Srinivasa Ramanujan

Srinivasa Ramanujan was a largely self-taught pure mathematician. Hindered by poverty and ill-health, his highly original work has considerably enriched number theory and, more recently, physics.

Beginnings

Srinivasa Ramanujan was born on December 8, 1820 in the town of Erode, in Tamil Nadu, in the south east of India. His father was K. Srinivasa Iyengar, an accounting clerk for a clothing merchant. His mother was Komalatammal, who earned a small amount of money each month as a singer at the local temple.

His family were Brahmins, the Hindu caste of priests and scholars. His mother ensured the boy was in tune with Brahmin traditions and culture. Although his family were high caste, they were very poor.

Ramanujan’s parents moved around a lot, and he attended a variety of different elementary schools. By the age of 10, he was the top student, not just in his school, but in his district.

The Discovery of Ramanujan as a Mathematician

The Hungry Years
At the beginning of 1907, at the age of 19, with minimal funds and a stomach all too often groaning with hunger, Ramanujan continued on the path he had chosen: total devotion to mathematics. The mathematics he was doing was highly original and very advanced.

Even though (or some might say because) he had very little formal mathematical education he was able to discover new theorems. He also independently discovered results originally discovered by some of the greatest mathematicians in history, such as Carl Friedrich Gauss and Leonhard Euler.

Ill-health was Ramanujan’s constant companion – as it would be for much of his short life.

By 1910 he realized he must find work to stay alive. In the city of Madras he found some students who needed mathematics tutoring and he also walked around the city offering to do accounting work for businesses.

And then a piece of luck came his way. Ramanujan tried to find work at the government revenue department, and there he met an official whose name was Ramaswamy Aiyer. Ramanujan did not have a resume to show Ramaswamy Aiyer; all he had was his notebooks – the results of his mathematical work.

Ramanujan’s good fortune was that Ramaswamy Aiyer was a mathematician. He had only recently founded the Indian Mathematical Society, and his jaw dropped when he saw Ramanujan’s work.

Number Theory and String Theory
In 1918 Ramanujan became the first Indian Mathematician to be elected a Fellow of the British Royal Society:

“Distinguished as a pure mathematician particularly for his investigation in elliptic functions and the theory of numbers.”

In his short lifetime he produced almost 4000 proofs, identities, conjectures and equations in pure mathematics.

His theta function lies at the heart of string theory in physics.

Some Personal Details and the End

In July 1909 Ramanujan married S. Janaki Ammal, who was then just 10 years old. The marriage had been arranged by Ramanujan’s mother. The couple began sharing a home in 1912.

When Ramanujan left to study at the University of Cambridge, his wife moved in with Ramanujan’s parents. Ramanujan’s scholarship was sufficient for his needs in Cambridge and the family’s needs in Kumbakonam.

For his first three years in Cambridge, Ramanujan was very happy. His health, however, had always been rather poor. The winter weather in England, much colder than anything he had ever imagined, made him ill for a time.

In 1917 he was diagnosed with tuberculosis and worryingly low vitamin levels. He spent months being cared for in sanitariums and nursing homes.

In February 1919 his health seemed to have recovered sufficiently for him to return to India, but sadly he would only live for about a year on his return.

Srinivasa Ramanujan died aged 32 in Madras on April 26, 1920. His death was most likely caused by hepatic amoebiasis caused by liver parasites common in Madras. His body was cremated.

Benjamin Franklin

Benjamin Franklin was one of the Founding Fathers of the United States. A renowned polymath, Franklin was a leading author, printer, political theorist, politician, freemason, postmaster, scientist, inventor, civic activist, statesman, and diplomat.

Benjamin Franklin’s Science, Innovation, and Inventions

Franklin was an original thinker, scientist and inventor. Dating his inventions is not always easy, because Franklin did not patent what he invented. He said that anyone who wanted to make money from his ideas was free to do so. This means the dates given to his inventions are approximate.

Bifocal Spectacles
The Franklin Stove

Franklin wore spectacles for most of his life.

He felt limited by the spectacles of his day, because a lens that was good for reading blurred his vision when he looked up. Working as a printer, this could be infuriating.

He defeated this problem in about 1739, aged 33, with his invention of split-lens bifocal spectacles. Each lens now had two focusing distances. Looking through the bottom part of the lens was good for reading, while looking through the upper part offered good vision at a greater distance.

As Franklin read more about science, he learned more about heat transfer. He looked at the design of a typical stove and concluded that it was inefficient. Much more heat was lost up the flue than necessary.

He decided to redesign the stove using the concept of heat-exchange/heat recovery.

The idea was that hot gases which would normally simply go up the flue would exchange their heat with cold air from the room, heating it up, and so heating the room up.

In 1741, the Franklin Stove came on to the market, allowing homeowners to get more heat into their homes for each unit of fuel they burned.

Electricity

In summer 1743, Franklin visited his hometown of Boston. Always seeking new knowledge, he visited a science show. There he saw Dr. Archibald Spencer, who had arrived from Scotland, demonstrating a variety of scientific phenomena. The electrical part of the show intrigued Franklin most: it featured the effects of static electricity.

Franklin left the show determined to learn more about electricity. It seemed to him that Dr. Spencer didn’t really understand it. This, of course, was true: nobody understood it! It was more a source of entertainment than a science.

In 1747, Franklin got hold of a long glass tube for the efficient generation of static electricity from Peter Collinsion in London.

Shaping our understanding of electricity

Franklin’s observations soon began to shape the world’s understanding of electricity and shape the language we use even today when we talk about it.

He identified that there was an electrical fluid that could flow from A to B. To describe the process he coined the terms positive and negative to describe the difference between A and B after the electrical fluid had flowed. Of course, today we would call the electrical fluid electrons, but remember: this was 1747; J.J. Thomson’s discovery of the electron lay 150 years in the future!

Franklin found that an excess of fluid led to positive charge (okay, we’ll have to pretend that electrons are positively charged for this) and a deficit of fluid led to negative charge.

Franklin was the first to write that electric charge cannot be created; it can only be ‘collected.’ This is a fundamental law of physics – the Law of Conservation of Electric Charge. It means that you cannot create (or destroy) electric charge.

Franklin was also the first person to use the words electrical battery. His meaning was not the same as ours though. His battery was made of capacitors (known as Leyden jars) wired together in series to store more charge than one alone could. This enabled Franklin to produce a bigger discharge of static electricity in his experiments.

In 1751, Franklin published the fruits of his labors in a book called Experiments and Observations on Electricity, which was widely read in Britain and then Europe, shaping a new understanding of electricity.

In 1752 Franklin’s most famous scientific work was carried out – the proof that lightning is electricity.

Franklin had an idea for an experiment to prove that lightning is electricity, making use of another of his own discoveries in electricity: that static electricity discharges to a sharp, pointed object more readily than to a blunt object.

King Louis XV saw a translation of Experiments and Observations on Electricity, and he asked French scientists to test Franklin’s lightning rod concept.

Jean Francois Dalibard used Franklin’s idea to confirm by experiment that lightning was indeed electrical in Paris in May 1752. Franklin himself carried out similar work in 1752, using a kite with a metal key connected to a Leyden Jar to prove his own theory. He didn’t write about his own experiment, however, until 1772.

The significance of the experiment was that it established the study of electricity as a serious scientific discipline.

Franklin had shown how to prove that electrical phenomena were a fundamental force of nature. Electricity would never again be thought of as just an interesting plaything for scientists and showmen to conjure up using glass rods.

Very soon, in 1753, when he was aged 47, the transformation in science that Franklin had brought about was recognized. Britain’s Royal Society honored his electrical work with its highest award, the Copley Medal – the equivalent of a modern Nobel Prize.

Meteorology

By observation of storms and winds, Franklin discovered that storms do not always travel in the direction of the prevailing wind. This was an important discovery in the development of the scientific discipline of meteorology.

More than a Scientist and Inventor

Franklin lived in turbulent times, which culminated in the United States’ Declaration of Independence in 1776: Franklin was one of the five men who drafted it. He had previously acted as British postmaster for the colonies; he was the American Ambassador in France from 1776 – 1785; and the governor of Pennsylvania from 1785 – 1788.

Benjamin Franklin’s Early Life and Education

Benjamin Franklin was born on January 17, 1706, in Boston, Massachusetts. His father, Josiah, was a tallow chandler, candle maker, and soap boiler who had moved to the American Colonies from England. His mother, Abiah Folger looked after the home and was the mother of ten children, including Benjamin, who was the eighth child in the family. She was born in Nantucket, Massachusetts.

Benjamin only had two years of formal education, which finished when he was ten years old, because his family could not afford the fees. His informal education then accelerated, because his mind was too restless to stop learning.

He had to work in his father’s business, but in his spare time he read everything he could, about every subject under the sun.

When he was twelve, Benjamin began working as an apprentice in a printing shop owned by one of his elder brothers, James. When his brother started printing a newspaper, Benjamin wrote to it in the name of “Mrs. Dogood” in defense of freedom of speech.

Aged 17, Benjamin Franklin left for Philadelphia, escaping from his apprenticeship, which was against the law. He was, however, free. After a few months in Philadelphia he left for London, England, where he learned more about printing, before returning to Philadelphia at the age of 20 to continue his career in printing.

The End

Benjamin Franklin died on April 17, 1790, at the age of 84. He was killed by pleurisy – a lung inflammation.

His wife, Deborah, had died sixteen years earlier. Franklin was survived by his daughter, Sarah, who looked after him in his later years and his son, William. William left America to live in Britain in 1782.

Today, the Benjamin Franklin Medal, named in Franklin’s honor, is one of the most prestigious awards in science. Its winners include Alexander Graham Bell, Marie and Pierre Curie, Albert Einstein and Stephen Hawking.

India is the land of glorious history in the field of science and technology. It is the birth place of the great scientist Aryabhatta, who was the first to introduce the concept of numbers in the ancient times and this legacy has been carried forward by the modern scientists of the country, who have greatly contribution to the world with their awe inspiring inventions and discoveries.

C. V. Raman

One of the most prominent Indian scientists in history, C.V. Raman was the first Indian person to win the Nobel Prize in science for his illustrious 1930 discovery, now commonly known as the “Raman Effect”. It is immensely surprising that Raman used equipment worth merely Rs.200 to make this discovery. The Raman Effect is now examined with the help of equipment worth almost millions of rupees.

Contributions and Achievements:

On a sea voyage to Europe in 1921, Raman curiously noticed the blue color of the glaciers and the Mediterranean. He was passionate to discover the reason for the blue color. Once Raman returned to India, he performed many experiments regarding the scattering of light from water and transparent blocks of ice. According to the results, he established the scientific explanation for the blue color of sea-water and sky.

There is a captivating event that served as the inspiration for the discovery of the Raman Effect. Raman was busy doing some work on a December evening in 1927, when his student, K.S. Krishnan (who later became the Director of the National Physical Laboratory, New Delhi), gave him the news that Professor Compton had won the Nobel Prize on scattering of X-rays. This led Raman to have some thoughts. He commented that if the Compton Effect is applicable for X-rays, it must also be true for light. He carried out some experiments to establish his opinion.

Raman employed monochromatic light from a mercury arc which penetrated transparent materials and was allowed to fall on a spectrograph to record its spectrum. During this, Raman detected some new lines in the spectrum which were later called ‘Raman Lines’. After a few months, Raman put forward his discovery of ‘Raman Effect’ in a meeting of scientists at Bangalore on March 16, 1928, for which he won the Nobel Prize in Physics in 1930.

The ‘Raman Effect’ is considered very significant in analyzing the molecular structure of chemical compounds. After a decade of its discovery, the structure of about 2000 compounds had been studied. Thanks to the invention of the laser, the ‘Raman Effect’ has proved to be a very useful tool for scientists.

Some of Raman’s other interests were the physiology of human vision, the optics of colloids and the electrical and magnetic anisotropy.

Early Life:

Chandrasekhara Venkata Raman was born at Tiruchirapalli in Tamil Nadu on 7th November 1888 to a physics teacher. Raman was a very sharp student. After doing his matriculation at 12, he was supposed to go abroad for higher studies, but after medical examination, a British surgeon suggested against it. Raman instead attended Presidency College, Madras. After completing his graduation in 1904, and M.Sc. in Physics in 1907, Raman put through various significant researches in the field of physics. He studied the diffraction of light and his thesis on the subject was published in 1906.

Raman was made the Deputy Accountant General in Calcutta in 1907, after a successful Civil Service competitive examination. Very much occupied due to his job, he spent his spare time in the evenings conducting scientific research at the laboratory of the Indian Association for Cultivation of Sciences. On certain occasions, he even spent entire nights there. Such was his passion that in 1917, he resigned from the position to become the Professor of Physics at Calcutta University.

Later Life and Death:

Sir C.V. Raman became the Fellow of the Royal Society of London in 1924. A year later, he set up Raman Research Institute near Bangalore, where he continued scientific research until his death which was caused by a strong heart attack on November 21, 1970. His sincere advice to aspiring scientists was that “scientific research needed independent thinking and hard work, not equipment.”

Stephen Hawking

Stephen William Hawking was born on 8 January 1942 (300 years after the death of Galileo) in Oxford, England. His parents' house was in north London, but during the second world war, Oxford was considered a safer place to have babies. When he was eight, his family moved to St. Albans, a town about 20 miles north of London. At the age of eleven, Stephen went to St. Albans School and then on to University College, Oxford; his father's old college. Stephen wanted to study Mathematics, although his father would have preferred medicine. Mathematics was not available at University College, so he pursued Physics instead. After three years and not very much work, he was awarded a first  class honours degree in Natural Science. 

Stephen then went on to Cambridge to do research in Cosmology, there being no one working in that area in Oxford at the time. His supervisor was Denis Sciama, although he had hoped to get Fred Hoyle who was working in Cambridge. After gaining his Ph.D. he became first a Research Fellow and later on a Professorial Fellow at Gonville and Caius College. After leaving the Institute of Astronomy in 1973, Stephen came to the Department of Applied Mathematics and Theoretical Physics in 1979, and held the post of Lucasian Professor of Mathematics from 1979 until 2009. The chair was founded in 1663 with money left in the will of the Reverend Henry Lucas who had been the Member of Parliament for the University. It was first held by Isaac Barrow and then in 1669 by Isaac Newton.  Stephen is still an active part of Cambridge University. His title is now the Dennis Stanton Avery and Sally Tsui Wong-Avery Director of Research at the Department of Applied Mathematics and Theoretical Physics. 

His many publications include The Large Scale Structure of Spacetime with G F R Ellis, General Relativity: An Einstein Centenary Survey, with W Israel, and 300 Years of Gravity, with W Israel. Among the popular books Stephen Hawking has published are his best seller A Brief History of Time, Black Holes and Baby Universes and Other Essays, The Universe in a Nutshell, The Grand Design and My Brief History. 

Professor Hawking has twelve honorary degrees. He was awarded the CBE in 1982, and was made a Companion of Honour in 1989. He is the recipient of many awards, medals and prizes, is a Fellow of The Royal Society and a Member of the US National Academy of Sciences. 

Stephen was diagnosed with ALS, a form of Motor Neurone Disease, shortly after his 21st birthday. In spite of being wheelchair bound and dependent on a computerised voice system for communication Stephen Hawking continues to combine family life (he has three children and three grandchildren), and his research into theoretical physics together with an extensive programme of travel and public lectures. He still hopes to make it into space one day.

Galileo

OCCUPATION

Astronomer, Scientist

BIRTH DATE

February 15, 1564

DEATH DATE

January 8, 1642

PLACE OF BIRTH

Pisa, Italy

PLACE OF DEATH

Arcetri, Italy

AKA

Galileo

NICKNAME

"The Father of Modern Scibence"

FULL NAME

Galileo Galilei

Born on February 15, 1564, in Pisa, Italy, Galileo Galilei was a mathematics professor who made pioneering observations of nature with long-lasting implications for the study of physics. He also constructed a telescope and supported the Copernican theory, which supports a sun-centered solar system. Galileo was accused twice of heresy by the church for his beliefs, and wrote books on his ideas. He died in Arcetri, Italy, on January 8, 1642.

Controversial Findings

In 1604, Galileo published The Operations of the Geometrical and Military Compass, revealing his skills with experiments and practical technological applications. He also constructed a hydrostatic balance for measuring small objects. These developments brought him additional income and more recognition. That same year, Galileo refined his theories on motion and falling objects, and developed the universal law of acceleration, which all objects in the universe obeyed. Galileo began to express openly his support of the Copernican theory that the earth and planets revolved around the sun. This challenged the doctrine of Aristotle and the established order set by the Catholic Church.

In July 1609, Galileo learned about a simple telescope built by Dutch eyeglass makers, and he soon developed one of his own. In August, he demonstrated it to some Venetian merchants, who saw its value for spotting ships and gave Galileo salary to manufacture several of them. However, Galileo’s ambition pushed him to go further, and in the fall of 1609 he made the fateful decision to turn his telescope toward the heavens. In March 1610, he published a small booklet, The Starry Messenger, revealing his discoveries that the moon was not flat and smooth, but a sphere with mountains and craters. He found Venus had phases like the moon, proving it rotated around the sun. He also discovered Jupiter had revolving moons, which didn’t revolve around the earth.