Subrahmanyan Chandrasekhar

Early life and education Chandrasekhar was born in Lahore on 19 October 1910 of the British Raj (present-day Pakistan) into a Tamil Brahmin family, to Sita Balakrishnan and C. Subrahmanya Ayyar, who was stationed in Lahore as Deputy Auditor General of the Northwestern Railways at the time of Chandrasekhar's birth. Chandra, as Chandrasekhar was known, had two elder sisters, Rajalakshmi and Balaparvathi, three younger brothers, Vishwanathan, Balakrishnan, and Ramanathan, and four younger sisters, Sarada, Vidya, Savitri, and Sundari. His paternal uncle was the Indian physicist and Nobel laureate C. V. Raman. His mother was devoted to intellectual pursuits, had translated Henrik Ibsen's A Doll's House into Tamil and is credited with arousing Chandra's intellectual curiosity at an early age. The family moved from Lahore to Allahabad in 1916, and finally settled in Madras in 1918.

Chandrasekhar was tutored at home until the age of 12. He obtained his bachelor's degree, BSc (Hon.), in physics, in June 1930. In July 1930, Chandrasekhar was awarded a Government of India scholarship to pursue graduate studies at the University of Cambridge, where he was admitted to Trinity College. The scholarship was secured by Ralph H. Fowler, to whom Chandrasekhar had sent his first paper. During his travels to England, Chandrasekhar spent his time working out the statistical mechanics of the degenerate electron gas in white dwarf stars, providing relativistic corrections to Fowler's previous work (see Legacy below).

University of Cambridge In his first year at Cambridge, as a research student of Fowler, Chandrasekhar spent his time calculating mean opacities and applying his results to the construction of an improved model for the limiting mass of a degenerate star. At the meetings of the Royal Astronomical Society, he met E. A. Milne. At the invitation of Max Born he spent the summer of 1931, his second year of post-graduate studies, at Born's institute at Göttingen, working on opacities, atomic absorption coefficients, and model stellar photospheres. On the advice of Paul Dirac, he spent his final year of graduate studies (September 1932 to May 1933) at the Institute for Theoretical Physics in Copenhagen, where he met Niels Bohr. At Copenhagen, he became friends with Victor Weisskopf, Léon Rosenfeld, George Placzek and Max Delbrück as they were all living in the same pension.

After receiving a bronze medal for his work on degenerate stars, Chandrasekhar was awarded his PhD degree at Cambridge in the summer of 1933, with a thesis on rotating self-gravitating polytropes. On 9 October, he was elected to a Prize Fellowship at Trinity College for the period 1933–1937, becoming only the second Indian to receive a Trinity Fellowship after Srinivasa Ramanujan 16 years earlier. He had been so certain of failing to obtain the fellowship that he had already made arrangements to study under Milne that autumn at Oxford, even going to the extent of renting a flat there.

Chandrasekhar remained at the University of Chicago for the rest of his career, 1937-1995. He was promoted to associate professor in 1941 and to full professor two years later at the age of 33.

After the Laboratory for Astrophysics and Space Research (LASR) was built by NASA in 1966 at the university, Chandrasekhar occupied one of the four corner offices on the second floor. (The other corners housed John A. Simpson, Peter Meyer, and Eugene N. Parker.) Chandrasekhar lived at 4800 Lake Shore Drive after the high-rise apartment complex was built in the late 1960s, and later at 5550 Dorchester Building.

Dispute with Eddington

After graduating from Cambridge, Chandrasekhar, who was in close contact with Arthur Eddington, presented a full solution to his stellar equation at the Royal Astronomical Society meeting in 1935. Eddington booked a talk right after Chandrasekhar, where he openly criticized Chandrasekhar's theory. This depressed Chandrasekhar and sparked a scientific dispute. Eddington refused to accept a limit for the mass of a star and proposed an alternative model.

Chandrasekhar sought support from prominent physicists like Léon Rosenfeld, Niels Bohr and Christian Møller who found Eddington's arguments lacking. The tension persisted through 1930s, as Eddington continued to openly criticize Chandrasekhar during meetings and the two compared each other's theories in publications. Chandrasekhar ultimately completed his theory of white dwarfs in 1939, receiving praise from others in the field. Eddington died in 1944, and despite their disagreements, Chandrasekhar continued to state that he admired Eddington and considered him a friend. On the Determination of the Velocity of a Projectile from the Beat Waves Produced by Interference with the Waves of Modified Frequency Reflected from the Projectile and The normal reflection of a blast wave. Chandrasekhar's expertise in hydrodynamics led Robert Oppenheimer to invite him to join the Manhattan Project at Los Alamos, but delays in the processing of his security clearance prevented him from contributing to the project. It has been rumoured that he visited the Calutron project.

Philosophy of systematization

He wrote that his scientific research was motivated by his desire to participate in the progress of different subjects in science to the best of his ability, and that the prime motive underlying his work was systematization. "What a scientist tries to do essentially is to select a certain domain, a certain aspect, or a certain detail, and see if that takes its appropriate place in a general scheme which has form and coherence; and, if not, to seek further information which would help him to do that".

Chandrasekhar developed a unique style of mastering several fields of physics and astrophysics; consequently, his working life can be divided into distinct periods. He would exhaustively study a specific area, publish several papers in it and then write a book summarizing the major concepts in the field. He would then move on to another field for the next decade and repeat the pattern. Thus he studied stellar structure, including the theory of white dwarfs, during the years 1929 to 1939, and subsequently focused on stellar dynamics, theory of Brownian motion from 1939 to 1943. Next, he concentrated on the theory of radiative transfer and the quantum theory of the negative ion of hydrogen from 1943 to 1950. This was followed by sustained work on turbulence and hydrodynamic and hydromagnetic stability from 1950 to 1961. In the 1960s, he studied both the equilibrium and the stability of ellipsoidal figures of equilibrium, and general relativity. During the period, 1971 to 1983 he studied the mathematical theory of black holes, and, finally, during the late 80s, he worked on the theory of colliding gravitational waves. Sagan recalled, "I discovered what true mathematical elegance is from Subrahmanyan Chandrasekhar."

Other activities

From 1952 to 1971 Chandrasekhar was editor of The Astrophysical Journal. When Eugene Parker submitted a paper on his discovery of solar wind in 1957, two eminent reviewers rejected the paper. However, since Chandra as an editor could not find any mathematical flaws in Parker's work, he went ahead and published the paper in 1958.

During the years 1990 to 1995, Chandrasekhar worked on a project devoted to explaining the detailed geometric arguments in Sir Isaac Newton's Philosophiae Naturalis Principia Mathematica using the language and methods of ordinary calculus. The effort resulted in the book Newton's Principia for the Common Reader, published in 1995.

Chandrasekhar also worked on collision of gravitational waves, and algebraically special perturbations. He had a strong interest in literature and the arts. In 1975, he lectured on patterns of creativity in Shakespeare, Beethoven and Newton.

Personal life

S. Chandrasekhar with his brothers and sisters in Madras [Chennai], India. From left to right seated are: Bala, Savitri, Chandra, Sarada, Rajam; standing: Vidya, Balakrishnan, Vishwam, Ramanathan, Sundari.

Chandrasekhar was the nephew of C. V. Raman, who was awarded the Nobel Prize for Physics in 1930.

Chandrasekhar married Lalitha Doraiswamy in September 1936. He met her as a fellow physics student at Presidency College. Doraiswamy's enthusiasm for physics mainly came from her interest in Marie Curie and India awarding the Nobel Prize in Physics to C. V. Raman. She wanted to continue her studies in England, but her mother did not agree to this, which led Doraiswamy to earn an LT (teaching degree) from the University of Madras and Lady Willingdon Training College in 1932. She spent the next few years teaching physics, chemistry, math, and physical education at various institutions. She earned her master's degree in physics from Presidency College in 1934. Doraiswamy eventually gave up her studies to focus on supporting her husband's career by primarily managing their household so he could focus on his work.

Chandrasekhar became a naturalized citizen of the U.S. in 1953. Many considered him warm, positive, generous, unassuming, meticulous, and open to debate, while others found him private, intimidating, impatient and stubborn about non-scientific matters, Chandrasekhar was a vegetarian. She was a serious student of literature and western classical music. This was also confirmed many times in his other talks. Kameshwar C. Wali quoted him saying: "I am not religious in any sense; in fact, I consider myself an atheist." In an October 1987 interview, Chandrasekhar said: "Of course, he (Otto Struve) knew I was an atheist, and he never brought up the subject with me". In deference to Chandrasekhar's atheistic views, his wife refrained from displaying the small religious icons of deities she had brought with her.

Awards, honours and legacy

Nobel prize

Chandrasekhar was awarded half of the Nobel Prize in Physics in 1983 for his studies on the physical processes important to the structure and evolution of stars. Chandrasekhar accepted this honour, but was upset the citation mentioned only his earliest work, seeing it as a denigration of a lifetime's achievement. He shared it with William A. Fowler.

Other awards and honors

Elected a Fellow of the Royal Society (FRS) in 1944 American Academy of Arts and Sciences, Member (1946) Henry Norris Russell Lectureship (1949) Bruce Medal (1952) Gold Medal of the Royal Astronomical Society (1953) United States National Academy of Sciences, Member (1955) Rumford Prize of the American Academy of Arts and Sciences (1957) National Medal of Science, USA (1966) Padma Vibhushan (1968) Henry Draper Medal of the National Academy of Sciences (1971) Marian Smoluchowski Medal (1973) Copley Medal of the Royal Society (1984) Gordon J. Laing Award (1989) Golden Plate Award of the American Academy of Achievement (1990) Jansky Lectureship before the National Radio Astronomy Observatory

Legacy

Chandrasekhar's most notable work is on the astrophysical Chandrasekhar limit. The limit gives the maximum mass of a white dwarf star, ~1.44 solar masses, or equivalently, the minimum mass that must be exceeded for a star to collapse into a neutron star or black hole (following a supernova). The limit was first calculated by Chandrasekhar in 1930 during his maiden voyage from India to Cambridge, England for his graduate studies. In 1979, NASA named the third of its four "Great Observatories" after Chandrasekhar. This followed a naming contest which attracted 6,000 entries from fifty states and sixty-one countries. The Chandra X-ray Observatory was launched and deployed by Space Shuttle Columbia on 23 July 1999. The Chandrasekhar number, an important dimensionless number of magnetohydrodynamics, is named after him. The asteroid 1958 Chandra is also named after Chandrasekhar. The Himalayan Chandra Telescope is named after him. In the Biographical Memoirs of Fellows of the Royal Society of London, R. J. Tayler wrote: "Chandrasekhar was a classical applied mathematician whose research was primarily applied in astronomy and whose like will probably never be seen again."

Chandrasekhar supervised 45 PhD students. After his death, his wife Lalitha Chandrasekhar made a gift of his Nobel Prize money to the University of Chicago towards the establishment of the Subrahmanyan Chandrasekhar Memorial Fellowship. First awarded in the year 2000, this fellowship is given annually to an outstanding applicant to graduate school in the PhD programs of the department of physics or the department of astronomy and astrophysics. S. Chandrasekhar Prize of Plasma Physics is an award given by Association of Asia Pacific Physical Societies (AAPS) to outstanding plasma physicists, started in the year 2014.

The Chandra Astrophysics Institute (CAI) is a program offered for high school students who are interested in astrophysics mentored by MIT scientists and sponsored by the Chandra X-ray Observatory.

In 2010, on account of Chandra's 100th birthday, University of Chicago conducted a symposium titled Chandrasekhar Centennial Symposium 2010 which was attended by leading astrophysicists such as Roger Penrose, Kip Thorne, Freeman Dyson, Jayant V. Narlikar, Rashid Sunyaev, G. Srinivasan, and Clifford Will. Its research talks were published in 2011 as a book titled Fluid flows to Black Holes: A tribute to S Chandrasekhar on his birth centenary.

On 19 October 2017, Chandrasekhar was celebrated in a Google Doodle honouring his 107th birthday.

Publications

Books