Dottie number

{{Short description|Mathematical constant related to the cosine function}}

file:Cosine_fixed_point.svg of the cosine function.]]

In mathematics, the Dottie number or the cosine constant is a constant that is the unique real root of the equation

: \cos x = x ,

where the argument of \cos is in radians.

The decimal expansion of the Dottie number is given by:

: {{mvar|D}} = {{val|0.739085133215160641655312087673}}... {{OEIS|id=A003957}}.

Since \cos(x) - x is decreasing and its derivative is non-zero at \cos(x) - x = 0, it only crosses zero at one point. This implies that the equation \cos(x) = x has only one real solution. It is the single real-valued fixed point of the cosine function and is a nontrivial example of a universal attracting fixed point. It is also a transcendental number because of the Lindemann–Weierstrass theorem.{{cite web|url=http://mathworld.wolfram.com/DottieNumber.html|author=Eric W. Weisstein|authorlink=Eric W. Weisstein|title=Dottie Number}} The generalised case \cos z = z for a complex variable z has infinitely many roots, but unlike the Dottie number, they are not attracting fixed points.

file:quadrisection.svg

History

The constant appeared in publications as early as 1860s.{{Cite web |last=Weisstein |first=Eric W. |title=Dottie Number |url=https://mathworld.wolfram.com/DottieNumber.html |access-date=2025-01-29 |website=mathworld.wolfram.com |language=en}} Norair Arakelian used lowercase ayb (ա) from the Armenian alphabet to denote the constant.

The constant name was coined by Samuel R. Kaplan in 2007. It originates from a professor of French named Dottie who observed the number by repeatedly pressing the cosine button on her calculator.{{refn|group=nb|If a calculator is set to take angles in degrees, the sequence of numbers will instead converge to 0.999847...,{{Cite OEIS|A330119}} the root of \cos\left(\frac{\pi}{180}x\right) = x.}}

The Dottie number, for which an exact series expansion can be obtained using the Faà di Bruno formula, has interesting connections with the Kepler and Bertrand's circle problems.{{cite arXiv |last=Pain |first=Jean-Christophe |date=2023 |title=An exact series expansion for the Dottie number |class=math.NT |eprint=2303.17962}}

Identities

The Dottie number appears in the closed form expression of some integrals:{{Citation |last=Michos |first=Alexander |title=A Brief Investigation of an Integral Representation of Dottie's Number |date=2023-03-03 |url=https://osf.io/3rzj5 |access-date=2024-09-24 |doi=10.31219/osf.io/3rzj5}}{{cite web |title=Integral Representation of the Dottie Number |url=https://math.stackexchange.com/questions/2446725/integral-representation-of-the-dottie-number |website=Mathematics Stack Exchange |language=en}}

:\int _0^{\infty }\ln \left(\frac{4\left(x+\sinh x\right)^2+\pi^2}{4(x-\sinh x)^2+\pi ^2}\right)\mathrm{d} x = \pi^2 - 2\pi D

:\int_{0 }^{\infty } \frac{3\pi^2+4(x-\sinh x)^2}{(3\pi^2+4(x-\sinh x)^2)^2 + 16\pi^2(x-\sinh x)^2} \, \mathrm dx = \frac1{8+8\sqrt{1-D^2}}

Using the Taylor series of the inverse of f(x) = \cos(x) - x at \frac{\pi}{2} (or equivalently, the Lagrange inversion theorem), the Dottie number can be expressed as the infinite series:

: D = \frac{\pi}{2}+\sum_{n\,\mathrm{odd}} a_{n} \pi^{n}

where each a_n is a rational number defined for odd n as{{cite journal |last1=Kaplan |first1=Samuel R |date=February 2007 |title=The Dottie Number |url=https://www.maa.org/sites/default/files/Kaplan2007-131105.pdf |journal=Mathematics Magazine |volume=80 |page=73 |doi=10.1080/0025570X.2007.11953455 |s2cid=125871044 |accessdate=29 November 2017}}{{Cite web |title=OEIS A302977 Numerators of the rational factor of Kaplan's series for the Dottie number. |url=https://oeis.org/A302977 |access-date=2019-05-26 |website=oeis.org}}{{Cite web |title=A306254 - OEIS |url=https://oeis.org/A306254 |access-date=2019-07-22 |website=oeis.org}}{{refn|group=nb|Kaplan does not give an explicit formula for the terms of the series, which follows trivially from the Lagrange inversion theorem.}}

:\begin{align}

a_n&=\frac{1}{n!2^n}\lim_{m\to\frac\pi2}

\frac{\partial^{n-1}}{\partial m^{n-1}}{\left(\frac{\cos m}{m-\pi/2}-1\right)^{-n}}

\\&=-\frac{1}{4},-\frac{1}{768},-\frac{1}{61440},-\frac{43}{165150720},\ldots

\end{align}

The Dottie number can also be expressed as:

:D=\sqrt{1-\left(2I^{-1}_\frac12\left(\frac 12,\frac 32\right)-1\right)^2},

where I^{-1} is the inverse of the regularized beta function. This value can be obtained using Kepler's equation, along with other equivalent closed forms.

In Microsoft Excel and LibreOffice Calc spreadsheets, the Dottie number can be expressed in closed form as {{code|SQRT(1-(2*BETA.INV(1/2,1/2,3/2)-1)^2)|dax|style=white-space:nowrap}}. In the Mathematica computer algebra system, the Dottie number is {{code|Sqrt[1 - (2 InverseBetaRegularized[1/2, 1/2, 3/2] - 1)^2]|mathematica|style=white-space:nowrap}}.

Another closed form representation:

:D=- \tanh\left(2\text{ arctanh}\left(\frac1{\sqrt3} \operatorname{InvT} \left(\frac14,3\right)\right)\right)=-\frac{2\sqrt3 {\operatorname{InvT}\left(\frac14,3\right)}}{\operatorname{InvT}^2\left(\frac14,3\right)+3},

where \operatorname{InvT} is the inverse survival function of Student's t-distribution. In Microsoft Excel and LibreOffice Calc, due to the specifics of the realization of `TINV` function, this can be expressed as formulas {{code|2 *SQRT(3)* TINV(1/2, 3)/(TINV(1/2, 3)^2+3)|dax|style=white-space:nowrap}} and {{code|TANH(2*ATANH(1/SQRT(3) * TINV(1/2,3)))|dax|style=white-space:nowrap}}.

Notes

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References

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