词条 | Dirac large numbers hypothesis |
释义 |
The Dirac large numbers hypothesis (LNH) is an observation made by Paul Dirac in 1937 relating ratios of size scales in the Universe to that of force scales. The ratios constitute very large, dimensionless numbers: some 40 orders of magnitude in the present cosmological epoch. According to Dirac's hypothesis, the apparent similarity of these ratios might not be a mere coincidence but instead could imply a cosmology with these unusual features:
Neither of these two features has gained wide acceptance in mainstream physics. BackgroundLNH was Dirac's personal response to a set of large number 'coincidences' that had intrigued other theorists of his time. The 'coincidences' began with Hermann Weyl (1919),[1][2] who speculated that the observed radius of the universe, RU, might also be the hypothetical radius of a particle whose rest energy is equal to the gravitational self-energy of the electron: where re is the classical electron radius, me is the mass of the electron, mH denotes the mass of the hypothetical particle, and rH is its electrostatic radius. The coincidence was further developed by Arthur Eddington (1931)[3] who related the above ratios to N, the estimated number of charged particles in the universe: In addition to the examples of Weyl and Eddington, Dirac was also influenced by the primeval-atom hypothesis of Georges Lemaître, who lectured on the topic in Cambridge in 1933. The notion of a varying-G cosmology first appears in the work of Edward Arthur Milne a few years before Dirac formulated LNH. Milne was inspired not by large number coincidences but by a dislike of Einstein's general theory of relativity.[4][5] For Milne, space was not a structured object but simply a system of reference in which relations such as this could accommodate Einstein's conclusions: where MU is the mass of the universe and t is the age of the universe in seconds. According to this relation, G increases over time. Dirac's interpretation of the large number coincidencesThe Weyl and Eddington ratios above can be rephrased in a variety of ways, as for instance in the context of time: where t is the age of the universe, is the speed of light and re is the classical electron radius. Hence, in units where {{nowrap|1=c = 1}} and {{nowrap|1=re = 1}}, the age of the universe is about 1040 units of time. This is the same order of magnitude as the ratio of the electrical to the gravitational forces between a proton and an electron: Hence, interpreting the charge of the electron, the masses and of the proton and electron, and the permittivity factor in atomic units (equal to 1), the value of the gravitational constant is approximately 10−40. Dirac interpreted this to mean that varies with time as . Although George Gamow noted that such a temporal variation does not necessarily follow from Dirac's assumptions,[6] a corresponding change of G has not been found.[7] According to general relativity, however, G is constant, otherwise the law of conserved energy is violated. Dirac met this difficulty by introducing into the Einstein field equations a gauge function {{lang|grc|β}} that describes the structure of spacetime in terms of a ratio of gravitational and electromagnetic units. He also provided alternative scenarios for the continuous creation of matter, one of the other significant issues in LNH:
Later developments and interpretationsDirac's theory has inspired and continues to inspire a significant body of scientific literature in a variety of disciplines. In the context of geophysics, for instance, Edward Teller seemed to raise a serious objection to LNH in 1948[8] when he argued that variations in the strength of gravity are not consistent with paleontological data. However, George Gamow demonstrated in 1962[9] how a simple revision of the parameters (in this case, the age of the Solar System) can invalidate Teller's conclusions. The debate is further complicated by the choice of LNH cosmologies: In 1978, G. Blake[10] argued that paleontological data is consistent with the 'multiplicative' scenario but not the 'additive' scenario. Arguments both for and against LNH are also made from astrophysical considerations. For example, D. Falik[11] argued that LNH is inconsistent with experimental results for microwave background radiation whereas Canuto and Hsieh[12][13] argued that it is consistent. One argument that has created significant controversy was put forward by Robert Dicke in 1961. Known as the anthropic coincidence or fine-tuned universe, it simply states that the large numbers in LNH are a necessary coincidence for intelligent beings since they parametrize fusion of hydrogen in stars and hence carbon-based life would not arise otherwise. Various authors have introduced new sets of numbers into the original 'coincidence' considered by Dirac and his contemporaries, thus broadening or even departing from Dirac's own conclusions. Jordan (1947)[14] noted that the mass ratio for a typical star and an electron approximates to 1060, an interesting variation on the 1040 and 1080 that are typically associated with Dirac and Eddington respectively. Several authors have recently identified and pondered the significance of yet another large number, approximately 120 orders of magnitude. This is for example the ratio of the theoretical and observational estimates of the energy density of the vacuum, which Nottale (1993)[15] and Matthews (1997)[16] associated in an LNH context with a scaling law for the cosmological constant. Carl Friedrich von Weizsäcker identified 10120 with the ratio of the universe's volume to the volume of a typical nucleon bounded by its Compton wavelength, and he identified this ratio with the sum of elementary events or bits of information in the universe.[17] See also{{Portal|Physics|Cosmology}}
References1. ^{{cite journal |author=H. Weyl |year=1917 |title=Zur Gravitationstheorie |journal=Annalen der Physik |volume=359 |issue=18 |pages=117–145 |bibcode=1917AnP...359..117W |doi=10.1002/andp.19173591804}} 2. ^{{cite journal |author=H. Weyl |year=1919 |title=Eine neue Erweiterung der Relativitätstheorie |journal=Annalen der Physik |volume=364 |issue=10 |pages=101–133 |bibcode=1919AnP...364..101W |doi=10.1002/andp.19193641002}} 3. ^{{cite journal |author=A. Eddington |year=1931 |title=Preliminary Note on the Masses of the Electron, the Proton, and the Universe |journal=Proceedings of the Cambridge Philosophical Society |volume=27 |issue= 1|pages=15 |bibcode=1931PCPS...27...15E |doi=10.1017/S0305004100009269}} 4. ^{{cite book |author=E. A. Milne |year=1935 |title=Relativity, Gravity and World Structure |publisher=Oxford University Press}} 5. ^{{cite book |author=H. Kragh |year=1996 |title=Cosmology and Controversy: The historical development of two theories of the universe |pages=61–62 |publisher=Princeton University Press |isbn=978-0-691-02623-7}} 6. ^{{cite book |author=H. Kragh |year=1990 |title=Dirac: A Scientific Biography |publisher=Cambridge University Press |page=177 |isbn=978-0-521-38089-8}} 7. ^{{cite journal |author=J. P.Uzan |year=2003 |title=The fundamental constants and their variation, Observational status and theoretical motivations |journal=Reviews of Modern Physics |volume=75 |issue=2 |page=403 |arxiv=hep-ph/0205340 |bibcode=2003RvMP...75..403U |doi=10.1103/RevModPhys.75.403}} 8. ^{{cite journal |author=E. Teller |year=1948 |title=On the change of physical constants |journal=Physical Review |volume=73 |issue=7 |pages=801–802 |bibcode=1948PhRv...73..801T |doi=10.1103/PhysRev.73.801}} 9. ^{{cite book |author=G. Gamow |year=1962 |title=Gravity |pages=138–141 |publisher=Doubleday |lccn=62008840}} 10. ^{{cite journal |author=G. Blake |year=1978 |title=The Large Numbers Hypothesis and the rotation of the Earth |journal=Monthly Notices of the Royal Astronomical Society |volume=185 |issue=2 |pages=399–408 |bibcode=1978MNRAS.185..399B |doi=10.1093/mnras/185.2.399}} 11. ^{{cite journal |author=D. Falik |year=1979 |title=Primordial Nucleosynthesis and Dirac's Large Numbers Hypothesis |journal=The Astrophysical Journal |volume=231 |page=L1 |bibcode=1979ApJ...231L...1F |doi=10.1086/182993}} 12. ^{{cite journal |author=V. Canuto, S. Hsieh |year=1978 |title=The 3 K blackbody radiation, Dirac's Large Numbers Hypothesis, and scale-covariant cosmology |journal=The Astrophysical Journal |volume=224 |pages=302 |bibcode=1978ApJ...224..302C |doi=10.1086/156378}} 13. ^{{cite journal |author=V. Canuto, S. Hsieh |year=1980 |title=Primordial nucleosynthesis and Dirac's large numbers hypothesis |journal=The Astrophysical Journal |volume=239 |pages=L91 |bibcode=1980ApJ...239L..91C |doi=10.1086/183299}} 14. ^{{Cite journal |author=P. Jordan |year=1947 |title=Die Herkunft der Sterne |journal=Astronomische Nachrichten |volume=275 |issue=10–12 |pages=191 |bibcode=1947dhds.book.....J|doi=10.1002/asna.19472751012}} 15. ^{{cite web |author=L. Nottale |title=Mach's Principle, Dirac's Large Numbers and the Cosmological Constant Problem |url=http://luth2.obspm.fr/~luthier/nottale/arlambda.pdf}} 16. ^{{cite journal |author=R. Matthews |title=Dirac's coincidences sixty years on |url=http://astrogeo.oxfordjournals.org/content/39/6/6.19.full.pdf |journal=Astronomy & Geophysics |year=1998 |volume=39 |issue=6|pages=19–20 |bibcode= |doi=10.1093/astrog/39.6.6.19}} 17. ^{{cite arXiv |author=H. Lyre |year=2003 |title=C. F. Weizsäcker's Reconstruction of Physics: Yesterday, Today and Tomorrow |eprint=quant-ph/0309183}} Further reading
|author=P. A. M. Dirac |year=1938 |title=A New Basis for Cosmology |journal=Proceedings of the Royal Society of London A |volume=165 |issue=921 |pages=199–208 |bibcode=1938RSPSA.165..199D |doi=10.1098/rspa.1938.0053 }}
|author=P. A. M. Dirac |year=1937 |title=The Cosmological Constants |journal=Nature |volume=139 |issue=3512 |pages=323 |bibcode=1937Natur.139..323D |doi=10.1038/139323a0 }}
|author=P. A. M. Dirac |year=1974 |title=Cosmological Models and the Large Numbers Hypothesis |journal=Proceedings of the Royal Society of London A |volume=338 |issue=1615 |pages=439–446 |bibcode=1974RSPSA.338..439D |doi=10.1098/rspa.1974.0095 }}
|author1=G. A. Mena Marugan |author2=S. Carneiro |year=2002 |title=Holography and the large number hypothesis |journal=Physical Review D |volume=65 |issue=8 |page=087303 |arxiv=gr-qc/0111034 |bibcode=2002PhRvD..65h7303M |doi=10.1103/PhysRevD.65.087303 }}
|author1=C.-G. Shao |author2=J. Shen |author3=B. Wang |author4=R.-K. Su |title=Dirac Cosmology and the Acceleration of the Contemporary Universe |year=2006 |journal=Classical and Quantum Gravity |volume=23 |issue=11 |pages=3707–3720 |arxiv=gr-qc/0508030 |bibcode=2006CQGra..23.3707S |doi=10.1088/0264-9381/23/11/003 }}
|author1=S. Ray |author2=U. Mukhopadhyay |author3=P. P. Ghosh |year=2007 |title=Large Number Hypothesis: A Review |class=gr-qc |eprint=0705.1836 }}
|author1=A. Unzicker |year=2009 |title=A Look at the Abandoned Contributions to Cosmology of Dirac, Sciama and Dicke |journal=Annalen der Physik |volume=18 |issue=1 |pages=57–70 |arxiv=0708.3518 |bibcode=2009AnP...521...57U |doi=10.1002/andp.200810335 }} External links
5 : Physical cosmology|Obsolete scientific theories|Paul Dirac|Astronomical hypotheses|1937 introductions |
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