Arctangent series explained
In mathematics, the arctangent series, traditionally called Gregory's series, is the Taylor series expansion at the origin of the arctangent function:
This series converges in the complex disk
except for
(where
It was first discovered in the 14th century by Indian mathematician Mādhava of Sangamagrāma (– c. 1425), the founder of the Kerala school, and is described in extant works by Nīlakaṇṭha Somayāji (c. 1500) and Jyeṣṭhadeva (c. 1530). Mādhava's work was unknown in Europe, and the arctangent series was independently rediscovered by James Gregory in 1671 and by Gottfried Leibniz in 1673. In recent literature the arctangent series is sometimes called the Mādhava–Gregory series to recognize Mādhava's priority (see also Mādhava series).[1]
The special case of the arctangent of is traditionally called the Leibniz formula for , or recently sometimes the Mādhava–Leibniz formula:
The extremely slow convergence of the arctangent series for
makes this formula impractical per se. Kerala-school mathematicians
used additional correction terms to speed convergence. John Machin (1706) expressed as a sum of arctangents of smaller values, eventually resulting in a variety of
Machin-like formulas for .
Isaac Newton (1684) and other mathematicians
accelerated the convergence of the series via various transformations.
Proof
If
then
The derivative is
Taking the reciprocal,
This sometimes is used as a definition of the arctangent:
The Maclaurin series for is a geometric series:
=1-x2+x4-x6+ … =
l({-x2}r){\vphantom)}k.
One can find the Maclaurin series for
by naïvely integrating term-by-term:
&=
\left(1-u2+u4-u6+ … \right)du\\[5mu]
&=x-
3+
5-
7+ …
=
.
\end{align}
While this turns out correctly, integrals and infinite sums cannot always be exchanged in this manner. To prove that the integral on the left converges to the sum on the right for real
can instead be written as the
finite sum,
[2]
=1-x2+x4- … +l({-x2}r){\vphantom)}N
+
N+1
}.
Again integrating both sides,
}\,du.
In the limit as
the integral on the right above tends to zero when
because
}\,du \,\Biggr|\,&\leq \int_0^1 \frac\,du\\[5mu]&< \int_0^1 u^du\,=\, \frac \,\to\, 0.\end
Therefore,
\begin{align}
\arctanx=
.
\end{align}
Convergence
The series for and
converge within the complex disk
, where both functions are
holomorphic. They diverge for
because when
, there is a
pole:
When
the partial sums
alternate between the values
and
never converging to the value
However, its term-by-term integral, the series for (barely) converges when
because
disagrees with its series only at the point
so the difference in integrals can be made arbitrarily small by taking sufficiently many terms:
Because of its exceedingly slow convergence (it takes five billion terms to obtain 10 correct decimal digits), the Leibniz formula is not a very effective practical method for computing Finding ways to get around this slow convergence has been a subject of great mathematical interest.
Accelerated series
Isaac Newton accelerated the convergence of the arctangent series in 1684 (in an unpublished work; others independently discovered the result and it was later popularized by Leonhard Euler's 1755 textbook; Euler wrote two proofs in 1779), yielding a series converging for
\begin{align}
\arctanx
&=
\\[10mu]
&=
+
2}+
3}
+
4}+ … \\[10mu]
&=C(x)\left(S(x)+
+
S(x)5
+
S(x)7+ …
\right),
\end{align}
where
and
Each term of this modified series is a rational function with its poles at
in the
complex plane, the same place where the arctangent function has its poles. By contrast, a polynomial such as the Taylor series for arctangent forces all of its poles to infinity.
History
The earliest person to whom the series can be attributed with confidence is Mādhava of Sangamagrāma (c. 1340 – c. 1425). The original reference (as with much of Mādhava's work) is lost, but he is credited with the discovery by several of his successors in the Kerala school of astronomy and mathematics founded by him. Specific citations to the series for
include
Nīlakaṇṭha Somayāji's
Tantrasaṅgraha (c. 1500),
[3] [4] Jyeṣṭhadeva's
Yuktibhāṣā (c. 1530),
[5] and the
Yukti-dipika commentary by
Sankara Variyar, where it is given in verses 2.206 - 2.209.
[6] See also
References
- Book: Berggren . Lennart . Borwein . Jonathan . Jonathan Borwein . Borwein . Peter . Peter Borwein . 2004 . Pi: A Source Book . 3rd . Springer . 10.1007/978-1-4757-4217-6 . 978-1-4419-1915-1 .
- Gupta . Radha Charan . Radha Charan Gupta . 1973 . The Mādhava–Gregory series . The Mathematics Education . 7 . B67–B70 .
- Roy . Ranjan . 1990 . The Discovery of the Series Formula for by Leibniz, Gregory and Nilakantha . Mathematics Magazine . 63 . 5 . 291–306 . 10.1080/0025570X.1990.11977541.
Notes and References
- For example:, ; Book: Joseph, George Gheverghese . George Gheverghese Joseph . The Crest of the Peacock: Non-European Roots of Mathematics . Princeton University Press . 2011 . 3rd . 428 . 1st ed. 1991. Levrie . Paul . 2011 . Lost and Found: An Unpublished -Proof . Mathematical Intelligencer . 33 . 29–32 . 10.1007/s00283-010-9179-y . 121133743. Other combinations of names include, Madhava–Gregory–Leibniz series: Benko . David . Molokach . John . 2013 . The Basel Problem as a Rearrangement of Series . College Mathematics Journal . 44 . 3 . 171–176 . 10.4169/college.math.j.44.3.171 . 124737638 . Madhava–Leibniz–Gregory series: Book: Danesi, Marcel . 2021 . 1. Discovery of π and Its Manifestations . Pi in Nature, Art, and Culture . Brill . 1–30 . 10.1163/9789004433397_002 . 978-90-04-43337-3 . 242107102 . Nilakantha–Gregory series: Campbell . Paul J. . 2004 . Reviews . Borwein, Jonathan, and David Bailey, Mathematics by Experiment . Mathematics Magazine . 77 . 2 . 163 . 10.1080/0025570X.2004.11953245. 218541218 . Gregory–Leibniz–Nilakantha formula: Gawrońska . Natalia . Słota . Damian . Wituła . Roman . Zielonka . Adam . 2013 . Some generalizations of Gregory's power series and their applications . Journal of Applied Mathematics and Computational Mechanics . 12 . 3 . 79–91 . 10.17512/jamcm.2013.3.09 .
- Shirali . Shailesh A. . 1997 . Nīlakaṇṭha, Euler and . Resonance . 2 . 5 . 29–43 . 10.1007/BF02838013 . 121433151 . Also see the erratum: Shirali . Shailesh A. . 1997 . Addendum to 'Nīlakaṇṭha, Euler and ' . Resonance . 2 . 11 . 112 . 10.1007/BF02862651 . free .
- Web site: Tantrasamgraha with English translation . K.V. Sarma . Translated by V.S. Narasimhan . Indian National Academy of Science . 48 . Sanskrit, English . 17 January 2010 . dead . https://web.archive.org/web/20120309014402/http://www.new.dli.ernet.in/rawdataupload/upload/insa/INSA_2/20005a5d_s1.pdf . 9 March 2012 .
- Tantrasamgraha, ed. K.V. Sarma, trans. V. S. Narasimhan in the Indian Journal of History of Science, issue starting Vol. 33, No. 1 of March 1998
- Web site: K. V. Sarma & S Hariharan. Yuktibhāṣā of Jyeṣṭhadeva. A book on rationales in Indian Mathematics and Astronomy—An analytic appraisal. 2006-07-09. https://web.archive.org/web/20060928203221/http://www.new.dli.ernet.in/insa/INSA_1/20005ac0_185.pdf . 28 September 2006.
- Book: C.K. Raju. Cultural Foundations of Mathematics : Nature of Mathematical Proof and the Transmission of the Calculus from India to Europe in the 16 c. CE. Centre for Studies in Civilisation. New Delhi. 2007. History of Science, Philosophy and Culture in Indian Civilisation. X Part 4. 231. 978-81-317-0871-2.