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ROOT
6.06/09
Reference Guide
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Definition at line 38 of file KelvinFunctions.h.
Public Member Functions | |
virtual | ~KelvinFunctions () |
Static Public Member Functions | |
static double | Ber (double x) |
Begin_Latex Ber(x) = Ber_{0}(x) = Re::left[J_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex J_{0}(z) End_Latex is the zeroth-order Bessel function of the first kind. More... | |
static double | Bei (double x) |
Begin_Latex Bei(x) = Bei_{0}(x) = Im::left[J_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex J_{0}(z) End_Latex is the zeroth-order Bessel function of the first kind. More... | |
static double | Ker (double x) |
Begin_Latex Ker(x) = Ker_{0}(x) = Re::left[K_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex K_{0}(z) End_Latex is the zeroth-order modified Bessel function of the second kind. More... | |
static double | Kei (double x) |
Begin_Latex Kei(x) = Kei_{0}(x) = Im::left[K_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex K_{0}(z) End_Latex is the zeroth-order modified Bessel function of the second kind. More... | |
static double | DBer (double x) |
Calculates the first derivative of Ber(x). More... | |
static double | DBei (double x) |
Calculates the first derivative of Bei(x). More... | |
static double | DKer (double x) |
Calculates the first derivative of Ker(x). More... | |
static double | DKei (double x) |
Calculates the first derivative of Kei(x). More... | |
static double | F1 (double x) |
Utility function appearing in the calculations of the Kelvin functions Bei(x) and Ber(x) (and their derivatives). More... | |
static double | F2 (double x) |
Utility function appearing in the calculations of the Kelvin functions Kei(x) and Ker(x) (and their derivatives). More... | |
static double | G1 (double x) |
Utility function appearing in the calculations of the Kelvin functions Bei(x) and Ber(x) (and their derivatives). More... | |
static double | G2 (double x) |
Utility function appearing in the calculations of the Kelvin functions Kei(x) and Ker(x) (and their derivatives). More... | |
static double | M (double x) |
Utility function appearing in the asymptotic expansions of DBer(x) and DBei(x). More... | |
static double | Theta (double x) |
Utility function appearing in the asymptotic expansions of DBer(x) and DBei(x). More... | |
static double | N (double x) |
Utility function appearing in the asymptotic expansions of DKer(x) and DKei(x). More... | |
static double | Phi (double x) |
Utility function appearing in the asymptotic expansions of DKer(x) and DKei(x). More... | |
Static Protected Attributes | |
static double | fgMin = 20 |
static double | fgEpsilon = 1.e-20 |
#include <Math/KelvinFunctions.h>
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Definition at line 63 of file KelvinFunctions.h.
Begin_Latex Bei(x) = Bei_{0}(x) = Im::left[J_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex J_{0}(z) End_Latex is the zeroth-order Bessel function of the first kind.
If x < fgMin (=20), Bei(x) is computed according to its polynomial approximation Begin_Latex Bei(x) = #sum_{n #geq 0}#frac{(-1)^{n}(x/2)^{4n+2}}{[(2n+1)!]^{2}} End_Latex For x > fgMin, Bei(x) is computed according to its asymptotic expansion: Begin_Latex Bei(x) = #frac{e^{x/sqrt{2}}}{sqrt{2#pix}} [F1(x) sin::alpha + G1(x) cos::alpha] - #frac{1}{pi}Ker(x) End_Latex where Begin_Latex #alpha = #frac{x}{sqrt{2}} - #frac{pi}{8} End_Latex See also F1(x) and G1(x).{
Definition at line 133 of file KelvinFunctions.cxx.
Begin_Latex Ber(x) = Ber_{0}(x) = Re::left[J_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex J_{0}(z) End_Latex is the zeroth-order Bessel function of the first kind.
If x < fgMin (=20), Ber(x) is computed according to its polynomial approximation Begin_Latex Ber(x) = 1 + #sum_{n #geq 1}#frac{(-1)^{n}(x/2)^{4n}}{[(2n)!]^{2}} End_Latex For x > fgMin, Ber(x) is computed according to its asymptotic expansion: Begin_Latex Ber(x) = #frac{e^{x/sqrt{2}}}{sqrt{2#pix}} [F1(x) cos::alpha + G1(x) sin::alpha] - #frac{1}{pi}Kei(x) End_Latex where Begin_Latex #alpha = #frac{x}{sqrt{2}} - #frac{pi}{8} End_Latex. See also F1(x) and G1(x).{
Definition at line 76 of file KelvinFunctions.cxx.
Calculates the first derivative of Bei(x).
If x < fgMin (=20), DBei(x) is computed according to the derivative of the polynomial approximation of Bei(x). Otherwise it is computed according to its asymptotic expansion Begin_Latex #frac{d}{dx} Bei(x) = M sin::left(#theta - #frac{pi}{4}#right) End_Latex See also M(x) and Theta(x).{
Definition at line 360 of file KelvinFunctions.cxx.
Calculates the first derivative of Ber(x).
If x < fgMin (=20), DBer(x) is computed according to the derivative of the polynomial approximation of Ber(x). Otherwise it is computed according to its asymptotic expansion Begin_Latex #frac{d}{dx} Ber(x) = M cos::left(#theta - #frac{pi}{4}#right) End_Latex See also M(x) and Theta(x).{
Definition at line 315 of file KelvinFunctions.cxx.
Calculates the first derivative of Kei(x).
If x < fgMin (=20), DKei(x) is computed according to the derivative of the polynomial approximation of Kei(x). Otherwise it is computed according to its asymptotic expansion Begin_Latex #frac{d}{dx} Kei(x) = N sin::left(#phi - #frac{pi}{4}#right) End_Latex See also N(x) and Phi(x).{
Definition at line 453 of file KelvinFunctions.cxx.
Calculates the first derivative of Ker(x).
If x < fgMin (=20), DKer(x) is computed according to the derivative of the polynomial approximation of Ker(x). Otherwise it is computed according to its asymptotic expansion Begin_Latex #frac{d}{dx} Ker(x) = N cos::left(#phi - #frac{pi}{4}#right) End_Latex See also N(x) and Phi(x).{
Definition at line 405 of file KelvinFunctions.cxx.
Utility function appearing in the calculations of the Kelvin functions Bei(x) and Ber(x) (and their derivatives).
F1(x) is given by Begin_Latex F1(x) = 1 + #sum_{n #geq 1} #frac{#prod_{m=1}^{n}(2m - 1)^{2}}{n! (8x)^{n}} cos::left(#frac{n::pi}{4}#right) End_Latex
Definition at line 488 of file KelvinFunctions.cxx.
Utility function appearing in the calculations of the Kelvin functions Kei(x) and Ker(x) (and their derivatives).
F2(x) is given by Begin_Latex F2(x) = 1 + #sum_{n #geq 1} (-1)^{n} #frac{#prod_{m=1}^{n}(2m - 1)^{2}}{n! (8x)^{n}} cos::left(#frac{n::pi}{4}#right) End_Latex
Definition at line 517 of file KelvinFunctions.cxx.
Utility function appearing in the calculations of the Kelvin functions Bei(x) and Ber(x) (and their derivatives).
G1(x) is given by Begin_Latex G1(x) = #sum_{n #geq 1} #frac{#prod_{m=1}^{n}(2m - 1)^{2}}{n! (8x)^{n}} sin::left(#frac{n::pi}{4}#right) End_Latex
Definition at line 548 of file KelvinFunctions.cxx.
Utility function appearing in the calculations of the Kelvin functions Kei(x) and Ker(x) (and their derivatives).
G2(x) is given by Begin_Latex G2(x) = #sum_{n #geq 1} (-1)^{n} #frac{#prod_{m=1}^{n}(2m - 1)^{2}}{n! (8x)^{n}} sin::left(#frac{n::pi}{4}#right) End_Latex
Definition at line 575 of file KelvinFunctions.cxx.
Begin_Latex Kei(x) = Kei_{0}(x) = Im::left[K_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex K_{0}(z) End_Latex is the zeroth-order modified Bessel function of the second kind.
If x < fgMin (=20), Kei(x) is computed according to its polynomial approximation Begin_Latex Kei(x) = -#left(ln #frac{x}{2} + #gamma#right) Bei(x) - #left(#frac{pi}{4} - #delta#right) Ber(x) + #sum_{n #geq 0} #frac{(-1)^{n}}{[(2n)!]^{2}} H_{2n} #left(#frac{x}{2}#right)^{4n+2} End_Latex where Begin_Latex #gamma = 0.577215664... End_Latex is the Euler-Mascheroni constant, Begin_Latex #delta = pi End_Latex for x < 0 and is otherwise zero, and Begin_Latex H_{n} = #sum_{k = 1}^{n} #frac{1}{k} End_Latex For x > fgMin, Kei(x) is computed according to its asymptotic expansion: Begin_Latex Kei(x) = - sqrt{#frac{pi}{2x}} e^{-x/sqrt{2}} [F2(x) sin::beta + G2(x) cos::beta] End_Latex where Begin_Latex beta = #frac{x}{sqrt{2}} + #frac{pi}{8} End_Latex See also F2(x) and G2(x).{
Definition at line 263 of file KelvinFunctions.cxx.
Referenced by Ber().
Begin_Latex Ker(x) = Ker_{0}(x) = Re::left[K_{0}#left(x e^{3#pii/4}#right)#right] End_Latex where x is real, and Begin_Latex K_{0}(z) End_Latex is the zeroth-order modified Bessel function of the second kind.
If x < fgMin (=20), Ker(x) is computed according to its polynomial approximation Begin_Latex Ker(x) = -#left(ln #frac{|x|}{2} + #gamma#right) Ber(x) + #left(#frac{pi}{4} - #delta#right) Bei(x) + #sum_{n #geq 0} #frac{(-1)^{n}}{[(2n)!]^{2}} H_{2n} #left(#frac{x}{2}#right)^{4n} End_Latex where Begin_Latex #gamma = 0.577215664... End_Latex is the Euler-Mascheroni constant, Begin_Latex #delta = pi End_Latex for x < 0 and is otherwise zero, and Begin_Latex H_{n} = #sum_{k = 1}^{n} #frac{1}{k} End_Latex For x > fgMin, Ker(x) is computed according to its asymptotic expansion: Begin_Latex Ker(x) = sqrt{#frac{pi}{2x}} e^{-x/sqrt{2}} [F2(x) cos::beta + G2(x) sin::beta] End_Latex where Begin_Latex beta = #frac{x}{sqrt{2}} + #frac{pi}{8} End_Latex See also F2(x) and G2(x).{
Definition at line 197 of file KelvinFunctions.cxx.
Referenced by Bei().
Utility function appearing in the asymptotic expansions of DBer(x) and DBei(x).
M(x) is given by Begin_Latex M(x) = #frac{e^{x/sqrt{2}}}{sqrt{2#pix}}#left(1 + #frac{1}{8sqrt{2} x} + #frac{1}{256 x^{2}} - #frac{399}{6144sqrt{2} x^{3}} + O::left(#frac{1}{x^{4}}#right)#right) End_Latex
Definition at line 604 of file KelvinFunctions.cxx.
Utility function appearing in the asymptotic expansions of DKer(x) and DKei(x).
(x) is given by Begin_Latex N(x) = sqrt{#frac{pi}{2x}} e^{-x/sqrt{2}} #left(1 - #frac{1}{8sqrt{2} x} + #frac{1}{256 x^{2}} + #frac{399}{6144sqrt{2} x^{3}} + O::left(#frac{1}{x^{4}}#right)#right) End_Latex
Definition at line 636 of file KelvinFunctions.cxx.
Utility function appearing in the asymptotic expansions of DKer(x) and DKei(x).
Begin_Latex #phi(x) #End_Latex is given by Begin_Latex #phi(x) = - #frac{x}{sqrt{2}} - #frac{pi}{8} + #frac{1}{8sqrt{2} x} - #frac{1}{16 x^{2}} + #frac{25}{384sqrt{2} x^{3}} + O::left(#frac{1}{x^{5}}#right) End_Latex
Definition at line 652 of file KelvinFunctions.cxx.
Utility function appearing in the asymptotic expansions of DBer(x) and DBei(x).
Begin_Latex #theta(x) #End_Latex is given by Begin_Latex #theta(x) = #frac{x}{sqrt{2}} - #frac{pi}{8} - #frac{1}{8sqrt{2} x} - #frac{1}{16 x^{2}} - #frac{25}{384sqrt{2} x^{3}} + O::left(#frac{1}{x^{5}}#right) End_Latex
Definition at line 620 of file KelvinFunctions.cxx.
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