In physics, natural units are physical units of measurement defined in such a way that certain selected universal physical constants are normalized to unity; that is, their numerical value becomes exactly 1 when measured in some system of natural units.

Contents

Introduction

Natural units are intended to elegantly simplify particular algebraic expressions appearing in physical law or to normalize some chosen physical quantities that are properties of universal elementary particles and that may be reasonably believed to be constant. However, what may be believed and forced to be constant in one system of natural units can very well be allowed or even assumed to vary in another natural unit system.

Natural units are natural because the origin of their definition comes only from properties of nature and not from any human construct. Planck units are often, without qualification, called "natural units", when in fact they are only one of several systems of natural units, albeit the best known such system. Planck units might be considered unique in that the set of units are not based on properties of any prototype, object, or particle but are solely derived from the properties of free space.

As with any set of base units or fundamental units the base units of a set of natural units will include definitions and values for length, mass, time, temperature, and electric charge. Some physicists do not recognize temperature as a fundamental physical quantity, since it simply expresses the energy per degree of freedom of a particle, which can be expressed in terms of energy (or mass, length, and time). Virtually every system of natural units normalizes Boltzmann's constant k to 1, which can be thought of as simply a way of defining the unit temperature.

In addition, some physicists recognize electric charge as a separate fundamental dimension of physical quantity, even if it has been expressed in terms of mass, length, and time in unit systems such as the electrostatic cgs system. Virtually every system of natural units normalizes the permittivity of free space to ε0=(4π)-1, an expression which can be thought of as defining the unit charge. This suggests that the controversial[1] adoption, first in CGS units and subsequently in SI units, of Georgi's preference for expressing Coulomb's law in the "rationalized" form F= (4πε0)-1q1q2r-2, rather than as F=kq1q2r-2, may not have been the most natural choice after all.

Candidate physical constants used in natural unit systems

The candidate physical constants to be normalized are chosen from those in the following table. Note that only a smaller subset of the following can be normalized in any one system of units without contradiction in definition (e.g., me and mp cannot both be defined as the unit mass in a single system).

Constant Symbol Dimension
speed of light in vacuum L T-1
Gravitational constant M-1L3T-2
Planck's constant (reduced) ML2T-1
Coulomb force constant where is the permittivity of free space Q-2 M L3 T-2
Elementary charge Q
Electron mass M
Proton mass M
Boltzmann constant ML2T-2Θ-1

Dimensionless physical constants such as the fine-structure constant

cannot take on a different numerical value no matter what system of units is used. Judiciously choosing units can only normalize physical constants that have dimension. Since α is a fixed dimensionless number not equal to 1, it is not possible to define a system of natural units that will normalize all of the physical constants that comprise α. Any 3 of the 4 constants: c, , e, or 4πε0, can be normalized (leaving the remaining physical constant to take on a value that is a simple function of α, attesting to the fundamental nature of the fine-structure constant) but not all 4.

Systems of natural units

Planck units

Main article: Planck units
Quantity Expression Metric value
Length (L) 1.61609735×10-35 m
Mass (M) 2.17644(11)×10-8 kg
Time (T) 5.3907205×10-44 s
Electric charge (Q) 1.87554573×10-18 C
Temperature (Θ) 1.4169206×1032 K

Planck units hold pride of place among systems of natural units, because they do not invoke any properties (specifically, the charge, mass, spin, or orbital radius) of any elementary particle. For example, the proton and electron are equally sensible choices, and thus are equally arbitrary. But their masses differ considerably, a fact having nontrivial implications for all other systems of natural units, because these all invoke one or more properties of protons or electrons.

By contrast, the physical constants that Planck units normalize are all properties of free space. In particular, the definition of Planck units does not invoke the elementary charge, whose numerical value, when measured in units of Planck charge, is the square root of the fine-structure constant α. Hence any observed variation over space or time in the value of α is attributed to variation in the elementary charge.

Stoney units

Quantity Expression Metric Value
Length (L) 1.38068×10-36 m
Mass (M) 1.85921×10-9 kg
Time (T) 4.60544×10-45 s
Electric charge (Q) 1.60218×10-19 C
Temperature (Θ) 1.21028×1031 K

George Johnstone Stoney was the first physicist to introduce the concept of natural units. He presented the idea in a lecture entitled "On the Physical Units of Nature" delivered to the British Association in 1874.[2] Stoney units fix the elementary charge and allow Planck's constant (only discovered after Stoney's proposal) to float. They can be obtained from Planck units with the substitution:

.

This removes Planck's constant from the definitions and the value it takes on in Stoney units is the reciprocal of the fine-structure constant, 1/α. Hence any observed variation over space or time in the value of α is attributed to variation in Planck's constant.

Heaviside-Lorentz units

Heaviside-Lorentz units are often used in relativistic calculations, and in particle and nuclear physics. The units are particularly convenient when performing calculations in spatial dimensions greater than three such as is done in string theory. Besides the speed of propagation of the electromagnetic interaction being normalized, so also is the characteristic impedance of electromagnetic waves.

This has the consequence that and so can be used to define a unit of electric charge so that the elementary charge is .

Similarly to geometrized units, without an additional independent constraint, Heaviside-Lorentz units do not define a complete set for length, time, and mass. Only the unit charge is fully defined. If the gravitational constant G is also constrained, Heaviside-Lorentz units would be identical to Planck units save for constant factors of or the reciprocal. If G is defined similarly to the Coulomb constant , then and, likewise to electromagnetic waves, the gravitational interaction propagates with normalized speed and normalized characteristic impedance.

"Schrödinger" units

Quantity Expression Metric Value
Length (L) 2.59276×10-32 m
Mass (M) 1.85921×10-9 kg
Time (T) 1.18516×10-38 s
Electric charge (Q) 1.602176487×10-19 C
Temperature (Θ) 6.44490×1026 K

The name was coined by Michael Duff [1]. They can be obtained from Planck units with the substitution:

.

This removes the speed of light from the definitions and the value it takes on in Schrödinger units is the reciprocal of the fine-structure constant, 1/α. Hence any observed variation over space or time in the value of α is attributed to variation in the speed of light,

Atomic units (Hartree)

Main article: Atomic units
Quantity Expression Metric Value
Length (L) 5.29177×10-11 m
Mass (M) 9.10938×10-31 kg
Time (T) 2.41889×10-17 s
Electric charge (Q) 1.60218×10-19 C
Temperature (Θ) 3.15774×105 K

First proposed by Douglas Hartree to simplify the physics of the Hydrogen atom. Michael Duff [2] calls these "Bohr units". The unit energy in this system is the total energy of the electron in the first circular orbit of the Bohr atom and called the Hartree energy, Eh. The unit velocity is the velocity of that electron, the unit mass is the electron mass, me, and the unit length is the Bohr radius, . They can be obtained from "Schrödinger" units with the substitution:

.

This removes the speed of light (as well as the gravitational constant) from the definitions and its numerical value in atomic units is the reciprocal of the fine-structure constant, 1/α. Hence any observed variation over space or time in the value of α is attributed to variation in the speed of light.

Natural Units (Particle Physics)

Quantity Expression Metric Value
Length (L) 3.86159×10-13 m
Mass (M) 9.10938×10-31 kg
Time (T) 1.28809×10-21 s
Electric charge (Q) 1.60218×10-19 C
Temperature (Θ) 5.92989×109 K

Used in high-energy particle physics and referred to in the SI handbook, however not officially endorsed [3]

Also known by the abbreviation "n.u.".

Electronic system of units

Quantity Expression
Length (L)
Mass (M)
Time (T)
Electric charge (Q)
Temperature (Θ)

Michael Duff [4] calls these "Dirac units". They can be obtained from Stoney units via the substitution:

.

They can be also obtained from atomic units with the substitution:

.

As is the case with Stoney units, any observed variation over space or time in the value of α is attributed to variation in Planck's constant.

Quantum chromodynamical system of units (Strong)

Quantity Expression
Length (L)
Mass (M)
Time (T)
Electric charge (Q)
Temperature (Θ)

The electron mass is replaced with that of the proton and the permittivity of free space is not fixed by definition. Strong units are convenient for work in QCD and nuclear physics, where quantum mechanics and relativity are omnipresent and the proton is an object of central interest[3]. In QCD, any observed variation over space or time in the value of α is attributed to variation in .

Geometrized units

Main article: Geometrized unit system

The geometrized unit system is not a completely defined or unique system. In this system, the base physical units are chosen so that the speed of light and the gravitational constant are set equal to unity leaving latitude to also set some other constant such as the Boltzmann constant and Coulomb force constant equal to unity:

If the reduced Planck constant is also set equal to unity,

then geometrized units are identical to Planck units.

N-body units

Quantity Expression
Length (R)
Mass (M)

N-body units are a completely self-contained system of units used for N-body simulations of self gravitating systems in astrophysics. In this system, the base physical units are chosen so that the total mass (M), the gravitational constant (G) and the virial radius (R) are set equal to unity. The underlying assumption is that the system of N objects (stars) satisfies the virial theorem. The consequence of standard N-body units is that the velocity dispersion of the system is and that the dynamical -crossing- time scales as . The first mention of standard N-body units was by Michel Hénon (1971) [5]. They were taken up by Haldan Cohn (1979) [6] and later widely advertised and generalized by Douglas Heggie and Robert Mathieu (1986). [7]

Conventional electrical units

Most natural unit systems were developed within the physics community to elegantly simplify particular algebraic expressions appearing in physical law. And most natural units are exclusively used within the physics community. However, one system of quasi-natural units, the conventional electrical units, are unique in that they were developed not for simplicity, but rather, to increase the precision of measurements. The conventional electrical units have achieved acceptance as an international standard and are commonly used outside of the physics community in both engineering and industry.

The conventional electrical units are “quasi-natural” in the sense that they are completely and exactly defined in terms of fundamental physical constants. They are the first set of measurement units to be defined in this way, and as such, represent a significant step towards using "natural" fundamental physics for practical measurement purposes. However, the conventional electrical units are unlike other natural units in that no set of physical constants is set to unity.

Four significant steps were taken in the last half century to increase the precision and utility of measurement units. In 1967 the Thirteenth General Conference on Weights and Measures defined the second of atomic time in the International System of Units as the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the cesium-133 atom. In 1983, the seventeenth CGPM redefined the metre in terms of the second and the speed of light, thus fixing the speed of light at exactly 299,792,458 m/s. And in 1990, the eighteenth CGPM adopted conventional values for the Josephson constant and the von Klitzing constant, fixing the conventional Josephson constant at exactly 483,597.9 × 109 Hz/V, and the conventional von Klitzing constant at exactly 25 812.807 Ω. The following table provides a comparison of these newly defined measurement units with other natural unit systems:

Quantity / Symbol Planck Stoney Schrödinger Atomic Electronic Conventional Electrical Units
speed of light in vacuum
Planck's constant
Dirac's constant
elementary charge
Josephson constant
von Klitzing constant
characteristic impedance of vacuum
electric constant (vacuum permittivity)
magnetic constant (vacuum permeability)
Newtonian constant of gravitation
electron mass
caesium ground state hyperfine transition frequency

See also

References

  1. ^ Kowalski, Ludwik, 1986, "A Short History of the SI Units in Electricity," The Physics Teacher 24(32): 97-99.
  2. ^ Ray, T.P. (1981). "Stoney's Fundamental Units". Irish Astronomical Journal 15: 152.
  3. ^ Wilczek, Frank, 2007, "Fundamental Constants," Frank Wilczek web site.

External links

Systems of measurement
Metric systems

International System of Units · metre-kilogram-second · centimetre-gram-second · metre-tonne-second · gravitational system

Natural units

Geometric systems · Planck · Stoney · "Schrödinger" · Atomic · Electronic · Quantum electrodynamical

Conventional systems

Astronomical · Electrical · Temperature

Customary systems

Avoirdupois · Troy · Apothecaries' · English · Imperial · Canadian · US · Danish · Dutch · Finnish · French · German · Irish · Maltese · Norwegian · Scottish · Spanish and Portuguese · Swedish · Polish · Romanian · Russian · Tatar · Hindu · Pegu · Chinese · Japanese · Taiwanese

Ancient systems

Greek · Roman · Egyptian · Hebrew · Arabic · Mesopotamian · Persian · Indian

Other systems

Non-standard · Mesures usuelles

Planck's natural units
Base Planck units Planck time · Planck length · Planck mass · Planck charge · Planck temperature
Derived Planck units Planck energy · Planck force · Planck power · Planck density · Planck angular frequency · Planck pressure · Planck current · Planck voltage · Planck impedance · Planck momentum

Categories: Natural units

 

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