|Who is it?||Astrophysicist|
|Birth Day||February 14, 1896|
|Birth Place||Kingston upon Hull, British|
|Age||123 YEARS OLD|
|Died On||21 September 1950(1950-09-21) (aged 54)\nDublin, Ireland|
|Alma mater||Trinity College, Cambridge|
|Known for||Milne model|
|Institutions||Victoria University of Manchester University of Oxford|
|Doctoral students||Thomas Cowling|
Milne was born in Hull, Yorkshire, England. He attended Hymers College and from there he won an open scholarship in mathematics and natural science to study at Trinity College, Cambridge in 1914, gaining the largest number of marks which had ever been awarded in the examination. In 1916 he joined a group of mathematicians led by A. V. Hill for the Ministry of munitions working on the ballistics of anti-aircraft gunnery, they became known as ′Hill's Brigands′. Later Milne became an expert on sound localisation. In 1917 he became a lieutenant in the Royal Navy Volunteer Reserve. He was a fellow of Trinity College, Cambridge, 1919–1925, being assistant Director of the solar physics observatory, 1920–1924, mathematical lecturer at Trinity, 1924–1925, and university lecturer in astrophysics, 1922–1925. He was Beyer professor of applied mathematics, Victoria University of Manchester, 1924–1928, before his appointment as Rouse Ball Professor of Mathematics and to a fellowship at Wadham College, Oxford, in 1928. Milne's earlier work was in mathematical astrophysics. Much of his research in the 1930s was concerned with the theory of relativity and cosmology. His later work, concerned with the interior structure of stars, aroused controversy. Milne was President of the Royal Astronomical Society, 1943–1945. During World War II he again worked on ballistics.
Milne worked on the structures and interiors of stars in the late 1920s and early 1930s. He often took opinions opposed to those of Arthur Eddington.
From the early 1930s, Milne's interests focused increasingly on relativity theory and cosmology.
From 1932 he worked on the Problem of the "expanding universe" and in Relativity, Gravitation, and World-Structure (1935), proposed an alternative to Albert Einstein's general relativity theory. With McCrea (1934) he also showed that the 3 Models which form the foundations of modern cosmology first proposed by Friedmann (1922) using the general theory of relativity, can also be derived using only Newtonian mechanics.
As of 1935, using this model, Milne published a prediction of the cosmic background radiation which appears to be of a much different character than that predicted by Eddington. In fact, many passages in Relativity, Gravitation and World Structure are devoted to attacking Eddington's preconceptions.