Trigonometric integral

From Wikipedia, the free encyclopedia
(Redirected from Integral sine)
Jump to navigation Jump to search
Plot of the hyperbolic sine integral function Shi(z) in the complex plane from −2 − 2i to 2 + 2i
Plot of the hyperbolic sine integral function Shi(z) in the complex plane from −2 − 2i to 2 + 2i

Si(x) (blue) and Ci(x) (green) shown on the same plot.
Sine integral in the complex plane, plotted with a variant of domain coloring.
Cosine integral in the complex plane. Note the branch cut along the negative real axis.

In mathematics, trigonometric integrals are a family of nonelementary integrals involving trigonometric functions.

Sine integral

[edit | edit source]
File:Sine integral.svg
Plot of Si(x) for 0 ≤ x ≤ 8π.
Plot of the cosine integral function Ci(z) in the complex plane from −2 − 2i to 2 + 2i
Plot of the cosine integral function Ci(z) in the complex plane from −2 − 2i to 2 + 2i

The different sine integral definitions are Si(x)=0xsinttdt si(x)=xsinttdt.

Note that the integrand sin(t)t is the sinc function, and also the zeroth spherical Bessel function. Since sinc is an even entire function (holomorphic over the entire complex plane), Si is entire, odd, and the integral in its definition can be taken along any path connecting the endpoints.

By definition, Si(x) is the antiderivative of sin x / x whose value is zero at x = 0, and si(x) is the antiderivative whose value is zero at x = ∞. Their difference is given by the Dirichlet integral, Si(x)si(x)=0sinttdt=π2 or Si(x)=π2+si(x).

In signal processing, the oscillations of the sine integral cause overshoot and ringing artifacts when using the sinc filter, and frequency domain ringing if using a truncated sinc filter as a low-pass filter.

Related is the Gibbs phenomenon: If the sine integral is considered as the convolution of the sinc function with the Heaviside step function, this corresponds to truncating the Fourier series, which is the cause of the Gibbs phenomenon.

Cosine integral

[edit | edit source]
File:Cosine integral.svg
Plot of Ci(x) for 0 < x ≤ 8π

The different cosine integral definitions are Cin(x)0x 1cost t dt.

Cin is an even, entire function. For that reason, some texts define Cin as the primary function, and derive Ci in terms of Cin .

Ci(x)x cost t dt =γ+lnx0x 1cost t dt

=γ+lnxCinx for | Arg(x) |<π , where γ ≈ 0.57721566490 ... is the Euler–Mascheroni constant. Some texts use ci instead of Ci. The restriction on Arg(x) is to avoid a discontinuity (shown as the orange vs blue area on the left half of the plot above) that arises because of a branch cut in the standard logarithm function (ln).

Ci(x) is the antiderivative of cos x/ x (which vanishes as  x ). The two definitions are related by Ci(x)=γ+lnxCin(x).

Hyperbolic sine integral

[edit | edit source]

The hyperbolic sine integral is defined as Shi(x)=0xsinh(t)tdt.

It is related to the ordinary sine integral by Si(ix)=iShi(x).

Hyperbolic cosine integral

[edit | edit source]

The hyperbolic cosine integral is

Plot of the hyperbolic cosine integral function Chi(z) in the complex plane from −2 − 2i to 2 + 2i
Plot of the hyperbolic cosine integral function Chi(z) in the complex plane from −2 − 2i to 2 + 2i

Chi(x)=γ+lnx+0xcosht1tdt for |Arg(x)|<π, where γ is the Euler–Mascheroni constant.

It has the series expansion Chi(x)=γ+ln(x)+x24+x496+x64320+x8322560+x1036288000+O(x12).

Auxiliary functions

[edit | edit source]

Trigonometric integrals can be understood in terms of the so-called "auxiliary functions" f(x)0sin(t)t+xdt=0extt2+1dt=Ci(x)sin(x)+[π2Si(x)]cos(x),g(x)0cos(t)t+xdt=0textt2+1dt=Ci(x)cos(x)+[π2Si(x)]sin(x). Using these functions, the trigonometric integrals may be re-expressed as (cf. Abramowitz & Stegun, p. 232) π2Si(x)=si(x)=f(x)cos(x)+g(x)sin(x), and Ci(x)=f(x)sin(x)g(x)cos(x).

Nielsen's spiral

[edit | edit source]
File:Nielsen's spiral.png
Nielsen's spiral.

The spiral formed by parametric plot of si, ci is known as Nielsen's spiral. x(t)=a×ci(t) y(t)=a×si(t)

The spiral is closely related to the Fresnel integrals and the Euler spiral. Nielsen's spiral has applications in vision processing, road and track construction and other areas.[1]

Expansion

[edit | edit source]

Various expansions can be used for evaluation of trigonometric integrals, depending on the range of the argument.

Asymptotic series (for large argument)

[edit | edit source]

Si(x)π2cosxx(12!x2+4!x46!x6)sinxx(1x3!x3+5!x57!x7) Ci(x)sinxx(12!x2+4!x46!x6)cosxx(1x3!x3+5!x57!x7).

These series are asymptotic and divergent, although can be used for estimates and even precise evaluation at ℜ(x) ≫ 1.

Convergent series

[edit | edit source]

Si(x)=n=0(1)nx2n+1(2n+1)(2n+1)!=xx33!3+x55!5x77!7± Ci(x)=γ+lnx+n=1(1)nx2n2n(2n)!=γ+lnxx22!2+x44!4

These series are convergent at any complex x, although for |x| ≫ 1, the series will converge slowly initially, requiring many terms for high precision.

Derivation of series expansion

[edit | edit source]

From the Maclaurin series expansion of sine: sinx=xx33!+x55!x77!+x99!x1111!+ sinxx=1x23!+x45!x67!+x89!x1011!+ sinxxdx=xx33!3+x55!5x77!7+x99!9x1111!11+

Relation with the exponential integral of imaginary argument

[edit | edit source]

The function E1(z)=1exp(zt)tdt for (z)0 is called the exponential integral. It is closely related to Si and Ci, E1(ix)=i(π2+Si(x))Ci(x)=isi(x)Ci(x) for x>0.

As each respective function is analytic except for the cut at negative values of the argument, the area of validity of the relation should be extended to (Outside this range, additional terms which are integer factors of π appear in the expression.)

Cases of imaginary argument of the generalized integro-exponential function are 1cos(ax)lnxxdx=π224+γ(γ2+lna)+ln2a2+n1(a2)n(2n)!(2n)2, which is the real part of 1eiaxlnxxdx=π224+γ(γ2+lna)+ln2a2π2i(γ+lna)+n1(ia)nn!n2.

Similarly 1eiaxlnxx2dx=1+ia[π224+γ(γ2+lna1)+ln2a2lna+1]+πa2(γ+lna1)+n1(ia)n+1(n+1)!n2.

Efficient evaluation

[edit | edit source]

Padé approximants of the convergent Taylor series provide an efficient way to evaluate the functions for small arguments. The following formulae, given by Rowe et al. (2015),[2] are accurate to better than 10−16 for 0 ≤ x ≤ 4, Si(x)x(14.54393409816329991102x2+1.15457225751016682103x41.41018536821330254105x6+9.43280809438713025108x83.532019789971683571010x10+7.082402822748759111013x126.053382120104224771016x141+1.01162145739225565102x2+4.99175116169755106105x4+1.55654986308745614107x6+3.280675710557897341010x8+4.50490975753865811013x10+3.211070511937121681016x12)Ci(x)γ+ln(x)+x2(0.25+7.51851524438898291103x21.27528342240267686104x4+1.05297363846239184106x64.68889508144848019109x8+1.064808028911892431011x109.937284888575854071015x121+1.1592605689110735102x2+6.72126800814254432105x4+2.55533277086129636107x6+6.970712957609589461010x8+1.385363527727786191012x10+1.891060547130597591015x12+1.397596167313768551018x14)

The integrals may be evaluated indirectly via auxiliary functions f(x) and g(x), which are defined by

Si(x)=π2f(x)cos(x)g(x)sin(x) Ci(x)=f(x)sin(x)g(x)cos(x)
or equivalently
f(x)[π2Si(x)]cos(x)+Ci(x)sin(x) g(x)[π2Si(x)]sin(x)Ci(x)cos(x)

For x4 the Padé rational functions given below approximate f(x) and g(x) with error less than 10−16:[2]

f(x)1x(1+7.44437068161936700618102x2+1.96396372895146869801105x4+2.37750310125431834034107x6+1.43073403821274636888109x8+4.337362388704325227651010x10+6.405338305740220229111011x12+4.209681805710769402081012x14+1.007951829803685746171013x16+4.948166881999519634821012x184.947011686454159599311011x201+7.46437068161927678031102x2+1.97865247031583951450105x4+2.41535670165126845144107x6+1.47478952192985464958109x8+4.585951158477657798301010x10+7.085013081495154015631011x12+5.060844645934750767741012x14+1.434685491715810164791013x16+1.115354935099142540971013x18)g(x)1x2(1+8.1359520115168615102x2+2.35239181626478200105x4+3.12557570795778731107x6+2.06297595146763354109x8+6.830522054236250071010x10+1.090495284503627861012x12+7.576645832578343491012x14+1.810044874646645751013x16+6.432916131430494851012x181.365171376708716891012x201+8.19595201151451564102x2+2.40036752835578777105x4+3.26026661647090822107x6+2.23355543278099360109x8+7.874650173418299301010x10+1.398667106964145651012x12+1.171647233717366051013x14+4.018390873076566201013x16+3.996532578874908111013x18)

See also

[edit | edit source]

References

[edit | edit source]
  1. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  2. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).

Further reading

[edit | edit source]
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value)..
[edit | edit source]
  • http://mathworld.wolfram.com/SineIntegral.html
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).