Trigonometric integral

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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 Template:Math in the complex plane from Template:Math to Template:Math

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Template:Math (blue) and Template:Math (green) shown on the same plot.
Sine integral in the complex plane, plotted with a variant of domain coloring.
Template:AnchorCosine 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

Plot of Template:Math for Template:Math.
Plot of the cosine integral function Ci(z) in the complex plane from −2 − 2i to 2 + 2i
Plot of the cosine integral function Template:Math in the complex plane from Template:Math to Template:Math

The different sine integral definitions are Si⁡(x)=−∫0xsin⁡ttdtsi⁡(x)=−∫x∞sin⁡ttdt.

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

By definition, Template:Tmath is the antiderivative of Template:Tmath whose value is zero at Template:Tmath, and Template:Tmath is the antiderivative whose value is zero at Template:Tmath. Their difference is given by the Dirichlet integral, Si⁡(x)−si⁡(x)=∫0∞sin⁡ttdt=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

Plot of Template:Math for Template:Math

The different cosine integral definitions are Cin⁡(x)≡∫0x1−cos⁡ttdt.

Template:Tmath is an even, entire function. For that reason, some texts define Template:Tmath as the primary function, and derive Template:Tmath in terms of Template:Tmath.Template:Sfnp

Ci⁡(x)≡−∫x∞cos⁡ttdt=γ+ln⁡x−∫0x1−cos⁡ttdt=γ+ln⁡x−Cin⁡(x), for Template:Tmath, where Template:Tmath is the Euler–Mascheroni constant. Some texts use Template:Tmath instead of Template:Tmath. The restriction on Template:Math 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 (Template:Tmath).

Template:Tmath is the antiderivative of Template:Tmath (which vanishes as Template:Tmath). The two definitions are related by Ci⁡(x)=γ+ln⁡x−Cin⁡(x).

Hyperbolic sine integral

The hyperbolic sine integral is defined as Shi⁡(x)=∫0xsinh⁡ttdt.

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

Hyperbolic cosine integral

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 Template:Math in the complex plane from Template:Math to Template:Math

Chi⁡(x)=γ+ln⁡x+∫0xcosh⁡(t)−1tdt 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

Trigonometric integrals can be understood in terms of the so-called "auxiliary functions" f(x)≡∫0∞sin⁡tt+xdt=∫0∞e−xtt2+1dt=−Ci⁡(x)sin⁡x−si⁡(x)cos⁡x=−Ci⁡(x)sin⁡x+[π2−Si⁡(x)]cos⁡x,g(x)≡∫0∞cos⁡tt+xdt=∫0∞te−xtt2+1dt=−Ci⁡(x)cos⁡x−si⁡(x)sin⁡x=−Ci⁡(x)cos⁡x+[π2−Si⁡(x)]sin⁡x. Using these functions, the trigonometric integrals may be re-expressed asTemplate:Sfnp Si⁡(x)=π2−f(x)cos⁡x+g(x)sin⁡x,Ci⁡(x)=π2−f(x)sin⁡x−g(x)cos⁡x.

Nielsen's spiral

Nielsen's spiral.

The spiral formed by parametric plot of Template:Tmath, Template:Tmath 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.[1]Template:Failed verification span

Expansion

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

Asymptotic series (for large argument)

Si⁡(x)∼π2−cos⁡xx(1−2!x2+4!x4−6!x6+⋯)−sin⁡xx(1x−3!x3+5!x5−7!x7+⋯),Ci⁡(x)∼π2−sin⁡xx(1−2!x2+4!x4−6!x6+⋯)−cos⁡xx(1x−3!x3+5!x5−7!x7+⋯).

These series are asymptotic and divergent, although can be used for estimates and even precise evaluation at Template:Tmath.

Convergent series

Si⁡(x)=∑n=0∞(−1)nx2n+1(2n+1)(2n+1)!=x−x33!⋅3+x55!⋅5−x77!⋅7±⋯ Ci⁡(x)=γ+ln⁡x+∑n=1∞(−1)nx2n2n(2n)!=γ+ln⁡x−x22!⋅2+x44!⋅4∓⋯

These series are convergent at any complex Template:Tmath, although for Template:Tmath, the series will converge slowly initially, requiring many terms for high precision.

Derivation of series expansion

From the Maclaurin series expansion of sine: sin⁡x=x−x33!+x55!−x77!+x99!−x1111!+⋯sin⁡xx=1−x23!+x45!−x67!+x89!−x1011!+⋯∴∫sin⁡xxdx=x−x33!⋅3+x55!⋅5−x77!⋅7+x99!⋅9−x1111!⋅11+⋯

Relation with the exponential integral of imaginary argument

The function E1(z)=∫1∞exp⁡(−zt)tdt for ℜ(z)≥0 is called the exponential integral. It is closely related to Template:Math and Template:Math, 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 Template:Math appear in the expression.)

Cases of imaginary argument of the generalized integro-exponential function are ∫1∞cos⁡(ax)ln⁡xxdx=−π224+γ(γ2+ln⁡a)+ln2a2+∑n≥1(−a2)n(2n)!(2n)2, which is the real part of ∫1∞eiaxln⁡xxdx=−π224+γ(γ2+ln⁡a)+ln2a2−π2i(γ+ln⁡a)+∑n≥1(ia)nn!n2.

Similarly ∫1∞eiaxln⁡xx2dx=1+ia[−π224+γ(γ2+ln⁡a−1)+ln2a2−ln⁡a+1]+πa2(γ+ln⁡a−1)+∑n≥1(ia)n+1(n+1)!n2.

Efficient evaluation

Padé approximants of the convergent Taylor series provide an efficient way to evaluate the functions for small arguments. The following formulae are accurate to better than Template:Val for Template:Tmath:[2] Si⁡(x)≈x⋅(1−4.54393409816329991⋅10−2⋅x2+1.15457225751016682⋅10−3⋅x4−1.41018536821330254⋅10−5⋅x6+9.43280809438713025⋅10−8⋅x8−3.53201978997168357⋅10−10⋅x10+7.08240282274875911⋅10−13⋅x12−6.05338212010422477⋅10−16⋅x141+1.01162145739225565⋅10−2⋅x2+4.99175116169755106⋅10−5⋅x4+1.55654986308745614⋅10−7⋅x6+3.28067571055789734⋅10−10⋅x8+4.5049097575386581⋅10−13⋅x10+3.21107051193712168⋅10−16⋅x12)Ci⁡(x)≈γ+ln⁡(x)+x2⋅(−0.25+7.51851524438898291⋅10−3⋅x2−1.27528342240267686⋅10−4⋅x4+1.05297363846239184⋅10−6⋅x6−4.68889508144848019⋅10−9⋅x8+1.06480802891189243⋅10−11⋅x10−9.93728488857585407⋅10−15⋅x121+1.1592605689110735⋅10−2⋅x2+6.72126800814254432⋅10−5⋅x4+2.55533277086129636⋅10−7⋅x6+6.97071295760958946⋅10−10⋅x8+1.38536352772778619⋅10−12⋅x10+1.89106054713059759⋅10−15⋅x12+1.39759616731376855⋅10−18⋅x14)

The integrals may be evaluated indirectly via auxiliary functions Template:Tmath and Template:Tmath Template:See above defined as: Si⁡(x)=π2−f(x)cos⁡x−g(x)sin⁡x,Ci⁡(x)=π2−f(x)sin⁡x−g(x)cos⁡x; or equivalently: f(x)≡[π2−Si⁡(x)]cos⁡x+Ci⁡(x)sin⁡x,g(x)≡[π2−Si⁡(x)]sin⁡x−Ci⁡(x)cos⁡x.

For x≥4 the Padé rational functions given below approximate f(x) and g(x) with error less than Template:Val:[2]

f(x)≈1x⋅(1+7.44437068161936700618⋅102⋅x−2+1.96396372895146869801⋅105⋅x−4+2.37750310125431834034⋅107⋅x−6+1.43073403821274636888⋅109⋅x−8+4.33736238870432522765⋅1010⋅x−10+6.40533830574022022911⋅1011⋅x−12+4.20968180571076940208⋅1012⋅x−14+1.00795182980368574617⋅1013⋅x−16+4.94816688199951963482⋅1012⋅x−18−4.94701168645415959931⋅1011⋅x−201+7.46437068161927678031⋅102⋅x−2+1.97865247031583951450⋅105⋅x−4+2.41535670165126845144⋅107⋅x−6+1.47478952192985464958⋅109⋅x−8+4.58595115847765779830⋅1010⋅x−10+7.08501308149515401563⋅1011⋅x−12+5.06084464593475076774⋅1012⋅x−14+1.43468549171581016479⋅1013⋅x−16+1.11535493509914254097⋅1013⋅x−18)g(x)≈1x2⋅(1+8.1359520115168615⋅102⋅x−2+2.35239181626478200⋅105⋅x−4+3.12557570795778731⋅107⋅x−6+2.06297595146763354⋅109⋅x−8+6.83052205423625007⋅1010⋅x−10+1.09049528450362786⋅1012⋅x−12+7.57664583257834349⋅1012⋅x−14+1.81004487464664575⋅1013⋅x−16+6.43291613143049485⋅1012⋅x−18−1.36517137670871689⋅1012⋅x−201+8.19595201151451564⋅102⋅x−2+2.40036752835578777⋅105⋅x−4+3.26026661647090822⋅107⋅x−6+2.23355543278099360⋅109⋅x−8+7.87465017341829930⋅1010⋅x−10+1.39866710696414565⋅1012⋅x−12+1.17164723371736605⋅1013⋅x−14+4.01839087307656620⋅1013⋅x−16+3.99653257887490811⋅1013⋅x−18)

See also

References

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Further reading

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Template:Nonelementary Integral