Eddington–Dirac Number
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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: *The strength of gravity, as represented by the
gravitational constant The gravitational constant (also known as the universal gravitational constant, the Newtonian constant of gravitation, or the Cavendish gravitational constant), denoted by the capital letter , is an empirical physical constant involved in ...
, is inversely proportional to the age of the universe: G \propto 1/t\, *The mass of the universe is proportional to the square of the universe's age: M \propto t^2. *Physical constants are actually not constant. Their values depend on the age of the Universe.


Background

LNH 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 Hermann Klaus Hugo Weyl, (; 9 November 1885 – 8 December 1955) was a German mathematician, theoretical physicist and philosopher. Although much of his working life was spent in Zürich, Switzerland, and then Princeton, New Jersey, he is assoc ...
(1919), who speculated that the observed radius of the universe, ''R''U, might also be the hypothetical radius of a particle whose rest energy is equal to the gravitational self-energy of the electron: :\frac \approx \frac \approx 4.1666763 \cdot 10^ \approx 10^ , where, :r_\text = \frac \approx 3.7612682 \cdot 10^ \mathrm :r_\text = \frac \approx 1,5671987 \cdot 10^ \,\mathrm with m_\text c^2 = \frac and ''r''e is the classical electron radius, ''m''e is the mass of the electron, ''m''H denotes the mass of the hypothetical particle, and ''r''H is its electrostatic radius. The coincidence was further developed by
Arthur Eddington Sir Arthur Stanley Eddington (28 December 1882 – 22 November 1944) was an English astronomer, physicist, and mathematician. He was also a philosopher of science and a populariser of science. The Eddington limit, the natural limit to the lumin ...
(1931) who related the above ratios to N, the estimated number of charged particles in the universe: :\frac \approx 4.1666763 \cdot 10^ \approx \sqrt . 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. 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: :G = \left(\!\frac\!\right)t, where ''M''U is the mass of the universe and ''t'' is the age of the universe. 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: :\frac \approx 3.47 \cdot 10^ \approx 10^, where ''t'' is the age of the universe, c is the speed of light and ''r''e is the classical electron radius. Hence, in units where and , 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
force In physics, a force is an influence that can change the motion of an object. A force can cause an object with mass to change its velocity (e.g. moving from a state of rest), i.e., to accelerate. Force can also be described intuitively as a p ...
s between a
proton A proton is a stable subatomic particle, symbol , H+, or 1H+ with a positive electric charge of +1 ''e'' elementary charge. Its mass is slightly less than that of a neutron and 1,836 times the mass of an electron (the proton–electron mass ...
and an electron: :\frac \approx 10^. Hence, interpreting the charge e of the electron, the masses m_\text and m_\text of the proton and electron, and the permittivity factor 4 \pi \epsilon_0 in atomic units (equal to 1), the value of the
gravitational constant The gravitational constant (also known as the universal gravitational constant, the Newtonian constant of gravitation, or the Cavendish gravitational constant), denoted by the capital letter , is an empirical physical constant involved in ...
is approximately 10−40. Dirac interpreted this to mean that G varies with time as G \approx 1/t. Although George Gamow noted that such a temporal variation does not necessarily follow from Dirac's assumptions, a corresponding change of ''G'' has not been found. 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 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: *'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 when he argued that variations in the strength of gravity are not consistent with paleontological data. However, George Gamow demonstrated in 1962 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 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 argued that LNH is inconsistent with experimental results for microwave background radiation whereas Canuto and Hsieh 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 The characterization of the universe as finely tuned suggests that the occurrence of life in the universe is very sensitive to the values of certain fundamental physical constants and that the observed values are, for some reason, improbable. If ...
or
fine-tuned universe The characterization of the universe as finely tuned suggests that the occurrence of life in the universe is very sensitive to the values of certain fundamental physical constants and that the observed values are, for some reason, improbable. If ...
, it simply states that the large numbers in LNH are a necessary coincidence for intelligent beings since they parametrize fusion of hydrogen in
star A star is an astronomical object comprising a luminous spheroid of plasma (physics), plasma held together by its gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked ...
s 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) noted that the mass ratio for a typical star (specifically, a star of the
Chandrasekhar mass The Chandrasekhar limit () is the maximum mass of a stable white dwarf star. The currently accepted value of the Chandrasekhar limit is about (). White dwarfs resist gravitational collapse primarily through electron degeneracy pressure, compare ...
, itself a constant of nature, approx. 1.44 solar masses) and an electron approximates to 1060, an interesting variation on the 1040 and 1080 that are typically associated with Dirac and Eddington respectively. (The physics defining the Chandrasekhar mass produces a ratio that is the −3/2 power of the gravitational fine-structure constant, 10−40.)


Modern studies

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) and Matthews (1997) 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
bit The bit is the most basic unit of information in computing and digital communications. The name is a portmanteau of binary digit. The bit represents a logical state with one of two possible values. These values are most commonly represented a ...
s of information in the universe. Valev (2019) found equation connecting cosmological parameters (for example density of the universe) and Planck units (for example Planck density). This ratio of densities, and other ratios (using four fundamental constants: speed of light in vacuum c, Newtonian constant of gravity G, reduced Planck constant ℏ, and Hubble constant H) computes to an exact number, . This provides evidence of the Dirac large numbers hypothesis by connecting the macro-world and the micro-world.


See also

* Dimensionless physical constant * Naturalness (physics) *
Time-variation of fundamental constants The term physical constant expresses the notion of a physical quantity subject to experimental measurement which is independent of the time or location of the experiment. The constancy (immutability) of any "physical constant" is thus subject to exp ...


References


Further reading

* * * * * * *


External links


Audio of Dirac talking about the large numbers hypothesis
{{DEFAULTSORT:Dirac Large Numbers Hypothesis Physical cosmology Obsolete scientific theories Large Numbers Hypothesis Astronomical hypotheses 1937 introductions Coincidence