NAME

Math::GSL::SF - Special Functions

SYNOPSIS

use Math::GSL::SF qw/:all/;

DESCRIPTION

This module contains a data structure named gsl_sf_result. To create a new one use

$r = Math::GSL::SF::gsl_sf_result_struct->new;

You can then access the elements of the structure in this way :

my $val   = $r->{val};

my $error = $r->{err};

Here is a list of all included functions:

gsl_sf_airy_Ai_e($x, $mode)

gsl_sf_airy_Ai($x, $mode, $result)

These routines compute the Airy function Ai($x) with an accuracy specified by $mode. $mode should be $GSL_PREC_DOUBLE, $GSL_PREC_SINGLE or $GSL_PREC_APPROX. $result is a gsl_sf_result structure.

gsl_sf_airy_Bi_e($x, $mode, $result)

gsl_sf_airy_Bi($x, $mode)

These routines compute the Airy function Bi($x) with an accuracy specified by $mode. $mode should be $GSL_PREC_DOUBLE, $GSL_PREC_SINGLE or $GSL_PREC_APPROX. $result is a gsl_sf_result structure.

gsl_sf_airy_Ai_scaled_e($x, $mode, $result)

gsl_sf_airy_Ai_scaled($x, $mode)

These routines compute a scaled version of the Airy function S_A($x) Ai($x). For $x>0 the scaling factor S_A($x) is \exp(+(2/3) $x**(3/2)), and is 1 for $x<0. $result is a gsl_sf_result structure.

gsl_sf_airy_Bi_scaled_e($x, $mode, $result)

gsl_sf_airy_Bi_scaled($x, $mode)

These routines compute a scaled version of the Airy function S_B($x) Bi($x). For $x>0 the scaling factor S_B($x) is exp(-(2/3) $x**(3/2)), and is 1 for $x<0. $result is a gsl_sf_result structure.

gsl_sf_airy_Ai_deriv_e($x, $mode, $result)

gsl_sf_airy_Ai_deriv($x, $mode)

These routines compute the Airy function derivative Ai'($x) with an accuracy specified by $mode. $result is a gsl_sf_result structure.

gsl_sf_airy_Bi_deriv_e($x, $mode, $result)
gsl_sf_airy_Bi_deriv($x, $mode): These routines compute the Airy function derivative Bi'($x) with an accuracy specified by $mode. $result is a gsl_sf_result structure.

gsl_sf_airy_Ai_deriv_scaled_e($x, $mode, $result)
gsl_sf_airy_Ai_deriv_scaled($x, $mode): These routines compute the scaled Airy function derivative S_A(x) Ai'(x). For x>0 the scaling factor S_A(x) is \exp(+(2/3) x^(3/2)), and is 1 for x<0. $result is a gsl_sf_result structure.

gsl_sf_airy_Bi_deriv_scaled_e($x, $mode, $result)
gsl_sf_airy_Bi_deriv_scaled($x, $mode): These routines compute the scaled Airy function derivative S_B(x) Bi'(x). For x>0 the scaling factor S_B(x) is exp(-(2/3) x^(3/2)), and is 1 for x<0. $result is a gsl_sf_result structure.

gsl_sf_airy_zero_Ai_e($s, $result)
gsl_sf_airy_zero_Ai($s): These routines compute the location of the s-th zero of the Airy function Ai($x). $result is a gsl_sf_result structure.

gsl_sf_airy_zero_Bi_e($s, $result)
gsl_sf_airy_zero_Bi($s): These routines compute the location of the s-th zero of the Airy function Bi($x). $result is a gsl_sf_result structure.

gsl_sf_airy_zero_Ai_deriv_e($s, $result)
gsl_sf_airy_zero_Ai_deriv($s): These routines compute the location of the s-th zero of the Airy function derivative Ai'(x). $result is a gsl_sf_result structure.

gsl_sf_airy_zero_Bi_deriv_e($s, $result)

gsl_sf_airy_zero_Bi_deriv($s)

These routines compute the location of the s-th zero of the Airy function derivative Bi'(x). $result is a gsl_sf_result structure.

gsl_sf_bessel_J0_e($x, $result)
gsl_sf_bessel_J0($x): These routines compute the regular cylindrical Bessel function of zeroth order, J_0($x). $result is a gsl_sf_result structure.

gsl_sf_bessel_J1_e($x, $result)

gsl_sf_bessel_J1($x)

These routines compute the regular cylindrical Bessel function of first order, J_1($x). $result is a gsl_sf_result structure.

gsl_sf_bessel_Jn_e($n, $x, $result)
gsl_sf_bessel_Jn($n, $x): These routines compute the regular cylindrical Bessel function of order n, J_n($x).

gsl_sf_bessel_Jn_array($nmin, $nmax, $x, $result_array): This routine computes the values of the regular cylindrical Bessel functions J_n($x) for n from $nmin to $nmax inclusive, storing the results in the array $result_array. The values are computed using recurrence relations for efficiency, and therefore may differ slightly from the exact values.

gsl_sf_bessel_Y0_e($x, $result)

gsl_sf_bessel_Y0($x)

These routines compute the irregular spherical Bessel function of zeroth order, y_0(x) = -\cos(x)/x.

gsl_sf_bessel_Y1_e($x, $result)
gsl_sf_bessel_Y1($x): These routines compute the irregular spherical Bessel function of first order, y_1(x) = -(\cos(x)/x + \sin(x))/x.

gsl_sf_bessel_Yn_e($n, $x, $result)
gsl_sf_bessel_Yn($n, $x): These routines compute the irregular cylindrical Bessel function of order $n, Y_n(x), for x>0.

gsl_sf_bessel_Yn_array

gsl_sf_bessel_I0_e($x, $result)
gsl_sf_bessel_I0($x): These routines compute the regular modified cylindrical Bessel function of zeroth order, I_0(x).

gsl_sf_bessel_I1_e($x, $result)
gsl_sf_bessel_I1($x): These routines compute the regular modified cylindrical Bessel function of first order, I_1(x).

gsl_sf_bessel_In_e($n, $x, $result)
gsl_sf_bessel_In($n, $x): These routines compute the regular modified cylindrical Bessel function of order $n, I_n(x).

gsl_sf_bessel_In_array

gsl_sf_bessel_I0_scaled_e($x, $result)
gsl_sf_bessel_I0_scaled($x): These routines compute the scaled regular modified cylindrical Bessel function of zeroth order \exp(-|x|) I_0(x).

gsl_sf_bessel_I1_scaled_e($x, $result)
gsl_sf_bessel_I1_scaled($x): These routines compute the scaled regular modified cylindrical Bessel function of first order \exp(-|x|) I_1(x).

gsl_sf_bessel_In_scaled_e($n, $x, $result)
gsl_sf_bessel_In_scaled($n, $x): These routines compute the scaled regular modified cylindrical Bessel function of order $n, \exp(-|x|) I_n(x)

gsl_sf_bessel_In_scaled_array

gsl_sf_bessel_K0_e($x, $result)
gsl_sf_bessel_K0($x): These routines compute the irregular modified cylindrical Bessel function of zeroth order, K_0(x), for x > 0.

gsl_sf_bessel_K1_e($x, $result)
gsl_sf_bessel_K1($x): These routines compute the irregular modified cylindrical Bessel function of first order, K_1(x), for x > 0.

gsl_sf_bessel_Kn_e($n, $x, $result)
gsl_sf_bessel_Kn($n, $x): These routines compute the irregular modified cylindrical Bessel function of order $n, K_n(x), for x > 0.

gsl_sf_bessel_Kn_array

gsl_sf_bessel_K0_scaled_e($x, $result)
gsl_sf_bessel_K0_scaled($x): These routines compute the scaled irregular modified cylindrical Bessel function of zeroth order \exp(x) K_0(x) for x>0.

gsl_sf_bessel_K1_scaled_e($x, $result)
gsl_sf_bessel_K1_scaled($x)

gsl_sf_bessel_Kn_scaled_e($n, $x, $result)
gsl_sf_bessel_Kn_scaled($n, $x)

gsl_sf_bessel_Kn_scaled_array

gsl_sf_bessel_j0_e($x, $result)
gsl_sf_bessel_j0($x)

gsl_sf_bessel_j1_e($x, $result)
gsl_sf_bessel_j1($x)

gsl_sf_bessel_j2_e($x, $result)
gsl_sf_bessel_j2($x)

gsl_sf_bessel_jl_e($l, $x, $result)
gsl_sf_bessel_jl($l, $x)

gsl_sf_bessel_jl_array

gsl_sf_bessel_jl_steed_array

gsl_sf_bessel_y0_e($x, $result)
gsl_sf_bessel_y0($x)

gsl_sf_bessel_y1_e($x, $result)
gsl_sf_bessel_y1($x)

gsl_sf_bessel_y2_e($x, $result)
gsl_sf_bessel_y2($x)

gsl_sf_bessel_yl_e($l, $x, $result)
gsl_sf_bessel_yl($l, $x)

gsl_sf_bessel_yl_array

gsl_sf_bessel_i0_scaled_e($x, $result)
gsl_sf_bessel_i0_scaled($x)

gsl_sf_bessel_i1_scaled_e($x, $result)
gsl_sf_bessel_i1_scaled($x)

gsl_sf_bessel_i2_scaled_e($x, $result)
gsl_sf_bessel_i2_scaled($x)

gsl_sf_bessel_il_scaled_e($l, $x, $result)
gsl_sf_bessel_il_scaled($x)

gsl_sf_bessel_il_scaled_array

gsl_sf_bessel_k0_scaled_e($x, $result)
gsl_sf_bessel_k0_scale($x)

gsl_sf_bessel_k1_scaled_e($x, $result)
gsl_sf_bessel_k1_scaled($x)

gsl_sf_bessel_k2_scaled_e($x, $result)
gsl_sf_bessel_k2_scaled($x)

gsl_sf_bessel_kl_scaled_e($l, $x, $result)
gsl_sf_bessel_kl_scaled($l, $x)

gsl_sf_bessel_kl_scaled_array

gsl_sf_bessel_Jnu_e($nu, $x, $result)
gsl_sf_bessel_Jnu($nu, $x)

gsl_sf_bessel_sequence_Jnu_e

gsl_sf_bessel_Ynu_e($nu, $x, $result)
gsl_sf_bessel_Ynu($nu, $x)

gsl_sf_bessel_Inu_scaled_e($nu, $x, $result)
gsl_sf_bessel_Inu_scaled($nu, $x)

gsl_sf_bessel_Inu_e($nu, $x, $result)
gsl_sf_bessel_Inu($nu, $x)

gsl_sf_bessel_Knu_scaled_e($nu, $x, $result)
gsl_sf_bessel_Knu_scaled($nu, $x)

gsl_sf_bessel_Knu_e($nu, $x, $result)
gsl_sf_bessel_Knu($nu, $x)

gsl_sf_bessel_lnKnu_e($nu, $x, $result)
gsl_sf_bessel_lnKnu($nu, $x)

gsl_sf_bessel_zero_J0_e($s, $result)
gsl_sf_bessel_zero_J0($s)

gsl_sf_bessel_zero_J1_e($s, $result)
gsl_sf_bessel_zero_J1($s)

gsl_sf_bessel_zero_Jnu_e($nu, $s, $result)
gsl_sf_bessel_zero_Jnu($nu, $s)

gsl_sf_clausen_e($x, $result)
gsl_sf_clausen($x)

gsl_sf_hydrogenicR_1_e($Z, $r, $result)
gsl_sf_hydrogenicR_1($Z, $r)

gsl_sf_hydrogenicR_e($n, $l, $Z, $r, $result)
gsl_sf_hydrogenicR($n, $l, $Z, $r)

gsl_sf_coulomb_wave_FG_e($eta, $x, $L_F, $k, $F, gsl_sf_result * Fp, gsl_sf_result * G, $Gp) - This function computes the Coulomb wave functions F_L(\eta,x), G_{L-k}(\eta,x) and their derivatives F'_L(\eta,x), G'_{L-k}(\eta,x) with respect to $x. The parameters are restricted to L, L-k > -1/2, x > 0 and integer $k. Note that L itself is not restricted to being an integer. The results are stored in the parameters $F, $G for the function values and $Fp, $Gp for the derivative values. $F, $G, $Fp, $Gp are all gsl_result structs. If an overflow occurs, $GSL_EOVRFLW is returned and scaling exponents are returned as second and third values.
gsl_sf_coulomb_wave_F_array -
gsl_sf_coulomb_wave_FG_array -
gsl_sf_coulomb_wave_FGp_array -
gsl_sf_coulomb_wave_sphF_array -
gsl_sf_coulomb_CL_e($L, $eta, $result) - This function computes the Coulomb wave function normalization constant C_L($eta) for $L > -1.
gsl_sf_coulomb_CL_arrayi -

gsl_sf_coupling_3j_e($two_ja, $two_jb, $two_jc, $two_ma, $two_mb, $two_mc, $result)

gsl_sf_coupling_3j($two_ja, $two_jb, $two_jc, $two_ma, $two_mb, $two_mc)

These routines compute the Wigner 3-j coefficient,
  (ja jb jc
   ma mb mc)
where the arguments are given in half-integer units, ja = $two_ja/2, ma = $two_ma/2, etc.

gsl_sf_coupling_6j_e($two_ja, $two_jb, $two_jc, $two_jd, $two_je, $two_jf, $result)

gsl_sf_coupling_6j($two_ja, $two_jb, $two_jc, $two_jd, $two_je, $two_jf)

These routines compute the Wigner 6-j coefficient,
  {ja jb jc
   jd je jf}
where the arguments are given in half-integer units, ja = $two_ja/2, ma = $two_ma/2, etc.

gsl_sf_coupling_RacahW_e
gsl_sf_coupling_RacahW

gsl_sf_coupling_9j_e($two_ja, $two_jb, $two_jc, $two_jd, $two_je, $two_jf, $two_jg, $two_jh, $two_ji, $result)

gsl_sf_coupling_9j($two_ja, $two_jb, $two_jc, $two_jd, $two_je, $two_jf, $two_jg, $two_jh, $two_ji)

These routines compute the Wigner 9-j coefficient,

         {ja jb jc
          jd je jf
          jg jh ji}
where the arguments are given in half-integer units, ja = two_ja/2, ma = two_ma/2, etc.

gsl_sf_dawson_e($x, $result)
gsl_sf_dawson($x): These routines compute the value of Dawson's integral for $x.

gsl_sf_debye_1_e($x, $result)
gsl_sf_debye_1($x): These routines compute the first-order Debye function D_1(x) = (1/x) \int_0^x dt (t/(e^t - 1)).

gsl_sf_debye_2_e($x, $result)
gsl_sf_debye_2($x): These routines compute the second-order Debye function D_2(x) = (2/x^2) \int_0^x dt (t^2/(e^t - 1)).

gsl_sf_debye_3_e($x, $result)
gsl_sf_debye_3($x): These routines compute the third-order Debye function D_3(x) = (3/x^3) \int_0^x dt (t^3/(e^t - 1)).

gsl_sf_debye_4_e($x, $result)
gsl_sf_debye_4($x): These routines compute the fourth-order Debye function D_4(x) = (4/x^4) \int_0^x dt (t^4/(e^t - 1)).

gsl_sf_debye_5_e($x, $result)
gsl_sf_debye_5($x): These routines compute the fifth-order Debye function D_5(x) = (5/x^5) \int_0^x dt (t^5/(e^t - 1)).

gsl_sf_debye_6_e($x, $result)
gsl_sf_debye_6($x): These routines compute the sixth-order Debye function D_6(x) = (6/x^6) \int_0^x dt (t^6/(e^t - 1)).

gsl_sf_dilog_e ($x, $result)

gsl_sf_dilog($x)

These routines compute the dilogarithm for a real argument. In Lewin's notation this is Li_2(x), the real part of the dilogarithm of a real x. It is defined by the integral representation Li_2(x) = - \Re \int_0^x ds \log(1-s) / s. Note that \Im(Li_2(x)) = 0 for x <= 1, and -\pi\log(x) for x > 1. Note that Abramowitz & Stegun refer to the Spence integral S(x)=Li_2(1-x) as the dilogarithm rather than Li_2(x).

gsl_sf_complex_dilog_xy_e -
gsl_sf_complex_dilog_e($r, $theta, $result_re, $result_im) - This function computes the full complex-valued dilogarithm for the complex argument z = r \exp(i \theta). The real and imaginary parts of the result are returned in the $result_re and $result_im gsl_result structs.
gsl_sf_complex_spence_xy_e -

gsl_sf_multiply
gsl_sf_multiply_e($x, $y, $result) - This function multiplies $x and $y storing the product and its associated error in $result.
gsl_sf_multiply_err_e($x, $dx, $y, $dy, $result) - This function multiplies $x and $y with associated absolute errors $dx and $dy. The product xy +/- xy \sqrt((dx/x)^2 +(dy/y)^2) is stored in $result.

gsl_sf_ellint_Kcomp_e($k, $mode, $result)
gsl_sf_ellint_Kcomp($k, $mode): These routines compute the complete elliptic integral K($k) to the accuracy specified by the mode variable mode. Note that Abramowitz & Stegun define this function in terms of the parameter m = k^2.

gsl_sf_ellint_Ecomp_e($k, $mode, $result)
gsl_sf_ellint_Ecomp($k, $mode)

gsl_sf_ellint_Pcomp_e($k, $n, $mode, $result)
gsl_sf_ellint_Pcomp($k, $n, $mode)

gsl_sf_ellint_Dcomp_e
gsl_sf_ellint_Dcomp

gsl_sf_ellint_F_e($phi, $k, $mode, $result)
gsl_sf_ellint_F($phi, $k, $mode): These routines compute the incomplete elliptic integral F($phi,$k) to the accuracy specified by the mode variable mode. Note that Abramowitz & Stegun define this function in terms of the parameter m = k^2.

gsl_sf_ellint_E_e($phi, $k, $mode, $result)
gsl_sf_ellint_E($phi, $k, $mode): These routines compute the incomplete elliptic integral E($phi,$k) to the accuracy specified by the mode variable mode. Note that Abramowitz & Stegun define this function in terms of the parameter m = k^2.

gsl_sf_ellint_P_e($phi, $k, $n, $mode, $result)
gsl_sf_ellint_P($phi, $k, $n, $mode): These routines compute the incomplete elliptic integral \Pi(\phi,k,n) to the accuracy specified by the mode variable mode. Note that Abramowitz & Stegun define this function in terms of the parameters m = k^2 and \sin^2(\alpha) = k^2, with the change of sign n \to -n.

gsl_sf_ellint_D_e($phi, $k, $n, $mode, $result)
gsl_sf_ellint_D($phi, $k, $n, $mode): These functions compute the incomplete elliptic integral D(\phi,k) which is defined through the Carlson form RD(x,y,z) by the following relation, D(\phi,k,n) = (1/3)(\sin(\phi))^3 RD (1-\sin^2(\phi), 1-k^2 \sin^2(\phi), 1). The argument $n is not used and will be removed in a future release.

gsl_sf_ellint_RC_e($x, $y, $mode, $result)

gsl_sf_ellint_RC($x, $y, $mode)

These routines compute the incomplete elliptic integral RC($x,$y) to the accuracy specified by the mode variable $mode.

gsl_sf_ellint_RD_e($x, $y, $z, $mode, $result)

gsl_sf_ellint_RD($x, $y, $z, $mode)

These routines compute the incomplete elliptic integral RD($x,$y,$z) to the accuracy specified by the mode variable $mode.

gsl_sf_ellint_RF_e($x, $y, $z, $mode, $result)

gsl_sf_ellint_RF($x, $y, $z, $mode)

These routines compute the incomplete elliptic integral RF($x,$y,$z) to the accuracy specified by the mode variable $mode.

gsl_sf_ellint_RJ_e($x, $y, $z, $p, $mode, $result)

gsl_sf_ellint_RJ($x, $y, $z, $p, $mode)

These routines compute the incomplete elliptic integral RJ($x,$y,$z,$p) to the accuracy specified by the mode variable $mode.

gsl_sf_elljac_e($u, $m) - This function computes the Jacobian elliptic functions sn(u|m), cn(u|m), dn(u|m) by descending Landen transformations. The function returns 0 if the operation succeded, 1 otherwise and then returns the result of sn, cn and dn in this order.
gsl_sf_erfc_e($x, $result)
gsl_sf_erfc($x): These routines compute the complementary error function erfc(x) = 1 - erf(x) = (2/\sqrt(\pi)) \int_x^\infty \exp(-t^2).

gsl_sf_log_erfc_e($x, $result)
gsl_sf_log_erfc($x): These routines compute the logarithm of the complementary error function \log(\erfc(x)).

gsl_sf_erf_e($x, $result)
gsl_sf_erf($x): These routines compute the error function erf(x), where erf(x) = (2/\sqrt(\pi)) \int_0^x dt \exp(-t^2).

gsl_sf_erf_Z_e($x, $result)
gsl_sf_erf_Z($x): These routines compute the Gaussian probability density function Z(x) = (1/\sqrt{2\pi}) \exp(-x^2/2).

gsl_sf_erf_Q_e($x, $result)

gsl_sf_erf_Q($x)

These routines compute the upper tail of the Gaussian probability function Q(x) = (1/\sqrt{2\pi}) \int_x^\infty dt \exp(-t^2/2). The hazard function for the normal distribution, also known as the inverse Mill's ratio, is defined as, h(x) = Z(x)/Q(x) = \sqrt{2/\pi} \exp(-x^2 / 2) / \erfc(x/\sqrt 2) It decreases rapidly as x approaches -\infty and asymptotes to h(x) \sim x as x approaches +\infty.

gsl_sf_hazard_e($x, $result)

gsl_sf_hazard($x)

These routines compute the hazard function for the normal distribution.

gsl_sf_exp_e($x, $result)

gsl_sf_exp($x)

These routines provide an exponential function \exp(x) using GSL semantics and error checking.

gsl_sf_exp_e10_e -

gsl_sf_exp_mult_e
gsl_sf_exp_mult

gsl_sf_exp_mult_e10_e -

gsl_sf_expm1_e($x, $result)
gsl_sf_expm1($x): These routines compute the quantity \exp(x)-1 using an algorithm that is accurate for small x.

gsl_sf_exprel_e($x, $result)
gsl_sf_exprel($x): These routines compute the quantity (\exp(x)-1)/x using an algorithm that is accurate for small x. For small x the algorithm is based on the expansion (\exp(x)-1)/x = 1 + x/2 + x^2/(2*3) + x^3/(2*3*4) + \dots.

gsl_sf_exprel_2_e($x, $result)
gsl_sf_exprel_2($x): These routines compute the quantity 2(\exp(x)-1-x)/x^2 using an algorithm that is accurate for small x. For small x the algorithm is based on the expansion 2(\exp(x)-1-x)/x^2 = 1 + x/3 + x^2/(3*4) + x^3/(3*4*5) + \dots.

gsl_sf_exprel_n_e($x, $result)
gsl_sf_exprel_n($x): These routines compute the N-relative exponential, which is the n-th generalization of the functions gsl_sf_exprel and gsl_sf_exprel2. The N-relative exponential is given by, exprel_N(x) = N!/x^N (\exp(x) - \sum_{k=0}^{N-1} x^k/k!) = 1 + x/(N+1) + x^2/((N+1)(N+2)) + ... = 1F1 (1,1+N,x)

gsl_sf_exp_err_e($x, $dx, $result) - This function exponentiates $x with an associated absolute error $dx.
gsl_sf_exp_err_e10_e -
gsl_sf_exp_mult_err_e($x, $dx, $y, $dy, $result) -
gsl_sf_exp_mult_err_e10_e -

gsl_sf_expint_E1_e($x, $result)
gsl_sf_expint_E1($x): These routines compute the exponential integral E_1(x), E_1(x) := \Re \int_1^\infty dt \exp(-xt)/t.

gsl_sf_expint_E2_e($x, $result)
gsl_sf_expint_E2($x): These routines compute the second-order exponential integral E_2(x), E_2(x) := \Re \int_1^\infty dt \exp(-xt)/t^2.

gsl_sf_expint_En_e($n, $x, $result)
gsl_sf_expint_En($n, $x): These routines compute the exponential integral E_n(x) of order n, E_n(x) := \Re \int_1^\infty dt \exp(-xt)/t^n.

gsl_sf_expint_E1_scaled_e
gsl_sf_expint_E1_scaled

gsl_sf_expint_E2_scaled_e
gsl_sf_expint_E2_scaled

gsl_sf_expint_En_scaled_e
gsl_sf_expint_En_scaled

gsl_sf_expint_Ei_e($x, $result)
gsl_sf_expint_Ei($x): These routines compute the exponential integral Ei(x), Ei(x) := - PV(\int_{-x}^\infty dt \exp(-t)/t) where PV denotes the principal value of the integral.

gsl_sf_expint_Ei_scaled_e
gsl_sf_expint_Ei_scaled

gsl_sf_Shi_e($x, $result)
gsl_sf_Shi($x): These routines compute the integral Shi(x) = \int_0^x dt \sinh(t)/t.

gsl_sf_Chi_e($x, $result)
gsl_sf_Chi($x): These routines compute the integral Chi(x) := \Re[ \gamma_E + \log(x) + \int_0^x dt (\cosh[t]-1)/t] , where \gamma_E is the Euler constant (available as $M_EULER from the Math::GSL::Const module).

gsl_sf_expint_3_e($x, $result)
gsl_sf_expint_3($x): These routines compute the third-order exponential integral Ei_3(x) = \int_0^xdt \exp(-t^3) for x >= 0.

gsl_sf_Si_e($x, $result)
gsl_sf_Si($x): These routines compute the Sine integral Si(x) = \int_0^x dt \sin(t)/t.

gsl_sf_Ci_e($x, $result)
gsl_sf_Ci($x): These routines compute the Cosine integral Ci(x) = -\int_x^\infty dt \cos(t)/t for x > 0.

gsl_sf_fermi_dirac_m1_e($x, $result)
gsl_sf_fermi_dirac_m1($x): These routines compute the complete Fermi-Dirac integral with an index of -1. This integral is given by F_{-1}(x) = e^x / (1 + e^x).

gsl_sf_fermi_dirac_0_e($x, $result)
gsl_sf_fermi_dirac_0($x): These routines compute the complete Fermi-Dirac integral with an index of 0. This integral is given by F_0(x) = \ln(1 + e^x).

gsl_sf_fermi_dirac_1_e($x, $result)
gsl_sf_fermi_dirac_1($x): These routines compute the complete Fermi-Dirac integral with an index of 1, F_1(x) = \int_0^\infty dt (t /(\exp(t-x)+1)).

gsl_sf_fermi_dirac_2_e($x, $result)
gsl_sf_fermi_dirac_2($x): These routines compute the complete Fermi-Dirac integral with an index of 2, F_2(x) = (1/2) \int_0^\infty dt (t^2 /(\exp(t-x)+1)).

gsl_sf_fermi_dirac_int_e($j, $x, $result)
gsl_sf_fermi_dirac_int($j, $x): These routines compute the complete Fermi-Dirac integral with an integer index of j, F_j(x) = (1/\Gamma(j+1)) \int_0^\infty dt (t^j /(\exp(t-x)+1)).

gsl_sf_fermi_dirac_mhalf_e($x, $result)
gsl_sf_fermi_dirac_mhalf($x): These routines compute the complete Fermi-Dirac integral F_{-1/2}(x).

gsl_sf_fermi_dirac_half_e($x, $result)
gsl_sf_fermi_dirac_half($x): These routines compute the complete Fermi-Dirac integral F_{1/2}(x).

gsl_sf_fermi_dirac_3half_e($x, $result)
gsl_sf_fermi_dirac_3half($x): These routines compute the complete Fermi-Dirac integral F_{3/2}(x).

gsl_sf_fermi_dirac_inc_0_e($x, $b, $result)
gsl_sf_fermi_dirac_inc_0($x, $b, $result): These routines compute the incomplete Fermi-Dirac integral with an index of zero, F_0(x,b) = \ln(1 + e^{b-x}) - (b-x).

gsl_sf_legendre_Pl_e($l, $x, $result)
gsl_sf_legendre_Pl($l, $x): These functions evaluate the Legendre polynomial P_l(x) for a specific value of l, x subject to l >= 0, |x| <= 1

gsl_sf_legendre_Pl_array
gsl_sf_legendre_Pl_deriv_array

gsl_sf_legendre_P1_e($x, $result)
gsl_sf_legendre_P2_e($x, $result)
gsl_sf_legendre_P3_e($x, $result)
gsl_sf_legendre_P1($x)
gsl_sf_legendre_P2($x)
gsl_sf_legendre_P3($x): These functions evaluate the Legendre polynomials P_l(x) using explicit representations for l=1, 2, 3.

gsl_sf_legendre_Q0_e($x, $result)
gsl_sf_legendre_Q0($x): These routines compute the Legendre function Q_0(x) for x > -1, x != 1.

gsl_sf_legendre_Q1_e($x, $result)
gsl_sf_legendre_Q1($x): These routines compute the Legendre function Q_1(x) for x > -1, x != 1.

gsl_sf_legendre_Ql_e($l, $x, $result)
gsl_sf_legendre_Ql($l, $x): These routines compute the Legendre function Q_l(x) for x > -1, x != 1 and l >= 0.

gsl_sf_legendre_Plm_e($l, $m, $x, $result)
gsl_sf_legendre_Plm($l, $m, $x): These routines compute the associated Legendre polynomial P_l^m(x) for m >= 0, l >= m, |x| <= 1.

gsl_sf_legendre_Plm_array
gsl_sf_legendre_Plm_deriv_array

gsl_sf_legendre_sphPlm_e($l, $m, $x, $result)
gsl_sf_legendre_sphPlm($l, $m, $x): These routines compute the normalized associated Legendre polynomial $\sqrt{(2l+1)/(4\pi)} \sqrt{(l-m)!/(l+m)!} P_l^m(x)$ suitable for use in spherical harmonics. The parameters must satisfy m >= 0, l >= m, |x| <= 1. Theses routines avoid the overflows that occur for the standard normalization of P_l^m(x).

gsl_sf_legendre_sphPlm_array
gsl_sf_legendre_sphPlm_deriv_array

gsl_sf_legendre_array_size -

gsl_sf_lngamma_e($x, $result)
gsl_sf_lngamma($x): These routines compute the logarithm of the Gamma function, \log(\Gamma(x)), subject to x not being a negative integer or zero. For x<0 the real part of \log(\Gamma(x)) is returned, which is equivalent to \log(|\Gamma(x)|). The function is computed using the real Lanczos method.

gsl_sf_lngamma_sgn_e($x, $result_lg) - This routine returns the sign of the gamma function and the logarithm of its magnitude into this order, subject to $x not being a negative integer or zero. The function is computed using the real Lanczos method. The value of the gamma function can be reconstructed using the relation \Gamma(x) = sgn * \exp(resultlg).

gsl_sf_gamma_e
gsl_sf_gamma

gsl_sf_gammastar_e
gsl_sf_gammastar

gsl_sf_gammainv_e
gsl_sf_gammainv

gsl_sf_lngamma_complex_e

gsl_sf_gamma_inc_Q_e
gsl_sf_gamma_inc_Q

gsl_sf_gamma_inc_P_e
gsl_sf_gamma_inc_P

gsl_sf_gamma_inc_e
gsl_sf_gamma_inc

gsl_sf_taylorcoeff_e
gsl_sf_taylorcoeff

gsl_sf_fact_e
gsl_sf_fact

gsl_sf_doublefact_e
gsl_sf_doublefact

gsl_sf_lnfact_e
gsl_sf_lnfact

gsl_sf_lndoublefact_e
gsl_sf_lndoublefact

gsl_sf_lnchoose_e
gsl_sf_lnchoose

gsl_sf_choose_e
gsl_sf_choose

gsl_sf_lnpoch_e
gsl_sf_lnpoch

gsl_sf_lnpoch_sgn_e

gsl_sf_poch_e
gsl_sf_poch

gsl_sf_pochrel_e
gsl_sf_pochrel

gsl_sf_lnbeta_e
gsl_sf_lnbeta

gsl_sf_lnbeta_sgn_e

gsl_sf_beta_e
gsl_sf_beta

gsl_sf_beta_inc_e
gsl_sf_beta_inc

gsl_sf_gegenpoly_1_e
gsl_sf_gegenpoly_2_e
gsl_sf_gegenpoly_3_e
gsl_sf_gegenpoly_1
gsl_sf_gegenpoly_2
gsl_sf_gegenpoly_3

gsl_sf_gegenpoly_n_e
gsl_sf_gegenpoly_n

gsl_sf_gegenpoly_array
gsl_sf_hyperg_0F1_e
gsl_sf_hyperg_0F1

gsl_sf_hyperg_1F1_int_e
gsl_sf_hyperg_1F1_int

gsl_sf_hyperg_1F1_e
gsl_sf_hyperg_1F1

gsl_sf_hyperg_U_int_e
gsl_sf_hyperg_U_int

gsl_sf_hyperg_U_int_e10_e

gsl_sf_hyperg_U_e
gsl_sf_hyperg_U

gsl_sf_hyperg_U_e10_e

gsl_sf_hyperg_2F1_e
gsl_sf_hyperg_2F1

gsl_sf_hyperg_2F1_conj_e
gsl_sf_hyperg_2F1_conj

gsl_sf_hyperg_2F1_renorm_e
gsl_sf_hyperg_2F1_renorm

gsl_sf_hyperg_2F1_conj_renorm_e
gsl_sf_hyperg_2F1_conj_renorm

gsl_sf_hyperg_2F0_e
gsl_sf_hyperg_2F0

gsl_sf_laguerre_1_e
gsl_sf_laguerre_2_e
gsl_sf_laguerre_3_e
gsl_sf_laguerre_1
gsl_sf_laguerre_2
gsl_sf_laguerre_3

gsl_sf_laguerre_n_e
gsl_sf_laguerre_n

gsl_sf_lambert_W0_e
gsl_sf_lambert_W0

gsl_sf_lambert_Wm1_e
gsl_sf_lambert_Wm1

gsl_sf_conicalP_half_e
gsl_sf_conicalP_half

gsl_sf_conicalP_mhalf_e
gsl_sf_conicalP_mhalf

gsl_sf_conicalP_0_e
gsl_sf_conicalP_0

gsl_sf_conicalP_1_e
gsl_sf_conicalP_1

gsl_sf_conicalP_sph_reg_e
gsl_sf_conicalP_sph_reg

gsl_sf_conicalP_cyl_reg_e
gsl_sf_conicalP_cyl_reg

gsl_sf_legendre_H3d_0_e
gsl_sf_legendre_H3d_0

gsl_sf_legendre_H3d_1_e
gsl_sf_legendre_H3d_1

gsl_sf_legendre_H3d_e
gsl_sf_legendre_H3d

gsl_sf_legendre_H3d_array

gsl_sf_log_e
gsl_sf_log

gsl_sf_log_abs_e
gsl_sf_log_abs

gsl_sf_complex_log_e

gsl_sf_log_1plusx_e
gsl_sf_log_1plusx

gsl_sf_log_1plusx_mx_e
gsl_sf_log_1plusx_mx

gsl_sf_mathieu_a_array
gsl_sf_mathieu_b_array

gsl_sf_mathieu_a
gsl_sf_mathieu_b

gsl_sf_mathieu_a_coeff
gsl_sf_mathieu_b_coeff

gsl_sf_mathieu_alloc

gsl_sf_mathieu_free

gsl_sf_mathieu_ce
gsl_sf_mathieu_se

gsl_sf_mathieu_ce_array
gsl_sf_mathieu_se_array

gsl_sf_mathieu_Mc
gsl_sf_mathieu_Ms

gsl_sf_mathieu_Mc_array
gsl_sf_mathieu_Ms_array

gsl_sf_pow_int_e
gsl_sf_pow_int

gsl_sf_psi_int_e
gsl_sf_psi_int

gsl_sf_psi_e
gsl_sf_psi

gsl_sf_psi_1piy_e
gsl_sf_psi_1piy

gsl_sf_complex_psi_e

gsl_sf_psi_1_int_e
gsl_sf_psi_1_int

gsl_sf_psi_1_e
gsl_sf_psi_1

gsl_sf_psi_n_e
gsl_sf_psi_n

gsl_sf_result_smash_e

gsl_sf_synchrotron_1_e
gsl_sf_synchrotron_1

gsl_sf_synchrotron_2_e
gsl_sf_synchrotron_2

gsl_sf_transport_2_e
gsl_sf_transport_2

gsl_sf_transport_3_e
gsl_sf_transport_3

gsl_sf_transport_4_e
gsl_sf_transport_4

gsl_sf_transport_5_e
gsl_sf_transport_5

gsl_sf_sin_e
gsl_sf_sin

gsl_sf_cos_e
gsl_sf_cos

gsl_sf_hypot_e
gsl_sf_hypot

gsl_sf_complex_sin_e

gsl_sf_complex_cos_e

gsl_sf_complex_logsin_e

gsl_sf_sinc_e
gsl_sf_sinc

gsl_sf_lnsinh_e
gsl_sf_lnsinh

gsl_sf_lncosh_e
gsl_sf_lncosh

gsl_sf_polar_to_rect

gsl_sf_rect_to_polar

gsl_sf_sin_err_e
gsl_sf_cos_err_e

gsl_sf_angle_restrict_symm_e
gsl_sf_angle_restrict_symm

gsl_sf_angle_restrict_pos_e
gsl_sf_angle_restrict_pos

gsl_sf_angle_restrict_symm_err_e

gsl_sf_angle_restrict_pos_err_e

gsl_sf_atanint_e
gsl_sf_atanint: These routines compute the Arctangent integral, which is defined as AtanInt(x) = \int_0^x dt \arctan(t)/t.

gsl_sf_zeta_int_e

gsl_sf_zeta_int

gsl_sf_zeta_e gsl_sf_zeta

gsl_sf_zetam1_e

gsl_sf_zetam1

gsl_sf_zetam1_int_e

gsl_sf_zetam1_int

gsl_sf_hzeta_e

gsl_sf_hzeta

gsl_sf_eta_int_e

gsl_sf_eta_int

gsl_sf_eta_e

gsl_sf_eta

This module also contains the following constants used as mode in various of those functions :

GSL_PREC_DOUBLE - Double-precision, a relative accuracy of approximately 2 * 10^-16.
GSL_PREC_SINGLE - Single-precision, a relative accuracy of approximately 10^-7.
GSL_PREC_APPROX - Approximate values, a relative accuracy of approximately 5 * 10^-4.

You can import the functions that you want to use by giving a space separated
list to Math::GSL::SF when you use the package.  You can also write 
use Math::GSL::SF qw/:all/ 
to use all avaible functions of the module. Note that
the tag names begin with a colon.  Other tags are also available, here is a
complete list of all tags for this module :

airy
bessel
clausen
hydrogenic
coulumb
coupling
dawson
debye
dilog
factorial
misc
elliptic
error
hypergeometric
laguerre
legendre
gamma
transport
trig
zeta
eta
vars

For more informations on the functions, we refer you to the GSL offcial documentation: http://www.gnu.org/software/gsl/manual/html_node/

EXAMPLES

This example computes the dilogarithm of 1/10 :

use Math::GSL::SF qw/dilog/;
my $x = gsl_sf_dilog(0.1);
print "gsl_sf_dilog(0.1) = $x\n";

An example using Math::GSL::SF and gnuplot is in the examples/sf folder of the source code.

AUTHORS

Jonathan "Duke" Leto <jonathan@leto.net> and Thierry Moisan <thierry.moisan@gmail.com>

COPYRIGHT AND LICENSE

This program is free software; you can redistribute it and/or modify it under the same terms as Perl itself.

To install Math::GSL, copy and paste the appropriate command in to your terminal.

cpanm

cpanm Math::GSL

CPAN shell

perl -MCPAN -e shell
install Math::GSL

For more information on module installation, please visit the detailed CPAN module installation guide.

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