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In [[physics]], a '''dimensionless physical constant''' is a [[physical constant]] that is [[dimensionless quantity|dimensionless]] – having no units attached, so its numerical value is the same under all possible [[systems of units]]. The best known example is the [[fine structure constant]] α, with the approximate value 1/137.036.
In [[physics]], a '''dimensionless physical constant''' is a [[physical constant]] that is [[dimensionless quantity|dimensionless]] – having no units attached, so its numerical value is the same under all possible [[systems of units]]. The best known example is the [[fine structure constant]] α, with the approximate value 1/137.036.
Dimensionless physical constants are a subset of '''fundamental physical constants''' [http://physics.nist.gov/cuu/Constants/ NIST] which are mostly '''dimensional''',for example, the [[speed of light]] ''c'', [[vacuum permittivity]] ''ε''<sub>0</sub>, [[Planck's constant]] ''h'', or the [[gravitational constant]] ''G''.
Dimensionless physical constants are a subset of '''fundamental physical constants''' [http://physics.nist.gov/cuu/Constants/ NIST] which are mostly '''dimensional''',for example, the [[speed of light]] ''c'', [[vacuum permittivity]] ''ε''<sub>0</sub>, [[Planck's constant]] ''h'', or the [[gravitational constant]] ''G''. [[exemple: dgheim number DG which is the ratio of the coriolis force over the viscosity force and then quantifies the preponderance of these two forces]].


==Introduction==
==Introduction==

Revision as of 17:03, 8 December 2013

In physics, a dimensionless physical constant is a physical constant that is dimensionless – having no units attached, so its numerical value is the same under all possible systems of units. The best known example is the fine structure constant α, with the approximate value 1/137.036. Dimensionless physical constants are a subset of fundamental physical constants NIST which are mostly dimensional,for example, the speed of light c, vacuum permittivity ε0, Planck's constant h, or the gravitational constant G. exemple: dgheim number DG which is the ratio of the coriolis force over the viscosity force and then quantifies the preponderance of these two forces.

Introduction

The numerical values of dimensional physical constants are dependent on the units used to express these physical constants. As such it is possible to define a basis set of units so that selected dimensional physical constants are normalized to 1 solely because of the choice of units. The basis set may consist of time, length, mass, charge, and temperature, or an equivalent set. A choice of units is called a system of units.

For example, the SI, the international system of units, is such a system of units solely defined as convenient to human use and the numerical values of dimensional physical constants have no natural significance, only in a manner that relates to the human experience. As another example, a system of natural units called Planck units are defined so that the numerical values of the speed of light (in a vacuum), the universal gravitational constant, and the constants of Planck, Coulomb, and Boltzmann, are all set to 1. Because, merely from the choice of units, these five dimensional physical constants disappear from equations of physical law, they are considered not fundamental in an operationally distinguishable sense.[1][2]

In contrast, the numerical values of dimensionless physical constants are independent of the units used. These constants cannot be eliminated by any choice of a system of units. Such constants include:

At the present time, the values of the dimensionless physical constants cannot be calculated; they are determined only by physical measurement. This is one of the unsolved problems of physics.

The best known of the dimensionless constants is the fine structure constant:

where e is the elementary charge, ħ is the reduced Planck's constant, c is the speed of light in a vacuum, and ε0 is the permittivity of free space. The fine structure constant is fixed to the strength of the electromagnetic force. Note that 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.

The analog of the fine structure constant for gravitation is the gravitational coupling constant. This constant requires the arbitrary choice of a pair of objects having mass. The electron and proton are natural choices because they are stable, and their properties are well measured and well understood. If αG is calculated from two protons, its value is ≈10−38.

The list of dimensionless physical constants increases in length whenever experiments measure new relationships between physical phenomena. The list of fundamental dimensionless constants, however, decreases when advances in physics show how some previously known constant can be computed in terms of others. A long-sought goal of theoretical physics is to find first principles from which all of the fundamental dimensionless constants can be calculated and compared to the measured values. A successful "Theory of Everything" would allow such a calculation, but so far, this goal has remained elusive.

Constants in the standard model and in cosmology

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.

The complete standard model requires 25 fundamental dimensionless constants (Baez, 2002). At present, their numerical values are not understood in terms of any widely accepted theory and are determined only from measurement. Based on Mp=1.22089(6)E19 GeV/c2, these 25 constants are:

One constant is required for cosmology:

Thus, currently there are 26 known fundamental dimensionless physical constants. However, this number may not be the final one. For example, if neutrinos turn out to be Majorana fermions, the Maki-Nakagawa-Sakata matrix has two additional parameters. Secondly, if dark matter is discovered, or if the description of dark energy requires more than the cosmological constant, further fundamental constants will be needed.

Well-known subsets

Certain dimensionless constants are discussed more frequently than others.

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, 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 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 cannot be measured. Hence most physicists would not deem it a dimensionless physical constant of the sort discussed in this entry. There are also compelling physical and mathematical reasons why D = 3.

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.

Variation of the constants

The question whether the fundamental dimensionless constants depend on space and time is being extensively researched. Despite several claims, no confirmed variation of the constants has been detected.[citation needed]

Calculation attempts

No formulae for the fundamental physical constants are known to this day.

The mathematician Simon Plouffe has made an extensive search of computer databases of mathematical formulae, seeking formulae for the mass ratios of the fundamental particles.

One well-known example of numerology is by the astrophysicist Arthur Eddington. He set out alleged mathematical reasons why the reciprocal of the fine structure constant had to be exactly 136. When its value was discovered to be closer to 137, he changed his argument to match that value. Experiments have since shown that Eddington was wrong; to six significant digits, the reciprocal of the fine-structure constant is 137.036.

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

See also

References

  1. ^ Michael Duff (2002) "Comment on time-variation of fundamental constants."
  2. ^ Michael Duff, O. Okun and Gabriele Veneziano (2002) "Trialogue on the number of fundamental constants," Journal of High Energy Physics 3: 023.
  3. ^ a b Rees, M. (2000), p. .
  4. ^ Rees, M. (2000), p. 53.
  5. ^ Rees, M. (2000), p. 110.
  6. ^ Rees, M. (2000), p. 118.

Bibliography

  • Martin Rees, 1999. Just Six Numbers: The Deep Forces that Shape the Universe. London: Weidenfeld & Nicolson. ISBN 0-7538-1022-0

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. (1986). The Anthropic Cosmological Principle (1st ed.). Oxford University Press. ISBN 978-0-19-282147-8. LCCN 87028148.
  • 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?"
  • Plouffe. Simon, 2004, "A search for a mathematical expression for mass ratios using a large database."
Do the fundamental constants vary?