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continuous.py
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continuous.py
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# Copyright 2022 The PyMC Developers
#
# Licensed under the Apache License, Version 2.0 (the "License");
# you may not use this file except in compliance with the License.
# You may obtain a copy of the License at
#
# http://www.apache.org/licenses/LICENSE-2.0
#
# Unless required by applicable law or agreed to in writing, software
# distributed under the License is distributed on an "AS IS" BASIS,
# WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
# See the License for the specific language governing permissions and
# limitations under the License.
# coding: utf-8
"""
Experimental probability distributions for stochastic nodes in PyMC.
The imports from pymc are not fully replicated here: add imports as necessary.
"""
import numpy as np
import pytensor.tensor as pt
from pymc import ChiSquared, CustomDist
from pymc.distributions import transforms
from pymc.distributions.dist_math import check_parameters
from pymc.distributions.distribution import Continuous
from pymc.distributions.shape_utils import rv_size_is_none
from pymc.logprob.utils import CheckParameterValue
from pymc.pytensorf import floatX
from pytensor.tensor.random.op import RandomVariable
from pytensor.tensor.variable import TensorVariable
from scipy import stats
class GenExtremeRV(RandomVariable):
name: str = "Generalized Extreme Value"
signature = "(),(),()->()"
dtype: str = "floatX"
_print_name: tuple[str, str] = ("Generalized Extreme Value", "\\operatorname{GEV}")
def __call__(self, mu=0.0, sigma=1.0, xi=0.0, size=None, **kwargs) -> TensorVariable:
return super().__call__(mu, sigma, xi, size=size, **kwargs)
@classmethod
def rng_fn(
cls,
rng: np.random.RandomState | np.random.Generator,
mu: np.ndarray,
sigma: np.ndarray,
xi: np.ndarray,
size: tuple[int, ...],
) -> np.ndarray:
# Notice negative here, since remainder of GenExtreme is based on Coles parametrization
return stats.genextreme.rvs(c=-xi, loc=mu, scale=sigma, random_state=rng, size=size)
gev = GenExtremeRV()
class GenExtreme(Continuous):
r"""
Univariate Generalized Extreme Value log-likelihood
The cdf of this distribution is
.. math::
G(x \mid \mu, \sigma, \xi) = \exp\left[ -\left(1 + \xi z\right)^{-\frac{1}{\xi}} \right]
where
.. math::
z = \frac{x - \mu}{\sigma}
and is defined on the set:
.. math::
\left\{x: 1 + \xi\left(\frac{x-\mu}{\sigma}\right) > 0 \right\}.
Note that this parametrization is per Coles (2001), and differs from that of
Scipy in the sign of the shape parameter, :math:`\xi`.
.. plot::
import matplotlib.pyplot as plt
import numpy as np
import scipy.stats as st
import arviz as az
plt.style.use('arviz-darkgrid')
x = np.linspace(-10, 20, 200)
mus = [0., 4., -1.]
sigmas = [2., 2., 4.]
xis = [-0.3, 0.0, 0.3]
for mu, sigma, xi in zip(mus, sigmas, xis):
pdf = st.genextreme.pdf(x, c=-xi, loc=mu, scale=sigma)
plt.plot(x, pdf, label=rf'$\mu$ = {mu}, $\sigma$ = {sigma}, $\xi$={xi}')
plt.xlabel('x', fontsize=12)
plt.ylabel('f(x)', fontsize=12)
plt.legend(loc=1)
plt.show()
======== =========================================================================
Support * :math:`x \in [\mu - \sigma/\xi, +\infty]`, when :math:`\xi > 0`
* :math:`x \in \mathbb{R}` when :math:`\xi = 0`
* :math:`x \in [-\infty, \mu - \sigma/\xi]`, when :math:`\xi < 0`
Mean * :math:`\mu + \sigma(g_1 - 1)/\xi`, when :math:`\xi \neq 0, \xi < 1`
* :math:`\mu + \sigma \gamma`, when :math:`\xi = 0`
* :math:`\infty`, when :math:`\xi \geq 1`
where :math:`\gamma` is the Euler-Mascheroni constant, and
:math:`g_k = \Gamma (1-k\xi)`
Variance * :math:`\sigma^2 (g_2 - g_1^2)/\xi^2`, when :math:`\xi \neq 0, \xi < 0.5`
* :math:`\frac{\pi^2}{6} \sigma^2`, when :math:`\xi = 0`
* :math:`\infty`, when :math:`\xi \geq 0.5`
======== =========================================================================
Parameters
----------
mu : float
Location parameter.
sigma : float
Scale parameter (sigma > 0).
xi : float
Shape parameter
scipy : bool
Whether or not to use the Scipy interpretation of the shape parameter
(defaults to `False`).
References
----------
.. [Coles2001] Coles, S.G. (2001).
An Introduction to the Statistical Modeling of Extreme Values
Springer-Verlag, London
"""
rv_op = gev
@classmethod
def dist(cls, mu=0, sigma=1, xi=0, scipy=False, **kwargs):
# If SciPy, use its parametrization, otherwise convert to standard
if scipy:
xi = -xi
mu = pt.as_tensor_variable(floatX(mu))
sigma = pt.as_tensor_variable(floatX(sigma))
xi = pt.as_tensor_variable(floatX(xi))
return super().dist([mu, sigma, xi], **kwargs)
def logp(value, mu, sigma, xi):
"""
Calculate log-probability of Generalized Extreme Value distribution
at specified value.
Parameters
----------
value: numeric
Value(s) for which log-probability is calculated. If the log probabilities for multiple
values are desired the values must be provided in a numpy array or Pytensor tensor
Returns
-------
TensorVariable
"""
scaled = (value - mu) / sigma
logp_expression = pt.switch(
pt.isclose(xi, 0),
-pt.log(sigma) - scaled - pt.exp(-scaled),
-pt.log(sigma)
- ((xi + 1) / xi) * pt.log1p(xi * scaled)
- pt.pow(1 + xi * scaled, -1 / xi),
)
logp = pt.switch(pt.gt(1 + xi * scaled, 0.0), logp_expression, -np.inf)
return check_parameters(
logp, sigma > 0, pt.and_(xi > -1, xi < 1), msg="sigma > 0 or -1 < xi < 1"
)
def logcdf(value, mu, sigma, xi):
"""
Compute the log of the cumulative distribution function for Generalized Extreme Value
distribution at the specified value.
Parameters
----------
value: numeric or np.ndarray or `TensorVariable`
Value(s) for which log CDF is calculated. If the log CDF for
multiple values are desired the values must be provided in a numpy
array or `TensorVariable`.
Returns
-------
TensorVariable
"""
scaled = (value - mu) / sigma
logc_expression = pt.switch(
pt.isclose(xi, 0), -pt.exp(-scaled), -pt.pow(1 + xi * scaled, -1 / xi)
)
logc = pt.switch(1 + xi * (value - mu) / sigma > 0, logc_expression, -np.inf)
return check_parameters(
logc, sigma > 0, pt.and_(xi > -1, xi < 1), msg="sigma > 0 or -1 < xi < 1"
)
def support_point(rv, size, mu, sigma, xi):
r"""
Using the mode, as the mean can be infinite when :math:`\xi > 1`
"""
mode = pt.switch(pt.isclose(xi, 0), mu, mu + sigma * (pt.pow(1 + xi, -xi) - 1) / xi)
if not rv_size_is_none(size):
mode = pt.full(size, mode)
return mode
class Chi:
r"""
:math:`\chi` log-likelihood.
The pdf of this distribution is
.. math::
f(x \mid \nu) = \frac{x^{\nu - 1}e^{-x^2/2}}{2^{\nu/2 - 1}\Gamma(\nu/2)}
.. plot::
:context: close-figs
import matplotlib.pyplot as plt
import numpy as np
import scipy.stats as st
import arviz as az
plt.style.use('arviz-darkgrid')
x = np.linspace(0, 10, 200)
for df in [1, 2, 3, 6, 9]:
pdf = st.chi.pdf(x, df)
plt.plot(x, pdf, label=r'$\nu$ = {}'.format(df))
plt.xlabel('x', fontsize=12)
plt.ylabel('f(x)', fontsize=12)
plt.legend(loc=1)
plt.show()
======== =========================================================================
Support :math:`x \in [0, \infty)`
Mean :math:`\sqrt{2}\frac{\Gamma((\nu + 1)/2)}{\Gamma(\nu/2)}`
Variance :math:`\nu - 2\left(\frac{\Gamma((\nu + 1)/2)}{\Gamma(\nu/2)}\right)^2`
======== =========================================================================
Parameters
----------
nu : tensor_like of float
Degrees of freedom (nu > 0).
Examples
--------
.. code-block:: python
import pymc as pm
from pymc_experimental.distributions import Chi
with pm.Model():
x = Chi('x', nu=1)
"""
@staticmethod
def chi_dist(nu: TensorVariable, size: TensorVariable) -> TensorVariable:
return pt.math.sqrt(ChiSquared.dist(nu=nu, size=size))
def __new__(cls, name, nu, **kwargs):
if "observed" not in kwargs:
kwargs.setdefault("default_transform", transforms.log)
return CustomDist(name, nu, dist=cls.chi_dist, class_name="Chi", **kwargs)
@classmethod
def dist(cls, nu, **kwargs):
return CustomDist.dist(nu, dist=cls.chi_dist, class_name="Chi", **kwargs)
class Maxwell:
R"""
The Maxwell-Boltzmann distribution
The pdf of this distribution is
.. math::
f(x \mid a) = {\displaystyle {\sqrt {\frac {2}{\pi }}}\,{\frac {x^{2}}{a^{3}}}\,\exp \left({\frac {-x^{2}}{2a^{2}}}\right)}
Read more about it on `Wikipedia <https://en.wikipedia.org/wiki/Maxwell%E2%80%93Boltzmann_distribution>`_
.. plot::
:context: close-figs
import matplotlib.pyplot as plt
import numpy as np
import scipy.stats as st
import arviz as az
plt.style.use('arviz-darkgrid')
x = np.linspace(0, 20, 200)
for a in [1, 2, 5]:
pdf = st.maxwell.pdf(x, scale=a)
plt.plot(x, pdf, label=r'$a$ = {}'.format(a))
plt.xlabel('x', fontsize=12)
plt.ylabel('f(x)', fontsize=12)
plt.legend(loc=1)
plt.show()
======== =========================================================================
Support :math:`x \in (0, \infty)`
Mean :math:`2a \sqrt{\frac{2}{\pi}}`
Variance :math:`\frac{a^2(3 \pi - 8)}{\pi}`
======== =========================================================================
Parameters
----------
a : tensor_like of float
Scale parameter (a > 0).
"""
@staticmethod
def maxwell_dist(a: TensorVariable, size: TensorVariable) -> TensorVariable:
if rv_size_is_none(size):
size = a.shape
a = CheckParameterValue("a > 0")(a, pt.all(pt.gt(a, 0)))
return Chi.dist(nu=3, size=size) * a
def __new__(cls, name, a, **kwargs):
return CustomDist(
name,
a,
dist=cls.maxwell_dist,
class_name="Maxwell",
**kwargs,
)
@classmethod
def dist(cls, a, **kwargs):
return CustomDist.dist(
a,
dist=cls.maxwell_dist,
class_name="Maxwell",
**kwargs,
)