dcTMD via Work

Introduction¶

One way to analyze nonequilibrium force time traces from constraint pulling simulations is by calculating the work first and then estimating the free energy $\Delta G$, via:

$$ \begin{align} \Delta G(s) &= \left< W(s) \right>_\text{N} -\frac{\beta}{2}\left<\delta W(s)^2\right>_\text{N} \\ &= \left<W(s)\right>_\text{N} - W_{diss}(s) \end{align} $$

with $\delta W(s) = W(s) -\left< W(s) \right>_\text{N}$. The expression is true if the work distribution is Gaussian. This allows to formulate the friction estimate:

$$\Gamma = \frac{1}{v_c}\frac{d~W_{diss}(s)}{ds}$$

This appraoch is implemented in the WorkEstimator class and computaionally more efficient than calculating the force autocorrelation function (which is implemented in the ForceEstimator class), because the class works with the work data via the integration of the force timetraces. This allows to reduce the resolution significantly while getting the same reults.

Therefore, we advide to use this approach for large datasets.

Workflow:¶

0. load packages and define variables¶

In [11]:

# load packages
import numpy as np
import dcTMD
from dcTMD.storing import WorkSet
from dcTMD.dcTMD import WorkEstimator

# load packages import numpy as np import dcTMD from dcTMD.storing import WorkSet from dcTMD.dcTMD import WorkEstimator

In [12]:

# define variables
velocity = 0.001
res = 1
verbose = True
temperature = 300

# define variables velocity = 0.001 res = 1 verbose = True temperature = 300

I. create a work set¶

To calculate free energy and friction estimates a workset is needed. It contains the integrated force time traces.

1. an array containing the filenames is generated. This can be done via the function dcTMD.io.load_pullf() which takes either a glob pattern or a file containing the pullf file names as argument.

In [13]:

pullf_files = '../../tests/testdata/pullf_filenames.dat'
pullf_files = '../../tests/testdata/*pullf.xvg'
filenames = dcTMD.io.load_pullf(pullf_files)

filenames

pullf_files = '../../tests/testdata/pullf_filenames.dat' pullf_files = '../../tests/testdata/*pullf.xvg' filenames = dcTMD.io.load_pullf(pullf_files) filenames

file ../../tests/testdata/*pullf.xvg not found. using glob.glob(../../tests/testdata/*pullf.xvg)

Out[13]:

['../../tests/testdata/t_middle_32_pullf.xvg',
 '../../tests/testdata/t_middle_03_pullf.xvg',
 '../../tests/testdata/t_middle_34_pullf.xvg',
 '../../tests/testdata/t_middle_24_pullf.xvg',
 '../../tests/testdata/t_middle_21_pullf.xvg',
 '../../tests/testdata/t_middle_04_pullf.xvg',
 '../../tests/testdata/t_middle_29_pullf.xvg',
 '../../tests/testdata/t_middle_16_pullf.xvg',
 '../../tests/testdata/t_middle_30_pullf.xvg',
 '../../tests/testdata/t_middle_19_pullf.xvg',
 '../../tests/testdata/t_middle_01_pullf.xvg',
 '../../tests/testdata/t_middle_28_pullf.xvg',
 '../../tests/testdata/t_middle_26_pullf.xvg',
 '../../tests/testdata/t_middle_31_pullf.xvg',
 '../../tests/testdata/t_middle_09_pullf.xvg',
 '../../tests/testdata/t_middle_17_pullf.xvg',
 '../../tests/testdata/t_middle_25_pullf.xvg',
 '../../tests/testdata/t_middle_05_pullf.xvg']

2. the workset is created by creating a WorkSet instance which is fitted with the filenames.

The resolution parameter controls the striding of the data set. The reduction is performed after integration the force time traces. For long trajectories e.g. 35,000,000 frames it is advisory to use a resolution > 1000 to not exceed your hardware.

In [14]:

# create WorkSet instance
workset = WorkSet(velocity=velocity,
                  resolution=res,
                  verbose=False,
                  )
workset

# create WorkSet instance workset = WorkSet(velocity=velocity, resolution=res, verbose=False, ) workset

Out[14]:

WorkSet(velocity=0.001)

In a Jupyter environment, please rerun this cell to show the HTML representation or trust the notebook.
On GitHub, the HTML representation is unable to render, please try loading this page with nbviewer.org.

In [15]:

# fit/fill workset
workset.fit(filenames)
# save workset
#dcTMD.storing.save('my_workset', workset)

# fit/fill workset workset.fit(filenames) # save workset #dcTMD.storing.save('my_workset', workset)

Loading & integrating force files: 100%|██████████| 18/18 [00:00<00:00, 99.35it/s]

Out[15]:

WorkSet(velocity=0.001)

In a Jupyter environment, please rerun this cell to show the HTML representation or trust the notebook.
On GitHub, the HTML representation is unable to render, please try loading this page with nbviewer.org.

In [16]:

print(vars(workset))

print(vars(workset))

{'velocity': 0.001, 'resolution': 1, 'verbose': False, 'X': ['../../tests/testdata/t_middle_32_pullf.xvg', '../../tests/testdata/t_middle_03_pullf.xvg', '../../tests/testdata/t_middle_34_pullf.xvg', '../../tests/testdata/t_middle_24_pullf.xvg', '../../tests/testdata/t_middle_21_pullf.xvg', '../../tests/testdata/t_middle_04_pullf.xvg', '../../tests/testdata/t_middle_29_pullf.xvg', '../../tests/testdata/t_middle_16_pullf.xvg', '../../tests/testdata/t_middle_30_pullf.xvg', '../../tests/testdata/t_middle_19_pullf.xvg', '../../tests/testdata/t_middle_01_pullf.xvg', '../../tests/testdata/t_middle_28_pullf.xvg', '../../tests/testdata/t_middle_26_pullf.xvg', '../../tests/testdata/t_middle_31_pullf.xvg', '../../tests/testdata/t_middle_09_pullf.xvg', '../../tests/testdata/t_middle_17_pullf.xvg', '../../tests/testdata/t_middle_25_pullf.xvg', '../../tests/testdata/t_middle_05_pullf.xvg'], 'time_': array([0.0000e+00, 1.0000e-01, 2.0000e-01, ..., 1.9998e+03, 1.9999e+03,
       2.0000e+03], shape=(20001,)), 'work_': array([[ 0.00000000e+00,  1.03698915e-01,  1.24836915e-01, ...,
         8.45118712e+01,  8.44347098e+01,  8.44165457e+01],
       [ 0.00000000e+00, -1.00744350e-01, -2.14093600e-01, ...,
         1.15331409e+02,  1.15265871e+02,  1.15229601e+02],
       [ 0.00000000e+00,  6.30896000e-02,  5.76634000e-02, ...,
         5.74830869e+01,  5.75868897e+01,  5.74908294e+01],
       ...,
       [ 0.00000000e+00, -8.02650000e-03,  1.56785000e-01, ...,
         5.20392642e+01,  5.21592937e+01,  5.21718456e+01],
       [ 0.00000000e+00,  1.79783900e-01,  3.88872900e-01, ...,
         8.74668694e+01,  8.72953927e+01,  8.72269519e+01],
       [ 0.00000000e+00,  2.15985500e-02, -4.17557500e-02, ...,
         9.99542344e+01,  9.98090948e+01,  9.98238686e+01]],
      shape=(18, 20001)), 'names_': array(['t_middle_32_pullf.xvg', 't_middle_03_pullf.xvg',
       't_middle_34_pullf.xvg', 't_middle_24_pullf.xvg',
       't_middle_21_pullf.xvg', 't_middle_04_pullf.xvg',
       't_middle_29_pullf.xvg', 't_middle_16_pullf.xvg',
       't_middle_30_pullf.xvg', 't_middle_19_pullf.xvg',
       't_middle_01_pullf.xvg', 't_middle_28_pullf.xvg',
       't_middle_26_pullf.xvg', 't_middle_31_pullf.xvg',
       't_middle_09_pullf.xvg', 't_middle_17_pullf.xvg',
       't_middle_25_pullf.xvg', 't_middle_05_pullf.xvg'], dtype='<U32'), 'position_': array([0.0000e+00, 1.0000e-04, 2.0000e-04, ..., 1.9998e+00, 1.9999e+00,
       2.0000e+00], shape=(20001,))}

II. check normality of work distribution¶

One of the main conditions which need to be fulfilled for dcTMD is a normally distributed work.

This can be checked via different methods. e.g. plotting the work time traces, normality checks at different x positions, Kolmogorov-Smirnov Test, Shapiro-Wilk Test, Anderson-Darling Test,

CAUTION: if the work distribution is not normal you results are compromised. And a path separation is necessary. For the theory on path separation see...

In [17]:

# plot workset
import matplotlib.pyplot as plt
from dcTMD.utils import plotting

fig, ax = plt.subplots()
plotting.plot_worklines(workset, ax)
plt.show()

# plot workset import matplotlib.pyplot as plt from dcTMD.utils import plotting fig, ax = plt.subplots() plotting.plot_worklines(workset, ax) plt.show()

In [18]:

from scipy.stats import probplot

def plot_worknormalitychecks(
    workset,
    index,
    x=None,
    worklinecolor='#777',
    colors=None,
    figsize=(6, 2),
    axs=None,
    res=10,
):
    """Plots the work values of trajectories individually.

    This function generates a plot with three subplots:
    1. Line plots of the work values for all trajectories.
    2. Work value histograms for the indices given `index`.
    3. As well as normality plot (Q-Q plot) for the work values the indices given `index`..

    Args:
        workset: workset object
        index (list of int): Indices of the positions. These indices
            are used to extract specific columns from `workset.work_` for
            histogram and normality plots.
        x (array-like, optional): The x-axis positions for the work values. If
            not provided, `workset.position_` is used.
        worklinecolor (str, optional): Color of the work line plot. Default is
            '#777'.
        colors (list of str, optional):
            Colors for the histogram and normality
            plots. If not provided, the `Dark2` colormap is used.
        figsize (tuple, optional):
            Size of the figure. Default is (6, 2).
        axs (list of matplotlib.axes.Axes, optional):
            Axes for the subplots. If
            not provided, new axes are created.
        res (int, optional): Resolution for the work line plot. Default is 10.

    Returns:
        list of matplotlib.axes.Axes: The axes containing the subplots.

    Example:
        >>> plot_worknormalitychecks(
        ...     workset=my_workset,
        ...     index=[0, 5, 10],
        ... )
        >>> plt.show()

    """
    if axs is None:
        print('No axs given. Create figure.')
        fig, axs = plt.subplots(
            ncols=3,
            nrows=1,
            figsize=figsize,
        )
    if x is None:
        x = workset.position_
    plotting.plot_worklines(workset, axs[0], x=x, res=res, color=worklinecolor)

    if not colors:
        cmap = plt.get_cmap('Dark2')
        colors = cmap.colors

    for j, idx in enumerate(index):
        work = workset.work_[:, idx].ravel()
        axs[1].set_title(r'Histogram at $x$')
        plotting.plot_histo_normaldist(work, axs[1], colors[j])
        axs[0].axvline(x[idx],
                       color=colors[j],
                       zorder=3,
                       label=rf'$x={x[idx]:.2f}$',
                       )

        probplot(work, plot=axs[2], fit=True)
        axs[2].get_lines()[j * 2].set_color(colors[j])  # noqa: WPS221
        axs[2].set_title('Normality plot')

    axs[0].legend()
    return axs

from scipy.stats import probplot def plot_worknormalitychecks( workset, index, x=None, worklinecolor='#777', colors=None, figsize=(6, 2), axs=None, res=10, ): """Plots the work values of trajectories individually. This function generates a plot with three subplots: 1. Line plots of the work values for all trajectories. 2. Work value histograms for the indices given `index`. 3. As well as normality plot (Q-Q plot) for the work values the indices given `index`.. Args: workset: workset object index (list of int): Indices of the positions. These indices are used to extract specific columns from `workset.work_` for histogram and normality plots. x (array-like, optional): The x-axis positions for the work values. If not provided, `workset.position_` is used. worklinecolor (str, optional): Color of the work line plot. Default is '#777'. colors (list of str, optional): Colors for the histogram and normality plots. If not provided, the `Dark2` colormap is used. figsize (tuple, optional): Size of the figure. Default is (6, 2). axs (list of matplotlib.axes.Axes, optional): Axes for the subplots. If not provided, new axes are created. res (int, optional): Resolution for the work line plot. Default is 10. Returns: list of matplotlib.axes.Axes: The axes containing the subplots. Example: >>> plot_worknormalitychecks( ... workset=my_workset, ... index=[0, 5, 10], ... ) >>> plt.show() """ if axs is None: print('No axs given. Create figure.') fig, axs = plt.subplots( ncols=3, nrows=1, figsize=figsize, ) if x is None: x = workset.position_ plotting.plot_worklines(workset, axs[0], x=x, res=res, color=worklinecolor) if not colors: cmap = plt.get_cmap('Dark2') colors = cmap.colors for j, idx in enumerate(index): work = workset.work_[:, idx].ravel() axs[1].set_title(r'Histogram at $x$') plotting.plot_histo_normaldist(work, axs[1], colors[j]) axs[0].axvline(x[idx], color=colors[j], zorder=3, label=rf'$x={x[idx]:.2f}$', ) probplot(work, plot=axs[2], fit=True) axs[2].get_lines()[j * 2].set_color(colors[j]) # noqa: WPS221 axs[2].set_title('Normality plot') axs[0].legend() return axs

In [19]:

# check if work distribution follows a normal distribution
from scipy.stats import kstest, shapiro, anderson
from dcTMD.utils import plotting

index = [5000, 15000]
x = workset.position_

plot_worknormalitychecks(workset, index)

for i, p in enumerate(index):
    # Shapiro-Wilk Test
    shapiro_test = shapiro(workset.work_[:,p])
    print(f'shapiro wilkins results at x={x[p]} is {shapiro_test}')
    # Anderson-Darling Test
    # If the test statsitics is larger than the critical value of a given
    # significance_level in percent, the null hypothesis that the work
    # is normally distributed has to be rejected.
    anderson_test = anderson(workset.work_[:,p], 'norm')
    print(f'anderson darling results at x={x[p]} is {anderson_test}.')
    # Kolmogorov-Smirnov Test (requires centering and scaling of input data)
    kstest_test = kstest(
        (workset.work_[:,p]-np.mean(workset.work_[:,p]))/np.std(workset.work_[:,p]),
        'norm'
    )
    print(f'Kolmogorov-Smirnov results at x={x[p]} is {kstest_test}')

# check if work distribution follows a normal distribution from scipy.stats import kstest, shapiro, anderson from dcTMD.utils import plotting index = [5000, 15000] x = workset.position_ plot_worknormalitychecks(workset, index) for i, p in enumerate(index): # Shapiro-Wilk Test shapiro_test = shapiro(workset.work_[:,p]) print(f'shapiro wilkins results at x={x[p]} is {shapiro_test}') # Anderson-Darling Test # If the test statsitics is larger than the critical value of a given # significance_level in percent, the null hypothesis that the work # is normally distributed has to be rejected. anderson_test = anderson(workset.work_[:,p], 'norm') print(f'anderson darling results at x={x[p]} is {anderson_test}.') # Kolmogorov-Smirnov Test (requires centering and scaling of input data) kstest_test = kstest( (workset.work_[:,p]-np.mean(workset.work_[:,p]))/np.std(workset.work_[:,p]), 'norm' ) print(f'Kolmogorov-Smirnov results at x={x[p]} is {kstest_test}')

No axs given. Create figure.
shapiro wilkins results at x=0.5 is ShapiroResult(statistic=np.float64(0.9809889406089324), pvalue=np.float64(0.95963623434336))
anderson darling results at x=0.5 is AndersonResult(statistic=np.float64(0.1889729620402001), critical_values=array([0.503, 0.573, 0.687, 0.802, 0.954]), significance_level=array([15. , 10. ,  5. ,  2.5,  1. ]), fit_result=  params: FitParams(loc=np.float64(67.2816159481796), scale=np.float64(12.135336573012399))
 success: True
 message: '`anderson` successfully fit the distribution to the data.').
Kolmogorov-Smirnov results at x=0.5 is KstestResult(statistic=np.float64(0.1222997987555296), pvalue=np.float64(0.920955734836253), statistic_location=np.float64(-1.013218181258685), statistic_sign=np.int8(1))
shapiro wilkins results at x=1.5 is ShapiroResult(statistic=np.float64(0.9350144421408513), pvalue=np.float64(0.237681372960928))
anderson darling results at x=1.5 is AndersonResult(statistic=np.float64(0.38109849215264546), critical_values=array([0.503, 0.573, 0.687, 0.802, 0.954]), significance_level=array([15. , 10. ,  5. ,  2.5,  1. ]), fit_result=  params: FitParams(loc=np.float64(92.54892049414023), scale=np.float64(19.147779388352493))
 success: True
 message: '`anderson` successfully fit the distribution to the data.').
Kolmogorov-Smirnov results at x=1.5 is KstestResult(statistic=np.float64(0.14917443864214264), pvalue=np.float64(0.7646028245726414), statistic_location=np.float64(0.5380536480357743), statistic_sign=np.int8(-1))

III. derive estimates from workset¶

1. create WorkEstimator instance
2. fit WorkEstimator instance with previously created workset

In [20]:

# create WorkEstimator instance
workestimator = WorkEstimator(temperature)
# fit existing workset
# or load an existing workset
# workset = dcTMD.storing.load(my_workset)
workestimator.fit(workset)
vars(workestimator)

# create WorkEstimator instance workestimator = WorkEstimator(temperature) # fit existing workset # or load an existing workset # workset = dcTMD.storing.load(my_workset) workestimator.fit(workset) vars(workestimator)

Out[20]:

{'temperature': 300,
 'verbose': False,
 'work_set': WorkSet(velocity=0.001),
 'position_': array([0.0000e+00, 1.0000e-04, 2.0000e-04, ..., 1.9998e+00, 1.9999e+00,
        2.0000e+00], shape=(20001,)),
 'names_': array(['t_middle_32_pullf.xvg', 't_middle_03_pullf.xvg',
        't_middle_34_pullf.xvg', 't_middle_24_pullf.xvg',
        't_middle_21_pullf.xvg', 't_middle_04_pullf.xvg',
        't_middle_29_pullf.xvg', 't_middle_16_pullf.xvg',
        't_middle_30_pullf.xvg', 't_middle_19_pullf.xvg',
        't_middle_01_pullf.xvg', 't_middle_28_pullf.xvg',
        't_middle_26_pullf.xvg', 't_middle_31_pullf.xvg',
        't_middle_09_pullf.xvg', 't_middle_17_pullf.xvg',
        't_middle_25_pullf.xvg', 't_middle_05_pullf.xvg'], dtype='<U32'),
 'W_mean_': array([0.00000000e+00, 4.41837458e-02, 4.44572742e-02, ...,
        9.33136501e+01, 9.32887153e+01, 9.32516402e+01], shape=(20001,)),
 'W_diss_': array([0.00000000e+00, 1.16301148e-03, 5.56596643e-03, ...,
        1.03329006e+02, 1.03220317e+02, 1.03098234e+02], shape=(20001,)),
 'dG_': array([  0.        ,   0.04302073,   0.03889131, ..., -10.01535586,
         -9.93160192,  -9.84659417], shape=(20001,)),
 'friction_': array([       0.        ,    11630.11484133,    44029.54944818, ...,
          750667.95818287, -1086887.96420736, -1220828.47757071],
       shape=(20001,))}

Visualize results¶

In the package a couple of simple plot functions to get an overview of the results are implemented. e.g. plot_dcTMD_results()

In [21]:

# plot dcTMD results
from dcTMD.utils import plotting

# plot free energy estimate
fig, ax = plt.subplots()
plotting.plot_dG(x, workestimator.dG_, ax, label='some system')
plt.legend()
plt.show()

# plot dcTMD results
fig, axs = plotting.plot_dcTMD_results(workestimator)
plt.show()

# plot dcTMD results from dcTMD.utils import plotting # plot free energy estimate fig, ax = plt.subplots() plotting.plot_dG(x, workestimator.dG_, ax, label='some system') plt.legend() plt.show() # plot dcTMD results fig, axs = plotting.plot_dcTMD_results(workestimator) plt.show()

Smooth friction estimate¶

Finally, the friction estimate needs to be smoothed. This can be done via dcTMD.utils.smoothing.gaussfilter_friction() or dcTMD.WorkEstimator.smooth_friction(sigma, mode) sigma is the standard deviation of gaussian kernel in nm the mode parameter determines how the input array is extended beyond its boundaries.

Caution: this can lead to long computations using large datasets and a big smoothing window.

In [22]:

# smooth friction and plot results
workestimator.smooth_friction(sigma=0.1)

# if the friction is smoothed that value is automatically plotted
fig, axs = plotting.plot_dcTMD_results(workestimator)
plt.show()

# but one can also specify the friction
#fig, axs = plotting.plot_dcTMD_results(
#    workestimator,
#    friction=workestimator.friction_
#)

# smooth friction and plot results workestimator.smooth_friction(sigma=0.1) # if the friction is smoothed that value is automatically plotted fig, axs = plotting.plot_dcTMD_results(workestimator) plt.show() # but one can also specify the friction #fig, axs = plotting.plot_dcTMD_results( # workestimator, # friction=workestimator.friction_ #)

Using different smoothing windows and modes changes the results significantly. Because of the different boundary handling in the modes. mode='nearest' leads to an overestimation at the right hand boarder (end of the simulation), while mode='reflect' leads to a wash out of the boarder on the left hand side.

Here, are some examples:

In [23]:

fig, axs = plt.subplots()

x = workestimator.position_
plotting.plot_Gamma(x,
                    workestimator.friction_smooth_,
                    axs,
                    label='default (reflect) 0.1nm'
                    )

# using different smoothing windows and modes changes the results significantly
smooth_friction = dcTMD.utils.gaussfilter_friction(workestimator.friction_,
                                                   x,
                                                   sigma=.01,
                                                   mode='reflect',
                                                   )
axs.plot(x, smooth_friction, label='reflect .01nm')
smooth_friction = dcTMD.utils.gaussfilter_friction(workestimator.friction_,
                                                   x,
                                                   sigma=.01, 
                                                   mode='nearest',
                                                   )
axs.plot(x, smooth_friction, label='nearest .01nm')
smooth_friction = dcTMD.utils.gaussfilter_friction(workestimator.friction_,
                                                   x,
                                                   sigma=0.2,
                                                   mode='reflect',
                                                   )
                                                   
axs.plot(x, smooth_friction, label='reflect .2nm')
axs.legend()

plt.show()

fig, axs = plt.subplots() x = workestimator.position_ plotting.plot_Gamma(x, workestimator.friction_smooth_, axs, label='default (reflect) 0.1nm' ) # using different smoothing windows and modes changes the results significantly smooth_friction = dcTMD.utils.gaussfilter_friction(workestimator.friction_, x, sigma=.01, mode='reflect', ) axs.plot(x, smooth_friction, label='reflect .01nm') smooth_friction = dcTMD.utils.gaussfilter_friction(workestimator.friction_, x, sigma=.01, mode='nearest', ) axs.plot(x, smooth_friction, label='nearest .01nm') smooth_friction = dcTMD.utils.gaussfilter_friction(workestimator.friction_, x, sigma=0.2, mode='reflect', ) axs.plot(x, smooth_friction, label='reflect .2nm') axs.legend() plt.show()

IV. Error estimation¶

The error estimation of the results is implemented via bootstrapping

In [24]:

n_resamples = 1000

# bootstrapping error in mode std
mode = 'std'
workestimator.estimate_free_energy_errors(n_resamples, mode)

fig, ax = plt.subplots()
plotting.plot_dG_werrors(workestimator, ax)
plt.show()

n_resamples = 1000 # bootstrapping error in mode std mode = 'std' workestimator.estimate_free_energy_errors(n_resamples, mode) fig, ax = plt.subplots() plotting.plot_dG_werrors(workestimator, ax) plt.show()

Bootstrapping progress: 100%|██████████| 1000/1000 [00:01<00:00, 982.54it/s]

In [25]:

# bootstrapping error in with confidence interval 
# this gives a lower and upperbound estimate
confidence_interval = 0.9
mode = confidence_interval
workestimator.estimate_free_energy_errors(n_resamples, mode)

fig, ax = plt.subplots()
plotting.plot_dG_werrors(workestimator, ax)
plt.show()

# bootstrapping error in with confidence interval # this gives a lower and upperbound estimate confidence_interval = 0.9 mode = confidence_interval workestimator.estimate_free_energy_errors(n_resamples, mode) fig, ax = plt.subplots() plotting.plot_dG_werrors(workestimator, ax) plt.show()

Bootstrapping progress: 100%|██████████| 1000/1000 [00:01<00:00, 772.36it/s]

V. Save and load results¶

In [26]:

# save workestimator instance
dcTMD.storing.save('my_workestimator', workestimator)

# save data as .npz and .dat file
outname = 'my_workestimator_results'
dcTMD.io.write_output(outname, workestimator)

# loas results
results = np.load(f'{outname}_N{len(workestimator.names_)}_dG.npz')

results.files

# save workestimator instance dcTMD.storing.save('my_workestimator', workestimator) # save data as .npz and .dat file outname = 'my_workestimator_results' dcTMD.io.write_output(outname, workestimator) # loas results results = np.load(f'{outname}_N{len(workestimator.names_)}_dG.npz') results.files

save file my_workestimator_results_N18.dat
save file my_workestimator_results_N18.npz

Out[26]:

['x',
 'Wmean',
 'Wdiss',
 'dG',
 'Gamma',
 's_W_mean',
 's_W_diss',
 's_dG',
 'Gamma_smooth']