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1
2 [section:mbessel Modified Bessel Functions of the First and Second Kinds]
3
4 [h4 Synopsis]
5
6 `#include <boost/math/special_functions/bessel.hpp>`
7
8 template <class T1, class T2>
9 ``__sf_result`` cyl_bessel_i(T1 v, T2 x);
10
11 template <class T1, class T2, class ``__Policy``>
12 ``__sf_result`` cyl_bessel_i(T1 v, T2 x, const ``__Policy``&);
13
14 template <class T1, class T2>
15 ``__sf_result`` cyl_bessel_k(T1 v, T2 x);
16
17 template <class T1, class T2, class ``__Policy``>
18 ``__sf_result`` cyl_bessel_k(T1 v, T2 x, const ``__Policy``&);
19
20
21 [h4 Description]
22
23 The functions __cyl_bessel_i and __cyl_bessel_k return the result of the
24 modified Bessel functions of the first and second kind respectively:
25
26 cyl_bessel_i(v, x) = I[sub v](x)
27
28 cyl_bessel_k(v, x) = K[sub v](x)
29
30 where:
31
32 [equation mbessel2]
33
34 [equation mbessel3]
35
36 The return type of these functions is computed using the __arg_promotion_rules
37 when T1 and T2 are different types. The functions are also optimised for the
38 relatively common case that T1 is an integer.
39
40 [optional_policy]
41
42 The functions return the result of __domain_error whenever the result is
43 undefined or complex. For __cyl_bessel_j this occurs when `x < 0` and v is not
44 an integer, or when `x == 0` and `v != 0`. For __cyl_neumann this occurs
45 when `x <= 0`.
46
47 The following graph illustrates the exponential behaviour of I[sub v].
48
49 [graph cyl_bessel_i]
50
51 The following graph illustrates the exponential decay of K[sub v].
52
53 [graph cyl_bessel_k]
54
55 [h4 Testing]
56
57 There are two sets of test values: spot values calculated using
58 [@http://functions.wolfram.com functions.wolfram.com],
59 and a much larger set of tests computed using
60 a simplified version of this implementation
61 (with all the special case handling removed).
62
63 [h4 Accuracy]
64
65 The following tables show how the accuracy of these functions
66 varies on various platforms, along with comparison to other libraries.
67 Note that only results for the widest floating-point type on the
68 system are given, as narrower types have __zero_error. All values
69 are relative errors in units of epsilon. Note that our test suite
70 includes some fairly extreme inputs which results in most of the worst
71 problem cases in other libraries:
72
73 [table_cyl_bessel_i_integer_orders_]
74
75 [table_cyl_bessel_i]
76
77 [table_cyl_bessel_k_integer_orders_]
78
79 [table_cyl_bessel_k]
80
81 [h4 Implementation]
82
83 The following are handled as special cases first:
84
85 When computing I[sub v][space] for ['x < 0], then [nu][space] must be an integer
86 or a domain error occurs. If [nu][space] is an integer, then the function is
87 odd if [nu][space] is odd and even if [nu][space] is even, and we can reflect to
88 ['x > 0].
89
90 For I[sub v][space] with v equal to 0, 1 or 0.5 are handled as special cases.
91
92 The 0 and 1 cases use minimax rational approximations on
93 finite and infinite intervals. The coefficients are from:
94
95 * J.M. Blair and C.A. Edwards, ['Stable rational minimax approximations
96 to the modified Bessel functions I_0(x) and I_1(x)], Atomic Energy of Canada
97 Limited Report 4928, Chalk River, 1974.
98 * S. Moshier, ['Methods and Programs for Mathematical Functions],
99 Ellis Horwood Ltd, Chichester, 1989.
100
101 While the 0.5 case is a simple trigonometric function:
102
103 I[sub 0.5](x) = sqrt(2 / [pi]x) * sinh(x)
104
105 For K[sub v][space] with /v/ an integer, the result is calculated using the
106 recurrence relation:
107
108 [equation mbessel5]
109
110 starting from K[sub 0][space] and K[sub 1][space] which are calculated
111 using rational the approximations above. These rational approximations are
112 accurate to around 19 digits, and are therefore only used when T has
113 no more than 64 binary digits of precision.
114
115 When /x/ is small compared to /v/, I[sub v]x[space] is best computed directly from the series:
116
117 [equation mbessel17]
118
119 In the general case, we first normalize [nu][space] to \[[^0, [inf]])
120 with the help of the reflection formulae:
121
122 [equation mbessel9]
123
124 [equation mbessel10]
125
126 Let [mu][space] = [nu] - floor([nu] + 1/2), then [mu][space] is the fractional part of
127 [nu][space] such that |[mu]| <= 1/2 (we need this for convergence later). The idea is to
128 calculate K[sub [mu]](x) and K[sub [mu]+1](x), and use them to obtain
129 I[sub [nu]](x) and K[sub [nu]](x).
130
131 The algorithm is proposed by Temme in
132 N.M. Temme, ['On the numerical evaluation of the modified bessel function
133 of the third kind], Journal of Computational Physics, vol 19, 324 (1975),
134 which needs two continued fractions as well as the Wronskian:
135
136 [equation mbessel11]
137
138 [equation mbessel12]
139
140 [equation mbessel8]
141
142 The continued fractions are computed using the modified Lentz's method
143 (W.J. Lentz, ['Generating Bessel functions in Mie scattering calculations
144 using continued fractions], Applied Optics, vol 15, 668 (1976)).
145 Their convergence rates depend on ['x], therefore we need
146 different strategies for large ['x] and small ['x].
147
148 ['x > v], CF1 needs O(['x]) iterations to converge, CF2 converges rapidly.
149
150 ['x <= v], CF1 converges rapidly, CF2 fails to converge when ['x] [^->] 0.
151
152 When ['x] is large (['x] > 2), both continued fractions converge (CF1
153 may be slow for really large ['x]). K[sub [mu]][space] and K[sub [mu]+1][space]
154 can be calculated by
155
156 [equation mbessel13]
157
158 where
159
160 [equation mbessel14]
161
162 ['S] is also a series that is summed along with CF2, see
163 I.J. Thompson and A.R. Barnett, ['Modified Bessel functions I_v and K_v
164 of real order and complex argument to selected accuracy], Computer Physics
165 Communications, vol 47, 245 (1987).
166
167 When ['x] is small (['x] <= 2), CF2 convergence may fail (but CF1
168 works very well). The solution here is Temme's series:
169
170 [equation mbessel15]
171
172 where
173
174 [equation mbessel16]
175
176 f[sub k][space] and h[sub k][space]
177 are also computed by recursions (involving gamma functions), but the
178 formulas are a little complicated, readers are referred to
179 N.M. Temme, ['On the numerical evaluation of the modified Bessel function
180 of the third kind], Journal of Computational Physics, vol 19, 324 (1975).
181 Note: Temme's series converge only for |[mu]| <= 1/2.
182
183 K[sub [nu]](x) is then calculated from the forward
184 recurrence, as is K[sub [nu]+1](x). With these two values and
185 f[sub [nu]], the Wronskian yields I[sub [nu]](x) directly.
186
187 [endsect]
188
189 [/
190 Copyright 2006 John Maddock, Paul A. Bristow and Xiaogang Zhang.
191 Distributed under the Boost Software License, Version 1.0.
192 (See accompanying file LICENSE_1_0.txt or copy at
193 http://www.boost.org/LICENSE_1_0.txt).
194 ]