if needed for mpl-data)"
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# sed -i s,\'/usr/share/matplotlib/mpl-data\',"f\"\{os.environ.get\('APPDIR'\,'/'\)\}/usr/share/matplotlib/mpl-data\"", ${TARGET_APPDIR}/usr/lib/python3/dist-packages/matplotlib/__init__.py
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files:
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exclude:
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- usr/share/man
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- usr/share/doc/*/README.*
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- usr/share/doc/*/changelog.*
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- usr/share/doc/*/NEWS.*
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- usr/share/doc/*/TODO.}*
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runtime:
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# if needed, apparently replaces hardcoded location with APPDIR location
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# path_mappings:
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# - /usr/share/matplotlib/mpl-data:$APPDIR/usr/share/matplotlib/mpl-data
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version: "continuous"
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env:
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PATH: '${APPDIR}/usr/bin:${PATH}'
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|
22
Makefile
22
Makefile
@ -8,27 +8,33 @@ PYRCC = pyrcc5
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RESOURCE_DIR = src/resources/_ui
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#Directory for compiled resources
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COMPILED_DIR = src/gui_qt/_py
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PYQT_DIR = src/gui_qt/_py
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#UI files to compile, uses every *.ui found in RESOURCE_DIR
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UI_FILES = $(foreach dir, $(RESOURCE_DIR), $(notdir $(wildcard $(dir)/*.ui)))
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COMPILED_UI = $(UI_FILES:%.ui=$(COMPILED_DIR)/%.py)
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PYQT_UI = $(UI_FILES:%.ui=$(PYQT_DIR)/%.py)
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SVG_FILES = $(foreach dir, $(RCC_DIR), $(notdir $(wildcard $(dir)/*.svg)))
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PNG_FILES = $(SVG_FILES:%.svg=$(RCC_DIR)/%.png)
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all : ui
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CC = gcc
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CFLAGS = -O2 -fPIC
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LDFLAGS = -shared
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ui : $(COMPILED_UI)
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C_DIR = src/nmreval/clib
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rcc: $(PNG_FILES)
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all : ui compile
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ui : $(PYQT_UI)
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rcc : $(PNG_FILES)
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# only one C file at the moment
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compile : $(C_DIR)/integrate.c
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$(CC) $(LDFLAGS) $(CFLAGS) -o $(C_DIR)/integrate.so $<
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$(COMPILED_DIR)/%.py : $(RESOURCE_DIR)/%.ui
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$(PYUIC) $< -o $@
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# replace import of ressource to correct path
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# @sed -i s/images_rc/nmrevalqt.$(COMPILED_DIR).images_rc/g $@
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# @sed -i /images_rc/d $@
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$(RCC_DIR)/%.png : $(RCC_DIR)/%.svg
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convert -background none $< $@
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|
158
src/nmreval/clib/integrate.c
Normal file
158
src/nmreval/clib/integrate.c
Normal file
@ -0,0 +1,158 @@
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/* integrands used in quadrature integration with scipy's LowLevelCallables */
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#include <math.h>
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const double KB = 8.617333262145179e-05;
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/* FFHS functions */
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double ffhsSD(double x, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau = c[1];
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double u = x*x;
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double res = u*u * tau;
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res /= 81. + 9.*u - 2.*u*u + u*u*u;
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res /= u*u + omega*omega * tau*tau;
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return res;
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}
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/* log-gaussian functions */
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double logNormalDist(double tau, double tau0, double sigma) {
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return exp(- pow((log(tau/tau0) / sigma), 2) / 2.) / sqrt(2*M_PI)/sigma;
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}
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double logGaussian_imag_high(double u, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau = c[1];
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double sigma = c[2];
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double uu = exp(-u);
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double dist = logNormalDist(1./uu, tau, sigma);
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return dist * omega * uu / (pow(uu, 2) + pow(omega, 2));
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}
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double logGaussian_imag_low(double u, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau = c[1];
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double sigma = c[2];
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double uu = exp(u);
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double dist = logNormalDist(uu, tau, sigma);
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return dist * omega * uu / (1. + pow(omega*uu, 2));
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}
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double logGaussian_real_high(double u, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau = c[1];
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double sigma = c[2];
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double uu = exp(-2.*u);
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double dist = logNormalDist(exp(uu), tau, sigma);
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return dist * uu / (uu + pow(omega, 2));
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}
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double logGaussian_real_low(double u, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau = c[1];
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double sigma = c[2];
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double uu = exp(u);
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double dist = logNormalDist(uu, tau, sigma);
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return dist / (1. + pow(omega*uu, 2));
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}
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double logGaussianCorrelation(double x, void *user_data) {
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double *c = (double *)user_data;
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double t = c[0];
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double tau = c[1];
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double sigma = c[2];
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double uu = exp(x);
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double dist = logNormalDist(uu, tau, sigma);
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return dist * exp(-t/uu);
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}
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// functions for distribution of energy
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double normalDist(double x, double x0, double sigma) {
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return exp(- pow((x-x0) / sigma, 2) / 2.) / sqrt(2 * M_PI) / sigma;
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}
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double rate(double tau0, double ea, double t) {
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return exp(-ea / t / KB) / tau0;
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}
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double energyDist_SD(double x, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau0 = c[1];
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double e_m = c[2];
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double e_b = c[3];
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double temp = c[4];
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double r = rate(tau0, x, temp);
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return r/(pow(r, 2) + pow(omega, 2)) * normalDist(x, e_m, e_b);
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}
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double energyDistSuscReal(double x, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau0 = c[1];
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double e_m = c[2];
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double e_b = c[3];
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double temp = c[4];
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double r = rate(tau0, x, temp);
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return 1 / (pow(r, 2) + pow(omega, 2)) * normalDist(x, e_m, e_b);
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}
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double energyDistSuscImag(double x, void *user_data) {
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double *c = (double *)user_data;
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double omega = c[0];
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double tau0 = c[1];
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double e_m = c[2];
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double e_b = c[3];
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double temp = c[4];
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double r = rate(tau0, x, temp);
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return omega * r / (pow(r, 2) + pow(omega, 2)) * normalDist(x, e_m, e_b);
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}
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double energyDistCorrelation(double x, void *user_data) {
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double *c = (double *)user_data;
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double t = c[0];
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double tau0 = c[1];
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double e_m = c[2];
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double e_b = c[3];
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double temp = c[4];
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double r = rate(tau0, x, temp);
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return normalDist(x, e_m, e_b) * exp(-t * r);
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}
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|
BIN
src/nmreval/clib/integrate.so
Executable file
BIN
src/nmreval/clib/integrate.so
Executable file
Binary file not shown.
@ -29,7 +29,7 @@ class Distribution(abc.ABC):
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@staticmethod
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@abc.abstractmethod
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def susceptibility(omega, tau, *args):
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def susceptibility(omega: ArrayLike, tau: ArrayLike, *args: Any):
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pass
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@classmethod
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|
@ -1,13 +1,18 @@
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from itertools import product
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from ctypes import c_double, cast, pointer, c_void_p
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import numpy as np
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from scipy import LowLevelCallable
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from scipy.integrate import quad, simps as simpson
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from .base import Distribution
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from ..lib.utils import ArrayLike
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from ..utils.constants import kB
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from .helper import HAS_C_FUNCS, lib
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# noinspection PyMethodOverriding
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class EnergyBarriers(Distribution):
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name = 'Energy barriers'
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parameter = [r'\tau_{0}', r'E_{m}', r'\Delta E']
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@ -23,24 +28,30 @@ class EnergyBarriers(Distribution):
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return np.exp(-e_a / (kB * te)) / t0
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@staticmethod
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def energydistribution(e_a, mu, sigma):
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def energy_distribution(e_a, mu, sigma):
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return np.exp(-0.5 * ((mu-e_a) / sigma) ** 2) / (np.sqrt(2 * np.pi) * sigma)
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@staticmethod
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def correlation(t, temperature, *args):
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tau0, e_m, e_b = args
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def integrand(e_a, ti, t0, mu, sigma, te):
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# correlation time would go to inf for higher energies, so we use rate
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return np.exp(-ti*EnergyBarriers.rate(t0, e_a, te)) * EnergyBarriers.energydistribution(e_a, mu, sigma)
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def correlation(t: ArrayLike, temperature: ArrayLike, tau0: float, e_m: float, e_b: float) -> ArrayLike:
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t = np.atleast_1d(t)
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temperature = np.atleast_1d(temperature)
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|
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e_axis = np.linspace(max(0, e_m-50*e_b), e_m+50*e_b, num=5001)
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if HAS_C_FUNCS:
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ret_val = _integrate_c(lib.energyDistCorrelation, t, temperature, tau0, e_m, e_b)
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else:
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ret_val = _integrate_py(_integrand_time, t, temperature, tau0, e_m, e_b)
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ret_val = np.array([simpson(integrand(e_axis, o, tau0, e_m, e_b, tt), e_axis)
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for o in t for tt in temperature])
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return ret_val
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||||
@staticmethod
|
||||
def specdens(omega: ArrayLike, temperature: ArrayLike, tau0: float, e_m: float, e_b: float) -> ArrayLike:
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omega = np.atleast_1d(omega)
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temperature = np.atleast_1d(temperature)
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|
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if HAS_C_FUNCS:
|
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ret_val = _integrate_c(lib.energyDist_SD, omega, temperature, tau0, e_m, e_b)
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||||
else:
|
||||
ret_val = _integrate_py(_integrand_sd, omega, temperature, tau0, e_m, e_b)
|
||||
|
||||
return ret_val
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||||
|
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@ -51,70 +62,73 @@ class EnergyBarriers(Distribution):
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omega = np.atleast_1d(omega)
|
||||
temperature = np.atleast_1d(temperature)
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||||
|
||||
e_axis = np.linspace(max(0, e_m-50*e_b), e_m+50*e_b, num=5001)
|
||||
ret_val = []
|
||||
for o, tt in product(omega, temperature):
|
||||
ret_val.append(simpson(_integrand_freq_real(e_axis, o, tau0, e_m, e_b, tt), e_axis) -
|
||||
1j * simpson(_integrand_freq_imag(e_axis, o, tau0, e_m, e_b, tt), e_axis))
|
||||
|
||||
return np.array(ret_val)
|
||||
|
||||
@staticmethod
|
||||
def specdens(omega, temperature, *args):
|
||||
# in contrast to other spectral densities, it's omega and temperature
|
||||
tau0, e_m, e_b = args
|
||||
|
||||
def integrand(e_a, w, t0, mu, sigma, t):
|
||||
r = EnergyBarriers.rate(t0, e_a, t)
|
||||
return r/(r**2 + w**2) * EnergyBarriers.energydistribution(e_a, mu, sigma)
|
||||
|
||||
omega = np.atleast_1d(omega)
|
||||
temperature = np.atleast_1d(temperature)
|
||||
|
||||
e_axis = np.linspace(max(0, e_m-50*e_b), e_m+50*e_b, num=5001)
|
||||
|
||||
ret_val = np.array([simpson(integrand(e_axis, o, tau0, e_m, e_b, tt), e_axis)
|
||||
for o in omega for tt in temperature])
|
||||
if HAS_C_FUNCS:
|
||||
ret_val = _integrate_c(lib.energyDistSuscReal, omega, temperature, tau0, e_m, e_b) + \
|
||||
1j * _integrate_c(lib.energyDistSuscImag, omega, temperature, tau0, e_m, e_b)
|
||||
else:
|
||||
ret_val = _integrate_py(_integrand_susc_real, omega, temperature, tau0, e_m, e_b) + \
|
||||
1j * _integrate_py(_integrand_susc_imag, omega, temperature, tau0, e_m, e_b)
|
||||
|
||||
return ret_val
|
||||
|
||||
@staticmethod
|
||||
def mean(*args):
|
||||
return args[1]*np.exp(args[2]/(kB*args[0]))
|
||||
def mean(temperature, tau0, ea):
|
||||
return tau0*np.exp(ea/(kB*temperature))
|
||||
|
||||
@staticmethod
|
||||
def logmean(*args):
|
||||
return args[1] + args[2] / (kB * args[0])
|
||||
def logmean(temperature, tau0, ea):
|
||||
return tau0 + ea / (kB * temperature)
|
||||
|
||||
@staticmethod
|
||||
def max(*args):
|
||||
return args[1] * np.exp(args[2] / (kB * args[0]))
|
||||
|
||||
|
||||
def _integrate_process_imag(args):
|
||||
pass
|
||||
# helper functions
|
||||
def _integrate_c(func, omega: np.ndarray, temperature: np.ndarray, tau0: float, e_m: float, e_b: float) -> np.ndarray:
|
||||
res = []
|
||||
for o, t in product(omega, temperature):
|
||||
c = (c_double * 5)(o, tau0, e_m, e_b, t)
|
||||
user_data = cast(pointer(c), c_void_p)
|
||||
area = quad(LowLevelCallable(func, user_data), 0, np.infty, epsabs=1e-13)[0]
|
||||
|
||||
res.append(area)
|
||||
|
||||
ret_val = np.array(res).reshape(omega.shape[0], temperature.shape[0])
|
||||
|
||||
return ret_val.squeeze()
|
||||
|
||||
|
||||
def _integrate_process_real(args):
|
||||
omega_i, t, tau0, mu, sigma, temp_j = args
|
||||
return quad(_integrand_freq_real(), 0, 10, args=(omega_i, t, tau0, mu, sigma, temp_j))[0]
|
||||
def _integrate_py(func, axis, temp, tau0, e_m, e_b):
|
||||
x = np.atleast_1d(axis)
|
||||
temperature = np.atleast_1d(temp)
|
||||
|
||||
e_axis = np.linspace(max(0., e_m - 50*e_b), e_m + 50*e_b, num=5001)
|
||||
ret_val = []
|
||||
for o, tt in product(x, temperature):
|
||||
ret_val.append(simpson(func(e_axis, o, tau0, e_m, e_b, tt), e_axis))
|
||||
|
||||
ret_val = np.array(ret_val).reshape(x.shape[0], temperature.shape[0])
|
||||
|
||||
return ret_val.squeeze()
|
||||
|
||||
|
||||
def _integrate_process_time(args):
|
||||
omega_i, t, tau0, mu, sigma, temp_j = args
|
||||
return quad(_integrand_time, 0, 10, args=(omega_i, t, tau0, mu, sigma, temp_j))[0]
|
||||
|
||||
|
||||
def _integrand_freq_real(u, omega, tau0, mu, sigma, temp):
|
||||
# python integrands
|
||||
def _integrand_sd(u, omega, tau0, mu, sigma, temp):
|
||||
r = EnergyBarriers.rate(tau0, u, temp)
|
||||
return 1 / (r**2 + omega**2) * EnergyBarriers.energydistribution(u, mu, sigma)
|
||||
return r / (r**2 + omega**2) * EnergyBarriers.energy_distribution(u, mu, sigma)
|
||||
|
||||
|
||||
def _integrand_freq_imag(u, omega, tau0, mu, sigma, temp):
|
||||
def _integrand_susc_real(u, omega, tau0, mu, sigma, temp):
|
||||
r = EnergyBarriers.rate(tau0, u, temp)
|
||||
return 1 / (r**2 + omega**2) * EnergyBarriers.energy_distribution(u, mu, sigma)
|
||||
|
||||
|
||||
def _integrand_susc_imag(u, omega, tau0, mu, sigma, temp):
|
||||
rate = EnergyBarriers.rate(tau0, u, temp)
|
||||
return omega * rate / (rate**2 + omega**2) * EnergyBarriers.energydistribution(u, mu, sigma)
|
||||
return omega * rate / (rate**2 + omega**2) * EnergyBarriers.energy_distribution(u, mu, sigma)
|
||||
|
||||
|
||||
def _integrand_time(u, t, tau0, mu, sigma, temp):
|
||||
rate = EnergyBarriers.rate(tau0, u, temp)
|
||||
return EnergyBarriers.energydistribution(u, mu, sigma) * np.exp(-t*rate)
|
||||
return EnergyBarriers.energy_distribution(u, mu, sigma) * np.exp(-t*rate)
|
||||
|
48
src/nmreval/distributions/helper.py
Normal file
48
src/nmreval/distributions/helper.py
Normal file
@ -0,0 +1,48 @@
|
||||
|
||||
from pathlib import Path
|
||||
from ctypes import CDLL, c_double, c_void_p
|
||||
|
||||
from ..lib.logger import logger
|
||||
|
||||
|
||||
lib = None
|
||||
try:
|
||||
lib = CDLL(str(Path(__file__).parents[1] / 'clib' / 'integrate.so'))
|
||||
|
||||
# FFHS integrand
|
||||
lib.ffhsSD.restype = c_double
|
||||
lib.ffhsSD.argtypes = (c_double, c_void_p)
|
||||
|
||||
# Log-Gaussian integrands
|
||||
lib.logGaussian_imag_high.restype = c_double
|
||||
lib.logGaussian_imag_high.argtypes = (c_double, c_void_p)
|
||||
lib.logGaussian_imag_low.restype = c_double
|
||||
lib.logGaussian_imag_low.argtypes = (c_double, c_void_p)
|
||||
|
||||
lib.logGaussian_real_high.restype = c_double
|
||||
lib.logGaussian_real_high.argtypes = (c_double, c_void_p)
|
||||
lib.logGaussian_real_low.restype = c_double
|
||||
lib.logGaussian_real_low.argtypes = (c_double, c_void_p)
|
||||
|
||||
lib.logGaussianCorrelation.restype = c_double
|
||||
lib.logGaussianCorrelation.argtypes = (c_double, c_void_p)
|
||||
|
||||
# integrands for distribution of energies
|
||||
lib.energyDist_SD.restype = c_double
|
||||
lib.energyDist_SD.argtypes = (c_double, c_void_p)
|
||||
|
||||
lib.energyDistCorrelation.restype = c_double
|
||||
lib.energyDistCorrelation.argtypes = (c_double, c_void_p)
|
||||
|
||||
lib.energyDistSuscReal.restype = c_double
|
||||
lib.energyDistSuscReal.argtypes = (c_double, c_void_p)
|
||||
lib.energyDistSuscImag.restype = c_double
|
||||
lib.energyDistSuscImag.argtypes = (c_double, c_void_p)
|
||||
|
||||
|
||||
HAS_C_FUNCS = True
|
||||
logger.info('Use C functions')
|
||||
except OSError:
|
||||
HAS_C_FUNCS = False
|
||||
logger.info('Use python functions')
|
||||
|
@ -1,9 +1,16 @@
|
||||
import ctypes
|
||||
|
||||
import numpy as np
|
||||
from scipy import LowLevelCallable
|
||||
from scipy.integrate import quad
|
||||
|
||||
from .helper import HAS_C_FUNCS, lib
|
||||
from .base import Distribution
|
||||
|
||||
|
||||
# Everything except spectral density is implemented in Python only because the only use case of FFHS is NMR
|
||||
# field cycling measurements with T1 results
|
||||
|
||||
class FFHS(Distribution):
|
||||
name = 'Intermolecular (FFHS)'
|
||||
parameter = None
|
||||
@ -24,7 +31,7 @@ class FFHS(Distribution):
|
||||
return ret_val
|
||||
|
||||
@staticmethod
|
||||
def specdens(omega, tau0, *args):
|
||||
def specdens_py(omega, tau0):
|
||||
def integrand(u, o, tau0):
|
||||
return u**4 * tau0 / (81 + 9*u**2 - 2*u**4 + u**6) / (u**4 + (o*tau0)**2)
|
||||
# return FFHS.distribution(u, tau0) * u / (1+o**2 * u**2)
|
||||
@ -33,6 +40,17 @@ class FFHS(Distribution):
|
||||
|
||||
return ret_val * 54 / np.pi
|
||||
|
||||
@staticmethod
|
||||
def specdens_c(omega, tau0):
|
||||
res = []
|
||||
for o in omega:
|
||||
c = (ctypes.c_double * 2)(o, tau0)
|
||||
user_data = ctypes.cast(ctypes.pointer(c), ctypes.c_void_p)
|
||||
func = LowLevelCallable(lib.ffhsSD, user_data)
|
||||
res.append(quad(func, 0, np.infty)[0])
|
||||
|
||||
return np.array(res) * 54 / np.pi
|
||||
|
||||
@staticmethod
|
||||
def susceptibility(omega, tau0, *args):
|
||||
def integrand_real(u, o, tau0):
|
||||
@ -48,6 +66,9 @@ class FFHS(Distribution):
|
||||
return ret_val
|
||||
|
||||
|
||||
FFHS.specdens = FFHS.specdens_c if HAS_C_FUNCS else FFHS.specdens_py
|
||||
|
||||
|
||||
# class Bessel(Distribution):
|
||||
# name = 'Intermolecular (Bessel)'
|
||||
# parameter = None
|
||||
|
@ -1,7 +1,12 @@
|
||||
import ctypes
|
||||
from multiprocessing import Pool, cpu_count
|
||||
from itertools import product
|
||||
from typing import Callable
|
||||
|
||||
import numpy as np
|
||||
from scipy import LowLevelCallable
|
||||
|
||||
from nmreval.lib.utils import ArrayLike
|
||||
|
||||
try:
|
||||
from scipy.integrate import simpson
|
||||
@ -9,19 +14,21 @@ except ImportError:
|
||||
from scipy.integrate import simps as simpson
|
||||
from scipy.integrate import quad
|
||||
|
||||
from .base import Distribution
|
||||
from nmreval.distributions.helper import HAS_C_FUNCS, lib
|
||||
from nmreval.distributions.base import Distribution
|
||||
|
||||
|
||||
__all__ = ['LogGaussian']
|
||||
|
||||
|
||||
# noinspection PyMethodOverriding
|
||||
class LogGaussian(Distribution):
|
||||
name = 'Log-Gaussian'
|
||||
parameter = [r'\sigma']
|
||||
bounds = [(0, 10)]
|
||||
|
||||
@staticmethod
|
||||
def distribution(tau, tau0, sigma: float):
|
||||
def distribution(tau: ArrayLike, tau0: ArrayLike, sigma: float) -> ArrayLike:
|
||||
return np.exp(-0.5*(np.log(tau/tau0)/sigma)**2)/np.sqrt(2*np.pi)/sigma
|
||||
|
||||
@staticmethod
|
||||
@ -29,54 +36,87 @@ class LogGaussian(Distribution):
|
||||
_t = np.atleast_1d(t)
|
||||
_tau = np.atleast_1d(tau0)
|
||||
|
||||
pool = Pool(processes=min(cpu_count(), 4))
|
||||
integration_ranges = [(omega_i, tau_j, sigma) for (omega_i, tau_j) in product(_t, _tau)]
|
||||
if HAS_C_FUNCS:
|
||||
res = _integrate_correlation_c(_t, _tau, sigma)
|
||||
else:
|
||||
res = _integration_parallel(_t, _tau, sigma, _integrate_process_time)
|
||||
|
||||
with np.errstate(divide='ignore'):
|
||||
res = np.array(pool.map(_integrate_process_time, integration_ranges))
|
||||
ret_val = res.reshape((_t.shape[0], _tau.shape[0]))
|
||||
|
||||
return ret_val.squeeze()
|
||||
return res.squeeze()
|
||||
|
||||
@staticmethod
|
||||
def susceptibility(omega, tau0, sigma: float):
|
||||
_omega = np.atleast_1d(omega)
|
||||
_tau = np.atleast_1d(tau0)
|
||||
|
||||
pool = Pool(processes=min(cpu_count(), 4))
|
||||
integration_ranges = [(omega_i, tau_j, sigma) for (omega_i, tau_j) in product(_omega, _tau)]
|
||||
if HAS_C_FUNCS:
|
||||
res_real = _integrate_susc_real_c(_omega, _tau, sigma)
|
||||
res_imag = _integrate_susc_imag_c(_omega, _tau, sigma)
|
||||
else:
|
||||
res_real = _integration_parallel(_omega, _tau, sigma, _integrate_process_imag)
|
||||
res_imag = _integration_parallel(_omega, _tau, sigma, _integrate_process_real)
|
||||
|
||||
with np.errstate(divide='ignore'):
|
||||
res_real = np.array(pool.map(_integrate_process_imag, integration_ranges))
|
||||
res_imag = np.array(pool.map(_integrate_process_real, integration_ranges))
|
||||
ret_val = (res_real+1j*res_imag).reshape((_omega.shape[0], _tau.shape[0]))
|
||||
|
||||
return ret_val.squeeze()
|
||||
return (res_real + 1j * res_imag).squeeze()
|
||||
|
||||
@staticmethod
|
||||
def specdens(omega, tau0, sigma):
|
||||
def specdens(omega: ArrayLike, tau: ArrayLike, sigma: float) -> np.ndarray:
|
||||
_omega = np.atleast_1d(omega)
|
||||
_tau = np.atleast_1d(tau0)
|
||||
_tau = np.atleast_1d(tau)
|
||||
|
||||
pool = Pool(processes=min(cpu_count(), 4))
|
||||
integration_ranges = [(omega_i, tau_j, sigma) for (omega_i, tau_j) in product(_omega, _tau)]
|
||||
|
||||
with np.errstate(divide='ignore'):
|
||||
res = np.array(pool.map(_integrate_process_imag, integration_ranges))
|
||||
ret_val = res.reshape((_omega.shape[0], _tau.shape[0]))
|
||||
if HAS_C_FUNCS:
|
||||
ret_val = _integrate_susc_imag_c(_omega, _tau, sigma)
|
||||
else:
|
||||
ret_val = _integration_parallel(_omega, _tau, sigma, _integrate_process_imag)
|
||||
|
||||
ret_val /= _omega[:, None]
|
||||
|
||||
return ret_val.squeeze()
|
||||
|
||||
def mean(*args):
|
||||
return args[0]*np.exp(args[1]**2 / 2)
|
||||
@staticmethod
|
||||
def mean(tau, sigma):
|
||||
return tau*np.exp(sigma**2 / 2)
|
||||
|
||||
|
||||
def _integration_parallel(x: np.ndarray, tau: np.ndarray, sigma: float, func: Callable) -> np.ndarray:
|
||||
pool = Pool(processes=min(cpu_count(), 4))
|
||||
integration_ranges = [(x_i, tau_j, sigma) for (x_i, tau_j) in product(x, tau)]
|
||||
|
||||
with np.errstate(divide='ignore'):
|
||||
res = pool.map(func, integration_ranges)
|
||||
|
||||
res = np.array(res).reshape((x.shape[0], tau.shape[0]))
|
||||
|
||||
return res
|
||||
|
||||
|
||||
def _integrate_susc_imag_c(omega: np.ndarray, tau: np.ndarray, sigma: float) -> np.ndarray:
|
||||
return _integrate_susc_c(lib.logGaussian_imag_low, lib.logGaussian_imag_high, omega, tau, sigma)
|
||||
|
||||
|
||||
def _integrate_susc_real_c(omega: np.ndarray, tau: np.ndarray, sigma: float) -> np.ndarray:
|
||||
return _integrate_susc_c(lib.logGaussian_real_low, lib.logGaussian_real_high, omega, tau, sigma)
|
||||
|
||||
|
||||
def _integrate_susc_c(lowfunc, highfunc, omega, tau, sigma):
|
||||
res = []
|
||||
|
||||
for o, t in product(omega, tau):
|
||||
c = (ctypes.c_double * 3)(o, t, sigma)
|
||||
user_data = ctypes.cast(ctypes.pointer(c), ctypes.c_void_p)
|
||||
|
||||
area = quad(LowLevelCallable(highfunc, user_data), 0, np.infty, epsabs=1e-12, epsrel=1e-12)[0]
|
||||
area += quad(LowLevelCallable(lowfunc, user_data), -np.infty, 0, epsabs=1e-12, epsrel=1e-12)[0]
|
||||
|
||||
res.append(area)
|
||||
|
||||
res = np.asanyarray(res).reshape((omega.shape[0], tau.shape[0]))
|
||||
|
||||
return res
|
||||
|
||||
|
||||
def _integrate_process_imag(args):
|
||||
omega_i, tau_j, sigma = args
|
||||
area = quad(_integrand_freq_imag_high, 0, 50, args=(omega_i, tau_j, sigma))[0]
|
||||
area += quad(_integrand_freq_imag_low, -50, 0, args=(omega_i, tau_j, sigma))[0]
|
||||
area = quad(_integrand_freq_imag_high, 0, 50, args=(omega_i, tau_j, sigma), epsabs=1e-12, epsrel=1e-12)[0]
|
||||
area += quad(_integrand_freq_imag_low, -50, 0, args=(omega_i, tau_j, sigma), epsabs=1e-12, epsrel=1e-12)[0]
|
||||
|
||||
return area
|
||||
|
||||
@ -89,9 +129,25 @@ def _integrate_process_real(args):
|
||||
return area
|
||||
|
||||
|
||||
def _integrate_correlation_c(t, tau, sigma):
|
||||
res = []
|
||||
|
||||
for t_i, tau_i in product(t, tau):
|
||||
c = (ctypes.c_double * 3)(t_i, tau_i, sigma)
|
||||
user_data = ctypes.cast(ctypes.pointer(c), ctypes.c_void_p)
|
||||
|
||||
area = quad(LowLevelCallable(lib.logGaussianCorrelation, user_data), -np.infty, np.infty)[0]
|
||||
|
||||
res.append(area)
|
||||
|
||||
res = np.asanyarray(res).reshape((t.shape[0], tau.shape[0]))
|
||||
|
||||
return res
|
||||
|
||||
|
||||
def _integrate_process_time(args):
|
||||
omega_i, tau_j, sigma = args
|
||||
return quad(_integrand_time, -50, 50, args=(omega_i, tau_j, sigma))[0]
|
||||
return quad(_integrand_time, -50, 50, args=(omega_i, tau_j, sigma), epsabs=1e-12, epsrel=1e-12)[0]
|
||||
|
||||
|
||||
def _integrand_time(u, t, tau, sigma):
|
||||
|
@ -1,4 +1,3 @@
|
||||
import time
|
||||
import warnings
|
||||
from itertools import product
|
||||
|
||||
|
@ -9,11 +9,14 @@ import _compat_pickle
|
||||
|
||||
from pickle import *
|
||||
from pickle import _Unframer, bytes_types, _Stop, _getattribute
|
||||
|
||||
from nmreval.lib.logger import logger
|
||||
|
||||
try:
|
||||
import bsddb3
|
||||
HAS_BSDDB3 = True
|
||||
except ImportError:
|
||||
warnings.warn('bsdbb3 is not installed, reading legacy .nmr files is not possible.')
|
||||
logger.warn('bsdbb3 is not installed, reading legacy .nmr files is not possible.')
|
||||
HAS_BSDDB3 = False
|
||||
|
||||
|
||||
|
@ -86,7 +86,7 @@ class EnergyFC(_AbstractFC):
|
||||
name = 'Energy distribution'
|
||||
params = ['C', 'T'] + EnergyBarriers.parameter
|
||||
bounds = [(0, None), (0, None), (0, None), (0, None)]
|
||||
ralax = Relaxation(distribution=EnergyBarriers)
|
||||
relax = Relaxation(distribution=EnergyBarriers)
|
||||
|
||||
|
||||
class _AbstractFCDipolar(_AbstractFC):
|
||||
|
@ -14,7 +14,7 @@ from collections import OrderedDict
|
||||
from ..utils.constants import gamma_full, hbar_joule, pi, gamma, mu0
|
||||
|
||||
|
||||
__all__ = ['Quadrupolar', 'Czjzek', 'HeteroDipolar',
|
||||
__all__ = ['Coupling', 'Quadrupolar', 'Czjzek', 'HeteroDipolar',
|
||||
'HomoDipolar', 'Constant', 'CSA']
|
||||
|
||||
|
||||
|
Loading…
Reference in New Issue
Block a user