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词条 Eddington number
释义

  1. History

  2. Recent theory

  3. See also

  4. References

  5. Bibliography

{{About|astrophysics|the measure in cycling|Arthur Eddington#Eddington number for cycling}}

In astrophysics, the Eddington number, NEdd, is the number of protons in the observable universe. The term is named for British astrophysicist Arthur Eddington, who in 1938 was the first to propose a value of NEdd and to explain why this number might be important for physical 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.[1] 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 {{nowrap|1=NEdd = 136 × 2256}}, or about {{val|1.57|e=79}}. Some estimates of NEdd point to a value of about {{val|e=80}}.[2] 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.[3]

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:

{{quote |I believe there are 15 747 724 136 275 002 577 605 653 961 181 555 468 044 717 914 527 116 709 366 231 425 076 185 631 031 296 protons in the universe and the same number of electrons.[4]}}

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.[5]

Recent theory

The most precise value of α (obtained experimentally in 2012) is:[6]

{{quote|}}

Consequently, no one maintains any longer that α is the reciprocal of an integer. Nor does anyone take seriously a mathematical relationship between α and NEdd.

On possible roles for NEdd in contemporary cosmology, especially its connection with large number coincidences, see Barrow (2002) (easier) and Barrow and Tipler (1986: 224–31) (harder).

See also

  • Combinatorial hierarchy
  • Eddington–Dirac number
  • Eddington number (cycling)
  • One-electron universe
  • The Sand Reckoner
  • Universe

References

1. ^{{Cite book |author=A. S. Eddington |year=1956 |chapter=The Constants of Nature |editor=J. R. Newman |title=The World of Mathematics |volume=2 |pages=1074–1093 |publisher=Simon & Schuster |isbn= |oclc= |lccn=}}
2. ^{{Cite web | url=http://mrob.com/pub/math/numbers-19.html | title=Notable Properties of Specific Numbers (page 19) at MROB}}
3. ^{{Cite journal |author=H. Kragh |year=2003 |title=Magic Number: A Partial History of the Fine-Structure Constant |journal=Archive for History of Exact Sciences |volume=57 |issue=5 |pages=395 |doi=10.1007/s00407-002-0065-7}}
4. ^Eddington (1939), lecture titled "The Philosophy of Physical Science".
5. ^Eddington (1946)
6. ^{{Cite journal |author1=Tatsumi Aoyama |author2=Masashi Hayakawa |author3=Toichiro Kinoshita |author4=Makiko Nio |year=2012 |title=Tenth-Order QED Contribution to the Electron g-2 and an Improved Value of the Fine Structure Constant |journal=Physical Review Letters |volume=109 |issue=11 |page=111807 |doi=10.1103/PhysRevLett.109.111807 |arxiv = 1205.5368 |bibcode = 2012PhRvL.109k1807A |pmid=23005618}}

Bibliography

  • {{cite book |last=John D. Barrow |edition= |editor= |date=2002 |title=The Constants of Nature from Alpha to Omega: The Numbers That Encode the Deepest Secrets of the Universe |page= |location= |publisher=Pantheon Books |isbn= 978-0-375-42221-8}}
  • {{cite book | author=John D. Barrow & Frank J. Tipler | title=The Anthropic Cosmological Principle | year=1986 | location=London | publisher=Oxford University Press| title-link=Anthropic Principle }}
  • {{cite book | author=Dingle, H. | year=1954 | title=The Sources of Eddington's Philosophy | location=London | publisher=Cambridge University Press }}
  • {{cite book | author=Arthur Eddington | title=The Nature of the Physical World | year=1928 | location=London | publisher=Cambridge University Press }}
  • {{cite book | author=-------- | title=New Pathways in Science | year=1935 | location=London | publisher=Cambridge University Press }}
  • {{cite book | author=-------- | title=The Philosophy of Physical Science | year=1939 | location=London | publisher=Cambridge University Press }}
  • {{cite book | author=-------- | title=Fundamental Theory | year=1946 | location=London | publisher=Cambridge University Press }}
  • {{cite book | author=Kilmister, C.W. & Tupper, B.O.J. | year=1962 | title=Eddington's Statistical Theory | location=London | publisher=Oxford University Press }}
  • {{cite journal |author1=Mohr, P.J. |author2=Taylor, B.N. | title=CODATA recommended values of the fundamental phh | pages=1–107 | doi=10.1103/RevModPhys.77.1 | year=2005 | journal=Reviews of Modern Physics | volume=77 |issue=1 | bibcode=2005RvMP...77....1M|citeseerx=10.1.1.245.4554 }}
  • {{cite book | author=Slater, N.B. | year=1957 | title=Development and Meaning in Eddington's Fundamental Theory | location=London | publisher=Cambridge University Press }}
  • {{cite book | author=Whittaker, E.T. | year=1951 | title=Eddington's Principle in the Philosophy of Science | publisher=Cambridge University Press | location=London }}
  • {{cite book | author=-------- | year=1958 | title=From Euclid to Eddington | publisher=Dover | location=New York }}

3 : Numerology|Astrophysics|Physical cosmology

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