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  1. Il y a 4 jours · Subrahmanyan Chandrasekhar (born October 19, 1910, Lahore, India [now in Pakistan]—died August 21, 1995, Chicago, Illinois, U.S.) was an Indian-born American astrophysicist who, with William A. Fowler, won the 1983 Nobel Prize for Physics for key discoveries that led to the currently accepted theory on the later evolutionary stages ...

    • The Editors of Encyclopaedia Britannica
  2. Il y a 4 jours · Subrahmanyan Chandrasekhar is back row, second from right, Arthur Eddington front row, second from right. Courtesy the AIP Emilio Segrè Visual Archives He presented this result at a meeting of the Royal Astronomical Society of London, but his findings were challenged by Eddington, who declared that Chandrasekhar’s ideas – based, as they were, solely on mathematics – bore no relation to ...

  3. Il y a 1 jour · Three more Indian-origin scientists have won — Hargovind Khorana in Medicine in 1968, Subrahmanyan Chandrasekhar in Physics in 1983, and Venkatraman Ramakrishnan in Chemistry 2009 — but they did their work outside India and were not Indian citizens when they were honoured.

  4. Il y a 1 jour · It has been 94 years since an Indian won a Nobel Prize in the sciences—Physics, Chemistry, or Medicine—while working in India. V. Raman’s Nobel Prize in Physics in 1930 remains the only accolade of its kind for India. Three additional Indian-origin scientists— Hargovind Khorana in Medicine (1968), Subrahmanyan Chandrasekhar in Physics ...

  5. Il y a 1 jour · Other Indian-origin Nobel laureates include Hargovind Khorana (Medicine, 1968), Subrahmanyan Chandrasekhar (Physics, 1983), and Venkatraman Ramakrishnan (Chemistry, 2009), but they did their work abroad and were not Indian citizens when awarded. Enroll now for UPSC Online Course. Challenges Hindering Scientific Advancement in India

  6. Il y a 4 jours · This term is neglected in the standard Chandrasekhar's treatment where only slower moving particles contribute to the decelerating drag. Here, we demonstrate that dynamical friction produced by the fast moving particles has a significant effect on the evolution of a massive binary within a dark matter spike.

  7. en.wikipedia.org › wiki › Black_holeBlack hole - Wikipedia

    Il y a 4 jours · In 1931, Subrahmanyan Chandrasekhar calculated, using special relativity, that a non-rotating body of electron-degenerate matter above a certain limiting mass (now called the Chandrasekhar limit at 1.4 M ☉) has no stable solutions. [23]