Dimensionless physical constant

Short description: Physical constant with no units

In physics, a dimensionless physical constant is a physical constant that is dimensionless, i.e. a pure number having no units attached and having a numerical value that is independent of whatever system of units may be used.[1]

The concept should not be confused with dimensionless numbers, that are not universally constant, and remain constant only for a particular phenomenon. In aerodynamics for example, if one considers one particular airfoil, the Reynolds number value of the laminar–turbulent transition is one relevant dimensionless number of the problem. However, it is strictly related to the particular problem: for example, it is related to the airfoil being considered and also to the type of fluid in which it moves.

The term fundamental physical constant is sometimes used to refer to some universal dimensionless constants. Perhaps the best-known example is the fine-structure constant, α, which has an approximate value of ​1⁄137.036.[2]

## Contents

* 1 Terminology
* 2 Characteristics
* 3 History
* 4 Examples
* 4.1 Fine-structure constant
* 4.2 Standard model
* 4.3 Cosmological constants
* 4.4 Barrow and Tipler
* 4.5 Martin Rees's Six Numbers
* 5 Relationships between Standard Model constants
* 6 See also
* 7 References
* 8 Bibliography
* 9 External articles

## Terminology

It has been argued the term fundamental physical constant should be restricted to the dimensionless universal physical constants that currently cannot be derived from any other source;[3][4][5][6][7] this stricter definition is followed here.

However, the term fundamental physical constant has also been used occasionally to refer to certain universal dimensioned physical constants, such as the speed of light c, vacuum permittivity ε0, Planck constant h, and the gravitational constant G, that appear in the most basic theories of physics.[8][9][10][11] NIST[8] and CODATA[12] sometimes used the term in this less strict manner.

## Characteristics

There is no exhaustive list of such constants but it does make sense to ask about the minimal number of fundamental constants necessary to determine a given physical theory. Thus, the Standard Model requires 25 physical constants, about half of them are the masses of fundamental particles (which become "dimensionless" when expressed relative to the Planck mass or, alternatively, as coupling strength with the Higgs field along with the gravitational constant).[13]

Fundamental physical constants cannot be derived and have to be measured. Developments in physics may lead to either a reduction or an extension of their number: discovery of new particles, or new relationships between physical phenomena, would introduce new constants, while the development of a more fundamental theory might allow the derivation of several constants from a more fundamental constant.

A long-sought goal of theoretical physics is to find first principles (theory of everything) from which all of the fundamental dimensionless constants can be calculated and compared to the measured values.

The large number of fundamental constants required in the Standard Model has been regarded as unsatisfactory since the theory's formulation in the 1970s. The desire for a theory that would allow the calculation of particle masses is a core motivation for the search for "Physics beyond the Standard Model".

## History

In the 1920s and 1930s, Arthur Eddington embarked upon extensive mathematical investigation into the relations between the fundamental quantities in basic physical theories, later used as part of his effort to construct an overarching theory unifying quantum mechanics and cosmological physics. For example, he speculated on the potential consequences of the ratio of the electron radius to its mass. Most notably, in a 1929 paper he set out an argument based on the Pauli exclusion principle and the Dirac equation that fixed the value of the reciprocal of the fine-structure constant as 𝛼−1 = 16 + ​1⁄2 × 16 × (16 − 1) = 136. When its value was discovered to be closer to 137, he changed his argument to match that value. His ideas were not widely accepted, and subsequent experiments have shown that they were wrong (for example, none of the measurements of the fine-structure constant suggest an integer value; in 2018 it was measured at α = 1/137.035999046(27)).[14]

Though his derivations and equations were unfounded, Eddington was the first physicist to recognize the significance of universal dimensionless constants, now considered among the most critical components of major physical theories such as the Standard Model and ΛCDM cosmology.[15] He was also the first to argue for the importance of the cosmological constant Λ itself, considering it vital for explaining the expansion of the universe, at a time when most physicists (including its discoverer, Albert Einstein) considered it an outright mistake or mathematical artifact and assumed a value of zero: this at least proved prescient, and a significant positive Λ features prominently in ΛCDM.

Eddington may have been the first to attempt in vain to derive the basic dimensionless constants from fundamental theories and equations, but he was certainly not the last. Many others would subsequently undertake similar endeavors, and efforts occasionally continue even today. None have yet produced convincing results or gained wide acceptance among theoretical physicists.[16][17]

An empirical relation between the masses of the electron, muon and tau has been discovered by physicist Yoshio Koide, but this formula remains unexplained.[18]

## Examples

Dimensionless fundamental physical constants include:

* α, the fine-structure constant, the coupling constant for the electromagnetic interaction (≈ ​1⁄137). Also the square of the electron charge, expressed in Planck units, which defines the scale of charge of elementary particles with charge.
* μ or β, the proton-to-electron mass ratio, the rest mass of the proton divided by that of the electron (≈1836). More generally, the ratio of the rest masses of any pair of elementary particles.
* αs, the coupling constant for the strong force (≈ 1)

### Fine-structure constant

One of the dimensionless fundamental constants is the fine-structure constant:

α=e24πε0 ℏc=e22ε0hc≈1137.035999084(21),

where e is the elementary charge, ħ is the reduced Planck constant, c is the speed of light in vacuum, and ε0 is the permittivity of free space. The fine-structure constant is fixed to the strength of the electromagnetic force. At low energies, α ≈ ​1⁄137, whereas at the scale of the Z boson, about 90 GeV, one measures α ≈ ​1⁄127. There is no accepted theory explaining the value of α; Richard Feynman elaborates:

> There is a most profound and beautiful question associated with the observed coupling constant, e - the amplitude for a real electron to emit or absorb a real photon. It is a simple number that has been experimentally determined to be close to 0.08542455. (My physicist friends won't recognize this number, because they like to remember it as the inverse of its square: about 137.03597 with about an uncertainty of about 2 in the last decimal place. It has been a mystery ever since it was discovered more than fifty years ago, and all good theoretical physicists put this number up on their wall and worry about it.) Immediately you would like to know where this number for a coupling comes from: is it related to pi or perhaps to the base of natural logarithms? Nobody knows. It's one of the greatest damn mysteries of physics: a magic number that comes to us with no understanding by man. You might say the "hand of God" wrote that number, and "we don't know how He pushed his pencil." We know what kind of a dance to do experimentally to measure this number very accurately, but we don't know what kind of dance to do on the computer to make this number come out, without putting it in secretly!

> -- Richard P. Feynman (1985). QED: The Strange Theory of Light and Matter. Princeton University Press. p. 129. ISBN 978-0-691-08388-9.

### Standard model

The original standard model of particle physics from the 1970s contained 19 fundamental dimensionless constants describing the masses of the particles and the strengths of the electroweak and strong forces. In the 1990s, neutrinos were discovered to have nonzero mass, and a quantity called the vacuum angle was found to be indistinguishable from zero.[citation needed]

The complete standard model requires 25 fundamental dimensionless constants (Baez, 2011). At present, their numerical values are not understood in terms of any widely accepted theory and are determined only from measurement. These 25 constants are:

* the fine structure constant;
* the strong coupling constant;
* fifteen masses of the fundamental particles (relative to the Planck mass mP = 1.22089(6)×1019 GeV/c2), namely:
* six quarks
* six leptons
* the Higgs boson
* the W boson
* the Z boson
* four parameters of the CKM matrix, describing how quarks oscillate between different forms;
* four parameters of the Pontecorvo–Maki–Nakagawa–Sakata matrix, which does the same thing for neutrinos.

Dimensionless constants of the Standard Model

Symbol  | Description  | Dimensionless value  | Alternative value representation
mu / mP | Up quark mass | 1.4×10−22 – 2.7×10−22 | 1.7–3.3 MeV/c2
md / mP | Down quark mass | 3.4×10−22 – 4.8×10−22 | 4.1–5.8 MeV/c2
mc / mP | Charm quark mass | 1.04431+0.0204768
−0.0286675×10−19 | 1.275+0.025
−0.035 GeV/c2
ms / mP | Strange quark mass | 8.27×10−21 | 95+9
−3 MeV/c2
mt / mP | Top quark mass | (1.415±0.00245721)×10−17 | 172.76±0.3 GeV/c2
mb / mP | Bottom quark mass | 3.43×10−19 | 4.19 GeV/c2
θ12,CKM | CKM 12-mixing angle | 0.22759±0.000873 | 13.04°±0.05°
θ23,CKM | CKM 23-mixing angle | 0.04154±0.00105 | 2.38°±0.06°
θ13,CKM | CKM 13-mixing angle | 0.003508±0.000192 | 0.201°±0.011°
δ13,CKM | CKM CP-violating Phase  | 1.201±0.0785 | 68.8°±4.5°
me / mP | electron mass  | 4.18546×10−23 | 511 keV/c2
mνe / mP | electron neutrino mass  | below 9.00978×10−30 | below 0.11 eV/c2
mμ / mP | Muon mass  | 8.65418×10−21 | 105.7 MeV/c2
mνμ / mP | muon neutrino mass  | below 1.6×10−28 | below 2 eV/c2
mτ / mP | tau mass  | 1.45535×10−19 | 1.78 GeV/c2
mντ / mP | tau neutrino mass  | below 1.6×10−28 | below 2 eV/c2
θ12,PMNS | PMNS 12-mixing angle | 0.58364±0.0122 | 33.44°+0.77°
−0.74°
θ23,PMNS | PMNS 23-mixing angle | 0.8587+0.0175
−0.0227 | 49.2°+1.0°
−1.3°
θ13,PMNS | PMNS 13-mixing angle | 0.1496+0.00227
−0.00209 | 8.57°+0.13°
−0.12°
δCp,PMNS | PMNS CP-violating Phase  | 2.95 ≤ δ ≤ 4.294  | 169° ≤ δ ≤ 246°
α | fine-structure constant | 0.00729735  | 1/137.036
αs | strong coupling constant | ≈1  | ≈1
mW± / mP | W boson mass  | (6.5841±0.0012)×10−18 | 80.385±0.015 GeV/c2
mZ0 / mP | Z boson mass  | (7.46888±0.00016)×10−18 | 91.1876±0.002 GeV/c2
mH / mP | Higgs boson mass  | ≈1.02×10−17 | 125.09±0.24 GeV/c2

### Cosmological constants

The cosmological constant, which can be thought of as the density of dark energy in the universe, is a fundamental constant in physical cosmology that has a dimensionless value of approximately 10−122.[19] Other dimensionless constants are the measure of homogeneity in the universe, denoted by Q, which is explained below by Martin Rees, the baryon mass per photon, the cold dark matter mass per photon and the neutrino mass per photon.[20]

### Barrow and Tipler

Barrow and Tipler (1986) anchor their broad-ranging discussion of astrophysics, cosmology, quantum physics, teleology, and the anthropic principle in the fine-structure constant, the proton-to-electron mass ratio (which they, along with Barrow (2002), call β), and the coupling constants for the strong force and gravitation.

### Martin Rees's Six Numbers

Martin Rees, in his book Just Six Numbers,[21] mulls over the following six dimensionless constants, whose values he deems fundamental to present-day physical theory and the known structure of the universe:

* N ≈ 1036: the ratio of the electrostatic and the gravitational forces between two protons. This ratio is denoted α/αG in Barrow and Tipler (1986). N governs the relative importance of gravity and electrostatic attraction/repulsion in explaining the properties of baryonic matter;[22]
* ε ≈ 0.007: The fraction of the mass of four protons that is released as energy when fused into a helium nucleus. ε governs the energy output of stars, and is determined by the coupling constant for the strong force;[23]
* Ω ≈ 0.3: the ratio of the actual density of the universe to the critical (minimum) density required for the universe to eventually collapse under its gravity. Ω determines the ultimate fate of the universe. If Ω ≥ 1, the universe may experience a Big Crunch. If Ω < 1, the universe may expand forever;[22]
* λ ≈ 0.7: The ratio of the energy density of the universe, due to the cosmological constant, to the critical density of the universe. Others denote this ratio by ΩΛ;[24]
* Q ≈ 10−5: The energy required to break up and disperse an instance of the largest known structures in the universe, namely a galactic cluster or supercluster, expressed as a fraction of the energy equivalent to the rest mass m of that structure, namely mc2;[25]
* D = 3: the number of macroscopic spatial dimensions.

N and ε govern the fundamental interactions of physics. The other constants (D excepted) govern the size, age, and expansion of the universe. These five constants must be estimated empirically. D, on the other hand, is necessarily a nonzero natural number and does not have an uncertainty. Hence most physicists would not deem it a dimensionless physical constant of the sort discussed in this entry.

Any plausible fundamental physical theory must be consistent with these six constants, and must either derive their values from the mathematics of the theory, or accept their values as empirical.

## Relationships between Standard Model constants

Another method to obtain dimensionless parameters is to use a non-fundamental particle with a mass around the GeV scale [26]. This provides a convenient way to derive relationships between parameters for symbolic regression, without sacrificing generality, since dimensional analysis is not affected by this technique. The presence of the mass of rho-meson mass (or any other particle masses used for obtaining dimensionless SM constants) can be considered a handy method for deriving short relationships. The final theory can be free of this constant after a successful variable substitution. In a paper [26] it was proposed to search for relationships between Standard Model parameters using genetic programming. The dimensionless parameters (masses) were obtained by re-scaling the masses of fundamental particles using the rho-meson mass instead of the Planck-scale mass. The latter was found to be too large for effective use in genetic programming. The obtained dimensionless relationships were made public with the goal of using this data for the analysis of patterns or structures that may reveal underlying relationships in high-dimensional functional space using generative artificial intelligence. The method allowed to reproduce known (likely coincidental) relationships, and provided several new relations that have not been observed in the past.

## See also

* Cabibbo–Kobayashi–Maskawa matrix (Cabibbo angle)
* Dimensionless numbers in fluid mechanics
* Dirac large numbers hypothesis
* Neutrino oscillation
* Physical cosmology
* Standard Model
* Weinberg angle
* Fine-tuned universe
* Koide formula

## References

1. ↑ Stroke, H. H., ed., The Physical Review: The First Hundred Years (Berlin/Heidelberg: Springer, 1995), p. 525.
2. ↑ Vértes, A., Nagy, S., Klencsár, Z., Lovas, R. G., & Rösch, F., eds., Handbook of Nuclear Chemistry, (Berlin/Heidelberg: Springer, 2011), p. 367.
3. ↑ Baez, John (2011-04-22). "How Many Fundamental Constants Are There?". http://math.ucr.edu/home/baez/constants.html.
4. ↑ Rich, James (2013-04-02). "Dimensionless constants and cosmological measurements". arXiv:1304.0577 [astro-ph.CO].
5. ↑ Michael Duff (2014). "How fundamental are fundamental constants?". Contemporary Physics 56 (1): 35–47. doi:10.1080/00107514.2014.980093. Bibcode: 2015ConPh..56...35D.
6. ↑ Duff, M. J. (13 August 2002). "Comment on time-variation of fundamental constants". arXiv:hep-th/0208093.
7. ↑ Duff, M. J.; Okun, L. B.; Veneziano, G. (2002). "Trialogue on the number of fundamental constants". Journal of High Energy Physics 2002 (3): 023. doi:10.1088/1126-6708/2002/03/023. Bibcode: 2002JHEP...03..023D.
8. ↑ 8.0 8.1 "Introduction to the Fundamental Physical Constants". https://physics.nist.gov/cuu/Constants/introduction.html.
9. ↑ http://physics.nist.gov/cuu/Constants/ NIST
10. ↑ "Physical constant" (in en). Encyclopedia Britannica. https://www.britannica.com/science/physical-constant. Retrieved 2018-04-13.
11. ↑ Karshenboim, Savely G. (August 2005). "Fundamental Physical Constants: Looking from Different Angles". Canadian Journal of Physics 83 (8): 767–811. doi:10.1139/p05-047. ISSN 0008-4204. Bibcode: 2005CaJPh..83..767K.
12. ↑ Mohr, Peter J.; Newell, David B.; Taylor, Barry N. (2016-09-26). "CODATA Recommended Values of the Fundamental Physical Constants: 2014". Reviews of Modern Physics 88 (3): 035009. doi:10.1103/RevModPhys.88.035009. ISSN 0034-6861. Bibcode: 2016RvMP...88c5009M.
13. ↑ Kuntz, I., Gravitational Theories Beyond General Relativity, (Berlin/Heidelberg: Springer, 2019), pp. 58–61.
14. ↑ Parker, Richard H.; Yu, Chenghui; Zhong, Weicheng; Estey, Brian; Müller, Holger (2018-04-13). "Measurement of the fine-structure constant as a test of the Standard Model" (in en). Science 360 (6385): 191–195. doi:10.1126/science.aap7706. ISSN 0036-8075. PMID 29650669. Bibcode: 2018Sci...360..191P.
15. ↑ Prialnik, D. K., An Introduction to the Theory of Stellar Structure and Evolution (Cambridge: Cambridge University Press , 2000), p. 82.
16. ↑ Kragh, Helge (2015-10-14). "On Arthur Eddington's Theory of Everything". arXiv:1510.04046 [physics.hist-ph].
17. ↑ Gamow, G. (1968-02-01). "Numerology of the Constants of Nature" (in en). Proceedings of the National Academy of Sciences 59 (2): 313–318. doi:10.1073/pnas.59.2.313. ISSN 0027-8424. PMID 16591598. Bibcode: 1968PNAS...59..313G.
18. ↑ Rivero, A.; Gsponer, A. (February 2, 2008). "The strange formula of Dr. Koide". p. 4\. arXiv:hep-ph/0505220.
19. ↑ Jaffe, R. L., & Taylor, W., The Physics of Energy (Cambridge: Cambridge University Press, 2018), p. 419.
20. ↑ Tegmark, Max (2014). Our Mathematical Universe: My Quest for the Ultimate Nature of Reality. Knopf Doubleday Publishing Group. p. 252. ISBN 9780307599803.
21. ↑ Radford, T., "Just Six Numbers: The Deep Forces that Shape the Universe by Martin Rees—review", The Guardian , June 8, 2012.
22. ↑ 22.0 22.1 Rees, M. (2000), p. .
23. ↑ Rees, M. (2000), p. 53.
24. ↑ Rees, M. (2000), p. 110.
25. ↑ Rees, M. (2000), p. 118.
26. ↑ 26.0 26.1 Chekanov, Sergei V.; Kjellerstrand, Hakan (2025). "Discovering the Underlying Analytic Structure within Standard Model Constants Using Artificial Intelligence". Particles 8 (4): 95. doi:doi.org/10.3390/particles8040095.

## Bibliography

* Martin Rees, 1999. Just Six Numbers: The Deep Forces that Shape the Universe. London: Weidenfeld & Nicolson. ISBN 0-7538-1022-0
* Josef Kuneš, 2012. Dimensionless Physical Quantities in Science and Engineering. Amsterdam: Elsevier. ISBN 978-0-12-416013-2

## External articles

General

* John D. Barrow, 2002. The Constants of Nature; From Alpha to Omega - The Numbers that Encode the Deepest Secrets of the Universe. Pantheon Books. ISBN 0-375-42221-8.
* Barrow, John D.; Tipler, Frank J. (1988). The Anthropic Cosmological Principle. Oxford University Press. ISBN 978-0-19-282147-8.
* Michio Kaku, 1994. Hyperspace: A Scientific Odyssey Through Parallel Universes, Time Warps, and the Tenth Dimension. Oxford University Press.
* Fundamental Physical Constants from NIST
* Values of fundamental constants. CODATA, 2002.
* John Baez, 2002, "How Many Fundamental Constants Are There?"
* Simon Plouffe, 2004, "A search for a mathematical expression for mass ratios using a large database."

Articles on variance of the fundamental constants

* Bahcall, John N.; Steinhardt, Charles L.; Schlegel, David (2004-01-10). "Does the Fine‐Structure Constant Vary with Cosmological Epoch?". The Astrophysical Journal 600 (2): 520–543. doi:10.1086/379971. ISSN 0004-637X. Bibcode: 2004ApJ...600..520B.
* John D. Barrow and Webb, J. K., "Inconstant Constants – Do the inner workings of nature change with time?" Scientific American (June 2005).
* Michael Duff, 2002 "Comment on time-variation of fundamental constants."
* Marion, H.; Pereira Dos Santos, F.; Abgrall, M.; Zhang, S.; Sortais, Y. et al. (2003-04-18). "Search for Variations of Fundamental Constants using Atomic Fountain Clocks". Physical Review Letters 90 (15): 150801. doi:10.1103/physrevlett.90.150801. ISSN 0031-9007. PMID 12732023. Bibcode: 2003PhRvL..90o0801M.
* Martins, C.J.A.P; Melchiorri, A; Rocha, G; Trotta, R; Avelino, P.P; Viana, P.T.P (2004). "WMAP constraints on varying α and the promise of reionization". Physics Letters B 585 (1–2): 29–34. doi:10.1016/j.physletb.2003.11.080. ISSN 0370-2693. Bibcode: 2004PhLB..585...29M.
* Olive, Keith A.; Pospelov, Maxim; Qian, Yong-Zhong; Coc, Alain; Cassé, Michel; Vangioni-Flam, Elisabeth (2002-08-23). "Constraints on the variations of the fundamental couplings". Physical Review D 66 (4): 045022. doi:10.1103/physrevd.66.045022. ISSN 0556-2821. Bibcode: 2002PhRvD..66d5022O.
* Uzan, Jean-Philippe (2003-04-07). "The fundamental constants and their variation: observational and theoretical status". Reviews of Modern Physics 75 (2): 403–455. doi:10.1103/revmodphys.75.403. ISSN 0034-6861. Bibcode: 2003RvMP...75..403U.
* Webb, J. K.; Murphy, M. T.; Flambaum, V. V.; Dzuba, V. A.; Barrow, J. D.; Churchill, C. W.; Prochaska, J. X.; Wolfe, A. M. (2001-08-09). "Further Evidence for Cosmological Evolution of the Fine Structure Constant". Physical Review Letters 87 (9): 091301. doi:10.1103/physrevlett.87.091301. ISSN 0031-9007. PMID 11531558. Bibcode: 2001PhRvL..87i1301W.

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