""" A collection of functions to find the weights and abscissas for Gaussian Quadrature. These calculations are done by finding the eigenvalues of a tridiagonal matrix whose entries are dependent on the coefficients in the recursion formula for the orthogonal polynomials with the corresponding weighting function over the interval. Many recursion relations for orthogonal polynomials are given: .. math:: a1n f_{n+1} (x) = (a2n + a3n x ) f_n (x) - a4n f_{n-1} (x) The recursion relation of interest is .. math:: P_{n+1} (x) = (x - A_n) P_n (x) - B_n P_{n-1} (x) where :math:`P` has a different normalization than :math:`f`. The coefficients can be found as: .. math:: A_n = -a2n / a3n \\qquad B_n = ( a4n / a3n \\sqrt{h_n-1 / h_n})^2 where .. math:: h_n = \\int_a^b w(x) f_n(x)^2 assume: .. math:: P_0 (x) = 1 \\qquad P_{-1} (x) == 0 For the mathematical background, see [golub.welsch-1969-mathcomp]_ and [abramowitz.stegun-1965]_. References ---------- .. [golub.welsch-1969-mathcomp] Golub, Gene H, and John H Welsch. 1969. Calculation of Gauss Quadrature Rules. *Mathematics of Computation* 23, 221-230+s1--s10. .. [abramowitz.stegun-1965] Abramowitz, Milton, and Irene A Stegun. (1965) *Handbook of Mathematical Functions: with Formulas, Graphs, and Mathematical Tables*. Gaithersburg, MD: National Bureau of Standards. http://www.math.sfu.ca/~cbm/aands/ .. [townsend.trogdon.olver-2014] Townsend, A. and Trogdon, T. and Olver, S. (2014) *Fast computation of Gauss quadrature nodes and weights on the whole real line*. :arXiv:`1410.5286`. .. [townsend.trogdon.olver-2015] Townsend, A. and Trogdon, T. and Olver, S. (2015) *Fast computation of Gauss quadrature nodes and weights on the whole real line*. IMA Journal of Numerical Analysis :doi:`10.1093/imanum/drv002`. """ # # Author: Travis Oliphant 2000 # Updated Sep. 2003 (fixed bugs --- tested to be accurate) # SciPy imports. import numpy as np from numpy import (exp, inf, pi, sqrt, floor, sin, cos, around, hstack, arccos, arange) from scipy import linalg from scipy.special import airy # Local imports. from . import _ufuncs from . import _ufuncs as cephes _gam = cephes.gamma from . import specfun _polyfuns = ['legendre', 'chebyt', 'chebyu', 'chebyc', 'chebys', 'jacobi', 'laguerre', 'genlaguerre', 'hermite', 'hermitenorm', 'gegenbauer', 'sh_legendre', 'sh_chebyt', 'sh_chebyu', 'sh_jacobi'] # Correspondence between new and old names of root functions _rootfuns_map = {'roots_legendre': 'p_roots', 'roots_chebyt': 't_roots', 'roots_chebyu': 'u_roots', 'roots_chebyc': 'c_roots', 'roots_chebys': 's_roots', 'roots_jacobi': 'j_roots', 'roots_laguerre': 'l_roots', 'roots_genlaguerre': 'la_roots', 'roots_hermite': 'h_roots', 'roots_hermitenorm': 'he_roots', 'roots_gegenbauer': 'cg_roots', 'roots_sh_legendre': 'ps_roots', 'roots_sh_chebyt': 'ts_roots', 'roots_sh_chebyu': 'us_roots', 'roots_sh_jacobi': 'js_roots'} _evalfuns = ['eval_legendre', 'eval_chebyt', 'eval_chebyu', 'eval_chebyc', 'eval_chebys', 'eval_jacobi', 'eval_laguerre', 'eval_genlaguerre', 'eval_hermite', 'eval_hermitenorm', 'eval_gegenbauer', 'eval_sh_legendre', 'eval_sh_chebyt', 'eval_sh_chebyu', 'eval_sh_jacobi'] __all__ = _polyfuns + list(_rootfuns_map.keys()) + _evalfuns + ['poch', 'binom'] class orthopoly1d(np.poly1d): def __init__(self, roots, weights=None, hn=1.0, kn=1.0, wfunc=None, limits=None, monic=False, eval_func=None): equiv_weights = [weights[k] / wfunc(roots[k]) for k in range(len(roots))] mu = sqrt(hn) if monic: evf = eval_func if evf: knn = kn eval_func = lambda x: evf(x) / knn mu = mu / abs(kn) kn = 1.0 # compute coefficients from roots, then scale poly = np.poly1d(roots, r=True) np.poly1d.__init__(self, poly.coeffs * float(kn)) self.weights = np.array(list(zip(roots, weights, equiv_weights))) self.weight_func = wfunc self.limits = limits self.normcoef = mu # Note: eval_func will be discarded on arithmetic self._eval_func = eval_func def __call__(self, v): if self._eval_func and not isinstance(v, np.poly1d): return self._eval_func(v) else: return np.poly1d.__call__(self, v) def _scale(self, p): if p == 1.0: return self._coeffs *= p evf = self._eval_func if evf: self._eval_func = lambda x: evf(x) * p self.normcoef *= p def _gen_roots_and_weights(n, mu0, an_func, bn_func, f, df, symmetrize, mu): """[x,w] = gen_roots_and_weights(n,an_func,sqrt_bn_func,mu) Returns the roots (x) of an nth order orthogonal polynomial, and weights (w) to use in appropriate Gaussian quadrature with that orthogonal polynomial. The polynomials have the recurrence relation P_n+1(x) = (x - A_n) P_n(x) - B_n P_n-1(x) an_func(n) should return A_n sqrt_bn_func(n) should return sqrt(B_n) mu ( = h_0 ) is the integral of the weight over the orthogonal interval """ k = np.arange(n, dtype='d') c = np.zeros((2, n)) c[0,1:] = bn_func(k[1:]) c[1,:] = an_func(k) x = linalg.eigvals_banded(c, overwrite_a_band=True) # improve roots by one application of Newton's method y = f(n, x) dy = df(n, x) x -= y/dy fm = f(n-1, x) fm /= np.abs(fm).max() dy /= np.abs(dy).max() w = 1.0 / (fm * dy) if symmetrize: w = (w + w[::-1]) / 2 x = (x - x[::-1]) / 2 w *= mu0 / w.sum() if mu: return x, w, mu0 else: return x, w # Jacobi Polynomials 1 P^(alpha,beta)_n(x) def roots_jacobi(n, alpha, beta, mu=False): r"""Gauss-Jacobi quadrature. Compute the sample points and weights for Gauss-Jacobi quadrature. The sample points are the roots of the nth degree Jacobi polynomial, :math:`P^{\alpha, \beta}_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-1, 1]` with weight function :math:`w(x) = (1 - x)^{\alpha} (1 + x)^{\beta}`. See 22.2.1 in [AS]_ for details. Parameters ---------- n : int quadrature order alpha : float alpha must be > -1 beta : float beta must be > -1 mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError("n must be a positive integer.") if alpha <= -1 or beta <= -1: raise ValueError("alpha and beta must be greater than -1.") if alpha == 0.0 and beta == 0.0: return roots_legendre(m, mu) if alpha == beta: return roots_gegenbauer(m, alpha+0.5, mu) mu0 = 2.0**(alpha+beta+1)*cephes.beta(alpha+1, beta+1) a = alpha b = beta if a + b == 0.0: an_func = lambda k: np.where(k == 0, (b-a)/(2+a+b), 0.0) else: an_func = lambda k: np.where(k == 0, (b-a)/(2+a+b), (b*b - a*a) / ((2.0*k+a+b)*(2.0*k+a+b+2))) bn_func = lambda k: 2.0 / (2.0*k+a+b)*np.sqrt((k+a)*(k+b) / (2*k+a+b+1)) \ * np.where(k == 1, 1.0, np.sqrt(k*(k+a+b) / (2.0*k+a+b-1))) f = lambda n, x: cephes.eval_jacobi(n, a, b, x) df = lambda n, x: 0.5 * (n + a + b + 1) \ * cephes.eval_jacobi(n-1, a+1, b+1, x) return _gen_roots_and_weights(m, mu0, an_func, bn_func, f, df, False, mu) def jacobi(n, alpha, beta, monic=False): r"""Jacobi polynomial. Defined to be the solution of .. math:: (1 - x^2)\frac{d^2}{dx^2}P_n^{(\alpha, \beta)} + (\beta - \alpha - (\alpha + \beta + 2)x) \frac{d}{dx}P_n^{(\alpha, \beta)} + n(n + \alpha + \beta + 1)P_n^{(\alpha, \beta)} = 0 for :math:`\alpha, \beta > -1`; :math:`P_n^{(\alpha, \beta)}` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. alpha : float Parameter, must be greater than -1. beta : float Parameter, must be greater than -1. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- P : orthopoly1d Jacobi polynomial. Notes ----- For fixed :math:`\alpha, \beta`, the polynomials :math:`P_n^{(\alpha, \beta)}` are orthogonal over :math:`[-1, 1]` with weight function :math:`(1 - x)^\alpha(1 + x)^\beta`. """ if n < 0: raise ValueError("n must be nonnegative.") wfunc = lambda x: (1 - x)**alpha * (1 + x)**beta if n == 0: return orthopoly1d([], [], 1.0, 1.0, wfunc, (-1, 1), monic, eval_func=np.ones_like) x, w, mu = roots_jacobi(n, alpha, beta, mu=True) ab1 = alpha + beta + 1.0 hn = 2**ab1 / (2 * n + ab1) * _gam(n + alpha + 1) hn *= _gam(n + beta + 1.0) / _gam(n + 1) / _gam(n + ab1) kn = _gam(2 * n + ab1) / 2.0**n / _gam(n + 1) / _gam(n + ab1) # here kn = coefficient on x^n term p = orthopoly1d(x, w, hn, kn, wfunc, (-1, 1), monic, lambda x: eval_jacobi(n, alpha, beta, x)) return p # Jacobi Polynomials shifted G_n(p,q,x) def roots_sh_jacobi(n, p1, q1, mu=False): """Gauss-Jacobi (shifted) quadrature. Compute the sample points and weights for Gauss-Jacobi (shifted) quadrature. The sample points are the roots of the nth degree shifted Jacobi polynomial, :math:`G^{p,q}_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[0, 1]` with weight function :math:`w(x) = (1 - x)^{p-q} x^{q-1}`. See 22.2.2 in [AS]_ for details. Parameters ---------- n : int quadrature order p1 : float (p1 - q1) must be > -1 q1 : float q1 must be > 0 mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ if (p1-q1) <= -1 or q1 <= 0: raise ValueError("(p - q) must be greater than -1, and q must be greater than 0.") x, w, m = roots_jacobi(n, p1-q1, q1-1, True) x = (x + 1) / 2 scale = 2.0**p1 w /= scale m /= scale if mu: return x, w, m else: return x, w def sh_jacobi(n, p, q, monic=False): r"""Shifted Jacobi polynomial. Defined by .. math:: G_n^{(p, q)}(x) = \binom{2n + p - 1}{n}^{-1}P_n^{(p - q, q - 1)}(2x - 1), where :math:`P_n^{(\cdot, \cdot)}` is the nth Jacobi polynomial. Parameters ---------- n : int Degree of the polynomial. p : float Parameter, must have :math:`p > q - 1`. q : float Parameter, must be greater than 0. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- G : orthopoly1d Shifted Jacobi polynomial. Notes ----- For fixed :math:`p, q`, the polynomials :math:`G_n^{(p, q)}` are orthogonal over :math:`[0, 1]` with weight function :math:`(1 - x)^{p - q}x^{q - 1}`. """ if n < 0: raise ValueError("n must be nonnegative.") wfunc = lambda x: (1.0 - x)**(p - q) * (x)**(q - 1.) if n == 0: return orthopoly1d([], [], 1.0, 1.0, wfunc, (-1, 1), monic, eval_func=np.ones_like) n1 = n x, w, mu0 = roots_sh_jacobi(n1, p, q, mu=True) hn = _gam(n + 1) * _gam(n + q) * _gam(n + p) * _gam(n + p - q + 1) hn /= (2 * n + p) * (_gam(2 * n + p)**2) # kn = 1.0 in standard form so monic is redundant. Kept for compatibility. kn = 1.0 pp = orthopoly1d(x, w, hn, kn, wfunc=wfunc, limits=(0, 1), monic=monic, eval_func=lambda x: eval_sh_jacobi(n, p, q, x)) return pp # Generalized Laguerre L^(alpha)_n(x) def roots_genlaguerre(n, alpha, mu=False): r"""Gauss-generalized Laguerre quadrature. Compute the sample points and weights for Gauss-generalized Laguerre quadrature. The sample points are the roots of the nth degree generalized Laguerre polynomial, :math:`L^{\alpha}_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[0, \infty]` with weight function :math:`w(x) = x^{\alpha} e^{-x}`. See 22.3.9 in [AS]_ for details. Parameters ---------- n : int quadrature order alpha : float alpha must be > -1 mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError("n must be a positive integer.") if alpha < -1: raise ValueError("alpha must be greater than -1.") mu0 = cephes.gamma(alpha + 1) if m == 1: x = np.array([alpha+1.0], 'd') w = np.array([mu0], 'd') if mu: return x, w, mu0 else: return x, w an_func = lambda k: 2 * k + alpha + 1 bn_func = lambda k: -np.sqrt(k * (k + alpha)) f = lambda n, x: cephes.eval_genlaguerre(n, alpha, x) df = lambda n, x: (n*cephes.eval_genlaguerre(n, alpha, x) - (n + alpha)*cephes.eval_genlaguerre(n-1, alpha, x))/x return _gen_roots_and_weights(m, mu0, an_func, bn_func, f, df, False, mu) def genlaguerre(n, alpha, monic=False): r"""Generalized (associated) Laguerre polynomial. Defined to be the solution of .. math:: x\frac{d^2}{dx^2}L_n^{(\alpha)} + (\alpha + 1 - x)\frac{d}{dx}L_n^{(\alpha)} + nL_n^{(\alpha)} = 0, where :math:`\alpha > -1`; :math:`L_n^{(\alpha)}` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. alpha : float Parameter, must be greater than -1. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- L : orthopoly1d Generalized Laguerre polynomial. Notes ----- For fixed :math:`\alpha`, the polynomials :math:`L_n^{(\alpha)}` are orthogonal over :math:`[0, \infty)` with weight function :math:`e^{-x}x^\alpha`. The Laguerre polynomials are the special case where :math:`\alpha = 0`. See Also -------- laguerre : Laguerre polynomial. """ if alpha <= -1: raise ValueError("alpha must be > -1") if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_genlaguerre(n1, alpha, mu=True) wfunc = lambda x: exp(-x) * x**alpha if n == 0: x, w = [], [] hn = _gam(n + alpha + 1) / _gam(n + 1) kn = (-1)**n / _gam(n + 1) p = orthopoly1d(x, w, hn, kn, wfunc, (0, inf), monic, lambda x: eval_genlaguerre(n, alpha, x)) return p # Laguerre L_n(x) def roots_laguerre(n, mu=False): r"""Gauss-Laguerre quadrature. Compute the sample points and weights for Gauss-Laguerre quadrature. The sample points are the roots of the nth degree Laguerre polynomial, :math:`L_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[0, \infty]` with weight function :math:`w(x) = e^{-x}`. See 22.2.13 in [AS]_ for details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad numpy.polynomial.laguerre.laggauss References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ return roots_genlaguerre(n, 0.0, mu=mu) def laguerre(n, monic=False): r"""Laguerre polynomial. Defined to be the solution of .. math:: x\frac{d^2}{dx^2}L_n + (1 - x)\frac{d}{dx}L_n + nL_n = 0; :math:`L_n` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- L : orthopoly1d Laguerre Polynomial. Notes ----- The polynomials :math:`L_n` are orthogonal over :math:`[0, \infty)` with weight function :math:`e^{-x}`. """ if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_laguerre(n1, mu=True) if n == 0: x, w = [], [] hn = 1.0 kn = (-1)**n / _gam(n + 1) p = orthopoly1d(x, w, hn, kn, lambda x: exp(-x), (0, inf), monic, lambda x: eval_laguerre(n, x)) return p # Hermite 1 H_n(x) def roots_hermite(n, mu=False): r"""Gauss-Hermite (physicist's) quadrature. Compute the sample points and weights for Gauss-Hermite quadrature. The sample points are the roots of the nth degree Hermite polynomial, :math:`H_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-\infty, \infty]` with weight function :math:`w(x) = e^{-x^2}`. See 22.2.14 in [AS]_ for details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights Notes ----- For small n up to 150 a modified version of the Golub-Welsch algorithm is used. Nodes are computed from the eigenvalue problem and improved by one step of a Newton iteration. The weights are computed from the well-known analytical formula. For n larger than 150 an optimal asymptotic algorithm is applied which computes nodes and weights in a numerically stable manner. The algorithm has linear runtime making computation for very large n (several thousand or more) feasible. See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad numpy.polynomial.hermite.hermgauss roots_hermitenorm References ---------- .. [townsend.trogdon.olver-2014] Townsend, A. and Trogdon, T. and Olver, S. (2014) *Fast computation of Gauss quadrature nodes and weights on the whole real line*. :arXiv:`1410.5286`. .. [townsend.trogdon.olver-2015] Townsend, A. and Trogdon, T. and Olver, S. (2015) *Fast computation of Gauss quadrature nodes and weights on the whole real line*. IMA Journal of Numerical Analysis :doi:`10.1093/imanum/drv002`. .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError("n must be a positive integer.") mu0 = np.sqrt(np.pi) if n <= 150: an_func = lambda k: 0.0*k bn_func = lambda k: np.sqrt(k/2.0) f = cephes.eval_hermite df = lambda n, x: 2.0 * n * cephes.eval_hermite(n-1, x) return _gen_roots_and_weights(m, mu0, an_func, bn_func, f, df, True, mu) else: nodes, weights = _roots_hermite_asy(m) if mu: return nodes, weights, mu0 else: return nodes, weights def _compute_tauk(n, k, maxit=5): """Helper function for Tricomi initial guesses For details, see formula 3.1 in lemma 3.1 in the original paper. Parameters ---------- n : int Quadrature order k : ndarray of type int Index of roots :math:`\tau_k` to compute maxit : int Number of Newton maxit performed, the default value of 5 is sufficient. Returns ------- tauk : ndarray Roots of equation 3.1 See Also -------- initial_nodes_a roots_hermite_asy """ a = n % 2 - 0.5 c = (4.0*floor(n/2.0) - 4.0*k + 3.0)*pi / (4.0*floor(n/2.0) + 2.0*a + 2.0) f = lambda x: x - sin(x) - c df = lambda x: 1.0 - cos(x) xi = 0.5*pi for i in range(maxit): xi = xi - f(xi)/df(xi) return xi def _initial_nodes_a(n, k): r"""Tricomi initial guesses Computes an initial approximation to the square of the `k`-th (positive) root :math:`x_k` of the Hermite polynomial :math:`H_n` of order :math:`n`. The formula is the one from lemma 3.1 in the original paper. The guesses are accurate except in the region near :math:`\sqrt{2n + 1}`. Parameters ---------- n : int Quadrature order k : ndarray of type int Index of roots to compute Returns ------- xksq : ndarray Square of the approximate roots See Also -------- initial_nodes roots_hermite_asy """ tauk = _compute_tauk(n, k) sigk = cos(0.5*tauk)**2 a = n % 2 - 0.5 nu = 4.0*floor(n/2.0) + 2.0*a + 2.0 # Initial approximation of Hermite roots (square) xksq = nu*sigk - 1.0/(3.0*nu) * (5.0/(4.0*(1.0-sigk)**2) - 1.0/(1.0-sigk) - 0.25) return xksq def _initial_nodes_b(n, k): r"""Gatteschi initial guesses Computes an initial approximation to the square of the kth (positive) root :math:`x_k` of the Hermite polynomial :math:`H_n` of order :math:`n`. The formula is the one from lemma 3.2 in the original paper. The guesses are accurate in the region just below :math:`\sqrt{2n + 1}`. Parameters ---------- n : int Quadrature order k : ndarray of type int Index of roots to compute Returns ------- xksq : ndarray Square of the approximate root See Also -------- initial_nodes roots_hermite_asy """ a = n % 2 - 0.5 nu = 4.0*floor(n/2.0) + 2.0*a + 2.0 # Airy roots by approximation ak = specfun.airyzo(k.max(), 1)[0][::-1] # Initial approximation of Hermite roots (square) xksq = (nu + 2.0**(2.0/3.0) * ak * nu**(1.0/3.0) + 1.0/5.0 * 2.0**(4.0/3.0) * ak**2 * nu**(-1.0/3.0) + (9.0/140.0 - 12.0/175.0 * ak**3) * nu**(-1.0) + (16.0/1575.0 * ak + 92.0/7875.0 * ak**4) * 2.0**(2.0/3.0) * nu**(-5.0/3.0) - (15152.0/3031875.0 * ak**5 + 1088.0/121275.0 * ak**2) * 2.0**(1.0/3.0) * nu**(-7.0/3.0)) return xksq def _initial_nodes(n): """Initial guesses for the Hermite roots Computes an initial approximation to the non-negative roots :math:`x_k` of the Hermite polynomial :math:`H_n` of order :math:`n`. The Tricomi and Gatteschi initial guesses are used in the region where they are accurate. Parameters ---------- n : int Quadrature order Returns ------- xk : ndarray Approximate roots See Also -------- roots_hermite_asy """ # Turnover point # linear polynomial fit to error of 10, 25, 40, ..., 1000 point rules fit = 0.49082003*n - 4.37859653 turnover = around(fit).astype(int) # Compute all approximations ia = arange(1, int(floor(n*0.5)+1)) ib = ia[::-1] xasq = _initial_nodes_a(n, ia[:turnover+1]) xbsq = _initial_nodes_b(n, ib[turnover+1:]) # Combine iv = sqrt(hstack([xasq, xbsq])) # Central node is always zero if n % 2 == 1: iv = hstack([0.0, iv]) return iv def _pbcf(n, theta): r"""Asymptotic series expansion of parabolic cylinder function The implementation is based on sections 3.2 and 3.3 from the original paper. Compared to the published version this code adds one more term to the asymptotic series. The detailed formulas can be found at [parabolic-asymptotics]_. The evaluation is done in a transformed variable :math:`\theta := \arccos(t)` where :math:`t := x / \mu` and :math:`\mu := \sqrt{2n + 1}`. Parameters ---------- n : int Quadrature order theta : ndarray Transformed position variable Returns ------- U : ndarray Value of the parabolic cylinder function :math:`U(a, \theta)`. Ud : ndarray Value of the derivative :math:`U^{\prime}(a, \theta)` of the parabolic cylinder function. See Also -------- roots_hermite_asy References ---------- .. [parabolic-asymptotics] https://dlmf.nist.gov/12.10#vii """ st = sin(theta) ct = cos(theta) # https://dlmf.nist.gov/12.10#vii mu = 2.0*n + 1.0 # https://dlmf.nist.gov/12.10#E23 eta = 0.5*theta - 0.5*st*ct # https://dlmf.nist.gov/12.10#E39 zeta = -(3.0*eta/2.0) ** (2.0/3.0) # https://dlmf.nist.gov/12.10#E40 phi = (-zeta / st**2) ** (0.25) # Coefficients # https://dlmf.nist.gov/12.10#E43 a0 = 1.0 a1 = 0.10416666666666666667 a2 = 0.08355034722222222222 a3 = 0.12822657455632716049 a4 = 0.29184902646414046425 a5 = 0.88162726744375765242 b0 = 1.0 b1 = -0.14583333333333333333 b2 = -0.09874131944444444444 b3 = -0.14331205391589506173 b4 = -0.31722720267841354810 b5 = -0.94242914795712024914 # Polynomials # https://dlmf.nist.gov/12.10#E9 # https://dlmf.nist.gov/12.10#E10 ctp = ct ** arange(16).reshape((-1,1)) u0 = 1.0 u1 = (1.0*ctp[3,:] - 6.0*ct) / 24.0 u2 = (-9.0*ctp[4,:] + 249.0*ctp[2,:] + 145.0) / 1152.0 u3 = (-4042.0*ctp[9,:] + 18189.0*ctp[7,:] - 28287.0*ctp[5,:] - 151995.0*ctp[3,:] - 259290.0*ct) / 414720.0 u4 = (72756.0*ctp[10,:] - 321339.0*ctp[8,:] - 154982.0*ctp[6,:] + 50938215.0*ctp[4,:] + 122602962.0*ctp[2,:] + 12773113.0) / 39813120.0 u5 = (82393456.0*ctp[15,:] - 617950920.0*ctp[13,:] + 1994971575.0*ctp[11,:] - 3630137104.0*ctp[9,:] + 4433574213.0*ctp[7,:] - 37370295816.0*ctp[5,:] - 119582875013.0*ctp[3,:] - 34009066266.0*ct) / 6688604160.0 v0 = 1.0 v1 = (1.0*ctp[3,:] + 6.0*ct) / 24.0 v2 = (15.0*ctp[4,:] - 327.0*ctp[2,:] - 143.0) / 1152.0 v3 = (-4042.0*ctp[9,:] + 18189.0*ctp[7,:] - 36387.0*ctp[5,:] + 238425.0*ctp[3,:] + 259290.0*ct) / 414720.0 v4 = (-121260.0*ctp[10,:] + 551733.0*ctp[8,:] - 151958.0*ctp[6,:] - 57484425.0*ctp[4,:] - 132752238.0*ctp[2,:] - 12118727) / 39813120.0 v5 = (82393456.0*ctp[15,:] - 617950920.0*ctp[13,:] + 2025529095.0*ctp[11,:] - 3750839308.0*ctp[9,:] + 3832454253.0*ctp[7,:] + 35213253348.0*ctp[5,:] + 130919230435.0*ctp[3,:] + 34009066266*ct) / 6688604160.0 # Airy Evaluation (Bi and Bip unused) Ai, Aip, Bi, Bip = airy(mu**(4.0/6.0) * zeta) # Prefactor for U P = 2.0*sqrt(pi) * mu**(1.0/6.0) * phi # Terms for U # https://dlmf.nist.gov/12.10#E42 phip = phi ** arange(6, 31, 6).reshape((-1,1)) A0 = b0*u0 A1 = (b2*u0 + phip[0,:]*b1*u1 + phip[1,:]*b0*u2) / zeta**3 A2 = (b4*u0 + phip[0,:]*b3*u1 + phip[1,:]*b2*u2 + phip[2,:]*b1*u3 + phip[3,:]*b0*u4) / zeta**6 B0 = -(a1*u0 + phip[0,:]*a0*u1) / zeta**2 B1 = -(a3*u0 + phip[0,:]*a2*u1 + phip[1,:]*a1*u2 + phip[2,:]*a0*u3) / zeta**5 B2 = -(a5*u0 + phip[0,:]*a4*u1 + phip[1,:]*a3*u2 + phip[2,:]*a2*u3 + phip[3,:]*a1*u4 + phip[4,:]*a0*u5) / zeta**8 # U # https://dlmf.nist.gov/12.10#E35 U = P * (Ai * (A0 + A1/mu**2.0 + A2/mu**4.0) + Aip * (B0 + B1/mu**2.0 + B2/mu**4.0) / mu**(8.0/6.0)) # Prefactor for derivative of U Pd = sqrt(2.0*pi) * mu**(2.0/6.0) / phi # Terms for derivative of U # https://dlmf.nist.gov/12.10#E46 C0 = -(b1*v0 + phip[0,:]*b0*v1) / zeta C1 = -(b3*v0 + phip[0,:]*b2*v1 + phip[1,:]*b1*v2 + phip[2,:]*b0*v3) / zeta**4 C2 = -(b5*v0 + phip[0,:]*b4*v1 + phip[1,:]*b3*v2 + phip[2,:]*b2*v3 + phip[3,:]*b1*v4 + phip[4,:]*b0*v5) / zeta**7 D0 = a0*v0 D1 = (a2*v0 + phip[0,:]*a1*v1 + phip[1,:]*a0*v2) / zeta**3 D2 = (a4*v0 + phip[0,:]*a3*v1 + phip[1,:]*a2*v2 + phip[2,:]*a1*v3 + phip[3,:]*a0*v4) / zeta**6 # Derivative of U # https://dlmf.nist.gov/12.10#E36 Ud = Pd * (Ai * (C0 + C1/mu**2.0 + C2/mu**4.0) / mu**(4.0/6.0) + Aip * (D0 + D1/mu**2.0 + D2/mu**4.0)) return U, Ud def _newton(n, x_initial, maxit=5): """Newton iteration for polishing the asymptotic approximation to the zeros of the Hermite polynomials. Parameters ---------- n : int Quadrature order x_initial : ndarray Initial guesses for the roots maxit : int Maximal number of Newton iterations. The default 5 is sufficient, usually only one or two steps are needed. Returns ------- nodes : ndarray Quadrature nodes weights : ndarray Quadrature weights See Also -------- roots_hermite_asy """ # Variable transformation mu = sqrt(2.0*n + 1.0) t = x_initial / mu theta = arccos(t) # Newton iteration for i in range(maxit): u, ud = _pbcf(n, theta) dtheta = u / (sqrt(2.0) * mu * sin(theta) * ud) theta = theta + dtheta if max(abs(dtheta)) < 1e-14: break # Undo variable transformation x = mu * cos(theta) # Central node is always zero if n % 2 == 1: x[0] = 0.0 # Compute weights w = exp(-x**2) / (2.0*ud**2) return x, w def _roots_hermite_asy(n): r"""Gauss-Hermite (physicist's) quadrature for large n. Computes the sample points and weights for Gauss-Hermite quadrature. The sample points are the roots of the nth degree Hermite polynomial, :math:`H_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-\infty, \infty]` with weight function :math:`f(x) = e^{-x^2}`. This method relies on asymptotic expansions which work best for n > 150. The algorithm has linear runtime making computation for very large n feasible. Parameters ---------- n : int quadrature order Returns ------- nodes : ndarray Quadrature nodes weights : ndarray Quadrature weights See Also -------- roots_hermite References ---------- .. [townsend.trogdon.olver-2014] Townsend, A. and Trogdon, T. and Olver, S. (2014) *Fast computation of Gauss quadrature nodes and weights on the whole real line*. :arXiv:`1410.5286`. .. [townsend.trogdon.olver-2015] Townsend, A. and Trogdon, T. and Olver, S. (2015) *Fast computation of Gauss quadrature nodes and weights on the whole real line*. IMA Journal of Numerical Analysis :doi:`10.1093/imanum/drv002`. """ iv = _initial_nodes(n) nodes, weights = _newton(n, iv) # Combine with negative parts if n % 2 == 0: nodes = hstack([-nodes[::-1], nodes]) weights = hstack([weights[::-1], weights]) else: nodes = hstack([-nodes[-1:0:-1], nodes]) weights = hstack([weights[-1:0:-1], weights]) # Scale weights weights *= sqrt(pi) / sum(weights) return nodes, weights def hermite(n, monic=False): r"""Physicist's Hermite polynomial. Defined by .. math:: H_n(x) = (-1)^ne^{x^2}\frac{d^n}{dx^n}e^{-x^2}; :math:`H_n` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- H : orthopoly1d Hermite polynomial. Notes ----- The polynomials :math:`H_n` are orthogonal over :math:`(-\infty, \infty)` with weight function :math:`e^{-x^2}`. """ if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_hermite(n1, mu=True) wfunc = lambda x: exp(-x * x) if n == 0: x, w = [], [] hn = 2**n * _gam(n + 1) * sqrt(pi) kn = 2**n p = orthopoly1d(x, w, hn, kn, wfunc, (-inf, inf), monic, lambda x: eval_hermite(n, x)) return p # Hermite 2 He_n(x) def roots_hermitenorm(n, mu=False): r"""Gauss-Hermite (statistician's) quadrature. Compute the sample points and weights for Gauss-Hermite quadrature. The sample points are the roots of the nth degree Hermite polynomial, :math:`He_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-\infty, \infty]` with weight function :math:`w(x) = e^{-x^2/2}`. See 22.2.15 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights Notes ----- For small n up to 150 a modified version of the Golub-Welsch algorithm is used. Nodes are computed from the eigenvalue problem and improved by one step of a Newton iteration. The weights are computed from the well-known analytical formula. For n larger than 150 an optimal asymptotic algorithm is used which computes nodes and weights in a numerical stable manner. The algorithm has linear runtime making computation for very large n (several thousand or more) feasible. See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad numpy.polynomial.hermite_e.hermegauss References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError("n must be a positive integer.") mu0 = np.sqrt(2.0*np.pi) if n <= 150: an_func = lambda k: 0.0*k bn_func = lambda k: np.sqrt(k) f = cephes.eval_hermitenorm df = lambda n, x: n * cephes.eval_hermitenorm(n-1, x) return _gen_roots_and_weights(m, mu0, an_func, bn_func, f, df, True, mu) else: nodes, weights = _roots_hermite_asy(m) # Transform nodes *= sqrt(2) weights *= sqrt(2) if mu: return nodes, weights, mu0 else: return nodes, weights def hermitenorm(n, monic=False): r"""Normalized (probabilist's) Hermite polynomial. Defined by .. math:: He_n(x) = (-1)^ne^{x^2/2}\frac{d^n}{dx^n}e^{-x^2/2}; :math:`He_n` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- He : orthopoly1d Hermite polynomial. Notes ----- The polynomials :math:`He_n` are orthogonal over :math:`(-\infty, \infty)` with weight function :math:`e^{-x^2/2}`. """ if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_hermitenorm(n1, mu=True) wfunc = lambda x: exp(-x * x / 2.0) if n == 0: x, w = [], [] hn = sqrt(2 * pi) * _gam(n + 1) kn = 1.0 p = orthopoly1d(x, w, hn, kn, wfunc=wfunc, limits=(-inf, inf), monic=monic, eval_func=lambda x: eval_hermitenorm(n, x)) return p # The remainder of the polynomials can be derived from the ones above. # Ultraspherical (Gegenbauer) C^(alpha)_n(x) def roots_gegenbauer(n, alpha, mu=False): r"""Gauss-Gegenbauer quadrature. Compute the sample points and weights for Gauss-Gegenbauer quadrature. The sample points are the roots of the nth degree Gegenbauer polynomial, :math:`C^{\alpha}_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-1, 1]` with weight function :math:`w(x) = (1 - x^2)^{\alpha - 1/2}`. See 22.2.3 in [AS]_ for more details. Parameters ---------- n : int quadrature order alpha : float alpha must be > -0.5 mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError("n must be a positive integer.") if alpha < -0.5: raise ValueError("alpha must be greater than -0.5.") elif alpha == 0.0: # C(n,0,x) == 0 uniformly, however, as alpha->0, C(n,alpha,x)->T(n,x) # strictly, we should just error out here, since the roots are not # really defined, but we used to return something useful, so let's # keep doing so. return roots_chebyt(n, mu) mu0 = np.sqrt(np.pi) * cephes.gamma(alpha + 0.5) / cephes.gamma(alpha + 1) an_func = lambda k: 0.0 * k bn_func = lambda k: np.sqrt(k * (k + 2 * alpha - 1) / (4 * (k + alpha) * (k + alpha - 1))) f = lambda n, x: cephes.eval_gegenbauer(n, alpha, x) df = lambda n, x: (-n*x*cephes.eval_gegenbauer(n, alpha, x) + (n + 2*alpha - 1)*cephes.eval_gegenbauer(n-1, alpha, x))/(1-x**2) return _gen_roots_and_weights(m, mu0, an_func, bn_func, f, df, True, mu) def gegenbauer(n, alpha, monic=False): r"""Gegenbauer (ultraspherical) polynomial. Defined to be the solution of .. math:: (1 - x^2)\frac{d^2}{dx^2}C_n^{(\alpha)} - (2\alpha + 1)x\frac{d}{dx}C_n^{(\alpha)} + n(n + 2\alpha)C_n^{(\alpha)} = 0 for :math:`\alpha > -1/2`; :math:`C_n^{(\alpha)}` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- C : orthopoly1d Gegenbauer polynomial. Notes ----- The polynomials :math:`C_n^{(\alpha)}` are orthogonal over :math:`[-1,1]` with weight function :math:`(1 - x^2)^{(\alpha - 1/2)}`. """ base = jacobi(n, alpha - 0.5, alpha - 0.5, monic=monic) if monic: return base # Abrahmowitz and Stegan 22.5.20 factor = (_gam(2*alpha + n) * _gam(alpha + 0.5) / _gam(2*alpha) / _gam(alpha + 0.5 + n)) base._scale(factor) base.__dict__['_eval_func'] = lambda x: eval_gegenbauer(float(n), alpha, x) return base # Chebyshev of the first kind: T_n(x) = # n! sqrt(pi) / _gam(n+1./2)* P^(-1/2,-1/2)_n(x) # Computed anew. def roots_chebyt(n, mu=False): r"""Gauss-Chebyshev (first kind) quadrature. Computes the sample points and weights for Gauss-Chebyshev quadrature. The sample points are the roots of the nth degree Chebyshev polynomial of the first kind, :math:`T_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-1, 1]` with weight function :math:`w(x) = 1/\sqrt{1 - x^2}`. See 22.2.4 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad numpy.polynomial.chebyshev.chebgauss References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError('n must be a positive integer.') x = _ufuncs._sinpi(np.arange(-m + 1, m, 2) / (2*m)) w = np.full_like(x, pi/m) if mu: return x, w, pi else: return x, w def chebyt(n, monic=False): r"""Chebyshev polynomial of the first kind. Defined to be the solution of .. math:: (1 - x^2)\frac{d^2}{dx^2}T_n - x\frac{d}{dx}T_n + n^2T_n = 0; :math:`T_n` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- T : orthopoly1d Chebyshev polynomial of the first kind. Notes ----- The polynomials :math:`T_n` are orthogonal over :math:`[-1, 1]` with weight function :math:`(1 - x^2)^{-1/2}`. See Also -------- chebyu : Chebyshev polynomial of the second kind. """ if n < 0: raise ValueError("n must be nonnegative.") wfunc = lambda x: 1.0 / sqrt(1 - x * x) if n == 0: return orthopoly1d([], [], pi, 1.0, wfunc, (-1, 1), monic, lambda x: eval_chebyt(n, x)) n1 = n x, w, mu = roots_chebyt(n1, mu=True) hn = pi / 2 kn = 2**(n - 1) p = orthopoly1d(x, w, hn, kn, wfunc, (-1, 1), monic, lambda x: eval_chebyt(n, x)) return p # Chebyshev of the second kind # U_n(x) = (n+1)! sqrt(pi) / (2*_gam(n+3./2)) * P^(1/2,1/2)_n(x) def roots_chebyu(n, mu=False): r"""Gauss-Chebyshev (second kind) quadrature. Computes the sample points and weights for Gauss-Chebyshev quadrature. The sample points are the roots of the nth degree Chebyshev polynomial of the second kind, :math:`U_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-1, 1]` with weight function :math:`w(x) = \sqrt{1 - x^2}`. See 22.2.5 in [AS]_ for details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError('n must be a positive integer.') t = np.arange(m, 0, -1) * pi / (m + 1) x = np.cos(t) w = pi * np.sin(t)**2 / (m + 1) if mu: return x, w, pi / 2 else: return x, w def chebyu(n, monic=False): r"""Chebyshev polynomial of the second kind. Defined to be the solution of .. math:: (1 - x^2)\frac{d^2}{dx^2}U_n - 3x\frac{d}{dx}U_n + n(n + 2)U_n = 0; :math:`U_n` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- U : orthopoly1d Chebyshev polynomial of the second kind. Notes ----- The polynomials :math:`U_n` are orthogonal over :math:`[-1, 1]` with weight function :math:`(1 - x^2)^{1/2}`. See Also -------- chebyt : Chebyshev polynomial of the first kind. """ base = jacobi(n, 0.5, 0.5, monic=monic) if monic: return base factor = sqrt(pi) / 2.0 * _gam(n + 2) / _gam(n + 1.5) base._scale(factor) return base # Chebyshev of the first kind C_n(x) def roots_chebyc(n, mu=False): r"""Gauss-Chebyshev (first kind) quadrature. Compute the sample points and weights for Gauss-Chebyshev quadrature. The sample points are the roots of the nth degree Chebyshev polynomial of the first kind, :math:`C_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-2, 2]` with weight function :math:`w(x) = 1 / \sqrt{1 - (x/2)^2}`. See 22.2.6 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ x, w, m = roots_chebyt(n, True) x *= 2 w *= 2 m *= 2 if mu: return x, w, m else: return x, w def chebyc(n, monic=False): r"""Chebyshev polynomial of the first kind on :math:`[-2, 2]`. Defined as :math:`C_n(x) = 2T_n(x/2)`, where :math:`T_n` is the nth Chebychev polynomial of the first kind. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- C : orthopoly1d Chebyshev polynomial of the first kind on :math:`[-2, 2]`. Notes ----- The polynomials :math:`C_n(x)` are orthogonal over :math:`[-2, 2]` with weight function :math:`1/\sqrt{1 - (x/2)^2}`. See Also -------- chebyt : Chebyshev polynomial of the first kind. References ---------- .. [1] Abramowitz and Stegun, "Handbook of Mathematical Functions" Section 22. National Bureau of Standards, 1972. """ if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_chebyc(n1, mu=True) if n == 0: x, w = [], [] hn = 4 * pi * ((n == 0) + 1) kn = 1.0 p = orthopoly1d(x, w, hn, kn, wfunc=lambda x: 1.0 / sqrt(1 - x * x / 4.0), limits=(-2, 2), monic=monic) if not monic: p._scale(2.0 / p(2)) p.__dict__['_eval_func'] = lambda x: eval_chebyc(n, x) return p # Chebyshev of the second kind S_n(x) def roots_chebys(n, mu=False): r"""Gauss-Chebyshev (second kind) quadrature. Compute the sample points and weights for Gauss-Chebyshev quadrature. The sample points are the roots of the nth degree Chebyshev polynomial of the second kind, :math:`S_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-2, 2]` with weight function :math:`w(x) = \sqrt{1 - (x/2)^2}`. See 22.2.7 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ x, w, m = roots_chebyu(n, True) x *= 2 w *= 2 m *= 2 if mu: return x, w, m else: return x, w def chebys(n, monic=False): r"""Chebyshev polynomial of the second kind on :math:`[-2, 2]`. Defined as :math:`S_n(x) = U_n(x/2)` where :math:`U_n` is the nth Chebychev polynomial of the second kind. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- S : orthopoly1d Chebyshev polynomial of the second kind on :math:`[-2, 2]`. Notes ----- The polynomials :math:`S_n(x)` are orthogonal over :math:`[-2, 2]` with weight function :math:`\sqrt{1 - (x/2)}^2`. See Also -------- chebyu : Chebyshev polynomial of the second kind References ---------- .. [1] Abramowitz and Stegun, "Handbook of Mathematical Functions" Section 22. National Bureau of Standards, 1972. """ if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_chebys(n1, mu=True) if n == 0: x, w = [], [] hn = pi kn = 1.0 p = orthopoly1d(x, w, hn, kn, wfunc=lambda x: sqrt(1 - x * x / 4.0), limits=(-2, 2), monic=monic) if not monic: factor = (n + 1.0) / p(2) p._scale(factor) p.__dict__['_eval_func'] = lambda x: eval_chebys(n, x) return p # Shifted Chebyshev of the first kind T^*_n(x) def roots_sh_chebyt(n, mu=False): r"""Gauss-Chebyshev (first kind, shifted) quadrature. Compute the sample points and weights for Gauss-Chebyshev quadrature. The sample points are the roots of the nth degree shifted Chebyshev polynomial of the first kind, :math:`T_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[0, 1]` with weight function :math:`w(x) = 1/\sqrt{x - x^2}`. See 22.2.8 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ xw = roots_chebyt(n, mu) return ((xw[0] + 1) / 2,) + xw[1:] def sh_chebyt(n, monic=False): r"""Shifted Chebyshev polynomial of the first kind. Defined as :math:`T^*_n(x) = T_n(2x - 1)` for :math:`T_n` the nth Chebyshev polynomial of the first kind. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- T : orthopoly1d Shifted Chebyshev polynomial of the first kind. Notes ----- The polynomials :math:`T^*_n` are orthogonal over :math:`[0, 1]` with weight function :math:`(x - x^2)^{-1/2}`. """ base = sh_jacobi(n, 0.0, 0.5, monic=monic) if monic: return base if n > 0: factor = 4**n / 2.0 else: factor = 1.0 base._scale(factor) return base # Shifted Chebyshev of the second kind U^*_n(x) def roots_sh_chebyu(n, mu=False): r"""Gauss-Chebyshev (second kind, shifted) quadrature. Computes the sample points and weights for Gauss-Chebyshev quadrature. The sample points are the roots of the nth degree shifted Chebyshev polynomial of the second kind, :math:`U_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[0, 1]` with weight function :math:`w(x) = \sqrt{x - x^2}`. See 22.2.9 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ x, w, m = roots_chebyu(n, True) x = (x + 1) / 2 m_us = cephes.beta(1.5, 1.5) w *= m_us / m if mu: return x, w, m_us else: return x, w def sh_chebyu(n, monic=False): r"""Shifted Chebyshev polynomial of the second kind. Defined as :math:`U^*_n(x) = U_n(2x - 1)` for :math:`U_n` the nth Chebyshev polynomial of the second kind. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- U : orthopoly1d Shifted Chebyshev polynomial of the second kind. Notes ----- The polynomials :math:`U^*_n` are orthogonal over :math:`[0, 1]` with weight function :math:`(x - x^2)^{1/2}`. """ base = sh_jacobi(n, 2.0, 1.5, monic=monic) if monic: return base factor = 4**n base._scale(factor) return base # Legendre def roots_legendre(n, mu=False): r"""Gauss-Legendre quadrature. Compute the sample points and weights for Gauss-Legendre quadrature. The sample points are the roots of the nth degree Legendre polynomial :math:`P_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[-1, 1]` with weight function :math:`w(x) = 1.0`. See 2.2.10 in [AS]_ for more details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad numpy.polynomial.legendre.leggauss References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ m = int(n) if n < 1 or n != m: raise ValueError("n must be a positive integer.") mu0 = 2.0 an_func = lambda k: 0.0 * k bn_func = lambda k: k * np.sqrt(1.0 / (4 * k * k - 1)) f = cephes.eval_legendre df = lambda n, x: (-n*x*cephes.eval_legendre(n, x) + n*cephes.eval_legendre(n-1, x))/(1-x**2) return _gen_roots_and_weights(m, mu0, an_func, bn_func, f, df, True, mu) def legendre(n, monic=False): r"""Legendre polynomial. Defined to be the solution of .. math:: \frac{d}{dx}\left[(1 - x^2)\frac{d}{dx}P_n(x)\right] + n(n + 1)P_n(x) = 0; :math:`P_n(x)` is a polynomial of degree :math:`n`. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- P : orthopoly1d Legendre polynomial. Notes ----- The polynomials :math:`P_n` are orthogonal over :math:`[-1, 1]` with weight function 1. Examples -------- Generate the 3rd-order Legendre polynomial 1/2*(5x^3 + 0x^2 - 3x + 0): >>> from scipy.special import legendre >>> legendre(3) poly1d([ 2.5, 0. , -1.5, 0. ]) """ if n < 0: raise ValueError("n must be nonnegative.") if n == 0: n1 = n + 1 else: n1 = n x, w, mu0 = roots_legendre(n1, mu=True) if n == 0: x, w = [], [] hn = 2.0 / (2 * n + 1) kn = _gam(2 * n + 1) / _gam(n + 1)**2 / 2.0**n p = orthopoly1d(x, w, hn, kn, wfunc=lambda x: 1.0, limits=(-1, 1), monic=monic, eval_func=lambda x: eval_legendre(n, x)) return p # Shifted Legendre P^*_n(x) def roots_sh_legendre(n, mu=False): r"""Gauss-Legendre (shifted) quadrature. Compute the sample points and weights for Gauss-Legendre quadrature. The sample points are the roots of the nth degree shifted Legendre polynomial :math:`P^*_n(x)`. These sample points and weights correctly integrate polynomials of degree :math:`2n - 1` or less over the interval :math:`[0, 1]` with weight function :math:`w(x) = 1.0`. See 2.2.11 in [AS]_ for details. Parameters ---------- n : int quadrature order mu : bool, optional If True, return the sum of the weights, optional. Returns ------- x : ndarray Sample points w : ndarray Weights mu : float Sum of the weights See Also -------- scipy.integrate.quadrature scipy.integrate.fixed_quad References ---------- .. [AS] Milton Abramowitz and Irene A. Stegun, eds. Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover, 1972. """ x, w = roots_legendre(n) x = (x + 1) / 2 w /= 2 if mu: return x, w, 1.0 else: return x, w def sh_legendre(n, monic=False): r"""Shifted Legendre polynomial. Defined as :math:`P^*_n(x) = P_n(2x - 1)` for :math:`P_n` the nth Legendre polynomial. Parameters ---------- n : int Degree of the polynomial. monic : bool, optional If `True`, scale the leading coefficient to be 1. Default is `False`. Returns ------- P : orthopoly1d Shifted Legendre polynomial. Notes ----- The polynomials :math:`P^*_n` are orthogonal over :math:`[0, 1]` with weight function 1. """ if n < 0: raise ValueError("n must be nonnegative.") wfunc = lambda x: 0.0 * x + 1.0 if n == 0: return orthopoly1d([], [], 1.0, 1.0, wfunc, (0, 1), monic, lambda x: eval_sh_legendre(n, x)) x, w, mu0 = roots_sh_legendre(n, mu=True) hn = 1.0 / (2 * n + 1.0) kn = _gam(2 * n + 1) / _gam(n + 1)**2 p = orthopoly1d(x, w, hn, kn, wfunc, limits=(0, 1), monic=monic, eval_func=lambda x: eval_sh_legendre(n, x)) return p # ----------------------------------------------------------------------------- # Code for backwards compatibility # ----------------------------------------------------------------------------- # Import functions in case someone is still calling the orthogonal # module directly. (They shouldn't be; it's not in the public API). poch = cephes.poch # eval_chebyu, eval_sh_chebyt and eval_sh_chebyu: These functions are not # used in orthogonal.py, they are not in _rootfuns_map, but their names # do appear in _evalfuns, so they must be kept. from ._ufuncs import (binom, eval_jacobi, eval_sh_jacobi, eval_gegenbauer, eval_chebyt, eval_chebyu, eval_chebys, eval_chebyc, eval_sh_chebyt, eval_sh_chebyu, eval_legendre, eval_sh_legendre, eval_genlaguerre, eval_laguerre, eval_hermite, eval_hermitenorm) # Make the old root function names an alias for the new ones _modattrs = globals() for newfun, oldfun in _rootfuns_map.items(): _modattrs[oldfun] = _modattrs[newfun] __all__.append(oldfun)