Sinc function
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In mathematics, the sinc function (for sinus cardinalis), also known as the interpolation function, filtering function or the first spherical Bessel function <math>j_0(x)\,</math>, is the product of a sine function and a monotonically decreasing function. It is defined by:
- <math>\operatorname{sinc}(x)
= \left\{ \begin{matrix} \frac{\sin(x)}{x}&:~x\ne 0 \\ \\ 1 &:~x=0 \end{matrix} \right. </math>
which oscillates within an envelope of ±1/x.
It is also sometimes defined as simply sin(x)/x, which has a removable singularity at zero since:
- <math>\lim_{x \to 0} \frac{\sin(x)}{x}=1\,</math>
Therefore the latter definition yields a function that is analytic everywhere.
An interesting property of the sinc function is that its local maxima and minima correspond to its intersections with the cosine curve. That is if <math>|\operatorname{sinc}(x)|</math> has a local maximum at <math>x = a\,</math>, then:
- <math>\mathrm{sinc}(a)=\textrm{cos}(a). \,</math>
Applications of the sinc function are found in digital signal processing, communication theory, control theory, and optics.
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Normalization and properties
A normalized sinc function is defined as:
- <math>\mathrm{sinc}_{\pi}(x) \equiv \textrm{sinc}(\pi x)\,</math>
It is important to note that <math>\mathrm{sinc}_{\pi}(x)\,</math> is also commonly referred to as the sinc function and written <math>\mathrm{sinc}(x)\,</math>. The normalization produces the simplest form of several properties and identities:
1. The zero-crossings occur at integer values of <math>x\,</math>.
2. The Fourier transform [to ordinary frequency] is <math>\mathrm{rect(f)}\,</math>. I.e., row 12 of important Fourier transforms, with <math>a = \pi\,</math>.
3. <math>\int_{-\infty}^\infty \mathrm{sinc}_{\pi}(x)\,dx = 1</math>,
- where the integral is regarded as an improper integral; it cannot be taken to be a Lebesgue integral because:
- <math>\int_{-\infty}^\infty \left|\mathrm{sinc}_{\pi}(x)\right|\,dx = \infty.</math>
4. <math>\mathrm{sinc}_{\pi}(x) = \prod_{n=1}^\infty \left(1 - \frac{x^2}{n^2}\right)</math>
5. <math>\mathrm{sinc}_{\pi}(x) = \frac{1}{\Gamma(1+x)\Gamma(1-x)} = \frac{1}{x! (-x)!}</math>
- where <math>\Gamma</math> is the gamma function.
Relationship to delta function
In the language of distributions, the sinc function is related to the delta function δ(x) by
- <math>\lim_{a\rightarrow 0}\frac{1}{\pi a}\textrm{sinc}(x/a)=\delta(x).</math>
This is not an ordinary limit, since the left side does not converge. Rather, it means that
- <math>\lim_{a\rightarrow 0}\int_{-\infty}^\infty \frac{1}{\pi a}\textrm{sinc}(x/a)\varphi(x)\,dx
=\int_{-\infty}^\infty\delta(x)\varphi(x)\,dx = \varphi(0),
</math>
for any smooth function <math>\varphi(x)</math> with compact support.
In the above expression, as a approaches zero, the number of oscillations per unit length of the sinc function approaches infinity. Nevertheless, the expression always oscillates inside an envelope of ±1/(πx), regardless of the value of a. This contradicts the informal picture of δ(x) as being zero for all x except at the point x=0 and illustrates the problem of thinking of the delta function as a function rather than as a distribution. A similar situation is found in the Gibbs phenomenon.
See also
- Anti-aliasing & Sinc filter
- Trigonometric function
- L'Hôpital's rule
- Nyquist-Shannon interpolation formula