 Dirac large numbers hypothesis

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 equivalence of these ratios might not be a mere coincidence but instead could imply a cosmology with these unusual features:
 The strength of gravity, as represented by the gravitational constant, is inversely proportional to the age of the universe: ;
 The mass of the universe is proportional to the square of the universe's age: .
Neither of these two features has gained acceptance in mainstream physics and, though some proponents of nonstandard cosmologies refer to Dirac's cosmology as a foundational basis for their own ideas and studies, some physicists harshly dismiss the large numbers in LNH as mere coincidences more suited to numerology than physics. A coincidence, however, may be defined optimally as 'an event that provides support for an alternative to a currently favoured causal theory, but not necessarily enough support to accept that alternative in light of its low prior probability.'^{[1]} Research into LNH, or the large number of coincidences that underpin it, appears to have gained new impetus from failures in standard cosmology to account for anomalies such as the recent discovery that the universe might be expanding at an accelerated rate.^{[2]}
Contents
Background
LNH was Dirac's personal response to a set of large number 'coincidences' that had intrigued other theorists at about the same time. The 'coincidences' began with Hermann Weyl (1919),^{[2]}^{[3]}^{[4]} who speculated that the observed radius of the universe might also be the hypothetical radius of a particle whose energy is equal to the gravitational selfenergy of the electron:
where r_{e} is the classical electron radius, m_{e} is the mass of the electron, m_{H} denotes the mass of the hypothetical particle, r_{H} is its electrostatic radius and R_{U} is the radius of the observable universe.
The coincidence was further developed by Arthur Eddington (1931) ^{[5]} 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 influenced also by the primevalatom hypothesis of Georges Lemaitre, who lectured on the topic in Cambridge in 1933.^{[2]} The notion of a varyingG 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.^{[6]}^{[7]} For Milne, space was not a structured object but simply a system of reference in which Einstein's conclusions could be accommodated by relations such as this:
where M_{U} 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 coincidences
The 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, c is the speed of light and r_{e} is the classical electron radius. Hence, in atomic units where c=1 and r_{e} = 1, the age of the Universe is about 10^{40} atomic 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 e of the electron, the mass m_{p}/m_{e} of the proton/electron, and the permittivity factor 4πε_{0} in atomic units (equal to 1), the value of the gravitational constant is approximately 10^{−40}. Dirac interpreted this to mean that G varies with time as , and thereby pointed to a cosmology that seems 'designermade' for a theory of quantum gravity. 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 equations a gauge function 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:^{[2]}
 'additive' creation (new matter is created uniformly throughout space) and
 'multiplicative' creation (new matter is created where there are already concentrations of mass).
Later developments and interpretations
Dirac'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 finetuned 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 carbonbased 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 10^{60}, an interesting variation on the 10^{40} and 10^{80} that are typically associated with Dirac and Eddington respectively. Various numbers of the order of 10^{60} were arrived at by V. E. ShemiZadah (2002) ^{[15]} through measuring cosmological entities in Planck units. P. Zizzi (1998) argued that there might be a modern mathematical interpretation of LNH in a Planckscale setting in the context of quantum foam.^{[16]} The relevance of the Planck scale to LNH was further demonstrated by S. Caneiro and G. Marugan (2002)^{[17]} by reference to the holographic principle. Previously, Carneiro (1997)^{[18]} arrived at an intermediate scaling factor 10^{20} when considering the possible quantization of cosmic structures and a rescaling of Planck's constant.
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)^{[19]} and Matthews (1997)^{[20]} associated in an LNH context with a scaling law for the cosmological constant. Carl Friedrich von Weizsaecker identified 10^{120} 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.^{[21]} T. Goernitz (1986), building on Weizsaecker's work, posited an explanation for large number 'coincidences' in the context of Bekenstein–Hawking entropy.^{[22]} Genreith (1999)^{[23]} has sketched out a fractal cosmology in which the smallest mass, which he identified as a neutrino, is about 120 orders of magnitude smaller than the mass of the universe (note: this 'neutrino' approximates in scale to the hypothetical particle m_{H} mentioned above in the context of Weyl's work in 1919). Sidharth (2005)^{[24]} interpreted a typical electromagnetic particle such as the pion as a collection of 10^{40} Planck oscillators and the universe as a collection of 10^{120} Planck oscillators. The fact that a number like 10^{120} can be represented in a variety of ways has been interpreted by Funkhouser (2006)^{[25]} as a new large numbers coincidence. Funkhouser claimed to have 'resolved' the LNH coincidences without departing from the standard model for cosmology. In a similar vein, Carneiro and Marugan (2002) claimed that the scaling relations in LNH can be explained entirely according to basic principles.^{[17]}
References
 ^ T.L. Griffiths, J.B. Tenenbaum (2007). "From mere coincidences to meaningful discoveries". Cognition 103 (2): 180–226. doi:10.1016/j.cognition.2006.03.004. PMID 16678145.
 ^ ^{a} ^{b} ^{c} ^{d} S. Ray, U. Mukhopadhyay, P.P. Ghosh (2007). "Large Number Hypothesis: A Review". arXiv:0705.1836 [grqc].
 ^ H. Weyl (1917). Annals of Physics 54: 117.
 ^ H. Weyl (1919). Annals of Physics 59: 101.
 ^ A. Eddington (1931). Proceedings of the Cambridge Philosophical Society 27.
 ^ E.A. Milne (1935). Relativity, Gravity and World Structure. Oxford University Press.
 ^ H. Kragh (1996). Cosmology and Controversy: The historical development of two theories of the universe. Princeton University Press. pp. 61–62.
 ^ E. Teller (1948). "On the change of physical constants". Physical Review 73 (7): 801–802. Bibcode 1948PhRv...73..801T. doi:10.1103/PhysRev.73.801.
 ^ G.Gamow (1962). Gravity. Doubleday. pp. 138–141.
 ^ G. Blake (1978). "The Large Numbers Hypothesis and the rotation of the Earth". Monthly Notices of the Royal Astronomical Society 185: 399. Bibcode 1978MNRAS.185..399B.
 ^ D. Falik (1979). "Primordial Nucleosynthesis and Dirac's Large Numbers Hypothesis". Astrophysical Journal 231: L1. Bibcode 1979ApJ...231L...1F. doi:10.1086/182993.
 ^ V. Canuto, S. Hsieh (1978). Astrophysical Journal 224.
 ^ V. Canuto, S. Hsieh (1980). Astrophysical Journal 239.
 ^ P. Jordan (1947). Die Herkunft der Sterne.
 ^ V. E. ShemiZadah (2002). "Coincidence of Large Numbers, exact value of cosmological parameters and their analytical representation". arXiv:grqc/0206084 [grqc].
 ^ P. Zizzi (1998). "Quantum Foam and de Sitterlike Universes". Int.J.Theor.Phys. 38: 2333–2348. arXiv:hepth/9808180. Bibcode 1999IJTP...38.2333Z.
 ^ ^{a} ^{b} S. Carneiro, G. Marugan (2001). "Holography and the large number hypothesis". Physical Review D 65 (8). arXiv:grqc/0111034. Bibcode 2002PhRvD..65h7303M. doi:10.1103/PhysRevD.65.087303.
 ^ S. Carneiro (1997). "The Large Numbers Hypothesis and Quantum Mechanics". Foundations of Physics Letters 11 (95): 95. arXiv:grqc/9712014. Bibcode 1998FoPhL..11...95C. doi:10.1023/A:1022411021285.
 ^ L. Nottale. "Mach's Principle, Dirac's Large Numbers and the Cosmological Constant Problem". http://luth2.obspm.fr/~luthier/nottale/arlambda.pdf.
 ^ R. Matthews. "Robert Matthews: Dirac's coincidences sixty years on". http://ourworld.compuserve.com/homepages/rajm/agdirac.htm.
 ^ H. Lyre (2003). "C. F. Weizsaecker's Reconstruction of Physics: Yesterday, Today and Tomorrow". arXiv:quantph/0309183 [quantph].
 ^ T. Gornitz (1986). "New Look at the Large Numbers". International Journal of Theoretical Physics 25 (8).
 ^ H. Genreith (1999). "The Large Numbers Hypothesis: Outline of a selfsimilar quantum cosmological Model". arXiv:grqc/9909009 [grqc].
 ^ B. Sidharth (2005). "The Planck Scale Underpinning for Spacetime". arXiv:physics/0509026 [physics.genph].
 ^ S. Funkhouser (2006). "A New Large Number Coincidence and a Scaling Law for the Cosmological Constant". Proc. R. Soc. A 464: 1345–1353. arXiv:physics/0611115. Bibcode 2008RSPSA.464.1345F. doi:10.1098/rspa.2007.0370.
 P.A.M. Dirac (1938). "A New Basis for Cosmology". Proceedings of the Royal Society of London A 165 (921): 199–208. Bibcode 1938RSPSA.165..199D. doi:10.1098/rspa.1938.0053.
 P.A.M. Dirac (1937). "The Cosmological Constants". Nature 139 (3512): 323. Bibcode 1937Natur.139..323D. doi:10.1038/139323a0.
 P.A.M. Dirac (1974). "Cosmological Models and the Large Numbers Hypothesis". Proceedings of the Royal Society of London A 338 (1615): 439–446. Bibcode 1974RSPSA.338..439D. doi:10.1098/rspa.1974.0095.
External links
 Audio of Dirac talking about the large numbers hypothesis
 Full transcript of Dirac's speech.
 ChengGang Shao, Jianyong Shen, Bin Wang: Dirac Cosmology and the Acceleration of the Contemporary Universe
 Saibal Ray, Utpal Mukhopadhyay, Partha Pratim Ghosh: Large Number Hypothesis: A Review
 grqc/0111034 Guillermo A. Mena Marugan, Saulo Carneiro: Holography and the large number hypothesis
 Robert Matthews: Dirac's coincidences sixty years on
 The Mysterious Eddington–Dirac Number
 A. Unzicker: A Look at the Abandoned Contributions to Cosmology of Dirac, Sciama and Dicke (arxiv:0708.3518)
Notes
Categories: Physical cosmology
 Obsolete scientific theories
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