Integration (:mod:`scipy.integrate`)
====================================

.. sectionauthor:: Travis E. Oliphant

.. currentmodule:: scipy.integrate

The :mod:`scipy.integrate` sub-package provides several integration
techniques including an ordinary differential equation integrator. An
overview of the module is provided by the help command:

.. literalinclude:: examples/4-1


General integration (:func:`quad`)
----------------------------------

The function :obj:`quad` is provided to integrate a function of one
variable between two points. The points can be :math:`\pm\infty`
(:math:`\pm` ``inf``) to indicate infinite limits. For example,
suppose you wish to integrate a bessel function ``jv(2.5,x)`` along
the interval :math:`[0,4.5].`

.. math::

    I=\int_{0}^{4.5}J_{2.5}\left(x\right)\, dx.


This could be computed using :obj:`quad`:

    >>> result = integrate.quad(lambda x: special.jv(2.5,x), 0, 4.5)
    >>> print result
    (1.1178179380783249, 7.8663172481899801e-09)

    >>> I = sqrt(2/pi)*(18.0/27*sqrt(2)*cos(4.5)-4.0/27*sqrt(2)*sin(4.5)+
        sqrt(2*pi)*special.fresnel(3/sqrt(pi))[0])
    >>> print I
    1.117817938088701

    >>> print abs(result[0]-I)
    1.03761443881e-11

The first argument to quad is a "callable" Python object (*i.e* a
function, method, or class instance). Notice the use of a lambda-
function in this case as the argument. The next two arguments are the
limits of integration. The return value is a tuple, with the first
element holding the estimated value of the integral and the second
element holding an upper bound on the error. Notice, that in this
case, the true value of this integral is

.. math::

    I=\sqrt{\frac{2}{\pi}}\left(\frac{18}{27}\sqrt{2}\cos\left(4.5\right)-\frac{4}{27}\sqrt{2}\sin\left(4.5\right)+\sqrt{2\pi}\textrm{Si}\left(\frac{3}{\sqrt{\pi}}\right)\right),

where

.. math::

    \textrm{Si}\left(x\right)=\int_{0}^{x}\sin\left(\frac{\pi}{2}t^{2}\right)\, dt.

is the Fresnel sine integral. Note that the numerically-computed integral is
within :math:`1.04\times10^{-11}` of the exact result --- well below the
reported error bound.


If the function to integrate takes additional parameters, the can be provided
in the `args` argument. Suppose that the following integral shall be calculated:

.. math::

    I(a,b)=\int_{0}^{1} ax^2+b \, dx.


This integral can be evaluated by using the following code:

>>> from scipy.integrate import quad
>>> def integrand(x, a, b):
...     return a * x + b
>>> a = 2
>>> b = 1
>>> I = quad(integrand, 0, 1, args=(a,b))
>>> I = (2.0, 2.220446049250313e-14)


Infinite inputs are also allowed in :obj:`quad` by using :math:`\pm`
``inf`` as one of the arguments. For example, suppose that a numerical
value for the exponential integral:

.. math::

    E_{n}\left(x\right)=\int_{1}^{\infty}\frac{e^{-xt}}{t^{n}}\, dt.

is desired (and the fact that this integral can be computed as
``special.expn(n,x)`` is forgotten). The functionality of the function
:obj:`special.expn` can be replicated by defining a new function
:obj:`vec_expint` based on the routine :obj:`quad`:

    >>> from scipy.integrate import quad
    >>> def integrand(t, n, x):
    ...     return exp(-x*t) / t**n

    >>> def expint(n, x):
    ...     return quad(integrand, 1, Inf, args=(n, x))[0]

    >>> vec_expint = vectorize(expint)

    >>> vec_expint(3,arange(1.0,4.0,0.5))
    array([ 0.1097,  0.0567,  0.0301,  0.0163,  0.0089,  0.0049])
    >>> special.expn(3,arange(1.0,4.0,0.5))
    array([ 0.1097,  0.0567,  0.0301,  0.0163,  0.0089,  0.0049])

The function which is integrated can even use the quad argument (though the
error bound may underestimate the error due to possible numerical error in the
integrand from the use of :obj:`quad` ). The integral in this case is

.. math::

    I_{n}=\int_{0}^{\infty}\int_{1}^{\infty}\frac{e^{-xt}}{t^{n}}\, dt\, dx=\frac{1}{n}.

>>> result = quad(lambda x: expint(3, x), 0, inf)
>>> print result
(0.33333333324560266, 2.8548934485373678e-09)

>>> I3 = 1.0/3.0
>>> print I3
0.333333333333

>>> print I3 - result[0]
8.77306560731e-11

This last example shows that multiple integration can be handled using
repeated calls to :func:`quad`.


General multiple integration (:func:`dblquad`, :func:`tplquad`, :func:`nquad`)
------------------------------------------------------------------------------

The mechanics for double and triple integration have been wrapped up into the
functions :obj:`dblquad` and :obj:`tplquad`. These functions take the function
to  integrate and four, or six arguments, respecively. The limits of all
inner integrals need to be defined as functions.

An example of using double integration to compute several values of
:math:`I_{n}` is shown below:

    >>> from scipy.integrate import quad, dblquad
    >>> def I(n):
    ...     return dblquad(lambda t, x: exp(-x*t)/t**n, 0, Inf, lambda x: 1, lambda x: Inf)

    >>> print I(4)
    (0.25000000000435768, 1.0518245707751597e-09)
    >>> print I(3)
    (0.33333333325010883, 2.8604069919261191e-09)
    >>> print I(2)
    (0.49999999999857514, 1.8855523253868967e-09)


As example for non-constant limits consider the integral

.. math::

    I=\int_{y=0}^{1/2}\int_{x=0}^{1-2y} x y \, dx\, dy=\frac{1}{96}.


This integral can be evaluated using the expression below (Note the use of the
non-constant lambda functions for the upper limit of the inner integral):

>>> from scipy.integrate import dblquad
>>> area = dblquad(lambda x, y: x*y, 0, 0.5, lambda x: 0, lambda x: 1-2*x)
>>> area
(0.010416666666666668, 1.1564823173178715e-16)


For n-fold integration, scipy provides the function :obj:`nquad`. The
integration bounds are an iterable object: either a list of constant bounds,
or a list of functions for the non-constant integration bounds. The order of
integration (and therefore the bounds) is from the innermost integral to the
outermost one.

The integral from above

.. math::

    I_{n}=\int_{0}^{\infty}\int_{1}^{\infty}\frac{e^{-xt}}{t^{n}}\, dt\, dx=\frac{1}{n}

can be calculated as

>>> from scipy import integrate
>>> N = 5
>>> def f(t, x):
>>>    return np.exp(-x*t) / t**N
>>> integrate.nquad(f, [[1, np.inf],[0, np.inf]])
(0.20000000000002294, 1.2239614263187945e-08)

Note that the order of arguments for `f` must match the order of the
integration bounds; i.e. the inner integral with respect to :math:`t` is on
the interval :math:`[1, \infty]` and the outer integral with respect to
:math:`x` is on the interval :math:`[0, \infty]`.

Non-constant integration bounds can be treated in a similar manner; the
example from above

.. math::

    I=\int_{y=0}^{1/2}\int_{x=0}^{1-2y} x y \, dx\, dy=\frac{1}{96}.

can be evaluated by means of

>>> from scipy import integrate
>>> def f(x, y):
>>>     return x*y
>>> def bounds_y():
>>>     return [0, 0.5]
>>> def bounds_x(y):
>>>     return [0, 1-2*y]
>>> integrate.nquad(f, [bounds_x, bounds_y])
(0.010416666666666668, 4.101620128472366e-16)

which is the same result as before.

Gaussian quadrature
-------------------

A few functions are also provided in order to perform simple Gaussian
quadrature over a fixed interval. The first is :obj:`fixed_quad` which
performs fixed-order Gaussian quadrature. The second function is
:obj:`quadrature` which performs Gaussian quadrature of multiple
orders until the difference in the integral estimate is beneath some
tolerance supplied by the user. These functions both use the module
:mod:`special.orthogonal` which can calculate the roots and quadrature
weights of a large variety of orthogonal polynomials (the polynomials
themselves are available as special functions returning instances of
the polynomial class --- e.g. :obj:`special.legendre <scipy.special.legendre>`).


Romberg Integration
-------------------

Romberg's method [WPR]_ is another method for numerically evaluating an
integral. See the help function for :func:`romberg` for further details.


Integrating using Samples
-------------------------

If the samples are equally-spaced and the number of samples available
is :math:`2^{k}+1` for some integer :math:`k`, then Romberg :obj:`romb`
integration can be used to obtain high-precision estimates of the
integral using the available samples. Romberg integration uses the
trapezoid rule at step-sizes related by a power of two and then
performs Richardson extrapolation on these estimates to approximate
the integral with a higher-degree of accuracy.

In case of arbitrary spaced samples, the two functions trapz (defined in numpy
[NPT]_) and :obj:`simps` are available. They are using Newton-Coates formulas
of order 1 and 2 respectively to perform integration. The trapezoidal rule
approximates the function as a straight line between adjacent points, while
Simpson's rule approximates the function between three adjacent points as a
parabola.

For an odd number of samples that are equally spaced Simpson's rule is exact
if the function is a polynomial of order 3 or less. If the samples are not
equally spaced, then the result is exact only if the function is a polynomial
of order 2 or less.

>>> from scipy.integrate import simps
>>> import numpy as np
>>> def f(x):
...    return x**2
>>> def f2(x):
...    return x**3
>>> x = np.array([1,3,4])
>>> y1 = f1(x)
>>> I1 = integrate.simps(y1, x)
>>> print(I1)
21.0


This corresponds exactly to

.. math::

    \int_{1}^{4} x^2 \, dx = 21,

whereas integrating the second function

>>> y2 = f2(x)
>>> I2 = integrate.simps(y2, x)
>>> print(I2)
61.5

does not correspond to

.. math::

    \int_{1}^{4} x^3 \, dx = 63.75

because the order of the polynomial in f2 is larger than two.


Ordinary differential equations (:func:`odeint`)
------------------------------------------------

Integrating a set of ordinary differential equations (ODEs) given
initial conditions is another useful example. The function
:obj:`odeint` is available in SciPy for integrating a first-order
vector differential equation:

.. math::

    \frac{d\mathbf{y}}{dt}=\mathbf{f}\left(\mathbf{y},t\right),

given initial conditions :math:`\mathbf{y}\left(0\right)=y_{0}`, where
:math:`\mathbf{y}` is a length :math:`N` vector and :math:`\mathbf{f}`
is a mapping from :math:`\mathcal{R}^{N}` to :math:`\mathcal{R}^{N}.`
A higher-order ordinary differential equation can always be reduced to
a differential equation of this type by introducing intermediate
derivatives into the :math:`\mathbf{y}` vector.

For example suppose it is desired to find the solution to the
following second-order differential equation:

.. math::

    \frac{d^{2}w}{dz^{2}}-zw(z)=0

with initial conditions :math:`w\left(0\right)=\frac{1}{\sqrt[3]{3^{2}}\Gamma\left(\frac{2}{3}\right)}` and :math:`\left.\frac{dw}{dz}\right|_{z=0}=-\frac{1}{\sqrt[3]{3}\Gamma\left(\frac{1}{3}\right)}.` It is known that the solution to this differential equation with these
boundary conditions is the Airy function

.. math::

    w=\textrm{Ai}\left(z\right),

which gives a means to check the integrator using :func:`special.airy <scipy.special.airy>`.

First, convert this ODE into standard form by setting
:math:`\mathbf{y}=\left[\frac{dw}{dz},w\right]` and :math:`t=z`. Thus,
the differential equation becomes

.. math::

    \frac{d\mathbf{y}}{dt}=\left[\begin{array}{c} ty_{1}\\ y_{0}\end{array}\right]=\left[\begin{array}{cc} 0 & t\\ 1 & 0\end{array}\right]\left[\begin{array}{c} y_{0}\\ y_{1}\end{array}\right]=\left[\begin{array}{cc} 0 & t\\ 1 & 0\end{array}\right]\mathbf{y}.

In other words,

.. math::

    \mathbf{f}\left(\mathbf{y},t\right)=\mathbf{A}\left(t\right)\mathbf{y}.

As an interesting reminder, if :math:`\mathbf{A}\left(t\right)`
commutes with :math:`\int_{0}^{t}\mathbf{A}\left(\tau\right)\, d\tau`
under matrix multiplication, then this linear differential equation
has an exact solution using the matrix exponential:

.. math::

    \mathbf{y}\left(t\right)=\exp\left(\int_{0}^{t}\mathbf{A}\left(\tau\right)d\tau\right)\mathbf{y}\left(0\right),

However, in this case, :math:`\mathbf{A}\left(t\right)` and its integral do not commute.

There are many optional inputs and outputs available when using odeint
which can help tune the solver. These additional inputs and outputs
are not needed much of the time, however, and the three required input
arguments and the output solution suffice. The required inputs are the
function defining the derivative, *fprime*, the initial conditions
vector, *y0*, and the time points to obtain a solution, *t*, (with
the initial value point as the first element of this sequence).  The
output to :obj:`odeint` is a matrix where each row contains the
solution vector at each requested time point (thus, the initial
conditions are given in the first output row).

The following example illustrates the use of odeint including the
usage of the *Dfun* option which allows the user to specify a gradient
(with respect to :math:`\mathbf{y}` ) of the function,
:math:`\mathbf{f}\left(\mathbf{y},t\right)`.

    >>> from scipy.integrate import odeint
    >>> from scipy.special import gamma, airy
    >>> y1_0 = 1.0 / 3**(2.0/3.0) / gamma(2.0/3.0)
    >>> y0_0 = -1.0 / 3**(1.0/3.0) / gamma(1.0/3.0)
    >>> y0 = [y0_0, y1_0]
    >>> def func(y, t):
    ...     return [t*y[1],y[0]]

    >>> def gradient(y, t):
    ...     return [[0,t], [1,0]]

    >>> x = arange(0, 4.0, 0.01)
    >>> t = x
    >>> ychk = airy(x)[0]
    >>> y = odeint(func, y0, t)
    >>> y2 = odeint(func, y0, t, Dfun=gradient)

    >>> print ychk[:36:6]
    [ 0.355028  0.339511  0.324068  0.308763  0.293658  0.278806]

    >>> print y[:36:6,1]
    [ 0.355028  0.339511  0.324067  0.308763  0.293658  0.278806]

    >>> print y2[:36:6,1]
    [ 0.355028  0.339511  0.324067  0.308763  0.293658  0.278806]


References
~~~~~~~~~~

.. [WPR] http://en.wikipedia.org/wiki/Romberg's_method

.. [NPT] http://docs.scipy.org/doc/numpy/reference/generated/numpy.trapz.html
