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In astrophysics, the Eddington number, ''N''Edd, is the number of protons in the observable universe. The term honors the British astrophysicist Arthur Eddington, who in 1938 was the first to propose a value of ''N''Edd and to explain why this number might be important for cosmology and the foundations of physics. ==History== Eddington argued that the value of the fine-structure constant, α, could be obtained by pure deduction. He related α to the Eddington number, which was his estimate of the number of protons in the universe.〔 〕 This led him in 1929 to conjecture that α was exactly 1/137. Other physicists did not adopt this conjecture and did not accept his argument. In the late 1930s, the best experimental value of the fine-structure constant, α, was approximately 1/136. Eddington then argued, from aesthetic and numerological considerations, that α should be exactly 1/136. He devised a "proof" that ''N''Edd = 136×2256, or about 1.57×1079. Some estimates of ''N''Edd point to a value of about 1080. These estimates assume that all matter can be taken to be hydrogen and require assumed values for the number and size of galaxies and stars in the universe.〔 〕 Attempts to find a mathematical basis for this dimensionless constant have continued up to the present time. In the 1938 Tarner Lecture at Trinity College, Cambridge, Eddington averred that: This large number was soon named the "Eddington number." Shortly thereafter, improved measurements of α yielded values closer to 1/137, whereupon Eddington changed his "proof" to show that α had to be exactly 1/137.〔Eddington (1946)〕 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Eddington number」の詳細全文を読む スポンサード リンク
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