Edward Arthur Milne

Edward Arthur Milne

Infobox Scientist
name = Arthur Milne
box_width =



image_width =
caption =
birth_date = birth date|1896|02|14
birth_place = Hull, Yorkshire, England
death_date = death date and age|1950|09|02|1896|02|14
death_place = Dublin, Ireland
residence =
citizenship =
nationality =
ethnicity =
field =
work_institutions =
alma_mater =
doctoral_advisor =
doctoral_students =
known_for =
author_abbrev_bot =
author_abbrev_zoo =
influences =
influenced =
prizes =
religion =
footnotes =

Edward Arthur Milne FRS (February 14 1896 – September 21 1950) was a British astrophysicist and mathematician.

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. 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. From 1932 he also 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. His later work, concerned with the interior structure of stars, aroused controversy. Milne was president of the Royal Astronomical Society, 1943–1945. He was, as would be the next Rouse Ball Professor of Mathematics, Charles Coulson, a pioneer in religion and science discussions.

He died in Dublin, Ireland, while preparing to give a set of lectures. These can be found written down in one of his last published books: "Modern Cosmology and the Christian Idea of God" (1952).

"Relativity, Gravitation, and World Structure"

The main difference between the Milne model of an expanding universe, and the current (Einstein's) model of an expanding universe was that Milne did not assume "a priori" that the universe has a homogeneous matter distribution. He didn't include the gravitation interaction into the model either.

Milne argued that under the context of Einstein's special relativity, and the relativity of simultaneity, that it is impossible for a nonstatic universe to be homogeneous. Namely, if the universe is spreading out, its density is decreasing over time, and that if two regions appeared to be at the same density at the same time to one observer, they would not appear to be the same density at the same time to another observer. However, if each observer measures its local density at the same agreed-upon proper time, the measured density should be the same. In Minkowskian coordinates, this constant proper time forms a hyperbolic surface which extends infinitely to the light-cone of the event of creation. This is true even when proper time approaches 0, the time of the creation. The universe is already infinite at the creation time!

Milne's model (shown below) is, therefore, that of a sphere, with an approximately homogeneous matter distribution within several billion light years of the center which then increases to an infinite density. It can be shown that this infinite density is actually the density of the universe when at the time of the big bang. The spherical distribution is unique in that it is essentially the same after a Lorentz transformation, except that a different stationary particle is at the center. As it is the only distribution that has this property, it is the only distribution which could satisfy the cosmological principle of "no preferred reference frame." Based on this cosmological principle Milne created a model that can be described entirely within Euclidean geometry.

The plate below shows that 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.

Honours

Awards
*Gold Medal of the Royal Astronomical Society (1935)
*Royal Society's Royal Medal (1941)
*Bruce Medal (1945)Named after him
*Milne crater on the Moon

Books by Milne

* "The White Dwarf Stars", Oxford: Clarendon Press, 1932.
* "Relativity, gravitation and world-structure", Oxford: Clarendon Press, 1935.
* "The Inverse Square Law of Gravitation", London: Harrison and Son, 1936.
* "The Fundamental Concepts of Natural Philosophy", Edinburgh: Oliver & Boyd, 1943.
* "Kinematic relativity; a sequel to Relativity, gravitation and world structure", Oxford: Clarendon Press, 1948.
* "Vectorial Mechanics", New York: Interscience Publishers, 1948.
* "Modern Cosmology and the Christian Idea of God", Oxford: Clarendon Press, 1952.
* "Sir James Jeans: A Biography", Cambridge University Press, 1952.

ee also

*Gale, George, " [http://setis.library.usyd.edu.au/stanford/entries/cosmology-30s/ Cosmology: Methodological Debates in the 1930s and 1940s,] " Stanford Encyclopedia of Philosophy. Milne was a major player in the cosmological controversies described in this article.
*Herbert Dingle#Controversies
*List of science and religion scholars

Bibliography (excerpt)

* Thermodynamics of the Stars (1930)
* The White Dwarf Stars (1932)
* Relativity, Gravitation and World-Structure (1935)
* Kinematic Relativity (1948)

External links

*


Wikimedia Foundation. 2010.

Игры ⚽ Нужно решить контрольную?

Look at other dictionaries:

  • Edward Arthur Milne — Edward Arthur Milne, debout à droite. Edward Arthur Milne (14 février 1896 21 septembre 1950) est un mathématicien et astrophysicien britannique. Sommaire …   Wikipédia en Français

  • Edward Arthur Milne — stehend, links nach rechts: Mark Gertler, Hewy Levy, Walter J. Turner, Edward Arthur Milne; sitzend, links nach rechts: Ralph Hodgson, J.W.N. Sullivan und S. S. Koteliansky. London, 1928 Edward Arthur Milne (* 14. Februar 1896 in Hull, Yorkshire; …   Deutsch Wikipedia

  • Arthur Milne — Edward Arthur Milne Edward Arthur Milne, debout à droite. Edward Arthur Milne (14 février 1896 21 septembre 1950) est un mathématicien et astrophysicien britannique. Sommaire …   Wikipédia en Français

  • Milne, Edward Arthur — ▪ British astrophysicist born Feb. 14, 1896, Hull, Yorkshire, Eng. died Sept. 21, 1950, Dublin       English astrophysicist and cosmologist best known for his development of kinematic relativity.       Milne was educated at the University of… …   Universalium

  • Edward Milne — Edward Arthur Milne Edward Arthur Milne, debout à droite. Edward Arthur Milne (14 février 1896 21 septembre 1950) est un mathématicien et astrophysicien britannique. Sommaire …   Wikipédia en Français

  • Milne (surname) — Milne /ˈmɪln/ is a surname of Scottish origin, and may refer to: In military: Sir Alexander Milne, 1st Baronet, British admiral Archibald Berkeley Milne (1855–1938), admiral of the Royal Navy Sir David Milne, British admiral Duncan Grinnell Milne …   Wikipedia

  • Milne (crater) — Coordinates 31°24′S 112°12′W / 31.4°S 112.2°W / …   Wikipedia

  • Milne — ist der Familienname folgender Personen: A. A. Milne (1882–1956), englischer Schriftsteller Alan Alexander Milne (1882–1956), englischer Schriftsteller Alphonse Milne Edwards (1835–1900), französischer Ornithologe, Karzinologe und Naturforscher… …   Deutsch Wikipedia

  • Edward Milne — may refer to*Edward Arthur Milne (1896 ndash;1950), British mathematician and astrophysicist *Eddie Milne (1915 ndash;1983), British Labour Party Member of Parliament for Blyth, afterwards re elected as an independent …   Wikipedia

  • Arthur Geoffrey Walker — (* 17. Juli 1909 in Watford, Hertfordshire, England; † 31. März 2001) war ein britischer Mathematiker, der sich mit Differentialgeometrie beschäftigte und bedeutende Beträge zur Kosmologie geleistet hat. Walker studierte ab 1931 an der… …   Deutsch Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”