Stoney units

Last updated

In physics, the Stoney units form a system of units named after the Irish physicist George Johnstone Stoney, who first proposed them in 1881. They are the earliest example of natural units, i.e., a coherent set of units of measurement designed so that chosen physical constants fully define and are included in the set.

Contents

Units

QuantityExpressionValue in SI units
Length (L)1.3807×10−36 m
Mass (M)1.8592×10−9 kg
Time (T)4.6054×10−45 s
Electric charge (Q)1.6022×10−19 C

The constants that Stoney used to define his set of units is the following: [1] [2]

Later authors typically replace the Coulomb constant with 1/4πε0. [3] [4]

This means that the numerical values of all these constants, when expressed in coherent Stoney units, is equal to one:

In Stoney units, the numerical value of the reduced Planck constant is

where α is the fine-structure constant.

History

George Stoney was one of the first scientists to understand that electric charge was quantized; from this quantization and three other constants that he perceived as being universal (a speed from electromagnetism, and the coefficients in the electrostatic and gravitational force equations) he derived the units that are now named after him. [5] [6] Stoney's derived estimate of the unit of charge, 10−20 ampere-second, was 116 of the modern value of the charge of the electron [7] due to Stoney using the approximated value of 1018 for the number of molecules presented in one cubic millimetre of gas at standard temperature and pressure. Using the modern values for the Avogadro constant 6.02214×1023 mol−1 and for the volume of a gram-molecule under these conditions of 22.4146×106 mm3, the modern value is 2.687×1016, instead of Stoney's 1018.

Stoney units and Planck units

Stoney's set of base units is similar to the one used in Planck units, proposed independently by Planck thirty years later, in which Planck normalized the Planck constant [lower-alpha 1] in place of the elementary charge. [8]

Planck units are more commonly used than Stoney units in modern physics, especially for quantum gravity (including string theory). Rarely, Planck units are referred to as Planck–Stoney units. [8]

The Stoney length and the Stoney energy, collectively called the Stoney scale, are not far from the Planck length and the Planck energy, the Planck scale. The Stoney scale and the Planck scale are the length and energy scales at which quantum processes and gravity occur together. At these scales, a unified theory of physics is thus required. The only notable attempt to construct such a theory from the Stoney scale was that of Hermann Weyl, who associated a gravitational unit of charge with the Stoney length [9] [10] [11] and who appears to have inspired Dirac's fascination with the large numbers hypothesis. [12] Since then, the Stoney scale has been largely neglected in the development of modern physics, although it is still occasionally discussed. [13]

The ratio of Stoney units to Planck units of length, time and mass is , where is the fine-structure constant: [14]

See also

Notes

  1. In modern usage, Planck units are understood to normalize the reduced Planck constant in place of the Planck constant.

Related Research Articles

<span class="mw-page-title-main">Kinetic energy</span> Energy of a moving physical body

In physics, the kinetic energy of an object is the form of energy that it possesses due to its motion.

In particle physics, the Dirac equation is a relativistic wave equation derived by British physicist Paul Dirac in 1928. In its free form, or including electromagnetic interactions, it describes all spin-1/2 massive particles, called "Dirac particles", such as electrons and quarks for which parity is a symmetry. It is consistent with both the principles of quantum mechanics and the theory of special relativity, and was the first theory to account fully for special relativity in the context of quantum mechanics. It was validated by accounting for the fine structure of the hydrogen spectrum in a completely rigorous way. It has become vital in the building of the Standard Model.

<span class="mw-page-title-main">Heat equation</span> Partial differential equation describing the evolution of temperature in a region

In mathematics and physics, the heat equation is a certain partial differential equation. Solutions of the heat equation are sometimes known as caloric functions. The theory of the heat equation was first developed by Joseph Fourier in 1822 for the purpose of modeling how a quantity such as heat diffuses through a given region.

In mathematics, the Laplace operator or Laplacian is a differential operator given by the divergence of the gradient of a scalar function on Euclidean space. It is usually denoted by the symbols , (where is the nabla operator), or . In a Cartesian coordinate system, the Laplacian is given by the sum of second partial derivatives of the function with respect to each independent variable. In other coordinate systems, such as cylindrical and spherical coordinates, the Laplacian also has a useful form. Informally, the Laplacian Δf (p) of a function f at a point p measures by how much the average value of f over small spheres or balls centered at p deviates from f (p).

The elementary charge, usually denoted by e, is a fundamental physical constant, defined as the electric charge carried by a single proton or, equivalently, the magnitude of the negative electric charge carried by a single electron, which has charge −1 e.

The Kerr metric or Kerr geometry describes the geometry of empty spacetime around a rotating uncharged axially symmetric black hole with a quasispherical event horizon. The Kerr metric is an exact solution of the Einstein field equations of general relativity; these equations are highly non-linear, which makes exact solutions very difficult to find.

<span class="mw-page-title-main">Hyperfine structure</span> Small shifts and splittings in the energy levels of atoms, molecules and ions

In atomic physics, hyperfine structure is defined by small shifts in otherwise degenerate electronic energy levels and the resulting splittings in those electronic energy levels of atoms, molecules, and ions, due to electromagnetic multipole interaction between the nucleus and electron clouds.

<span class="mw-page-title-main">Coupling constant</span> Parameter describing the strength of a force

In physics, a coupling constant or gauge coupling parameter, is a number that determines the strength of the force exerted in an interaction. Originally, the coupling constant related the force acting between two static bodies to the "charges" of the bodies divided by the distance squared, , between the bodies; thus: in for Newtonian gravity and in for electrostatic. This description remains valid in modern physics for linear theories with static bodies and massless force carriers.

In mathematics and in theoretical physics, the Stone–von Neumann theorem refers to any one of a number of different formulations of the uniqueness of the canonical commutation relations between position and momentum operators. It is named after Marshall Stone and John von Neumann.

<span class="mw-page-title-main">Dirac large numbers hypothesis</span> Hypothesis relating age of the universe to physical constants

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:

A multipole expansion is a mathematical series representing a function that depends on angles—usually the two angles used in the spherical coordinate system for three-dimensional Euclidean space, . Similarly to Taylor series, multipole expansions are useful because oftentimes only the first few terms are needed to provide a good approximation of the original function. The function being expanded may be real- or complex-valued and is defined either on , or less often on for some other .

The Compton wavelength is a quantum mechanical property of a particle, defined as the wavelength of a photon whose energy is the same as the rest energy of that particle. It was introduced by Arthur Compton in 1923 in his explanation of the scattering of photons by electrons.

In the field of mathematics, norms are defined for elements within a vector space. Specifically, when the vector space comprises matrices, such norms are referred to as matrix norms. Matrix norms differ from vector norms in that they must also interact with matrix multiplication.

Scalar–tensor–vector gravity (STVG) is a modified theory of gravity developed by John Moffat, a researcher at the Perimeter Institute for Theoretical Physics in Waterloo, Ontario. The theory is also often referred to by the acronym MOG.

The Gamow factor, Sommerfeld factor or Gamow–Sommerfeld factor, named after its discoverer George Gamow or after Arnold Sommerfeld, is a probability factor for two nuclear particles' chance of overcoming the Coulomb barrier in order to undergo nuclear reactions, for example in nuclear fusion. By classical physics, there is almost no possibility for protons to fuse by crossing each other's Coulomb barrier at temperatures commonly observed to cause fusion, such as those found in the Sun. When George Gamow instead applied quantum mechanics to the problem, he found that there was a significant chance for the fusion due to tunneling.

An LC circuit can be quantized using the same methods as for the quantum harmonic oscillator. An LC circuit is a variety of resonant circuit, and consists of an inductor, represented by the letter L, and a capacitor, represented by the letter C. When connected together, an electric current can alternate between them at the circuit's resonant frequency:

In particle physics and physical cosmology, Planck units are a system of units of measurement defined exclusively in terms of four universal physical constants: c, G, ħ, and kB. Expressing one of these physical constants in terms of Planck units yields a numerical value of 1. They are a system of natural units, defined using fundamental properties of nature rather than properties of a chosen prototype object. Originally proposed in 1899 by German physicist Max Planck, they are relevant in research on unified theories such as quantum gravity.

In physics, natural unit systems are measurement systems for which selected physical constants have been set to 1 through nondimensionalization of physical units. For example, the speed of light c may be set to 1, and it may then be omitted, equating mass and energy directly E = m rather than using c as a conversion factor in the typical mass–energy equivalence equation E = mc2. A purely natural system of units has all of its dimensions collapsed, such that the physical constants completely define the system of units and the relevant physical laws contain no conversion constants.

<span class="mw-page-title-main">Relativistic Lagrangian mechanics</span> Mathematical formulation of special and general relativity

In theoretical physics, relativistic Lagrangian mechanics is Lagrangian mechanics applied in the context of special relativity and general relativity.

Lagrangian field theory is a formalism in classical field theory. It is the field-theoretic analogue of Lagrangian mechanics. Lagrangian mechanics is used to analyze the motion of a system of discrete particles each with a finite number of degrees of freedom. Lagrangian field theory applies to continua and fields, which have an infinite number of degrees of freedom.

References

  1. Ray, T. P. (1981), "Stoney's fundamental units", Irish Astronomical Journal, 15: 152, Bibcode:1981IrAJ...15..152R
  2. Stoney, G. Johnstone (May 1881), "LII. On the physical units of nature", The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science, 11 (69): 381–390, doi:10.1080/14786448108627031, ISSN   1941-5982
  3. Barrow, John D.; Tipler, Frank (1988), The anthropic cosmological principle, Oxford University Press, p. 291, ISBN   978-0-192-82147-8
  4. Flowers, Jeff; Petley, Brian (2004), "Constants, Units and Standards", in Karshenboim, Savely G.; Peik, Ekkehard (eds.), Astrophysics, clocks and fundamental constants, Springer, p. 79, ISBN   978-3-540-21967-5
  5. Stoney, G. (1881), "On The Physical Units of Nature", Phil. Mag., 11 (69): 381–391, doi:10.1080/14786448108627031
  6. Stoney, G. Johnstone (1883), "On The Physical Units of Nature", The Scientific Proceedings of the Royal Dublin Society, 3: 51–60, retrieved 2010-11-28
  7. O'Hara, J. G. (1993), "George Johnstone Stoney and the Conceptual Discovery of the Electron", Occasional Papers in Science and Technology, 8: 5–28
  8. 1 2 Barrow, John D. (2004), "Outer Space", in Penz, François; Radick, Gregory; Howell, Robert (eds.), Space: in science, art and society, Cambridge University Press, p. 191, ISBN   978-0-521-82376-0
  9. Tomilin, K. (2000), "Natural System of Units", Proc. of the XX11 International Workshop on High Energy Physics and Field Theory: 289
  10. Weyl, H. (1918), "Gravitation und Elekrizitaet", Koniglich Preussische Akademie der Wissenschaften: 465–78
  11. Weyl, H. (1919), "Eine Neue Erweiterung der Relativitaetstheorie", Annalen der Physik, 59 (10): 101–103, Bibcode:1919AnP...364..101W, doi:10.1002/andp.19193641002
  12. Gorelik, G. (2002), "Hermann Weyl and Large Numbers in Relativistic Cosmology", in Balashov, Y.; Vizgin, V. (eds.), Einstein Studies in Russia, Birkhaeuser
  13. Uzan, Jean-Philippe (2011), "Varying Constants, Gravitation and Cosmology", Living Rev. Relativ., 14 (1): 15–16, arXiv: 1009.5514 , Bibcode:2011LRR....14....2U, doi: 10.12942/lrr-2011-2 , PMC   5256069 , PMID   28179829
  14. Duff, M. J.; Okun, L. B.; Veneziano, G. (2002-03-09), "Trialogue on the number of fundamental constants", Journal of High Energy Physics, 2002 (3): 3, arXiv: physics/0110060 , Bibcode:2002JHEP...03..023D, doi:10.1088/1126-6708/2002/03/023, ISSN   1029-8479, S2CID   15806354