New series expansions of the Gauss hypergeometric function
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1 New series expansions of the Gauss hypergeometric function José L. López and Nico. M. Temme 2 Departamento de Matemática e Informática, Universidad Pública de Navarra, 36-Pamplona, Spain. jl.lopez@unavarra.es. 2 CWI, Science Park 23, 98 XG Amsterdam, The Netherlands. Nico.Temme@cwi.nl. ABSTRACT. The Gauss hypergeometric function 2 F (a, b, c; z) can be computed by using the power series in powers of z, z/(z ), z, /z, /( z), (z )/z. With these expansions 2 F (a, b, c; z) is not completely computable for all complex values of z. As pointed out in Gil, et al. [27, 2.3], the points z = e ±iπ/3 are always excluded from the domains of convergence of these expansions. Bühring [987] has given a power series expansion that allows computation at and near these points. But, when b a is an integer, the coefficients of that expansion become indeterminate and its computation requires a nontrivial limiting process. Moreover, the convergence becomes slower and slower in that case. In this paper we obtain new expansions of the Gauss hypergeometric function in terms of rational functions of z for which the points z = e ±iπ/3 are well inside their domains of convergence. In addition, these expansion are well defined when b a is an integer and no limits are needed in that case. Numerical computations show that these expansions converge faster than Bühring s expansion for z in the neighborhood of the points e ±iπ/3, especially when b a is close to an integer number. 2 AMS Mathematics Subject Classification: 33C5; 4A58; 4A2, 65D2 Keywords & Phrases: Gauss hypergeometric function. Approximation by rational functions. Two and three-point Taylor expansions.. Introduction The power series of the Gauss hypergeometric function 2 F (a, b, c; z), 2F (a, b, c; z) = (a) n (b) n z n, () (c) n n! converges inside the unit disk. For numerical computations we can use the right hand side of () to compute 2F (a, b, c; z) only in the disk z ρ <, with ρ depending on numerical requirements, such as precision and efficiency. From [[3], 2.3. and 2.3.2] or [[7], eq and 5.8(i) and 5.8(ii)], we see that the Gauss hypergeometric function 2 F (a, b, c; z) may be written in terms of one or two other 2 F functions with any of the following arguments z, z, z, z z, z. (2) z
2 As explained in [[3], 2.3.2], when these formulas are combined with the series expansion (), we obtain a set of series expansions of 2 F (a, b, c; z) in powers of some of the rational functions given in (2). The domains of convergence of the whole set of the expansions obtained in this way are the regions z ρ <, z ρ <, z ρ <, z ρ <, z z ρ <, z z ρ <. (3) These regions (interior or exterior of certain circles) do not cover the entire z plane, the points z = e ±iπ/3, that are the intersection points of the circles z = and z =, are excluded for any value of ρ < (see Fig. ). 2 = = Figure. Regions given by formulas (3) for two particular values of ρ. The points e ±iπ/3 are indicated by black dots. When ρ, the set of points of the z plane excluded from the union of these regions shrinks to the exceptional points z = e ±iπ/3, in addition, the convergence of those expansions becomes slower and slower when z e ±iπ/3. To compute the Gauss hypergeometric function in a neighborhood of these points, other methods are indicated in [3], the most useful one being Bühring s analytic continuation formula []. Bühring s expansion reads as follows [[3], 2.3.2]. If b a is not an integer, we have for ph(z z) < π the continuation formula Γ(c)Γ(b a) 2F (a, b, c; z) = Γ(b)Γ(c a) (z z) a d n (a, z )(z z ) n + Γ(c)Γ(a b) Γ(a)Γ(c b) (z z) b d n (b, z )(z z ) n, where both series converge outside the circle z z = max{ z, z } and the coefficients are given by the three-term recurrence relation n + s d n (s, z ) = n(n + 2s a b) {z ( z )(n + s 2)d n 2 (s, z ) + [(n + s)( 2z ) + (a + b + )z c]d n (s, z )}, (4)
3 3 with n =, 2, 3,... and starting values d (s, z ) =, d (s, z ) =. For the case when b a is an integer, the coefficients of expansion (4) become indeterminate and a limiting process is needed (see [] for further details). When we take z = /2, the series in (4) converges outside the circle z /2 = /2, and both points z = e ±iπ/3 are inside the domain of convergence. But, when b a approaches an integer value, the convergence of the expansion becomes slower and slower. In this paper we investigate new convergent expansions of the Gauss hypergeometric function 2 F (a, b, c; z) that include the points z = e ±iπ/3 inside their domain of convergence and which do not require any further computation when b a is an integer. The starting point is the integral representation [[7], eq. 5.6.] 2F (a, b, c; z) = valid for Rc > Rb > and ph( z) < π. Γ(c) Γ(b)Γ(c b) t b ( t) c b ( zt) a dt, (5) When we replace f(t) := ( zt) a in this integral by the standard Taylor series expansion of f(t) at t = and interchange summation and integration, we obtain the power series expansion (). The Taylor series expansion of f(t) at t = converges uniformly in z for any t (, ) (for any t in the integration domain of (5)) if z <. Then, the expansion () is convergent in the disk z <. For purposes that will become clear later, it is more convenient to consider the above argument about the region of convergence of the right hand side of () from a different point of view, which is the following. The domain of convergence of () (the disk z < ) is determined by the two following requirements: (i) The interval of integration (, ) in (5) must be completely contained in the domain of convergence of the series expansion of f(t), a disk D r of center t = and radius r, D r = {t C/, t < r}. (ii) The branch point t = /z of f(t) must be located outside that domain D r, which means that z must be located in a region S r = the inverse to the exterior of D r : S r = (Dr EXT ) = {z C/, z < r }. Therefore, the smaller D r is (the smaller r), the bigger the domain S r of validity of () is. But D r must satisfy (i) and then the largest possible r is r = and S r = {z C/, z < } (see Fig. 2). In this paper we explore the following idea. Instead of the Taylor series expansion of f(t) at t =, consider new different convergent expansions of f(t) in a certain domain D satisfying the two above mentioned requirements: (i) (, ) D (The interval of integration (, ) must be completely contained in D); (ii) z S := (D EXT ) (z must be located in a region S = the inverse to the exterior of D). Then, replacing f(t) in (5) by this new expansion and interchanging summation and integration, we will obtain an expansion of 2 F (a, b, c; z) convergent for z S. The larger S is, the better, and one expects that, the smaller D is (containing the interval (, ) in its interior), the bigger S will be. The first possibility that we explore in Section 2 is an expansion of f(t) at t = /2, halfway the interval of integration (, ). In Section 3 we generalize this idea expanding f(t) at a generic point t = w. In Section 4 we explore a two-point Taylor expansion of f(t) at t = and t =. In Section 5 we explore a three-point Taylor expansion of f(t) at t =, t = /2 and t =. Some final remarks and comments are given in Section 6.
4 4 /z Im t Im z D r r Re t S r /r Re z z (a) (b) Figure 2. The disk of convergence D r of the Taylor expansion of f(t) at t = is shown in figure (a) for a certain r (> ), and the region S r, inverse of the exterior of D r is shown in figure (b). The smaller D r is, the larger S r is. The smallest possible value of r for which the integration interval (, ) D r is r =. Before we conclude this section, we want to mention other methods for computing the Gauss hypergeometric function. Continued fractions [[2], Chap. 5, Sec. 3] and Padé approximation [], [[3], Chap. 9, Sec. 2.4], [[2], Chap. 5, Sec. 4] give uniformly convergent expansions on compact subsets of C/ \ [, ). In both methods, the approximation is only known explicitly for the exceptional case a = and c > b >. A different approach using optimal conformal mappings and re-expansions is considered in [] to approximate the Gauss hypergeometric function for z. A regularization and re-expansion method is used in [8] and [9] for computing F (a, b, c; z) in the neighborhoods of singular points z = and z =. 2. An expansion for Rz < Consider the Taylor expansion of the function f(t) = ( zt) a at t = /2: f(t) = z n (a) n n! ( z ) ( a n t n. (6) 2 2) This expansion satisfies condition (i) for D = {t C/, t /2 < /2} and (, ) D (the disk D is the minimal disk centered at t = /2 that contains the domain of integration of (5)); also, it satisfies condition (ii), that is, /z / D, for S = {z C/, Rz < } (see Fig. 3). obtain Then, for Rz <, we can introduce the expansion (6) in (5) and interchange summation and integration to 2F (a, b, c; z) = ( z ) a ( ) n (a) n z Φ n (b, c), (7) 2 n! z 2 with Therefore, Φ n (b, c) := Γ(c) Γ(b)Γ(c b) 2F (a, b, c; z) = t b ( t) c b ( 2t) n dt = 2 F ( n, b, c; 2). ( z ) a ( ) n (a) n z 2F ( n, b, c; 2). (8) 2 n! z 2
5 We have Φ (b, c) =, Φ (b, c) = 2b/c and, for n =, 2, 3,..., the remaining Φ n (b, c) may be obtained from the three-terms recurrence relation [[7], eq. 5.5.] (c + n) 2 F ( n, b, c; 2) + (2b c) 2 F ( n, b, c; 2) n 2 F ( n, b, c; 2) =. It is straightforward to show that Φ n (b, c) also satisfies the contiguous relation Φ n (b, c) = Φ n (b, c) 2b c Φ n (b +, c + ). The functions Φ n (b, c) are polynomials of b and rational functions of c. 5 Im t Im z /z D Re t S Re z /2 z (a) Figure 3. The minimal domain of convergence D of the standard Taylor expansion of f(t) at t = /2 containing the interval (, ) is a disk of radius /2 (figure (a)). The region S, inverse of the exterior of D is the region shown in figure (b): S = {z C/, Rz < }. The following table shows some numerical experiments comparing the accuracy of Bühring s expansion and expansion (8). For values of z near the exceptional points e ±iπ/3, expansion (8) is more competitive than Bühring s expansion. Away from these points, Bühring s expansion becomes more competitive. Parameter values: a =.2, b = 2., c = 3, z = e iπ/3, z = /2. (b) Bühring s formula.263e+2.879e+.3e+.955e-.83e-2 Formula (8).29E+.995E-2.43E-3.223E-4.8E-5 Parameter values: a =.2, b = 2.5, c = 3, z = e iπ/3, z = /2. Bühring s formula.596e+.93e+.228e+.2e-.78e-2 Formula (8).467E+.228E-.26E-3.734E-4.437E-5 Parameter values: a =.2, b = 2., c = 3, z =, z = /2. Bühring s formula.55e+2.33e+.248e-2.48e-4.796e-7 Formula (8).3E+.338E-3.876E-6.34E-8.E-
6 6 Parameter values: a =.2, b = 2., c = 3, z = + I, z = /2. Bühring s formula.4e+2.972e-.29e-3.69e-6.49e-8 Formula (8).7E+.92E-2.26E-4.326E-6.466E-8 Parameter values: a =.2, b = 2., c = 3.5, z = 5, z = /2. Bühring s formula.475e+.47e-3.69e-8.852e-3.56e-3 Formula (8).974E-2.53E-2.49E-3.67E-4.934E-5 Table. The first row represents the number n of terms used in either Bühring s expansion or expansion (8). The second row represents the relative error obtained with Bühring s approximation. The third row represents the relative error resulting from approximation (8). 3. An expansion for 2R(wz) < with arbitrary w C / We can generalize the expansion introduced in the above section considering a standard Taylor expansion of the function f(t) = ( zt) a, not at t = /2, but at a generic point w = u + vi C/, u, v R : f(t) = (a) n z n ( wz) a n (t w) n. (9) n! This expansion satisfies condition (i) for D = {t C/, t w <max{ w, w }}. It also satisfies condition (ii), that is, /z / D, for S = {z C/, wz > z max{ w, w }}. For u = Rw /2 the domain S is the semi-plane S = {z = x + iy; x, y R, 2R(wz) = 2ux 2vy < }. For u < /2 it is the disk S = {z C/, z + ( 2u) w < ( 2u) w } (see Figure 4). Then, for Rz S, we can introduce the expansion (9) in (5) and interchange summation and integration to obtain ( ) n 2F (a, b, c; z) = ( wz) a (a) n wz Φ n (b, c, w), () n! wz with Therefore we have Φ n (b, c, w) := Γ(c) Γ(b)Γ(c b) 2F (a, b, c; z) = ( wz) a ( t b ( t) c b t ) n ( dt = 2 F n, b, c; ). w w (a) n n! ( ) n ( wz 2F n, b, c; ). () wz w We have Φ (b, c, w) =, Φ (b, c, w) = b/(cw) and, for n =, 2, 3,..., the remaining Φ n (b, c, w) may be obtained from the three-terms recurrence relation [[7], eq. 5.5.] ( (c + n) 2 F n, b, c; ) ( ) ( b + n + w w 2n c 2F n, b, c; ) ( + n ) ( 2F n, b, c; ) =. w w w It is straightforward to show that Φ n (b, c) also satisfies the contiguous relation Φ n (b, c, w) = Φ n (b, c, w) b cw Φ n (b +, c +, w). The functions Φ n (b, c, w) are polynomials of b and rational functions of c.
7 7 Im t Im z /z D (+i)/2 Re t S Re z z -i (a) w = + i 2. (b) w = + i 2. Im z Im t i S i D Re t z Re z /z (c) w = i. (d) w = i. Figure 4. The minimal domain of convergence D of the standard Taylor expansion of f(t) at t = w containing the interval (, ) is a disk of center at t = w and radius max{ w, w } (figures (a) and (c)). The region S, inverse of the exterior of D is: the half-plane S = {z = x + iy; x, y R, 2R(wz) > } if Rw /2 (figure (b)) or the disk of center w /(2Rw ) and radius w /( 2Rw) if Rw < /2 (figure (d)). The following table shows some numerical experiments comparing the accuracy of Bühring s expansion and expansion () for w = ( + i)/2. For values of z near the exceptional points e ±iπ/3, expansion () is more competitive than Bühring s expansion. Away from these points, Bühring s expansion becomes more competitive. Parameter values: a =.2, b = 2., c = 3, z = e iπ/3, z = /2. Bühring s formula.263e+2.879e+.954e-.e+.83e-2 Formula ().48E+.66E-2.56E-3.476E-5.5E-6 Table 2. The first row represents the number n of terms used in either Bühring s expansion or expansion () with w = ( + i)/2. The second row represents the relative error obtained with Bühring s approximation. The third row represents the relative error resulting from approximation () with w = ( + i)/2.
8 8 Parameter values: a =.2, b = 2.5, c = 3, z = e iπ/3, z = /2. Bühring s formula.596e+.92e+.228e+.2e-.78e-2 Formula ().48E+.27E-.48E-3.38E-4.477E-6 Parameter values: a =.2, b = 2., c = 3, z =, z = /2. Bühring s formula.54e+2.33e+.248e-2.48e-4.796e-7 Formula ().4E+.267E-2.3E-4.43E-6.677E-8 Parameter values: a =.2, b = 2., c = 3, z = + I, z = /2. Bühring s formula.4e+2.972e-.29e-3.69e-6.49e-8 Formula ().49E+.472E-2.937E-4.243E-5.663E-7 Parameter values: a =.2, b = 2., c = 3.5, z = 5, z = /2. Bühring s formula.475e+.47e-3.69e-8.852e-3.56e-4 Formula ().68E+.56E-.537E-2.4E-2.627E-3 4. An expansion for z 2 < 4 z As has been pointed out in [6] (in a different context), the use of a multi-point Taylor expansion [4], [5] with base points in the interval (, ) is preferable to using a standard Taylor expansion. With a multi-point Taylor expansion we can avoid the singularity t = /z of f(t) in its domain of convergence in a better way, and, at the same time, include the whole interval (, ) in its interior (see Fig. 5(a)). Therefore, we consider the two-point Taylor expansion of the function f(t) = ( zt) a at t = and t = [4]: f(t) = [A n (a, z) + B n (a, z)t]t n (t ) n. (2) An explicit formula for the coefficients A n (a, z) and B n (a, z) is given in [4]: A (a, z) =, B (a, z) = ( z) a and, for n =, 2, 3,..., A n (a, z) = n! B n (a, z) = n! n k= n k= (n + k )! [( ) n n ( ) k k( z) k a n ](a) n k z n k. k!(n k)! (n + k)! k!(n k)! [( )k ( z) k a n + ( ) n+ ](a) n k z n k.
9 Also, a recurrence relation for A n (a, z) and B n (a, z) may be obtained by using the differential equation satisfied by f(t): ( zt)f = azf. Introducing expansion (2) and f (t) = {[(2n + )B n (a, z) (n + )A n+ (a, z)] + (n + )(2A n+ (a, z) + B n+ (a, z))t}t n (t ) n, in the differential equation ( zt)f = azf, and equating coefficients of t n (t ) n and t n+ (t ) n we obtain: 9 A n+ (a, z) = z(a + 2n)A n(a, z) + [ + n(2 z)]b n (a, z), n + B n+ (a, z) = z(2 z)(a + 2n)A n(a, z) + [z(a + 2) + n(6z z 2 4) 2]B n (a, z). (n + )( z) (3) Im t D r /2 /z Re t Im z 4 2 z S r Re z (a) Figure 5. The minimal domain of convergence D r of the two-point Taylor expansion of f(t) at t = and t = containing the interval (, ) is a Cassini oval of radius /4 and foci t = and t = (figure (a)). The region S r, inverse of the exterior of D r is the region shown in figure (b): S r = {z C/; z 2 < 4 z }. Expansion (2) converges inside a Cassini oval with foci at t = and t = and radius r > of the form D r = {t C/, t(t ) < r}. The interval (, ) is completely contained in this Cassini oval if its middle point t = /2 is contained. This happens for r t 2 = /4 and then, expansion (2) satisfies condition (i) for r /4. On the other hand, it satisfies condition (ii) if /z / D r [4], that is, for any ( ) r < z z. The smallest r we can take is r = /4 and then, the largest S r we can choose is (see Fig. 5(b)) S r = {z C/; z 2 < 4 z } = {x + iy; x, y R, y 4 + (2x 2 6)y 2 + [x 4 6x x 6] < }. (b) Then, for z S r, we can introduce the expansion (2) in (5) and interchange summation and integration to obtain 2F (a, b, c; z) = [A n (a, z)φ n (b, c) + B n (a, z)ψ n (b, c)], (4) with Φ n (b, c) := ( ) n Γ(c) Γ(b)Γ(c b) Ψ n (b, c) := ( ) n Γ(c) Γ(b)Γ(c b) t b+n ( t) n+c b dt = ( ) n (b) n(c b) n (c) 2n, t b+n ( t) n+c b dt = ( ) n (b) n+(c b) n (c) 2n+.
10 Therefore, we have 2F (a, b, c; z) = ( ) n (b) n(c b) n [(c + 2n)A n (a, z) + (b + n)b n (a, z)], (5) (c) 2n+ with A n (a, z) and B n (a, z) given by the recursion (3) and A (a, z) =, B (a, z) = ( z) a. This expansion is a series of elementary functions of z: a linear combination of and ( z) n a whose coefficients are polynomials in z. The following table shows some numerical experiments comparing the accuracy of Bühring s expansion and expansion (5). For values of z near the exceptional points e ±iπ/3, expansion (5) is more competitive than Bühring s expansion. Away from these points, Bühring s expansion becomes more competitive. Parameter values: a =.2, b = 2., c = 3, z =, z = /2. Bühring s formula.54e+2.33e+.248e-2.48e-4.796e-7 Formula (5).2E+.242E-5.63E-.43E-4.48E-5 Parameter values: a =.2, b = 2.5, c = 3, z = 2, z = /2. Bühring s formula.8e+.294e-2.75e-5.85e-9.339e-2 Formula (5).22E+.546E-3.87E-5.688E-8.26E- Parameter values: a =.2, b = 2., c = 3, z = e iπ/3, z = /2. Bühring s formula.263e+2.879e+.955e-.e+.83e-2 Formula (5).2E+.42E-3.8E-6.4E-9.936E-3 Parameter values: a =.2, b = 2.5, c = 3, z = e iπ/3, z = /2. Bühring s formula.596e+.93e+.228e+.2e-.78e-2 Formula (5).4E+.753E-4.63E-7.522E-.467E-3 Table 3. The first row represents the number n of terms used in either Bühring s expansion or expansion (5). The second row represents the relative error obtained with Bühring s approximation. The third row represents the relative error resulting from approximation (5).
11 5. An expansion for z 3 < 6 3 ( z)(2 z) As has been pointed out in [6], the use of a three-point Taylor expansion [5] with base points in the interval (, ) is preferable to the use of a two-point Taylor expansion in order to better avoid the singularity t = /z of f(t) in its domain of convergence, and, at the same time, to include the whole interval (, ) in its interior (see Fig. 6(a)). Therefore, we consider the three-point Taylor expansion of the function f(t) = ( zt) a at t =, t = /2 and t = : f(t) = [A n (a, z)t + B n (a, z)t + C n (a, z)t 2 ][t(t )(t /2)] n, (6) with A (a, z) =, B (a, z) = 4( z/2) a ( z) a 3 and C (a, z) = 2 + 2( z) a 4( z/2) a. We have that [6] f (t) = [A n(a, z) + B n(a, z)t + C n(a, z)t 2 ][t(t )(t /2)] n, (7) with A n(a, z) := n + A n+ (a, z) + (3n + )B n (a, z) + 3n 2 2 C n(a, z), B n(a, z) :=(3n + 2)C n (a, z) 3(n + )A n+ (a, z) (n + )B n+ (a, z) C n(a, z) :=3(n + )A n+ (a, z) + 3(n + ) B n+ (a, z) + 2 5(n + ) C n+ (a, z). 4 3(n + ) C n+ (a, z), 4 Introducing (6) and (7) into the differential equation ( zt)f = azf and equating coefficients of [t(t )(t /2)] n we obtain A n+ (a, z) = 2(n + ) {2[3n(z 2) 2]B n(a, z) + 4z(3n + a)a n (a, z) + n(5z 6)C n (a, z)}, B n+ (a, z) = 2(n + )(z 2 3z + 2) {4z(3n + a)(26z 3z2 24)A n (a, z) + 2[48 4z(8 + 5a) + 6z 2 (4 + 3a)+ 3n(48 96z + 5z 2 3z 3 )]B n (a, z) + [4(2 6z(5 + a) + 5z 2 (2 + a))+ n(264 56z + 262z 2 5z 3 )]C n (a, z)}, C n+ (a, z) = 2(n + )(z 2 3z + 2) {4z(3n + a)(2 2z + z2 )A n (a, z) + 2[2(6(3 + a)z (6 + 5a)z 2 2)+ 3n(z 3 24z z 24)]B n (a, z) + [4(2z(9 + 2a) 3z 2 (2 + a) 2)+ n(5z 3 32z z 44)]C n (a, z)}. Expansion (6) converges inside a Cassini oval with foci at t =, t = /2 and t = and radius r > of the form D r = {t C/, t(t )(t /2) < r}. The interval (, ) is completely contained in this Cassini oval if the points t = ± 3 2, at which R(t) := t(t )(t /2) gets its maximum value, is contained in D r. This happens for r R(t ) = (2 3) and then, expansion (6) satisfies condition (i) for r (2 3). On the other hand, it satisfies condition (ii) if /z / D r, that is, for any r < z ( ) ( z z ). 2 The smallest r we can take is r = (2 3) and then, the largest S r we can choose is (see Fig. 6(b)) S r = {z C/; z 3 < 6 3 ( z)(2 z) } = {x + iy; x, y R, 8[( x) 2 + y 2 ][(2 x) 2 + y 2 ] > (x 2 + y 2 ) 3 }. (8)
12 2 Im t Im z D r Re t S r 5 z Re z /z (a) (b) Figure 6. The minimal domain of convergence D r of the three-points Taylor expansion of f(t) at t =, t = /2 and t = containing the interval (, ) is a Cassini oval of radius (2 3) and foci at t =, t = /2 and t = (figure (a)). The region S r, inverse of the exterior of D r is the region shown in figure (b): S r = {z C/; z 3 < 6 3 ( z)(2 z) }. Then, for z S r, we can introduce the expansion (6) in (5) and interchange summation and integration to obtain [ 2F (a, b, c; z) = ( ) n A n (a, z) + b ] c B b(b + ) n(a, z) + c(c + ) C n(a, z) Φ n (b, c), (9) with Φ n (b, c) := Therefore we have 2F (a, b, c; z) = Γ(c) Γ(b)Γ(c b) t n+b ( t) n+c b (t /2) n dt = ( ) n (b) n(c b) n 2 n (c) 2n 2F ( n, b + n; c + 2n; 2). [ A n (a, z) + b ] c B b(b + ) n(a, z) + c(c + ) C (b)n (c b) n n(a, z) 2 n 2F ( n, b + n; c + 2n; 2), (2) (c) 2n with A n (a, z), B n (a, z) and C n (a, z) given by the recursion (8) and A (a, z) =, B (a, z) = 4( z/2) a ( z) a 3 and C (a, z) = 2 + 2( z) a 4( z/2) a. A recursion relation for Φ n (b, c) with respect to n can be obtained by using Zeilberger s algorithm (e.g. via its Maple realization) for hypergeometric functions, and it follows that the functions Φ n (b, c) satisfy the three-terms recurrence relation X n Φ n (b, c) + Y n Φ n (b, c) + Z n Φ n+ (b, c) =, where b(b c)(2b c) Φ (b, c) =, Φ (b, c) = 2c(c + )(c + 2). The coefficients are given by X n := n( c 2n 5nc 6n 2 4bc + 4b 2 )( n + b c + )(n + b ), We thank Dr. Raimundas Vidunas for his help.
13 3 Y n := 2(2b c)(p + p n + p 2 n 2 + p 3 n 3 ), where and p :=6b( + b)(b c + )(b c), p := 4 + 2c + 4b 2 7c 2 32b 2 c + 32bc 2 4bc, p 2 :=24bc b 2 + 5c 2 57c, p 3 :=8(c 2), Z n := 6(3n + c))(3n + + c)(3n c)( 5nc 6n 2 + n + 4b 2 4bc + 4c 4). On the other hand, it is straightforward to see that Φ (b, c) = and that Φ n (b, c) satisfies the contiguous relation b(b + )(c b) Φ n+ (b, c) = c(c + )(c + 2) Φ b(c b) n(b + 2, c + 3) 2c(c + ) Φ n(b +, c + 2). Expansion (2) is a series of elementary functions of z: a linear combination of, ( z) n a and ( z/2) n a whose coefficients are polynomials in z. The following table shows some numerical experiments comparing the accuracy of Bühring s expansion and expansion (2). For values of z near the exceptional points e ±iπ/3, expansion (2) is more competitive than Bühring s expansion. Away from these points, Bühring s expansion becomes more competitive. Parameter values: a =.2, b = 2., c = 3, z = e iπ/3, z = /2. n Bühring s formula.263e+2.77e+2.879e+.253e+.3e+ Formula (2).33E-.647E-5.8E-7.96E-.527E-4 Parameter values: a =.2, b = 2.5, c = 3, z = e iπ/3, z = /2. n Bühring s formula.596e+.386e+.93e+.56e+.228e- Formula (2).35E-.496E-5.37E-7.84E-.523E-4 Parameter values: a =..2, b = 2., c = 3, z = 5, z = /2. n Bühring s formula.84e+.65e-2.26e-4.236e-7.238e-9 Formula (2).7E+.429E-2.36E-3.465E-5.36E-6 Parameter values: a =.2, b = 2., c = 3, z = 5, z = /2. n Bühring s formula.269e+.7e-2.86e-4.966e-7.973e-9 Formula (2).99E-.526E-2.39E-3.277E-5.26E-6
14 Table 4. The first row represents the number n of terms used in either Bühring s expansion or expansion (2). The second row represents the relative error obtained with Bühring s approximation. The third row represents the relative error resulting from approximation (2) Concluding remarks In Sections 2 and 3 we have used a standard one-point Taylor expansion of f(t) = ( zt) a with the smallest possible convergence region D containing the integration interval (, ): an expansion at the point t = /2 and convergence radius r = /2 or at any point t = w and convergence radius r =max{ w, w }. Then, the inverse of the complement of this disk D is the largest possible region that we can obtain with one-point Taylor expansions of f(t): Rz < or, in general, the semi-plane 2R(zw) < (when Rw /2). In Section 4 we have used a two-point Taylor expansion of f(t), with two base points located in the interval (, ) and, in Section 5, a three-point Taylor expansion. One may consider the possibility of expanding f(t) at four or more points located in the interval (, ). In fact, one gets new approximations valid in regions S r larger than the ones shown in Figs. 5(b) and 6(b); but the integrals defining the functions Φ n (b, c), as well as the recurrences of the coefficients (A n (a, z), B n (a, z),...) become more complicated. 7. Acknowledgments The Dirección General de Ciencia y Tecnología (REF. MTM2-237) is acknowledged by its financial support. NMT acknowledges support from Ministerio de Ciencia e Innovación, project MTM
15 5 References [] W. Bühring, An analytic continuation of the hypergeometric series, SIAM J. Math. Anal., 8 (987) [2] A.Cuyt, V.B.Petersen, B.Verdonk, H.Waadeland and W.B.Jones, Handbook of Continued Fractions for Special Functions, Springer, 28. [3] A. Gil, J. Segura and N. M. Temme, Numerical Methods for Special Functions, SIAM, Philadelphia, 27. [4] J. L. Lopez and N. M. Temme, Two-point Taylor expansions of analytic functions, Stud. Appl. Math., 9 (22) [5] J. L. Lopez and N. M. Temme, Multi-point Taylor expansions of analytic functions, Trans. Amer. Math. Soc., 356 n. (24) [6] J. L. Lopez, E. Pérez and N. M. Temme, Multi-point Taylor approximations in one-dimensional linear boundary value problems, Appl. Math. Comput., 27 n. 2 (29) [7] A. B. Olde Daalhuis, Chapter 5, Hypergeometric Function, NIST Handbook of Mathematical Functions, NIST and Cambridge Univ. Press, 2. [8] S.L. Skorokhodov, Regularization method for computing hypergeometric function F (a, b, c; z) in the neighborhoods of singular points z = and z =, Comput. Math. Math. Phys., 4 n. 2 (2), [9] S.L. Skorokhodov, Computer Algebra and Computing Special Functions, Programming and Computer Software, 29 n. 2 (23) [] S.L. Skorokhodov, Advanced techniques for computing divergent series, Nucl. Instr. Meth. Phys. Res. A, 52 (23)
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