1. Madhava of Sangamagrama formulated a rule equivalent to the Gregory series for calculating the inverse tangent function.
2. The rule expresses the inverse tangent as a sum of terms involving sines and cosines, equivalent to the Gregory series.
3. Ancient Indian mathematicians provided proofs of the rule, equivalent to modern proofs through term-by-term integration, showing they understood the concept of infinite series well before Western mathematicians formulated them explicitly.
This document discusses ancient Indian values of Pi that were used in mathematics. It provides 5 ancient approximations of Pi that were used in India and other parts of the world:
1. The simplest approximation of Pi = 3, which was used by the ancient Babylonians, in the Bible, and in ancient Chinese works. Similar approximations are found in ancient Indian texts.
2. The "Jaina value" of Pi = 22/7, which was frequently used in Jain texts and first appeared in India around the 1st century AD.
3. The Archimedean value of Pi = 22/7, which was recognized as a satisfactory approximation after Archimedes showed Pi is between 3 1/
1. Aryabhata, an Indian astronomer and mathematician from the 5th century AD, approximated pi (π) to 3.1416 in his famous work the Aryabhatiya. This approximation correct to four decimal places was one of the most accurate approximations of pi used anywhere in the ancient world.
2. Aryabhata expressed pi as a fraction 62832/20000, which can be expressed in continued fractions as 3 + (4/16). This value of pi was later used and referenced by many Indian and foreign mathematicians and astronomers over subsequent centuries.
3. Scholars debate whether Aryabhata's value of pi was influenced by the Greeks
Bhaskara I, an Indian mathematician from around 600 AD, developed an elegant algebraic formula for approximating trigonometric sine values. This formula, described in his text Mahabhaskariya, expresses sine as a function of the angular arc in degrees. Several subsequent Indian texts, including works by Brahmagupta, Varahamihira, and Bhaskara II, reference or derive equivalent forms of Bhaskara I's approximation formula. The document discusses the accuracy of the formula and compares it to actual sine values, providing historical context on the development and transmission of trigonometric concepts in early Indian and Western mathematics.
1) The ancient Indian mathematician Bhaskara II first described the addition and subtraction theorems for sines in his work Jyotpatti from 1150 AD. These theorems state that the sine of the sum of two arcs is equal to the sum of the sines of individual arcs multiplied by their cosines, and the sine of the difference of two arcs is equal to the difference of the sines.
2) Bhaskara II provided two formulas based on these theorems to tabulate sines at intervals of 225 minutes and 60 minutes. These formulas allow constructing tables of 24 sines and 90 sines respectively using recurrence relations.
3) The article discusses Bhaskara II's contribution to trigon
Bhaskara II, an Indian mathematician from the 12th century, derived the formula for the surface area of a sphere. He used a crude form of integration by dividing the surface into thin circular sections and approximating their areas. This led to the formula of circumference x diameter. Earlier, Aryabhata II had provided the same formula, though Bhaskara criticized another mathematician, Lalla, for providing an incorrect formula. Bhaskara's derivation showed originality compared to Archimedes' method, though it lacked the same level of ingenuity.
This document summarizes a rule from the ancient Indian mathematics text Lilavati for computing the sides of regular polygons inscribed in a circle. The rule provides coefficients that when multiplied by the circle's diameter and divided by 12,000 yield the side lengths of triangles, squares, pentagons, etc. up to nonagons. While the rationales for some coefficients are clear, others are less accurate, possibly due to limitations in available sine tables or knowledge of exact solutions. The document discusses methods that may have been used to derive the coefficients and compares the original values to more accurate modern calculations.
1) Ancient Indian mathematicians developed rational approximations to trigonometric functions like sine, cosine, and versine that were found in Sanskrit works from the 7th to 17th centuries AD.
2) These approximations took the form of algebraic formulas relating the functions to angles in degrees. For example, one approximation for sine was sin(A) ≈ 16A(180-A)/(32400-A^2).
3) These formulas, which were popular in India, can be found in many original Indian mathematical works and show that such approximations were well-established by the 7th century.
The document discusses addition and subtraction theorems for the sine and cosine functions in medieval Indian mathematics. It provides statements of the theorems as found in several important Indian works from the 12th to 17th centuries. These theorems are equivalent to the modern mathematical formulas for trigonometric addition and subtraction. The document also outlines various proofs and derivations of the theorems found in Indian works, which indicate how Indians understood the rationales behind the theorems.
This document discusses ancient Indian values of Pi that were used in mathematics. It provides 5 ancient approximations of Pi that were used in India and other parts of the world:
1. The simplest approximation of Pi = 3, which was used by the ancient Babylonians, in the Bible, and in ancient Chinese works. Similar approximations are found in ancient Indian texts.
2. The "Jaina value" of Pi = 22/7, which was frequently used in Jain texts and first appeared in India around the 1st century AD.
3. The Archimedean value of Pi = 22/7, which was recognized as a satisfactory approximation after Archimedes showed Pi is between 3 1/
1. Aryabhata, an Indian astronomer and mathematician from the 5th century AD, approximated pi (π) to 3.1416 in his famous work the Aryabhatiya. This approximation correct to four decimal places was one of the most accurate approximations of pi used anywhere in the ancient world.
2. Aryabhata expressed pi as a fraction 62832/20000, which can be expressed in continued fractions as 3 + (4/16). This value of pi was later used and referenced by many Indian and foreign mathematicians and astronomers over subsequent centuries.
3. Scholars debate whether Aryabhata's value of pi was influenced by the Greeks
Bhaskara I, an Indian mathematician from around 600 AD, developed an elegant algebraic formula for approximating trigonometric sine values. This formula, described in his text Mahabhaskariya, expresses sine as a function of the angular arc in degrees. Several subsequent Indian texts, including works by Brahmagupta, Varahamihira, and Bhaskara II, reference or derive equivalent forms of Bhaskara I's approximation formula. The document discusses the accuracy of the formula and compares it to actual sine values, providing historical context on the development and transmission of trigonometric concepts in early Indian and Western mathematics.
1) The ancient Indian mathematician Bhaskara II first described the addition and subtraction theorems for sines in his work Jyotpatti from 1150 AD. These theorems state that the sine of the sum of two arcs is equal to the sum of the sines of individual arcs multiplied by their cosines, and the sine of the difference of two arcs is equal to the difference of the sines.
2) Bhaskara II provided two formulas based on these theorems to tabulate sines at intervals of 225 minutes and 60 minutes. These formulas allow constructing tables of 24 sines and 90 sines respectively using recurrence relations.
3) The article discusses Bhaskara II's contribution to trigon
Bhaskara II, an Indian mathematician from the 12th century, derived the formula for the surface area of a sphere. He used a crude form of integration by dividing the surface into thin circular sections and approximating their areas. This led to the formula of circumference x diameter. Earlier, Aryabhata II had provided the same formula, though Bhaskara criticized another mathematician, Lalla, for providing an incorrect formula. Bhaskara's derivation showed originality compared to Archimedes' method, though it lacked the same level of ingenuity.
This document summarizes a rule from the ancient Indian mathematics text Lilavati for computing the sides of regular polygons inscribed in a circle. The rule provides coefficients that when multiplied by the circle's diameter and divided by 12,000 yield the side lengths of triangles, squares, pentagons, etc. up to nonagons. While the rationales for some coefficients are clear, others are less accurate, possibly due to limitations in available sine tables or knowledge of exact solutions. The document discusses methods that may have been used to derive the coefficients and compares the original values to more accurate modern calculations.
1) Ancient Indian mathematicians developed rational approximations to trigonometric functions like sine, cosine, and versine that were found in Sanskrit works from the 7th to 17th centuries AD.
2) These approximations took the form of algebraic formulas relating the functions to angles in degrees. For example, one approximation for sine was sin(A) ≈ 16A(180-A)/(32400-A^2).
3) These formulas, which were popular in India, can be found in many original Indian mathematical works and show that such approximations were well-established by the 7th century.
The document discusses addition and subtraction theorems for the sine and cosine functions in medieval Indian mathematics. It provides statements of the theorems as found in several important Indian works from the 12th to 17th centuries. These theorems are equivalent to the modern mathematical formulas for trigonometric addition and subtraction. The document also outlines various proofs and derivations of the theorems found in Indian works, which indicate how Indians understood the rationales behind the theorems.
1) Brahmagupta, an ancient Indian mathematician from the 7th century AD, developed formulas for calculating the area and diagonals of a cyclic quadrilateral using only the lengths of its four sides.
2) His formula for accurate area involved taking the square root of the product of terms involving the differences between half sums of opposite sides.
3) His expressions for the diagonals involved dividing and multiplying terms involving products of the sides, and took the square root of the results. These formulas are considered some of the most remarkable in Hindu geometry.
1. The property that the second order differences of sines are proportional to the sines themselves was known in early Indian mathematics, dating back to Aryabhata I in the 5th century AD.
2. The paper describes various formulations of this proportionality found in important Indian astronomical works from the 5th to 15th centuries. It also outlines Nilakantha Somayaji's ingenious geometric proof of the property from his commentary on Aryabhatiya in the early 16th century.
3. The Indian mathematical method of computing sine tables using this difference property, which involves an implied differential process, was considered novel by Western scholars despite being used in India since ancient times
The document summarizes rules for calculating the perimeter and area of an ellipse from an ancient Indian mathematics text from the 9th century AD. It provides the ancient text's approximate formulas for perimeter and area, and explains how they were likely empirically derived by comparing an ellipse to simpler shapes like a semicircle or circular segment. It also gives the correct elliptic integral formulas, and shows how the ancient approximations compare to the precise solutions for a numerical example.
This document discusses fractional parts of Aryabhata's sine differences that are found in Govindasvami's commentary on Mahabhashya. Specifically:
1. Govindasvami's commentary provides the sexagesimal fractional parts (seconds and thirds) of Aryabhata's 24 tabular sine differences, allowing for a more accurate sine table with values given to the second order of sexagesimal fractions.
2. These fractional parts found in Govindasvami's commentary are subtracted from or added to Aryabhata's sine differences to improve the accuracy of the table.
3. In addition to improving Aryabhata's sine table, the
Brahmagupta was an ancient Indian mathematician from the 7th century AD who made important contributions to mathematics. This document discusses one of Brahmagupta's formulas for calculating the volume of frustum-like solids (solids with parallel ends of different shapes and sizes). The formula provides a method to calculate both the practical volume and gross volume, and uses the difference between the two to find the accurate volume. The formula is shown to apply to specific cases like truncated wedges and cones. The formula demonstrates Brahmagupta's sophisticated mathematical abilities and had influence in both India and other parts of the ancient world.
1) The ancient Indian text Baudhayana's Sulba Sutra from around 800-400 BC contains a rule for approximating the square root of two. The rule increases the side of a square by one-third and one-fourth parts to get an approximation of 1.41421.
2) This approximation method of linear interpolation was popular in ancient India. The rule can be explained through a two-term interpolation formula.
3) Repeated use of this interpolation process yields the four-term approximation found in the Sulba Sutra, equivalent to methods used by later mathematicians like Neugebauer. While an improvement, the Indian approximation was still less accurate than the sexagesimal
The document discusses the benefits of exercise for mental health. Regular physical activity can help reduce anxiety and depression and improve mood and cognitive functioning. Exercise causes chemical changes in the brain that may help boost feelings of calmness, happiness and focus.
1. According to Jaina cosmography, the Jambu Island is circular with a diameter of 100,000 yojanas.
2. Ancient Jaina texts provided approximations for the circumference of the Jambu Island using simple formulas like C=3D. More accurate values were also calculated using the formula C=√(10D2) which is better than C=3D.
3. The article examines various circumference values found in ancient Jaina texts like the Tiloya-Pannatti and expresses them using the detailed unit system from the text to compare to the precise modern calculation of the circumference.
Narayana Pandita, an important ancient Indian mathematician who lived in the 14th century, developed a method for approximating quadratic surds (square roots of non-perfect squares). His method involved finding integer solutions to the indeterminate equation x2 - Ny2 = 1 and taking the ratio of the solutions as the approximation. The article describes Narayana's method using the example of approximating √10 and relates his method to other ancient approaches like the binomial approximation and Newton's method. It highlights the significance of Narayana's works in the development of ancient Indian mathematics.
1) Neelakantha Somaydji was an important mathematician from medieval India who lived from 1443-1543 AD and wrote several astronomical works.
2) In one of his works called Golasara, Neelakantha provides a formula for computing the length of a small circular arc given the Indian Sine and Versed Sine.
3) The formula, which is equivalent to the modern formula, enables the approximate computation of an angle when its sine or cosine is given.
The document presents a new interpretation of a rule in the Ganita-siira-sa4graha (GSS), an ancient Indian mathematics text, for calculating the surface area of a spherical segment.
Previous interpretations by Rangacharya and Jain assumed the rule treated the spherical segment as a flat circular base. The document suggests an alternate interpretation where the Sanskrit term "viskambha" refers to the curvilinear breadth of the segment, not its diameter. This new interpretation matches the true mathematical formula and has less error than the previous views.
1) The document discusses an ancient Indian mathematics problem involving using gnomons (vertical rods) to measure the height of a lamp post and the distance between shadow tips.
2) It presents the original rule from the Aryabhatiya, and provides examples and explanations of how to use the rule to calculate heights and distances.
3) The rule involves using ratios between shadow lengths, distance between shadow tips, and gnomon length to determine the "upright" distance and lamp post height.
This document contains questions from a Material Science and Metallurgy exam. It covers various topics:
- Crystal structures of BCC, FCC and HCP lattices and their properties. Diffusion of iron atoms in BCC lattice.
- Mechanical properties in the plastic region from stress-strain diagrams. True and conventional strain expressions. Twinning mechanism of plastic deformation.
- Fracture mechanisms based on Griffith's theory of brittle fracture. Factors affecting creep. Fatigue testing and S-N curves for materials.
- Solidification process and expression for critical nucleus radius. Cast metal structures. Solid solutions and Hume-Rothery rules. Phase diagrams and Gibbs phase rule.
Five Dimensional Bianchi Type-V Space-Time in f (R,T) Theory of GravitywIJERA Editor
We study the spatially homogeneous anisotropic Bianchi type-V universe in f(R,T) theory of gravity, where R is
the Ricci scalar and T is the trace of the energy-momentum tensor. We assume the variation law of mean
Hubble parameter and constant deceleration parameter to find two different five dimensional exact solutions of
the modified field equations. The first solution yields a singular model for n 0 while the second gives a nonsingular
model for n 0. The physical quantities are discussed for both models in future evolution of the
universe.
Five Dimensional Bianchi Type-V Space-Time in f (R,T) Theory of GravitywIJERA Editor
We study the spatially homogeneous anisotropic Bianchi type-V universe in f(R,T) theory of gravity, where R is
the Ricci scalar and T is the trace of the energy-momentum tensor. We assume the variation law of mean
Hubble parameter and constant deceleration parameter to find two different five dimensional exact solutions of
the modified field equations. The first solution yields a singular model for
n 0
while the second gives a nonsingular
model for
n 0.
The physical quantities are discussed for both models in future evolution of the
universe
Aryabhata was a famous mathematician and astronomer from the classical age of Indian mathematics and astronomy. Some of his major works, which are still extant, include the Aryabhatiya, a compendium of mathematics and astronomy. In it, he worked on approximations for pi and found it to be approximately equal to 3.1416. He also believed that the earth rotates and revolves around the sun. Aryabhata made several important contributions in the fields of mathematics and astronomy.
This document describes an automatic essay paraphrasing system that can take an input essay of up to 300 words and generate a new output essay that summarizes the content in a non-redundant manner using different sentences. The system performs dependency and phrase structure parsing of the input text and uses the analysis to generate grammatically correct paraphrases while maintaining coherence. It includes components for parsing, establishing dependencies across sentences, generating sentence paraphrases, and controlling the logical sequence of the output. The current version requires word class assignments and grammatical information to be provided in the input text.
Stability criterion of periodic oscillations in a (13)Alexander Decker
This document discusses domination problems on isosceles triangular chessboards using different chess pieces. It examines placing a minimum number of pieces such that all unoccupied positions are attacked (the domination number). For a single piece type, it determines the domination number and possible solutions for rooks, bishops, and kings on isosceles triangular boards. It also considers domination numbers when using two piece types together, such as kings and rooks or kings and bishops. Key results include formulas for the domination number and total solutions in terms of the board size for each piece type.
1) Brahmagupta, an ancient Indian mathematician from the 7th century AD, developed formulas for calculating the area and diagonals of a cyclic quadrilateral using only the lengths of its four sides.
2) His formula for accurate area involved taking the square root of the product of terms involving the differences between half sums of opposite sides.
3) His expressions for the diagonals involved dividing and multiplying terms involving products of the sides, and took the square root of the results. These formulas are considered some of the most remarkable in Hindu geometry.
1. The property that the second order differences of sines are proportional to the sines themselves was known in early Indian mathematics, dating back to Aryabhata I in the 5th century AD.
2. The paper describes various formulations of this proportionality found in important Indian astronomical works from the 5th to 15th centuries. It also outlines Nilakantha Somayaji's ingenious geometric proof of the property from his commentary on Aryabhatiya in the early 16th century.
3. The Indian mathematical method of computing sine tables using this difference property, which involves an implied differential process, was considered novel by Western scholars despite being used in India since ancient times
The document summarizes rules for calculating the perimeter and area of an ellipse from an ancient Indian mathematics text from the 9th century AD. It provides the ancient text's approximate formulas for perimeter and area, and explains how they were likely empirically derived by comparing an ellipse to simpler shapes like a semicircle or circular segment. It also gives the correct elliptic integral formulas, and shows how the ancient approximations compare to the precise solutions for a numerical example.
This document discusses fractional parts of Aryabhata's sine differences that are found in Govindasvami's commentary on Mahabhashya. Specifically:
1. Govindasvami's commentary provides the sexagesimal fractional parts (seconds and thirds) of Aryabhata's 24 tabular sine differences, allowing for a more accurate sine table with values given to the second order of sexagesimal fractions.
2. These fractional parts found in Govindasvami's commentary are subtracted from or added to Aryabhata's sine differences to improve the accuracy of the table.
3. In addition to improving Aryabhata's sine table, the
Brahmagupta was an ancient Indian mathematician from the 7th century AD who made important contributions to mathematics. This document discusses one of Brahmagupta's formulas for calculating the volume of frustum-like solids (solids with parallel ends of different shapes and sizes). The formula provides a method to calculate both the practical volume and gross volume, and uses the difference between the two to find the accurate volume. The formula is shown to apply to specific cases like truncated wedges and cones. The formula demonstrates Brahmagupta's sophisticated mathematical abilities and had influence in both India and other parts of the ancient world.
1) The ancient Indian text Baudhayana's Sulba Sutra from around 800-400 BC contains a rule for approximating the square root of two. The rule increases the side of a square by one-third and one-fourth parts to get an approximation of 1.41421.
2) This approximation method of linear interpolation was popular in ancient India. The rule can be explained through a two-term interpolation formula.
3) Repeated use of this interpolation process yields the four-term approximation found in the Sulba Sutra, equivalent to methods used by later mathematicians like Neugebauer. While an improvement, the Indian approximation was still less accurate than the sexagesimal
The document discusses the benefits of exercise for mental health. Regular physical activity can help reduce anxiety and depression and improve mood and cognitive functioning. Exercise causes chemical changes in the brain that may help boost feelings of calmness, happiness and focus.
1. According to Jaina cosmography, the Jambu Island is circular with a diameter of 100,000 yojanas.
2. Ancient Jaina texts provided approximations for the circumference of the Jambu Island using simple formulas like C=3D. More accurate values were also calculated using the formula C=√(10D2) which is better than C=3D.
3. The article examines various circumference values found in ancient Jaina texts like the Tiloya-Pannatti and expresses them using the detailed unit system from the text to compare to the precise modern calculation of the circumference.
Narayana Pandita, an important ancient Indian mathematician who lived in the 14th century, developed a method for approximating quadratic surds (square roots of non-perfect squares). His method involved finding integer solutions to the indeterminate equation x2 - Ny2 = 1 and taking the ratio of the solutions as the approximation. The article describes Narayana's method using the example of approximating √10 and relates his method to other ancient approaches like the binomial approximation and Newton's method. It highlights the significance of Narayana's works in the development of ancient Indian mathematics.
1) Neelakantha Somaydji was an important mathematician from medieval India who lived from 1443-1543 AD and wrote several astronomical works.
2) In one of his works called Golasara, Neelakantha provides a formula for computing the length of a small circular arc given the Indian Sine and Versed Sine.
3) The formula, which is equivalent to the modern formula, enables the approximate computation of an angle when its sine or cosine is given.
The document presents a new interpretation of a rule in the Ganita-siira-sa4graha (GSS), an ancient Indian mathematics text, for calculating the surface area of a spherical segment.
Previous interpretations by Rangacharya and Jain assumed the rule treated the spherical segment as a flat circular base. The document suggests an alternate interpretation where the Sanskrit term "viskambha" refers to the curvilinear breadth of the segment, not its diameter. This new interpretation matches the true mathematical formula and has less error than the previous views.
1) The document discusses an ancient Indian mathematics problem involving using gnomons (vertical rods) to measure the height of a lamp post and the distance between shadow tips.
2) It presents the original rule from the Aryabhatiya, and provides examples and explanations of how to use the rule to calculate heights and distances.
3) The rule involves using ratios between shadow lengths, distance between shadow tips, and gnomon length to determine the "upright" distance and lamp post height.
This document contains questions from a Material Science and Metallurgy exam. It covers various topics:
- Crystal structures of BCC, FCC and HCP lattices and their properties. Diffusion of iron atoms in BCC lattice.
- Mechanical properties in the plastic region from stress-strain diagrams. True and conventional strain expressions. Twinning mechanism of plastic deformation.
- Fracture mechanisms based on Griffith's theory of brittle fracture. Factors affecting creep. Fatigue testing and S-N curves for materials.
- Solidification process and expression for critical nucleus radius. Cast metal structures. Solid solutions and Hume-Rothery rules. Phase diagrams and Gibbs phase rule.
Five Dimensional Bianchi Type-V Space-Time in f (R,T) Theory of GravitywIJERA Editor
We study the spatially homogeneous anisotropic Bianchi type-V universe in f(R,T) theory of gravity, where R is
the Ricci scalar and T is the trace of the energy-momentum tensor. We assume the variation law of mean
Hubble parameter and constant deceleration parameter to find two different five dimensional exact solutions of
the modified field equations. The first solution yields a singular model for n 0 while the second gives a nonsingular
model for n 0. The physical quantities are discussed for both models in future evolution of the
universe.
Five Dimensional Bianchi Type-V Space-Time in f (R,T) Theory of GravitywIJERA Editor
We study the spatially homogeneous anisotropic Bianchi type-V universe in f(R,T) theory of gravity, where R is
the Ricci scalar and T is the trace of the energy-momentum tensor. We assume the variation law of mean
Hubble parameter and constant deceleration parameter to find two different five dimensional exact solutions of
the modified field equations. The first solution yields a singular model for
n 0
while the second gives a nonsingular
model for
n 0.
The physical quantities are discussed for both models in future evolution of the
universe
Aryabhata was a famous mathematician and astronomer from the classical age of Indian mathematics and astronomy. Some of his major works, which are still extant, include the Aryabhatiya, a compendium of mathematics and astronomy. In it, he worked on approximations for pi and found it to be approximately equal to 3.1416. He also believed that the earth rotates and revolves around the sun. Aryabhata made several important contributions in the fields of mathematics and astronomy.
This document describes an automatic essay paraphrasing system that can take an input essay of up to 300 words and generate a new output essay that summarizes the content in a non-redundant manner using different sentences. The system performs dependency and phrase structure parsing of the input text and uses the analysis to generate grammatically correct paraphrases while maintaining coherence. It includes components for parsing, establishing dependencies across sentences, generating sentence paraphrases, and controlling the logical sequence of the output. The current version requires word class assignments and grammatical information to be provided in the input text.
Stability criterion of periodic oscillations in a (13)Alexander Decker
This document discusses domination problems on isosceles triangular chessboards using different chess pieces. It examines placing a minimum number of pieces such that all unoccupied positions are attacked (the domination number). For a single piece type, it determines the domination number and possible solutions for rooks, bishops, and kings on isosceles triangular boards. It also considers domination numbers when using two piece types together, such as kings and rooks or kings and bishops. Key results include formulas for the domination number and total solutions in terms of the board size for each piece type.
The International Journal of Engineering & Science is aimed at providing a platform for researchers, engineers, scientists, or educators to publish their original research results, to exchange new ideas, to disseminate information in innovative designs, engineering experiences and technological skills. It is also the Journal's objective to promote engineering and technology education. All papers submitted to the Journal will be blind peer-reviewed. Only original articles will be published.
The papers for publication in The International Journal of Engineering& Science are selected through rigorous peer reviews to ensure originality, timeliness, relevance, and readability.
This document appears to contain questions from an engineering mathematics exam. It includes questions on several topics:
1. Differential equations, evaluating integrals using Cauchy's integral formula, Bessel functions, and Legendre polynomials.
2. Vector calculus topics like divergence and curl of vector fields, and finding equations of planes and lines.
3. Probability and statistics problems involving binomial, normal and Poisson distributions.
4. Graph theory questions about planar graphs, chromatic polynomials, and finding minimum spanning trees.
5. Combinatorics problems involving counting arrangements and distributions with restrictions.
The document provides instructions for a 3-hour physics exam for Class 11 students. It contains 30 questions ranging from 1 to 5 marks each. The questions cover a range of physics topics including fundamental forces, motion, mechanics, heat, waves, and electricity. Students are informed that calculators are not permitted and various physical constants may be used. They are advised that all questions are compulsory and instructed on the internal choices provided in some questions.
This document appears to contain exam questions for the subject "Electronic Circuits". It includes questions related to BJT operating point, UJT construction and operation, MOSFET and CMOS characteristics, photoconductors and optocouplers. Some sample calculations are provided related to photodiode parameters like NEP, detectivity, quantum efficiency. The document tests knowledge of fundamental electronic devices and circuits.
The document discusses Bhaskara II's treatise on Jyotpatti, the science of trigonometry in ancient India. It begins by providing context for the treatise as the last section of Bhaskara's comprehensive work Siddhanta Siromani. It then describes the graphical method used in ancient India to define and obtain values of trigonometric functions like jya (sine). Subsequently, it presents Bhaskara's mathematical method for calculating jya and other functions through formulas involving the radius of the reference circle. Key contributions of the treatise included the first accurate values for sines of particular angles derived through inscribing regular polygons in a circle.
International Journal of Mathematics and Statistics Invention (IJMSI) is an international journal intended for professionals and researchers in all fields of computer science and electronics. IJMSI publishes research articles and reviews within the whole field Mathematics and Statistics, new teaching methods, assessment, validation and the impact of new technologies and it will continue to provide information on the latest trends and developments in this ever-expanding subject. The publications of papers are selected through double peer reviewed to ensure originality, relevance, and readability. The articles published in our journal can be accessed online.
International Journal of Mathematics and Statistics Invention (IJMSI) is an international journal intended for professionals and researchers in all fields of computer science and electronics. IJMSI publishes research articles and reviews within the whole field Mathematics and Statistics, new teaching methods, assessment, validation and the impact of new technologies and it will continue to provide information on the latest trends and developments in this ever-expanding subject. The publications of papers are selected through double peer reviewed to ensure originality, relevance, and readability. The articles published in our journal can be accessed online.
International Journal of Mathematics and Statistics Invention (IJMSI)inventionjournals
This document defines and studies various weak forms of nano-open sets, including nano α-open sets, nano semi-open sets, and nano pre-open sets. It introduces these concepts in a nano topological space based on lower and upper approximations. Some key results shown are: 1) every nano-open set is nano α-open, 2) the family of nano α-open sets is contained within the families of nano semi-open and nano pre-open sets, and 3) the nano α-open sets equal the intersection of nano semi-open and nano pre-open sets. Examples are provided to illustrate these concepts.
A multithreaded web server uses a cache to avoid disk reads for frequently accessed pages. When a request is received, a worker thread first checks the cache and will only perform a disk read if the page is not found in the cache. The document asks whether kernel-level threads should be used instead of user-level threads for the worker threads.
A real-time system has 3 periodic tasks. The document asks whether each of rate monotonic scheduling and earliest deadline first scheduling can produce a feasible schedule for the tasks, showing the schedules with Gantt charts.
The document also discusses using semaphores to solve the producer-consumer problem, evaluating their use and explaining the purpose of wait and signal operations on se
A multithreaded web server uses a cache to avoid disk reads for frequently accessed pages. When a request is received, a worker thread first checks the cache and will perform a disk read only if the page is not found in the cache. Kernel-level threads should be used instead of user-level threads to allow preemption for better response times under heavy loads.
The document summarizes a two-day international seminar on the history of mathematics held in New Delhi in 2012. Over 150 mathematicians from 16 countries participated in the event, which celebrated the 125th birth anniversary of Srinivasa Ramanujan and covered various aspects of mathematics history, especially ancient Indian history. There were 11 sessions over the two days featuring talks and papers from scholars. The seminar concluded with positive feedback and was considered a great success in arranging such a large international event.
The document discusses the benefits of exercise for mental health. Regular physical activity can help reduce anxiety and depression and improve mood and cognitive function. Exercise causes chemical changes in the brain that may help protect against mental illness and improve symptoms.
In the rapidly evolving landscape of technologies, XML continues to play a vital role in structuring, storing, and transporting data across diverse systems. The recent advancements in artificial intelligence (AI) present new methodologies for enhancing XML development workflows, introducing efficiency, automation, and intelligent capabilities. This presentation will outline the scope and perspective of utilizing AI in XML development. The potential benefits and the possible pitfalls will be highlighted, providing a balanced view of the subject.
We will explore the capabilities of AI in understanding XML markup languages and autonomously creating structured XML content. Additionally, we will examine the capacity of AI to enrich plain text with appropriate XML markup. Practical examples and methodological guidelines will be provided to elucidate how AI can be effectively prompted to interpret and generate accurate XML markup.
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Gupta1973e
1. The Mathematics Education SECTION B
Vol. V I I . N o . 3 , S e p t . 1 97 3
G L I M PS E S OF A N C IE N T INDIAN M ATH. NO. 7
The nnadfrava-Gre€ory Series
D7Radha Charan Gupta, Dept. of MatltematicsBirla Institute of Technolog7
P,O. Mcsra,
RANCHI ( India )
( Re ce ive d l0 Ju ly 1973 )
l. Introduction:
fn current mathematical literature the series
a rc ta n x :x -x s l a -| x ,l u -... (l )
is called the Gregory's seriesfor the inverse tangent function after the Scottish mathemat-
cianJames Gregory ( 1638-75)1 who knew it about the year 1670. In India, an equiva:
lent of the series(l) is found enunciated in a rule which is attributed to the famous
Madhava of Saigamagrdma ( circa 1340-1425)s who is also called as Golvid ( .Master of
Spherics') by later astronomers.
Madhava's rules is found the Keralite commentary Krir,trkramakari
quoted in
(fn+rnt+tt ) 1:fffl on Bldskara JI's Lilavati (dtoref,t), the most poptrlar work of
ancient Indian mathematicr. The authorship of KKK has been a matter of con.jecture.
lfowever, according to K. V. Sarma, 'there arerclear evidences..to show that the KKK is
a work of Ndr-;'aLra Vdriar ( circa.l500-6-0) as conje-
( circa 1500-75)a andinot 6f Sar.r[a1a
ctured by some scholarss. wron S-, @ t {-..- f+it ,,8 u-vL
The Sanskrit verses( comprising the rule ) which are attributed to Midhava in the
KKK are also found mentioned in the YuktiBh:isa (:YB)0, a popular Malal'alam work
whose authorhas been identified to be one called stsatsJyesthadeva (circa 1500-1601)?.
Another Sanskrit stanza which contains the velbal enunciation of an equivalent of
th e se r ies( l) is f ound i n th e Ka ra rl a -Pa d d h a ti(:K P, C hap. V I, V erse l B )8 of P utumana
Somayaji ( about 1660-1740)e.
Ilel<;rvwe give the Sanskrit text of the M:ldhava's rule, its transliteration, a transla-
tion, its explar.ration modern form, arrd indicate an ancient Indian proof of it.
in
2. Enunciation of the Series :
The Sanskrit text of the rule attributed to M.idlsva i51o
qsesqrfssqqleiarq diaqrcacqq ssq I
gsrifi' E'ffi siflas{ s AIIF{ ll
crrTEri
2. 6B TE! TIII| TTITtCE !I'I'C I| IIO | I
rscTf(so*-qlsq tqr r.'Fdfilt6: I
gs'sqrqtq ierrflqiis'Ats{3l rnE II
qlqrqi dgt<a*<r grcdq qgfts t
<):rlaqheqttq +erdtlfrq €get I
oadtilqqfli (qr;il;qqrFqgg: gt tt
Istajl'd-trijyayor gh tet kotyaptarp prathamaqr phalarp I
Jyavargaqr gurlakarl kltvf kotivargap ca harakam ll
Pratham:1di-phalebhyo' tha ney:t phalatatatir muhuh I
Eka-tryldyo jasalikhl'lbhir bhaktesv etesv-anukramf,t ll
Ojana p sapyutes-tyaktvf, yugma-yogarp dhanur-bhabet I
Dohkotyor-alpam-eveha kalpaniyam-iha smrtamll
Labdhinam-avasdnar.n sy-nninyathSpi muhuh krite I
We may translate the above as follows:lr
The product of the given Sine and the radius divided by the Cosine is the first
result. From the first, (and then, second, third,) etc., results obtain (successively)a seque-
nce of results by taking repeatedlythe square of the Sine as the multiplier and the square of
the Cosine as the divisor. Divide (the above results) in srder by the odd numbers one' three'
etc. (to get the full sequenceof terms). From the sum of the odd terms' subtract the sum of
the even terms. (The results) becomes the arc. In this connection, it is laid down that the
(Sine of the) arc or ( that of ) its complement, which ever is smaller, should be taken here
(as the'given Sine'); otherwise, the terms, obtained by the (alrove) repeatedProcesswill not
tend to the vanishing-magnitudo.
That is, we are asked to form the sequence
(Rlr). (s/c), (,s/c)"
(s/c).
(n/3). (R/5).
(s/c). (sic)"..
(sic),.
:T T z , I s , ' . . s a ],
whereR is the radius (norm or sinus totus) of the circle reference and
S:R sin 0
C -R c o s 0 .
Then, according to the rule
v y s : ( T t { Tr* ...) - (Ir* 7 r* ...)
- - T r - T z* T s -T r* ... (2)
That is,
/R sin0) r R' ( Rsin r
0)
=lllnioJO)': - x
R 0 :3 II
,t"
9 j ; (1( 0)' r s. (R .oioF- "'
.*
Or
0 :ta n 0 -(ta n a 0 )/3 f (ta n 5 0)/5-...
which is equivalent to (l).
It may be noted that the condition given tolr'ards the end of the rule amounts to
saying that we should have R sin 0 to be less than R cos 0, 0 being accute. That is, tan 0 or
3. N. O. GUPTI 69
x should be less than trnity which is the condition for the absolute convergence of the series
(l ). Incidently this justifies the re-arrangement of the terms of the sequence the form (2)
in
which rvas known to the Indians of the period as is clear from the proof given by them (see
Section 3 belor.r').
The statement of the Midhava-Gregory seriesas found in the IfP, VI, l8 (p. l9)
is contained in the verse
aqrwfq {en*rrrgq6: r}aqrcaqtv su
E4rqiiur fqflerqrfqqq.d aftc,o set( |
5(ql$'ifegor*l dTg q*6+tftqotl|EftT-
ridoslqgiiee+iq eqfi dtargflcrsat tl tc rl
It r.r'ill be noted that the r.r'ordingof this stanza is similar to that of the first four
lines of the Sanskrit passageu'hich we have translated above. The meaning is almost the
same and need not to be repeated.
Still another Sanskrit stanza which gives the game seriesis found in the Sadratna-
ma l a of S ank ala V a rma (A .D . te 2 3 ;tr.
3. Derivation of the Series :
An ancient fndian derivation of the Mldhava-Gregory seriesis found in the YB (pp.
ll3-16). The proof starts rvith a geornetrical derivation of the rule which is basically
equivalent to what is implied in the modern formula dT:d ( tan 0 )/( lf tanz 0 ). The
elaborate proof then consistsof stepswhich amount to what, in modern analysis,is called
expansionar,d tcrm-by-term integration. However, it must be remembered that the proof
belongs lo the pre-calculusperiod in the modern sense.
The YII derivation has been published in various presentations by scholars such ar
C. T. Rajagopala, according to whom the proof "would even today be regalded as
satisfactory except for the abscnce of a fervjustificatory remarks", and othersrs. The
itrtelestedreader may refer to their publicatiorrsfor details,
References and Notec
l. C. B. Bo1-er: A lTislor2 of Mathematicr.Wiley, New York, 196'8,pp. 421'22.
2. K. V. Sarma ! Historl of Kerala School of Hindu Astronoml,t ( in Perspectittcz
:i s h v e s h v a ra n a n d s t., H oshi arpur, 1972,p' 51.
fn
T.A. Sara:watl i : "f'he Development of Mathematical Seriesin India after Bhaskara
II". Bull. A'ational Inst. of Sciences India, No. 2l ( 1963 ),
of
p .3 3 7 ; a rrd S a rm a , OP. ci t., p.20.
1. Sar m a, OP. c i t., p p . 5 7 -5 9 .
5. K. Kunjunni Raja : "Astronomy and Mathematics in Kerala (an Account of the Litera-
ttrre )" Ad y a r L i l -rra ryBul l , N o. 27 (1963)' pp. 154-55; and S ara-
sr,r'athi, cit., p.320.
oP.
6. The Yukti-EI:asa (in Malalalam). Part I, edited with noted by Rama Varma Maru
4. 70 T IIE X.[T IIEM IIIICg E D U C ITION
Thampuran and A.R. Akhileswar Aiyar, Mangalodayam press,
Trichur, 1948,pp. ll3-14. Also seethe Garlita-Yukti-Bhasa edited by
T. Chandrasekharan and others, lvfadras Government Oriental
I4anuscripts Selies No. 32, Madras, 1953,pp. 52-53 (the text as
edited here is corrupt).
7. Sarma, Op. cit., pp. 59-60.
B. The Kararla Paddhati: edited by K. Sambasiva Sastri, Trivandrum Sanskrit SeriesNo.
126, 'Irivandrum, 1937, p. 19. Also seethe KP along rvith two
Malayalam commentariesedited by S.K. Nayar Government Orie-
ntal Manuscripts Library, Madras; 1956, pp. 196-97.
9. Sarma, Op. cit., pp. 68-69.
It may be noted here that the arguments given by A. K. Bag, "Trigonometrical
Seriesin KP and the probable date of the text", IndianJ. Hist. Sci., vol.l (1966), pp. 102-105,
for a much earlier date of the work cannot be accepted becausehe has not fully analysed
the views found in the introduction of Nayar's edition cited above and also those summari-
zed by Raja, op. cit., etc.
lC. See referencesunder serial nos. 3 and 6 above. We have followed the text as given
in the YB in the Malayalam script. The text given by Sarma is slightly different.
I l. We have tried to give our own translation which is more or less a literal one. For a
different translation seeC. T. Rajagopal and T. V. Vedamurthi Aiyar, "Or the Hindu
Proof of Gregory's Series", ScriptaMathematica, Vol. l7 (1951), p. 67; Or Sarma,
" op. cit., pp.20-21 where the translation of Rajagopal and Ai1'ar has bee reproduced.
It may alsobe noted here that these two joint authors mention the nrle (quoted in the
YB) as a quotation from the Tantra-Samgraha (:TS, 1500 A.D.). So also Sarasr,,,a.
thi, op. cit., p. 337. Of course in the printed YB ( seeref. 6 above ) the work TS is
mentioned within brackets after one more rule given, besidesthe one which we have
quoted. The Ganita-YB does not montion TS at this place. Moreover the printed
TS (edited by S. K. Pillai, Trivandrum, l35B), which seemsto be complete in itself,
does not contain the lines. According to Sarma, op. cit., p. lB, the information, given
to Saraswathi, op. cit., p.32+, foot-note 9, that the printed TS is not complete, is not
likely to be correct.
12. Govt. Oriental Manuscripts Libray, Madras, lvls. No. R 4448, Ch. III, verse 10. For
date, seeSarma, oP.cit., p. 78.
13. Some referencesare :
(i) C. T. Rajagopal : "A Neglected Chapter of Hindu Mathematics". Soipta Math.,
V ol. l5 ( 19 4 9 ), p p . 2 0 1 -2 0 9 .
(ii) Rajagopala andVedanurthi Aiyar, op. cit., pp.65-74.
(iii) C. N. Srinivasiengar' : The Historlt of Ancient Indian Mathematics, World Press,
Calc ut t a, 19 6 7 ,p p . 1 4 6 -4 7 .
Horvever, the reader should be careful about the dates of the concerned Indian works
as given in the above three refcrences.