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Subrahmanyan Chandrasekhar ( tamil: சுப்பிரமணியன் சந்திரசேகர்) ( Lahore, 19 ottobre 1910 – Chicago, 21 agosto 1995) è stato un fisico, astrofisico e matematico indiano naturalizzato statunitense . Indice. 1 Biografia. 1.1 Limite di Chandrasekhar. 2 Curiosità. 3 Premi. 4 Onorificenze. 5 Note. 6 Voci correlate. 7 Altri progetti.
Subrahmanyan Chandrasekhar FRS (/ ˌ tʃ æ n d r ə ˈ ʃ eɪ k ər /; 19 October 1910 – 21 August 1995) was an Indian-American theoretical physicist who made significant contributions to understanding of stellar evolution, black holes, and the structure of stars.
30 apr 2024 · 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
The Nobel Prize in Physics 1983 was divided equally between Subrahmanyan Chandrasekhar "for his theoretical studies of the physical processes of importance to the structure and evolution of the stars" and William Alfred Fowler "for his theoretical and experimental studies of the nuclear reactions of importance in the formation of the chemical ...
21 ago 1995 · Subrahmanyan Chandrasekhar. The Nobel Prize in Physics 1983. Born: 19 October 1910, Lahore, India (now Pakistan) Died: 21 August 1995, Chicago, IL, USA. Affiliation at the time of the award: University of Chicago, Chicago, IL, USA.
Subrahmanyan Chandrasekhar nasce il 19 ottobre 1910. Biografia della rubrica “Vita da genio” a cura di Chiara Oppedisano. Il nome di Subrahmanyan Chandrasekhar, chiamato amichevolmente “Chandra” da amici e colleghi, è indissolubilmente legato all’evoluzione delle stelle e alla loro fine….
Subrahmanyan Chandrasekhar was one of the foremost astrophysicists of the twentieth century. He was one of the first scientists to couple the study of physics with the study of astronomy. Chandra proved that there was an upper limit to the mass of a white dwarf.
