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Article

Asymptotic Expansion of the Modified Exponential Integral Involving the Mittag-Leffler Function

Division of Computing and Mathematics, Abertay University, Dundee DD1 1HG, UK
Mathematics 2020, 8(3), 428; https://doi.org/10.3390/math8030428
Submission received: 21 February 2020 / Revised: 6 March 2020 / Accepted: 10 March 2020 / Published: 16 March 2020
(This article belongs to the Special Issue Special Functions with Applications to Mathematical Physics)

Abstract

:
We consider the asymptotic expansion of the generalised exponential integral involving the Mittag-Leffler function introduced recently by Mainardi and Masina [Fract. Calc. Appl. Anal. 21 (2018) 1156–1169]. We extend the definition of this function using the two-parameter Mittag-Leffler function. The expansions of the similarly extended sine and cosine integrals are also discussed. Numerical examples are presented to illustrate the accuracy of each type of expansion obtained.

1. Introduction

The complementary exponential integral Ein ( z ) is defined by
Ein ( z ) = 0 z 1 e t t d t = n = 1 ( ) n 1 z n n n ! ( z C )
and is an entire function. Its connection with the classical exponential integral E 1 ( z ) = z t 1 e t d t , valid in the cut plane | arg z | < π , is [1], p. 150.
Ein ( z ) = log z + γ + E 1 ( z ) ,
where γ = 0.5772156 is the Euler-Mascheroni constant.
In a recent paper, Mainardi and Masina [2] proposed an extension of Ein ( z ) by replacing the exponential function in (1) by the one-parameter Mittag-Leffler function
E α ( z ) = n = 0 z n Γ ( α n + 1 ) ( z C , α > 0 ) ,
which generalises the exponential function e z . They introduced the function for any α > 0 in the cut plane | arg z | < π
Ein α ( z ) = 0 z 1 E α ( t α ) t α d t = n = 0 ( ) n z α n + 1 ( α n + 1 ) Γ ( α n + α + 1 ) ,
which when α = 1 reduces to the function Ein ( z ) . A physical application of this function for 0 α 1 arises in the study of the creep features of a linear viscoelastic model; see Reference [3] for details. An analogous extension of the generalised sine and cosine integrals was also considered in Reference [2]. Plots of all these functions for α [ 0 , 1 ] were given.
Here we consider a slightly more general version of (3) based on the two-parameter Mittag-Leffler function given by
E α , β ( z ) = n = 0 z n Γ ( α n + β ) ( z C , α > 0 ) ,
where β will be taken to be real. Then the extended complementary exponential integral we shall consider is
Ein α , β ( z ) = 0 z 1 E α , β ( t α ) t α d t = n = 1 ( ) n 1 Γ ( α n + β ) 0 z t α n α d t = z n = 0 ( ) n z α n ( α n + 1 ) Γ ( α n + α + β ) ,
upon replacement of n 1 by n in the last summation. When β = 1 this reduces to (3) so that Ein α , 1 ( z ) = Ein α ( z ) .
The asymptotic expansion of this function will be obtained for large complex z with the parameters α , β held fixed. We achieve this by consideration of the asymptotics of a related function using the theory developed for integral functions of hypergeometric type as discussed, for example, in Reference [4], §2.3. An interesting feature of the expansion of Ein α , β ( x ) for x + when α ( 0 , 1 ] is the appearance of a logarithmic term whenever α = 1 , 1 2 , 1 3 , . Similar expansions are obtained for the extended sine and cosine integrals in Section 4. The paper concludes with the presentation of some numerical results that demonstrate the accuracy of the different expansions obtained.

2. The Asymptotic Expansion of a Related Function for | z |

To determine the asymptotic expansion of Ein α , β ( z ) for large complex z with the parameters α and β held fixed, we shall find it convenient to consider the related function defined by
F ( χ ) : = n = 0 χ n ( α n + γ ) Γ ( α n + α + β ) = n = 0 g ( n ) χ n n ! ( χ C ) ,
where
g ( n ) = Γ ( n + 1 ) ( α n + γ ) Γ ( α n + α + β ) = Γ ( α n + γ ) Γ ( n + 1 ) Γ ( α n + γ + 1 ) Γ ( α n + α + β ) .
It is readily seen that, when γ = 1 ,
Ein α , β ( z ) = z F ( z α ) .
The parameter γ > 0 , but will be chosen to have two specific values in Section 3 and Section 4; namely, γ = 1 and γ = 1 + α . It will be shown that the asymptotic expansion of F ( χ ) consists of an algebraic and an exponential expansion valid in different sectors of the complex χ -plane.
The function F ( χ ) in (5) is a case of the Fox-Wright function
p Ψ q ( χ ) = n = 0 r = 1 p Γ ( α r n + a r ) r = 1 q Γ ( β r n + b r ) χ n n ! ,
corresponding to p = q = 2 . In (6) the parameters α r and β r are real and positive and a r and b r are arbitrary complex numbers. We also assume that the α r and a r are subject to the restriction
α r n + a r 0 , 1 , 2 , ( n = 0 , 1 , 2 , ; 1 r p )
so that no gamma function in the numerator in (6) is singular. We introduce the following parameters associated (empty sums and products are to be interpreted as zero and unity, respectively) with p Ψ q ( χ ) which play a key role in the analysis of its asymptotic behaviour. are given by
κ = 1 + r = 1 q β r r = 1 p α r , h = r = 1 p α r α r r = 1 q β r β r ,
ϑ = r = 1 p a r r = 1 q b r + 1 2 ( q p ) , ϑ = 1 ϑ .
The asymptotic expansion of F ( χ ) is discussed in detail in Reference [5] Section 12, and is summarised in [4,6]. The algebraic expansion of F ( χ ) is obtained from the Mellin-Barnes integral representation [4], p. 56.
F ( χ ) = 1 2 π i c i c + i Γ ( s ) Γ ( 1 + s ) ( χ e π i ) s ( α s + γ ) Γ ( α s + α + β ) d s , | arg ( χ ) | < π ( 1 1 2 α ) ,
where, with γ / α < c < 0 , the integration path lies to the left of the poles of Γ ( s ) at s = 0 , 1 , 2 , but to the right of the poles at s = γ / α and s = k 1 , k = 0 , 1 , 2 , . The upper or lower sign is taken according as arg χ > 0 or arg χ < 0 , respectively. It is seen that when α = γ / m , m = 1 , 2 , the pole at s = m is double and its residue must be evaluated accordingly. Displacement of the integration path to the left when 0 < α < 2 and evaluation of the residues then produces the algebraic expansion H ( χ e π i ) , where
H ( χ ) = π / α sin γ π / α χ γ / α Γ ( α + β γ ) + k = 0 ( ) k χ k 1 ( γ α ( k + 1 ) ) Γ ( β α k ) ( α γ m ) ( ) m 1 χ m Γ ( α + β γ ) m γ log χ ψ ( α + β γ ) + k = 0 k m 1 ( ) k χ k 1 ( γ α ( k + 1 ) ) Γ ( β α k ) ( α = γ m ) ,
and ψ denotes the logarithmic derivative of the gamma function.
The exponential expansion associated with p Ψ q ( χ ) is given by [6] p. 299, [4] p. 57.
E ( χ ) : = X ϑ e X j = 0 A j X j , X = κ ( h χ ) 1 / κ ,
where the coefficients A j are those appearing in the inverse factorial expansion
1 Γ ( 1 + s ) r = 1 p Γ ( α r n + a r ) r = 1 q Γ ( β r n + b r ) = κ A 0 ( h κ κ ) s j = 0 M 1 c j Γ ( κ s + ϑ + j ) + ρ M ( s ) Γ ( κ s + ϑ + M )
with c 0 = 1 . Here M is a positive integer and ρ M ( s ) = O ( 1 ) for | s | in | arg s | < π . The constant A 0 is specified by
A 0 = ( 2 π ) 1 2 ( p q ) κ 1 2 ϑ r = 1 p α r a r 1 2 r = 1 q β r 1 2 b r .
The coefficients c j are independent of s and depend only on the parameters p, q, α r , β r , a r and b r .
For the function F ( χ ) , we have
κ = α , h = α α , ϑ = α β , A 0 = α 1 .
We are in the fortunate position that the normalised coefficients c j in this case can be determined explicitly as c j = ( α + β γ ) j . This follows from the well-known (convergent) expansion given in Reference [4,7], p. 41.
1 ( α s + γ ) Γ ( α s + α + β ) = j = 0 ( α + β γ ) j Γ ( α s + ϑ + j ) ( ( s ) > γ / α ) ,
to which, in the case of F ( χ ) , the ratio of gamma functions appearing on the left-hand side of (10) reduces. Then, with X = χ 1 / α we have from (9) the exponential expansion associated with F ( χ ) given by
E ( χ ) = 1 α χ ϑ / α exp [ χ 1 / α ] j = 0 ( α + β γ ) j χ j / α .
From Reference [4] pp. 57–58, we then obtain the asymptotic expansion for | χ | when 0 < α < 2
F ( χ ) E ( χ ) + H ( χ e π i ) | arg χ | < 1 2 π α H ( χ e π i ) | arg ( χ ) | < π ( 1 1 2 α )
and, when α = 2 ,
F ( χ ) E ( χ ) + E ( χ e 2 π i ) + H ( χ e π i ) | arg χ | π .
The upper and lower signs are chosen according as arg χ > 0 or arg χ < 0 , respectively. It may be noted that the expansions E ( χ e 2 π i ) in (14) only become significant in the neighbourhood of arg χ = ± π . When α > 2 , the expansion of F ( χ ) is exponentially large for all values of arg χ (see Reference [4], p. 58) and accordingly we omit this case as it is unlikely to be of physical interest.
Remark 1.
The exponential expansion E ( χ ) in (13) continues to hold beyond the sector | arg χ | < 1 2 π α , where it becomes exponentially small in the sectors π α | arg χ | < 1 2 π α when 0 < α 1 . The rays arg χ = ± π α are Stokes lines, where E ( χ ) is maximally subdominant relative to the algebraic expansion H ( χ e π i ) . On these rays, E ( χ ) undergoes a Stokes phenomenon, where the exponentially small expansion “switches off” in a smooth manner as | arg χ | increases [1], §2.11(iv), with its value to leading order given by 1 2 E ( χ ) ; see Reference [8] for a more detailed discussion of this point in the context of the confluent hypergeometric functions. We do not consider exponentially small contributions to F ( χ ) here, except to briefly mention in Section 3 the situation pertaining to the case α = 1 .

3. The Asymptotic Expansion of Ein α , β ( z ) for | z |

The asymptotic expansion of Ein α , β ( z ) defined in (4) can now be constructed from that of F ( χ ) with the parameter γ = 1 . It is sufficient, for real α , β , to consider 0 arg z π , since the expansion when arg z < 0 is given by the conjugate value. With χ = z α = e π i z α , the exponentially large sector | arg χ | < 1 2 π α becomes | π + α arg z | < 1 2 π α ; that is
θ 0 < arg z < θ 0 + π , θ 0 : = π 2 α ( 2 α ) .
On the boundaries of this sector the exponential expansion is of an oscillatory character. When 0 < α < 2 3 , we note that the exponentially large sector (15) lies outside the sector of interest 0 arg z π .
We define the algebraic and exponential asymptotic expansions
H α , β ( z ) = π / α sin ( π / α ) Γ ( α + β 1 ) + k = 0 ( ) k z 1 α ( k + 1 ) ( 1 α ( k + 1 ) ) Γ ( β α k ) ( α m 1 ) ( ) m 1 Γ ( α + β 1 ) { log z ψ ( α + β 1 ) } + k = 0 k m 1 ( ) k z 1 α ( k + 1 ) ( 1 α ( k + 1 ) ) Γ ( β α k ) ( α = m 1 ) ,
where m = 1 , 2 , , and
E α , β ( z ) = ( e π i / α z ) ϑ α exp [ e π i / α z ] j = 0 ( α + β 1 ) j ( e π i / α z ) j
where we recall that ϑ = α β . Then the following result holds:
Theorem 1.
Let m be a positive integer, with α > 0 and β real and θ 0 = π ( 2 α ) / ( 2 α ) . Then the following expansions hold for | z |
Ein α , β ( z ) H α , β ( z ) ( 0 arg z π )
when 0 < α < 2 3 , and
Ein α , β ( z ) H α , β ( z ) ( 0 arg z < θ 0 ) z E α , β ( z ) + H α , β ( z ) ( θ 0 arg z π )
when 2 3 α < 2 . Finally, when α = 2 we have Ein 2 , β ( z ) = Ein 2 , β ( z ) and it is therefore sufficient to consider 0 arg z 1 2 π . Then, from (14), we obtain the expansion when α = 2
Ein 2 , β ( z ) z { E 2 , β ( z ) + E 2 , β ( z e π i ) } + H 2 , β ( z ) ( 0 arg z 1 2 π ) .
We note from Theorem 1 that when z the value of Ein α , β ( z ) is, in general, complex-valued.
In the case of main physical interest, when z = x > 0 is a real variable, we have the following expansion:
Theorem 2.
When z = x ( > 0 ) we have from Theorem 1 the expansions
Ein α , β ( x ) H α , β ( x )
for 0 < α < 2 , and from (17) and (20) when α = 2
Ein 2 , β ( x ) H 2 , β ( x ) x 1 β j = 0 ( 1 + β ) j x j cos [ x 1 2 π ( β + j ) ]
as x + .
It is worth noting that a logarithmic term is present in the asymptotic expansion of Ein α , β ( x ) whenever α = 1 , 1 2 , 1 3 , .

The Case α = 1

The special case α = 1 deserves further consideration. From (16) and (21) we obtain the expansion
Ein 1 , β ( x ) 1 Γ ( β ) { log x ψ ( β ) } k = 1 ( x ) k k Γ ( β k ) ( x + ) .
If β = 1 , the asymptotic sum in (23) vanishes and
Ein 1 , 1 ( x ) log x + γ
for large x. But we have the exact evaluation (compare (2))
Ein 1 , 1 ( x ) = x n = 0 ( x ) n ( n + 1 ) 2 n ! = log x + γ + E 1 ( x ) log x + γ + e x x j = 0 ( ) j j ! x j ( x + )
by Reference [1], (6.12.1). The additional asymptotic sum appearing in (25) is exponentially small as x + and is consequently not accounted for in the result (24).
From Remark 1, it is seen that there are Stokes lines at arg z = ± π ( 1 α ) , which coalesce on the positive real axis when α = 1 . In the sense of increasing arg z in the neighbourhood of the positive real axis, the exponential expansion E 1 , β ( z ) is in the process of switching on across arg z = π ( 1 α ) and E 1 , β ( z ) ¯ (where the bar denotes the complex conjugate) is in the process of switching off across arg z = π ( 1 α ) . When α = 1 , this produces the exponential contribution
1 2 x { E 1 , β ( x ) + E 1 , β ( x ) ¯ } = e x x β cos π β j = 0 ( ) j + 1 ( β ) j x j
for large x. Thus, the more accurate version of (23) should read
Ein 1 , β ( x ) 1 Γ ( β ) { log x ψ ( β ) } k = 1 ( x ) k k Γ ( β k ) e x x β cos π β j = 0 ( ) j ( β ) j x j
as x + . When β = 1 , this correctly reduces to (25).
When β = 2 , we have [9]
Ein 1 , 2 ( x ) = x n = 0 ( x ) n ( n + 1 ) 2 ( n + 2 ) n ! = log x ψ ( 2 ) + 1 x + E 1 ( x ) e x x
log x ψ ( 2 ) + 1 x + e x x j = 1 ( ) j j ! x j ( x + ) .
This can be seen also to agree with (26) after a little rearrangement.

4. The Generalised Sine and Cosine Integrals

The sine and cosine integrals are defined by [1], §6.2,
Si ( z ) = 0 z sin t t d t , Cin ( z ) = 0 z 1 cos t t d t .
Mainardi and Masina [2] generalised these definitions by replacing the trigonometric functions by
sin α ( t ) = t α E 2 α , α + β ( t 2 α ) = n = 0 ( ) n t ( 2 n + 1 ) α Γ ( 2 n α + α + β ) , cos α ( t ) = E 2 α , β ( t 2 α ) = n = 0 ( ) n t 2 n α Γ ( 2 n α + β )
with β = 1 to produce
Sin α ( z ) = 0 z sin α ( t ) t α d t = n = 0 ( ) n z 2 n α + 1 ( 2 n α + 1 ) Γ ( 2 n α + α + 1 ) Cin α ( z ) = 0 1 cos α ( t ) t α d t = n = 0 ( ) n z 2 n α + α + 1 ( 2 n α + α + 1 ) Γ ( 2 n α + 2 α + 1 ) .
Here we extend the definitions (27) by including the additional parameter β R in the Mittag-Leffler functions and consider the functions
Sin α , β ( z ) = z n = 0 ( ) n z 2 n α ( 2 n α + 1 ) Γ ( 2 n α + α + β ) Cin α , β ( z ) = z 1 + α n = 0 ( ) n z 2 n α ( 2 n α + α + 1 ) Γ ( 2 n α + 2 α + β ) .
The asymptotics of Sin α , β ( z ) and Cin α , β ( z ) can be deduced from the results in Section 2. However, here we restrict ourselves to determining the asymptotic expansion of these functions for large | z | in a sector enclosing the positive real z-axis, where for 0 < α < 1 they only have an algebraic-type expansion. We observe in passing that
Sin α , β ( z ) = Ein 2 α , β α ( z ) .
Comparison of the series expansion for Sin α , β ( z ) with F ( χ ) in Section 2, with the substitutions α 2 α , β β α and γ = 1 (or from the above identity combined with Theorems 1 and 2), produces the following expansion:
Theorem 3.
For m = 1 , 2 , and 0 < α < 1 we have the algebraic expansions
Sin α , β ( z ) π / ( 2 α ) sin ( π / ( 2 α ) ) Γ ( α + β 1 ) + k = 0 ( ) k z 1 2 α ( k + 1 ) ( 1 2 α ( k + 1 ) ) Γ ( β ( 2 k + 1 ) α ) ( α ( 2 m ) 1 ) ( ) m 1 Γ ( α + β 1 ) { log z ψ ( α + β 1 ) } + k = 0 k m 1 ( ) k z 1 2 α ( k + 1 ) ( 1 2 α ( k + 1 ) ) Γ ( β ( 2 k + 1 ) α ) ( α = ( 2 m ) 1 )
as | z | in the sector | arg z | < π ( 1 α ) / ( 2 α ) .
A similar treatment for Cin α , β ( z ) shows that with the substitutions α 2 α , β β and γ = 1 + α we obtain the following expansion:
Theorem 4.
For m = 1 , 2 , and 0 < α < 1 we have the algebraic expansions
Cin α , β ( z ) π / ( 2 α ) cos ( π / ( 2 α ) ) Γ ( α + β 1 ) + k = 0 ( ) k z 1 ( 2 k + 1 ) α ( 1 ( 2 k + 1 ) α ) Γ ( β 2 α k ) ( α ( 2 m 1 ) 1 ) ( ) m 1 Γ ( α + β 1 ) { log z ψ ( α + β 1 ) } + k = 0 k m 1 ( ) k z 1 ( 2 k + 1 ) α ( 1 ( 2 k + 1 ) α ) Γ ( β 2 α k ) ( α = ( 2 m 1 ) 1 )
as | z | in the sector | arg z | < π ( 1 α ) / ( 2 α ) .
The expansions of Sin α , β ( x ) and Cin α , β ( x ) as x + when 0 < α < 1 follow immediately from Theorems 3 and 4.
As x + when α = 1 , the exponentially oscillatory contribution to Sin 1 , β ( x ) can be obtained directly from (22) together with (29). In the case of Cin 1 , β ( x ) , we obtain from (9) with κ = 2 , h = 1 4 , ϑ = 2 β , X = χ 1 / 2 and A 0 = 1 2 the exponential expansion
E ( χ ) = 1 2 χ ϑ / 2 exp [ χ 1 / 2 ] j = 0 c j χ j / 2 , χ = e π i x 2 ,
with the coefficients c j = ( β ) j . Then the exponential contribution to Cin 1 , β ( x ) is
x 2 { E ( χ ) + E ( χ e π i ) } = x β j = 0 ( β ) j x j cos [ x 1 2 π ( β + j ) ] ( x + ) .
Collecting together these results we finally obtain the following theorem.
Theorem 5.
When α = 1 and β is real the following expansions hold:
Sin 1 , β ( x ) π 2 Γ ( β ) k = 0 ( ) k x 2 k 1 ( 2 k + 1 ) Γ ( β 1 2 k ) + x β j = 0 ( β ) j x j sin [ x 1 2 π ( β + j ) ]
and
Cin 1 , β ( x ) 1 Γ ( β ) { log x ψ ( β ) } k = 1 ( ) k x 2 k 2 k Γ ( β 2 k ) x β j = 0 ( β ) j x j cos [ x 1 2 π ( β + j ) ]
as x + .
When β > 0 , it is seen that Sin 1 , β ( x ) approaches the constant value π / ( 2 Γ ( β ) ) whereas Cin 1 , β ( x ) grows logarithmically like log ( x ) / Γ ( β ) as x + .

5. Numerical Results

In this section we present numerical results confirming the accuracy of the various expansions obtained in this paper. In all cases we have employed optimal truncation (that is truncation at, or near, the least term in modulus) of the algebraic and (when appropriate) the exponential expansions. The numerical values of Ein α , β ( x ) were computed from (4) using high-precision evaluation of the terms in the suitably truncated sum.
We first present results in the physically interesting case of 0 < α 1 and β = 1 considered in Reference [2]. Table 1 shows the values (In the tables we write the values as x ( y ) instead of x × 10 y .) of the absolute relative error in the computation of Ein α , 1 ( x ) from the asymptotic expansions in Theorem 2 for several values of x and different α in the extended range 0 < α 2 . The expansion for 0 < α < 2 is given by the algebraic expansion in (21); this contains a logarithmic term for the values α = 1 4 , 1 2 , 1 . The progressive loss of accuracy when α > 1 can be attributed to the presence of the approaching exponentially large sector, whose lower boundary is, from (15), given by θ 0 = π ( 2 α ) / ( 2 α ) . In the final case α = 2 , the accuracy is seen to suddenly increase considerably. This is due to the inclusion of the (oscillatory) exponential contribution, which from (22), takes the form
Ein 2 , 1 ( x ) 1 2 π 1 x j = 1 j ! x j + 1 cos ( x 1 2 π j ) ( x + ) .
In Figure 1 we show some plots of Ein α , 1 ( x ) for values of α in the range 0 < α 1 . In Figure 2 the asymptotic approximations for two values of α are shown compared with the corresponding curves of Ein α , 1 ( x ) .
Table 2 shows the values of the absolute relative error in the computation of Ein α , β ( z ) from the asymptotic expansions in Theorem 1 for complex z for values of α in the range 0 < α 2 . It will noticed that there is a sudden reduction in the error when α = 1 and θ = π / 4 . In this case, the value of θ 0 = 1 2 π and a more accurate treatment would include the exponentially small contribution z E α , β ( z ) . When this term is included we find the absolute relative error equal to 6.935 × 10 11 .
Finally, in Table 3 we present the error associated with the expansions of the generalised sine and cosine integrals Sin α , β ( x ) and Cin α , β ( x ) as x + given in Theorems 3–5. For Sin α , β ( x ) , the logarithmic expansion in (30) arises for α = 1 4 and α = 1 2 ; for Cin α , β ( x ) the logarithmic expansion in (31) arises for α = 1 3 . In Figure 3 are shown plots (We remark that the plot of Cin α 1 ( x ) in Figure 3b differs from that shown in Figure 4 of Reference [2].) of Sin α , 1 ( x ) and Cin α , 1 ( x ) for different α and in Figure 4 the leading asymptotic approximations from the expansions in Theorem 5 are compared with the corresponding plots of these functions.
In conclusion, it is worth mentioning that the function Ein α , β ( z ) , and also the generalised sine and cosine integrals, can be extended by using the three-parameter Mittag-Leffler function (or Prabhakar function) defined by
E α , β ρ ( z ) = n = 0 ( ρ ) n Γ ( α n + β ) z n n ! .
A comprehensive discussion of this function and its applications can be found in Reference [10]; see also Reference [6] Section 5.1, for details of its large-z asymptotic expansion.

6. Conclusions

The large-z asymptotic expansions of the modified exponential integral Ein α , β ( z ) involving the two-parameter Mittag-Leffer function have been determined by exploiting the known asymptotic theory developed for integral functions of hypergeometric type, namely the Fox-Wright function. The appearance of logarithmic terms in the expansion of Ein α , β ( x ) for x + for certain values of α ( 0 , 1 ] is emphasised. Similar expansions have been obtained for the extended sine and cosine integrals.

Funding

This research received no external funding.

Acknowledgments

I would like to thank Francesco Mainardi for the invitation to contribute to this special edition.

Conflicts of Interest

The author declares no conflict of interest.

References

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Figure 1. Plots of Ein α , 1 ( x ) for different values of α .
Figure 1. Plots of Ein α , 1 ( x ) for different values of α .
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Figure 2. Plots of Ein α , 1 ( x ) (solid curves) and the leading asymptotic approximation (dashed curves) for (a) α = 0.75 and (b) α = 1 .
Figure 2. Plots of Ein α , 1 ( x ) (solid curves) and the leading asymptotic approximation (dashed curves) for (a) α = 0.75 and (b) α = 1 .
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Figure 3. Plots of the generalised sine and cosine integrals (a) Sin α , 1 ( x ) and (b) Cin α , 1 ( x ) for α = 0.25 , 0.50 , 0.75 , 1 .
Figure 3. Plots of the generalised sine and cosine integrals (a) Sin α , 1 ( x ) and (b) Cin α , 1 ( x ) for α = 0.25 , 0.50 , 0.75 , 1 .
Mathematics 08 00428 g003
Figure 4. Plots of the generalised sine and cosine integrals (solid curves) and their leading asymptotic approximations (dashed curves) from Theorems 3, 4 and 5: (a) Sin α , 1 ( x ) when α = 0.25 , 0.75 , (b) Sin α , 1 ( x ) when α = 1 , (c) Cin α , 1 ( x ) when α = 0.25 , 0.75 and (d) Cin α , 1 ( x ) when α = 1 .
Figure 4. Plots of the generalised sine and cosine integrals (solid curves) and their leading asymptotic approximations (dashed curves) from Theorems 3, 4 and 5: (a) Sin α , 1 ( x ) when α = 0.25 , 0.75 , (b) Sin α , 1 ( x ) when α = 1 , (c) Cin α , 1 ( x ) when α = 0.25 , 0.75 and (d) Cin α , 1 ( x ) when α = 1 .
Mathematics 08 00428 g004aMathematics 08 00428 g004b
Table 1. The absolute relative error in the computation of Ein α , β ( x ) from Theorem 2 for different values of α and x when β = 1 .
Table 1. The absolute relative error in the computation of Ein α , β ( x ) from Theorem 2 for different values of α and x when β = 1 .
x α = 0.25 α = 0.40 α = 0.50 α = 0.75 α = 1.00
5 1.602 × 10 4 1.678 × 10 5 2.012 × 10 4 2.115 × 10 4 5.249 × 10 4
10 5.733 × 10 7 1.735 × 10 7 4.413 × 10 7 2.339 × 10 7 1.442 × 10 6
20 3.680 × 10 11 3.031 × 10 11 6.526 × 10 12 9.362 × 10 12 2.753 × 10 11
30 1.808 × 10 16 9.384 × 10 16 1.543 × 10 16 1.337 × 10 16 7.595 × 10 16
x α = 1.20 α = 1.40 α = 1.60 α = 1.80 α = 2.00
5 1.121 × 10 3 1.301 × 10 4 5.279 × 10 3 1.407 × 10 2 1.550 × 10 3
10 4.345 × 10 6 3.168 × 10 5 2.103 × 10 4 1.536 × 10 4 2.849 × 10 6
20 2.147 × 10 10 2.277 × 10 8 1.671 × 10 6 4.751 × 10 5 4.926 × 10 10
30 4.388 × 10 14 2.363 × 10 11 2.125 × 10 8 6.216 × 10 6 1.613 × 10 14
Table 2. The absolute relative error in the computation of Ein α , β ( z ) from Theorem 1 for different α and θ when z = 20 e i θ and β = 1 / 3 .
Table 2. The absolute relative error in the computation of Ein α , β ( z ) from Theorem 1 for different α and θ when z = 20 e i θ and β = 1 / 3 .
θ α = 0.40 α = 0.50 α = 1.00 α = 1.50 α = 2.00
0 2.400 × 10 8 5.494 × 10 10 2.702 × 10 10 1.572 × 10 6 5.119 × 10 10
π / 4 2.553 × 10 8 1.820 × 10 9 1.142 × 10 7 1.202 × 10 8 8.204 × 10 8
π / 2 3.026 × 10 8 4.057 × 10 9 1.756 × 10 10 2.021 × 10 8 3.684 × 10 7
3 π / 4 3.897 × 10 8 8.028 × 10 9 1.423 × 10 9 2.320 × 10 7 8.204 × 10 8
π 5.398 × 10 8 1.617 × 10 8 6.457 × 10 9 3.005 × 10 3 5.119 × 10 10
Table 3. The absolute relative error in the computation of Sin α , β ( x ) and Cin α , β ( x ) from Theorems 3–5 for different α and x when β = 4 / 3 .
Table 3. The absolute relative error in the computation of Sin α , β ( x ) and Cin α , β ( x ) from Theorems 3–5 for different α and x when β = 4 / 3 .
Sin α , β ( x )
x α = 1 / 4 α = 1 / 3 α = 1 / 2 α = 2 / 3 α = 1
10 4.396 × 10 7 1.394 × 10 8 1.785 × 10 6 3.410 × 10 6 1.012 × 10 5
20 3.213 × 10 11 1.171 × 10 13 3.920 × 10 11 2.076 × 10 8 3.094 × 10 11
25 2.373 × 10 13 3.792 × 10 14 2.098 × 10 13 4.437 × 10 10 3.270 × 10 12
30 1.879 × 10 15 5.065 × 10 15 1.172 × 10 15 8.197 × 10 12 8.010 × 10 15
Cin α , β ( x )
x α = 1 / 4 α = 1 / 3 α = 1 / 2 α = 2 / 3 α = 1
10 9.237 × 10 8 3.787 × 10 7 6.608 × 10 7 2.270 × 10 5 7.756 × 10 6
20 1.293 × 10 12 4.473 × 10 12 1.090 × 10 11 2.462 × 10 10 2.576 × 10 10
25 8.066 × 10 14 2.334 × 10 16 5.326 × 10 14 6.881 × 10 11 1.437 × 10 12
30 1.160 × 10 16 9.285 × 10 17 2.764 × 10 16 2.934 × 10 12 7.716 × 10 15

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Paris, R. Asymptotic Expansion of the Modified Exponential Integral Involving the Mittag-Leffler Function. Mathematics 2020, 8, 428. https://doi.org/10.3390/math8030428

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Paris R. Asymptotic Expansion of the Modified Exponential Integral Involving the Mittag-Leffler Function. Mathematics. 2020; 8(3):428. https://doi.org/10.3390/math8030428

Chicago/Turabian Style

Paris, Richard. 2020. "Asymptotic Expansion of the Modified Exponential Integral Involving the Mittag-Leffler Function" Mathematics 8, no. 3: 428. https://doi.org/10.3390/math8030428

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