Intro

Kerala School

Terminology

π value

Madhava’s series

Sine table

Analysis

Comparison

Conclusion

On Sangamagr¯ama M¯adhava’s (c.1350 - c.1425) Algorithms for the Computation of Sine and Cosine Functions V.N. Krishnachandran, Reji C. Joy, Siji K.B. Vidya Academy of Science and Technology, Thrissur - 680501, Kerala.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Outline 1 Introduction 2 Kerala School of Astronomy and Mathematics 3 Some terminology 4 Madhava’s value for π 5 Madhava’s series 6 Madhava’s sine table 7 Analysis of Madhava’s computational schemes 8 Comparison with modern algorithms 9 Conclusion 10 Bibliography V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

Comparison

Conclusion

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Introduction

Classical period in Indian mathematics: Aryabhata I (476 - 550 CE) : Author of Aryabhatiya. Varahamihira (505 - 587 CE) Brhamagupta (598 - 670 CE) Bhaskara I (c.600 - c.680 CE) Govindasvami (c.800 - c.860 CE) Aryabhata II (c.920 - c.1000 CE) Bhaskara II (1114 - 1185 CE) : Author of Lilavati.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

Conclusion

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Introduction

Development of mathematics in India did not end with Bhaskara II Mathematics continued to flourish in Kerala unknown to the rest of the world! C.M. Whish, an East India Company official, wrote about the Kerala School of Astronomy and Mathematics in 1832. But nobody noticed it.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Kerala School : Geographical area (Trikkandiyur)

Map showing Trikkandiyur and nearby places V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

Conclusion

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Intro

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Terminology

π value

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Sine table

Analysis

Comparison

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Kerala School : Period

Pre-Madhava period : Begins with Vararuci (4 th century CE) ending with Govinda Bhattathiri (1237 - 1295 CE) Madhava and his disciples (c.1350 - c.1650 CE) Later period (c.1650 - c.1850)

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Kerala School : Founder

Sangamagrama Madhava (c.1350 - c.1425 CE) No personal details about M¯adhava has come to light. Sangamagr¯ama is surmised to be a reference to his place of residence. Some historians have identified Sangamagr¯ama as modern day Irinjalakuda in Thrissur District in Kerala. There are references and tributes to M¯adhava in the works of other authors about whom accurate details are available.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Kerala School : Prominent members

Paramesvara (c.1380 - c.1460), a pupil of Sangamagrama M¯adhava : Promulgator of Drigganita system of astronomical computations in Kerala. Da.modara, another prominent member of the Kerala school, was Paramesvara’s son and also his pupil. N¯ilakant.ha S¯omay¯aji (1444 - 1544), a pupil of Parameshvara. Author of Tantrasamgraha completed in 1501.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Kerala School : Other prominent members

Jy¯es.t.had¯eva (c.1500 - c.1600) Author of Yukt.ibh¯as.a. Yukt.ibh¯as.a is composed in Malayalam. It contains clear statements of the power series expansions of the sine and cosine functions and also their proofs. This treatise proves that the idea of proof is not alien to Indian mathematics.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Some terminology: C¯apa, jy¯a, koti-jy¯a, utkrama-jy¯a

Diagram showing c¯apa, jy¯a , etc.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Some terminology: C¯apa, jy¯a, koti-jy¯a, utkrama-jy¯a

jy¯a of arc AB = BM = R sin

s R



koti-jy¯a of arc AB = OM = R cos

s R



utkrama-jy¯a (or ´sara of arc AB) = MA = R 1 − cos V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

s R



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Some terminology: Katapayadi scheme The Kat.apay¯adi scheme is a method for representing numbers using letters of the Sanskrit alphabet. Table: Mapping of digits to letters in katapay¯adi scheme

1

2

3

4

5

6

7

8

9

0

ka

kha

ga

gha

na ˙

ca

cha

ja

jha

n˜a

t.a pa

t.ha pha

d.a ba

d.ha bha

n.a ma

ta

tha

da

dha

na

-

-

-

-

-

ya

ra

la

va

´sa

s.a

sa

ha

-

-

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Some terminology: Katapayadi scheme

Consonants have numerals assigned as per Table in previous slide. All stand-alone vowels like a and i are assigned to 0. In case of a conjunct, consonants attached to a non-vowel will be valueless. Numbers are written in increasing place values from left to right. The number 386 which denotes 3 × 100 + 8 × 10 + 6 in modern notations would be written as 683 in pre-modern Indian traditions.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Madhava’s value for π

Madhava derived the following series for the computation of π: 1 1 1 π = 1 − + − + ··· 4 3 5 7 The series is known as the Gregory (1638 1675) series. But it was known in Kerala more than two centuries before Gregory. Using this series and several correction terms M¯adhava computed the following value for π: π = 3.1415926535922.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Madhava’s series for sine: In Madhava’s own words

Multiply the arc by the square of the arc, and take the result of repeating that (any number of times). Divide (each of the above numerators) by the squares of the successive even numbers increased by that number and multiplied by the square of the radius. Place the arc and the successive results so obtained one below the other, and subtract each from the one above. These together give the j¯iva, as collected together in the verse beginning with “vidv¯an” etc.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Madhava’s series for sine: Rendering in modern notations Madhava’s series for sine function: j¯iva

= s h − s·

s2 (22 + 2)r 2 h s2 − s· 2 (2 + 2)r 2 h s2 − s· 2 (2 + 2)r 2 iii − ···

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

s2 (42 + 4)r 2 s2 s2 · 2 · (4 + 4)r 2 (62 + 6)r 2 ·

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Madhava’s series for sine: As power series for sine

Let θ be the angle subtended by the arc s at the center of the circle. s = r θ and j¯iva = rsinθ. Substitute these in the expression given by Madhava. We get θ3 θ5 θ7 + − + ··· 3! 5! 7! This is the infinite power series expansion of the sine function. sin θ = θ −

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Madhava’s series for sine: Reformulation for computation

M¯adhava considers one quarter of a circle. The length of the quarter-circle is taken as 5400 minutes (say C minutes). He computes the radius R of the circle: R = 2 × 5400/π = 3437.74677078493925 = 34370

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

4400

48000

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Madhava’s series for sine: Reformulation for computation

The expression for j¯iva is now put in the following form: s5 s3 + − ··· R 2 (22 + 2) R 4 (22 + 2)(42 + 4)  s 3 h R π  3  s 2 h R π  5 ii 2 2 =s− − − ··· C 3! C 5!

jiva = s −

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Madhava’s series for sine: Pre-computaion of coefficients

No. 1

Expression R × (π/2)3 /3!

22200 3900 40000

Value

2

R × (π/2)5 /5!

2730 5700 47000

3

R × (π/2)7 /7!

160 0500 41000

4 5

R × (π/2)9 /9! R × (π/2)11 /11!

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

3300 06000 44000

In kat.apay¯adi system ni-rvi-ddh¯a-ngana-r¯e-ndra-rung sa-rv¯a-rtha´s¯i-la-sthi-ro ka-v¯i-´sani-ca-ya tu-nna-ba-la vi-dv¯an

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Madhava’s series for sine: Reformulation for computation

Madhava’s polynomial approximation to sine function: jiva = s − (s/C )3 [(22200 3900 40000 ) − (s/C )2 [(2730 5700 47000 − (s/C )2 [(160 0500 41000 ) − (s/C )2 [(3300 06000 ) − (s/C )2 (44000 )]]]]

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Madhava’s series for cosine Madhava’s polynomial approximation to cosine function: ´sara = (s/C )2 [(42410 0900 00000 ) − (s/C )2 [(8720 03000 05000 ) − (s/C )2 [(0710 4300 24000 ) − (s/C )2 [(030 09000 37000 ) − (s/C )2 [(0500 12000 ) − (s/C )2 (06000 )]]]]]

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

Conclusion

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Madhava’s sine table

(continued in next slide) V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Madhava’s sine table

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: These are algorithms!

Madhava and his followers were developing algorithms for the computation of sine and cosine functions. The expansions are given as a step by step procedure for computations the function values. In Jy¯es.t.had¯eva’s Yuktibh¯as.a, the author has used the term kriya-krama which translates into procedure or an algorithm.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Use of polynomial approximation

M¯adhava uses polynomial approximations. For sine function, an 11 th degree polynomial is used. For the cosine function, a 12 th degree polynomial is used. The orders of the polynomials were decided by the requirements of accuracy. The values computed by M¯adhava could also be obtained by other methods. But M¯adhava did seek and get a general method in the form of power series expansions.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Pre-computation of the coefficients

Madhava pre-computed the coefficients appearing in the polynomial approximations.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Use of Horner’s scheme

M¯adhava had applied what is now known as the Horner’s scheme for the computation of polynomials. The scheme is now attributed to William George Horner (1786 1837) who was a British mathematician and schoolmaster.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Horner’s scheme

Given the polynomial p(x) =

n X

ai x i = a0 + a1 x + a2 x 2 + a3 x 3 + · · · + an x n ,

i=0

let it be required to evaluate p(x) at a specific value of x.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Horner’s scheme To compute p(x), the polynomial is expressed in the form p(x) = a0 + x(a1 + x(a2 + · · · + x(an−1 + an x) · · · )). Then apply the following algorithm for computing p(x): bn = an bn−1 = an−1 + bn x ··· b1 = a1 + b2 x b0 = a0 + b1 x. b0 is the required value of the polynomial. V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Use of Horner’s scheme

M¯adhava had actually implemented Horner’s scheme in his algorithms. The method was known to Isaac Newton in 1669, the Chinese mathematician Qin Jiushao in the 13th century, and even earlier to the Persian Muslim mathematicians. M¯adhava’s was the first conscious and deliberate application of the scheme in a computational algorithm with the intention of reducing the complexity of numerical procedures.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Analysis: Simultaneous computation of sine and cosine In many modern implementations of routines for the calculations of the sine and cosine functions, there would be one routine for the simultaneous computation of sine and cosine. Whenever sine or cosine is required, the other would also be required. So a common algorithm which returns both values simultaneously would be more time efficient and economical. It would appear that M¯adhava had anticipated such a scenario. This is evidenced by the description of one common procedure for the evaluation of sine and cosine functions in Yuktibh¯as.a.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Comparison with programmes in Open64 Compiler

Compare, for example, with the programme included in the Open64 Compiler developed by Computer Architecture and Parallel Systems Laboratory in University of Delaware. These programs are not using the polynomials used by M¯adhava. They are using the minimax polynomial computed using the Remez algorithm to improve the accuracy of computations.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Comparison: Coefficients for computation of sine 00135 /* coefficients for polynomial approximation of sin on +/- pi/4 */ 00136 00137 static const du S[] = 00138 00139 D(0x3ff00000, 0x00000000), 00140 D(0xbfc55555, 0x55555548), 00141 D(0x3f811111, 0x1110f7d0), 00142 D(0xbf2a01a0, 0x19bfdf03), 00143 D(0x3ec71de3, 0x567d4896), 00144 D(0xbe5ae5e5, 0xa9291691), 00145 D(0x3de5d8fd, 0x1fcf0ec1), 00146 ; V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Comparison: Coefficients for computation of cosine 00148 /* coefficients for polynomial approximation of cos on +/- pi/4 */ 00149 00150 static const du C[] = 00151 00152 D(0x3ff00000, 0x00000000), 00153 D(0xbfdfffff, 0xffffff96), 00154 D(0x3fa55555, 0x5554f0ab), 00155 D(0xbf56c16c, 0x1640aaca), 00156 D(0x3efa019f, 0x81cb6a1d), 00157 D(0xbe927df4, 0x609cb202), 00158 D(0x3e21b8b9, 0x947ab5c8), 00159 ; V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Comparison: Polynomial approximations

00329 00330 00331 00332 00333 00334 00335 00336 00337

xsq = x*x; cospoly = (((((C[6].d*xsq + C[5].d)*xsq + C[4].d)*xsq + C[3].d)*xsq + C[2].d)*xsq + C[1].d)*xsq + C[0].d; sinpoly = (((((S[6].d*xsq + S[5].d)*xsq + S[4].d)*xsq + S[3].d)*xsq + S[2].d)*xsq + S[1].d)*(xsq*x) + x;

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

Conclusion

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Conclusion

Madhava was a great computationalist. Madhava pioneered several new ideas and techniques for the efficient computaion of functions. In particular, Madhava implemented the following concepts to devise a scheme for the computation of sine and cosine functions: Use of an approximating polynomial. Pre-computation of coefficients. Use of Horner’s scheme for the evaluation of polynomials. Simultaneous computation of sine and cosine functions.

V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Bibliography 1 G. G. Joseph, A Passage to Infinity: Medieval Indian Mathematics from Kerala and Its Impact. New Delhi: Sage Publications Pvt. Ltd, 2009. 2 C. M. Whish, On the hindu quadrature of the circle and the infinite series of the proportion of the circumference to the diameter exhibited in the four sastras, the tantra sahgraham, yucti bhasha, carana padhati and sadratnamala, Transactions of the Royal Asiatic Society of Great Britain and Ireland (Royal Asiatic Society of Great Britain and Ireland, vol. 3 (3), pp. 509 523, 1834. 3 I. S. B. Murthy, A modern introduction to ancient Indian mathematics. New Delhi: New Age International Publishers, 1992. V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Bibliography 4 V. J. Katz, The mathematics of Egypt, Mesopotemia, China, India and Islam: A source book. Princeton: Princeton University Press, 2007, ch. Chapter 4 : Mathematics in India IV. Kerala School (pp. 480 - 495). 5 K. Plofker, Mathematics in India. Princeton, NJ: Princeton University Press, 2010. 6 Madhava of sangamagramma. [Online]. Available: http://wwwgap. dcs.st-and.ac.uk/ history/Projects/Pearce/Chapters/Ch9 3.html 7 K. V. Sarma and V. S. Narasimhan, Tantrasamgraha, Indian Journal of History of Science, vol. 33 (1), Mar. 1998.

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Bibliography 8 K. V. Sarma and S. Hariharan, Yuktibhasa of jyesthadeva : a book of rationales in indian mathematics and astronomy - an analytical appraisal, Indian Journal of History of Science, vol. 26 (2), pp. 185 207, 1991. 9 A. V. Raman, The katapayadi formula and the modern hashing technique, Annals of the History of Computing, vol. 19 (4), pp. 4952, 1997. 10 R. Roy, Article The discovery of the series formula for π by Leibniz, Gregory, and Nilakantha in Sherlock Holmes in Babylon and other tales of mathematical history, R. W. Marlow Anderson, Victor Katz, Ed. The Mathematical Association of America, 2004. V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Bibliography 11 C. K. Raju, Cultural foundations of mathematics : The nature of mathematical proof and the transmission of the calculus from India to Europe in the 16th c. CE. Delhi: Centre for Studies in Civilizations, 2007. 12 F. Cajori, A history of mathematics, 5th ed. Chelsea Publishing Series, 1999. 13 Jyeshthadeva, Ganita-yukti-bhasha, K. V. Sarma, Ed. New Delhi: Hindustan Book Agency, 2008. 14 osprey/libm/mips/sincos.c. [Online]. Available: http:// www.open64.net/ doc/d6/d08/ sincos 8c-source.html 15 k sin.c. [Online]. Available: http://www.netlib.org/fdlibm/k sin.c 16 k cos.c. [Online]. Available: http://www.netlib.org/fdlibm/k cos.c V N Krishnachandran, Reji C Joy, Siji K B On Sangamagr¯ ama M¯ adhava’s (c.1350 - c.1425) Algorithms

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Thanks

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Conclusion

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On Sangamagrama Madhava's (c.1350 - c.1425 ...

Kerala School of Astronomy and Mathematics in 1832. But ..... University Press, 2010. 6 Madhava of sangamagramma. [Online]. Available: http://wwwgap. ... analytical appraisal, Indian Journal of History of Science, vol. 26 (2), pp. 185 207 ...

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