In physics, natural units are physical units of measurement based only on universal physical constants. For example the elementary charge e is a natural unit of electric charge, and the speed of light c is a natural unit of speed. A purely natural system of units is defined in such a way that some set of selected universal physical constants are each normalized to unity; that is, their numerical values in terms of these units are exactly 1. While this has the advantage of simplicity, there is a potential disadvantage in terms of loss of clarity and understanding, as these constants are then omitted from mathematical expressions of physical laws.
Contents

Introduction 1

Notation and use 2

Advantages and disadvantages 2.1

Choosing constants to normalize 3

Electromagnetism units 4

Systems of natural units 5

See also 6

Notes and references 7

External links 8
Introduction
Natural units are intended to elegantly simplify particular algebraic expressions appearing in the laws of physics or to normalize some chosen physical quantities that are properties of universal elementary particles and are reasonably believed to be constant. However there is a choice of the set of natural units chosen, and quantities which are set to unity in one system may take a different value or even be 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", although they constitute only one of several systems of natural units, albeit the best known such system. Planck units (up to a simple multiplier for each unit) might be considered one of the most "natural" systems in that the set of units is not based on properties of any prototype, object, or particle but are solely derived from the properties of free space.
As with other systems of units, the base units of a set of natural units will include definitions and values for length, mass, time, temperature, and electric charge (in lieu of electric current). Some physicists do not recognize temperature as a fundamental physical quantity, since it 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_{B} to 1, which can be thought of as simply a way of defining the unit temperature.
In the SI unit system, electric charge is a separate fundamental dimension of physical quantity, but in natural unit systems charge is expressed in terms of the mechanical units of mass, length, and time, similarly to cgs. There are two common ways to relate charge to mass, length, and time: In Lorentz–Heaviside units (also called "rationalized"), Coulomb's law is F = q_{1}q_{2}/(4πr^{2}), and in Gaussian units (also called "nonrationalized"), Coulomb's law is F = q_{1}q_{2}/r^{2}.^{[1]} Both possibilities are incorporated into different natural unit systems.
Notation and use
Natural units are most commonly used by setting the units to one. For example, many natural unit systems include the equation c = 1 in the unitsystem definition, where c is the speed of light. If a velocity v is half the speed of light, then as v = 1/2c and c = 1, hence v = 1/2. The equation v = 1/2 means "the velocity v has the value onehalf when measured in Planck units", or "the velocity v is onehalf the Planck unit of velocity".
The equation c = 1 can be plugged in anywhere else. For example, Einstein's equation E = mc^{2} can be rewritten in Planck units as E = m. This equation means "The energy of a particle, measured in Planck units of energy, equals the mass of the particle, measured in Planck units of mass."
Advantages and disadvantages
Compared to SI or other unit systems, natural units have both advantages and disadvantages:

Simplified equations: By setting constants to 1, equations containing those constants appear more compact and in some cases may be simpler to understand. For example, the special relativity equation E^{2} = p^{2}c^{2} + m^{2}c^{4} appears somewhat complicated, but the natural units version, E^{2} = p^{2} + m^{2}, appears simpler.

Physical interpretation: Natural unit systems automatically subsume dimensional analysis. For example, in Planck units, the units are defined by properties of quantum mechanics and gravity. Not coincidentally, the Planck unit of length is approximately the distance at which quantum gravity effects become important. Likewise, atomic units are based on the mass and charge of an electron, and not coincidentally the atomic unit of length is the Bohr radius describing the orbit of the electron in a hydrogen atom.

No prototypes: A prototype is a physical object that defines a unit, such as the International Prototype Kilogram, a physical cylinder of metal whose mass is by definition exactly one kilogram. A prototype definition always has imperfect reproducibility between different places and between different times, and it is an advantage of natural unit systems that they use no prototypes. (They share this advantage with other nonnatural unit systems, such as conventional electrical units.)

Less precise measurements: SI units are designed to be used in precision measurements. For example, the second is defined by an atomic transition frequency in cesium atoms, because this transition frequency can be precisely reproduced with atomic clock technology. Natural unit systems are generally not based on quantities that can be precisely reproduced in a lab. Therefore, in order to retain the same degree of precision, the fundamental constants used still have to be measured in a laboratory in terms of physical objects that can be directly observed. If this is not possible, then a quantity expressed in natural units can be less precise than the same quantity expressed in SI units. For example, Planck units use the gravitational constant G, which is measurable in a laboratory only to four significant digits.

Greater ambiguity: Consider the equation a = 10^{10} in Planck units. If a represents a length, then the equation means a = 1.6×10^{−25} m. If a represents a mass, then the equation means a = 220 kg. Therefore, if the variable a was not clearly defined, then the equation a = 10^{10} might be misinterpreted. By contrast, in SI units, the equation would be (for example) a = 220 kg, and it would be clear that a represents a mass, not a length or anything else. In fact, natural units are especially useful when this ambiguity is deliberate: For example, in special relativity space and time are so closely related that it can be useful not to have to specify whether a variable represents a distance or a time.
Choosing constants to normalize
Out of the many physical constants, the designer of a system of natural unit systems must choose a few of these constants to normalize (set equal to 1). It is not possible to normalize just any set of constants. For example, the mass of a proton and the mass of an electron cannot both be normalized: if the mass of an electron is defined to be 1, then the mass of a proton has to be approximately 1836. In a less trivial example, the finestructure constant, α ≈ 1/137, cannot be set to 1, because it is a dimensionless number. The finestructure constant is related to other fundamental constants

\alpha = \frac{k_\text{e} e^2}{\hbar c},
where k_{e} is the Coulomb constant, e is the elementary charge, ℏ is the reduced Planck constant, and c is the speed of light. Therefore it is not possible to simultaneously normalize all four of the constants c, ℏ, e, and k_{e}.
Electromagnetism units
In SI units, electric charge is expressed in coulombs, a separate unit which is additional to the "mechanical" units (mass, length, time), even though the traditional definition of the ampere refers to some of these other units. In natural unit systems, however, electric charge has units of [mass]^{1/2} [length]^{3/2} [time]^{−1}.
There are two main natural unit systems for electromagnetism:
Of these, Lorentz–Heaviside is somewhat more common,^{[2]} mainly because Maxwell's equations are simpler in LorentzHeaviside units than they are in Gaussian units.
In the two unit systems, the elementary charge e satisfies:

e = \sqrt{4 \pi \alpha \hbar c} (Lorentz–Heaviside),

e = \sqrt{\alpha \hbar c} (Gaussian)
where ℏ is the reduced Planck constant, c is the speed of light, and α ≈ 1/137 is the finestructure constant.
In a natural unit system where c = 1, Lorentz–Heaviside units can be derived from SI units by setting ε_{0} = μ_{0} = 1. Gaussian units can be derived from SI units by a more complicated set of transformations, such as multiplying all electric fields by (4πε_{0})^{−1/2}, multiplying all magnetic susceptibilities by 4π, and so on.^{[3]}
Systems of natural units
Planck units
Quantity

Expression

Metric value

Name

Length (L)

l_\text{P} = \sqrt{\frac{\hbar G}{c^3}}

1.616×10^{−35} m

Planck length

Mass (M)

m_\text{P} = \sqrt{\frac{\hbar c}{G}}

2.176×10^{−8} kg

Planck mass

Time (T)

t_\text{P} = \sqrt{\frac{\hbar G}{c^5}}

5.3912×10^{−44} s

Planck time

Temperature (Θ)

T_\text{P} = \sqrt{\frac{\hbar c^5}{G {k_\text{B}}^2}}

1.417×10^{32} K

Planck temperature

Electric charge (Q)

q_\text{P} = e/\sqrt{4\pi\alpha} (L–H)

5.291×10^{−19} C


q_\text{P} = e/\sqrt{\alpha} (G)

1.876×10^{−18} C


Planck units are defined by

c = G = \hbar = k_\text{B} = 1 \
where c is the speed of light, G is the gravitational constant, ℏ is the reduced Planck constant, and k_{B} is the Boltzmann constant.
Planck units are a system of natural units that is not defined in terms of properties of any prototype, physical object, or even elementary particle. They only refer to the basic structure of the laws of physics: c and G are part of the structure of spacetime in general relativity, and ℏ captures the relationship between energy and frequency which is at the foundation of quantum mechanics. This makes Planck units particularly useful and common in theories of quantum gravity, including string theory.
Planck units may be considered "more natural" even than other natural unit systems discussed below, as Planck units are not based on any arbitrarily chosen prototype object or particle. For example, some other systems use the mass of an electron as a parameter to be normalized. But the electron is just one of 16 known massive elementary particles, all with different masses, and there is no compelling reason, within fundamental physics, to emphasize the electron mass over some other elementary particle's mass.
Like the other systems (see above), the electromagnetism units in Planck units can be based on either Lorentz–Heaviside units or Gaussian units. The unit of charge is different in each.
"Natural units" (particle physics and cosmology)
Unit

Metric value

Derivation

1 eV^{−1} of length

1.97×10^{−7} m

=(1\,\text{eV}^{1})\hbar c

1 eV of mass

1.78×10^{−36} kg

= (1\,\text{eV})/c^2

1 eV^{−1} of time

6.58×10^{−16} s

=(1\,\text{eV}^{1})\hbar

1 eV of temperature

1.16×10^{4} K

= 1\,\text{eV}/k_\text{B}

1 unit of electric charge
(L–H)

5.29×10^{−19} C

=e/\sqrt{4\pi\alpha}

1 unit of electric charge
(G)

1.88×10^{−18} C

=e/\sqrt{\alpha}

In particle physics and cosmology, the phrase "natural units" generally means:^{[4]}^{[5]}

\hbar = c = k_\text{B} = 1.
where \hbar is the reduced Planck constant, c is the speed of light, and k_{B} is the Boltzmann constant.
Like the other systems (see above), the electromagnetism units in Planck units can be based on either Lorentz–Heaviside units or Gaussian units. The unit of charge is different in each.
Finally, one more unit is needed to construct a usable system of units that includes energy and mass. Most commonly, electronvolt (eV) is used, despite the fact that this is not a "natural" unit in the sense discussed above – it is defined by a natural property, the elementary charge, and the anthropogenic unit of electric potential, the volt. (The SI prefixed multiples of eV are used as well: keV, MeV, GeV, etc.)
With the addition of eV (or any other auxiliary unit with the proper dimension), any quantity can be expressed. For example, a distance of 1.0 cm can be expressed in terms of eV, in natural units, as:^{[5]}

1.0\, \text{cm} = \frac{1.0\, \text{cm}}{\hbar c} \approx 51000\, \text{eV}^{1}
Stoney units
Quantity

Expression

Metric value

Length (L)

l_\text{S} = \sqrt{\frac{G e^2}{c^4 (4 \pi \epsilon_0)}}

1.381×10^{−36} m

Mass (M)

m_\text{S} = \sqrt{\frac{e^2}{G (4 \pi \epsilon_0)}}

1.859×10^{−9} kg

Time (T)

t_\text{S} = \sqrt{\frac{G e^2}{c^6 (4 \pi \epsilon_0)}}

4.605×10^{−45} s

Temperature (Θ)

T_\text{S} = \sqrt{\frac{c^4 e^2}{G (4 \pi \epsilon_0) {k_\text{B}}^2}}

1.210×10^{31} K

Electric charge (Q)

q_\text{S} = e \

1.602×10^{−19} C

Stoney units are defined by:

c = G = e = k_\text{B} = 1 \

\hbar = \frac{1}{\alpha} \
where c is the speed of light, G is the gravitational constant, e is the elementary charge, k_{B} is the Boltzmann constant, ℏ is the reduced Planck constant, and α is the finestructure constant.
British Association in 1874.^{[6]} Stoney units differ from Planck units by fixing the elementary charge at 1, instead of Planck's constant (only discovered after Stoney's proposal).
Stoney units are rarely used in modern physics for calculations, but they are of historical interest.
Atomic units
Quantity

Expression
(Hartree atomic units)

Metric value
(Hartree atomic units)

Length (L)

l_\text{A} = \frac{\hbar^2 (4 \pi \epsilon_0)}{m_\text{e} e^2}

5.292×10^{−11} m

Mass (M)

m_\text{A} = m_\text{e} \

9.109×10^{−31} kg

Time (T)

t_\text{A} = \frac{\hbar^3 (4 \pi \epsilon_0)^2}{m_\text{e} e^4}

2.419×10^{−17} s

Electric charge (Q)

q_\text{A} = e \

1.602×10^{−19} C

Temperature (Θ)

T_\text{A} = \frac{m_\text{e} e^4}{\hbar^2 (4 \pi \epsilon_0)^2 k_\text{B}}

3.158×10^{5} K

There are two types of atomic units, closely related.
Hartree atomic units:

e = m_\text{e} = \hbar = k_\text{B} = 1 \

c = \frac{1}{\alpha} \
Rydberg atomic units:^{[7]}

\frac{e}{\sqrt{2}} = 2m_\text{e} = \hbar = k_\text{B} = 1 \

c = \frac{2}{\alpha} \
These units are designed to simplify atomic and molecular physics and chemistry, especially the hydrogen atom, and are widely used in these fields. The Hartree units were first proposed by Douglas Hartree, and are more common than the Rydberg units.
The units are designed especially to characterize the behavior of an electron in the ground state of a hydrogen atom. For example, using the Hartree convention, in the Bohr model of the hydrogen atom, an electron in the ground state has orbital velocity = 1, orbital radius = 1, angular momentum = 1, ionization energy = 1/2, etc.
The unit of energy is called the Hartree energy in the Hartree system and the Rydberg energy in the Rydberg system. They differ by a factor of 2. The speed of light is relatively large in atomic units (137 in Hartree or 274 in Rydberg), which comes from the fact that an electron in hydrogen tends to move much slower than the speed of light. The gravitational constant is extremely small in atomic units (around 10^{−45}), which comes from the fact that the gravitational force between two electrons is far weaker than the Coulomb force. The unit length, l_{A}, is the Bohr radius, a_{0}.
The values of c and e shown above imply that e=(αℏc)^{1/2}, as in Gaussian units, not Lorentz–Heaviside units.^{[8]} However, hybrids of the Gaussian and Lorentz–Heaviside units are sometimes used, leading to inconsistent conventions for magnetismrelated units.^{[9]}
Quantum chromodynamics (QCD) system of units
Quantity

Expression

Metric value

Length (L)

l_{\mathrm{QCD}} = \frac{\hbar}{m_\text{p} c}

2.103×10^{−16} m

Mass (M)

m_{\mathrm{QCD}} = m_\text{p} \

1.673×10^{−27} kg

Time (T)

t_{\mathrm{QCD}} = \frac{\hbar}{m_\text{p} c^2}

7.015×10^{−25} s

Temperature (Θ)

T_{\mathrm{QCD}} = \frac{m_\text{p} c^2}{k_\text{B}}

1.089×10^{13} K

Electric charge (Q)

q_\mathrm{QCD} = e/\sqrt{4\pi\alpha} (L–H)

5.291×10^{−19} C

q_\mathrm{QCD} = e/\sqrt{\alpha} (G)

1.876×10^{−18} C


c = m_\text{p} = \hbar = k_\text{B} = 1 \
The electron mass is replaced with that of the proton. 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".^{[10]}
Geometrized units

c = G = 1 \
The geometrized unit system, used in general relativity, is not a completely defined 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. Other units may be treated however desired. By normalizing other appropriate units, geometrized units become identical to Planck units.
Summary table
Quantity / Symbol

Planck
(with Gauss)

Stoney

Hartree

Rydberg

"Natural"
(with LH)

"Natural"
(with Gauss)

Speed of light in vacuum
c \,

1 \,

1 \,

\frac{1}{\alpha} \

\frac{2}{\alpha} \

1 \,

1 \,

Planck's constant (reduced)
\hbar=\frac{h}{2 \pi}

1 \,

\frac{1}{\alpha} \

1 \,

1 \,

1 \,

1 \,

Elementary charge
e \,

\sqrt{\alpha} \,

1 \,

1 \,

\sqrt{2} \,

\sqrt{4\pi\alpha}

\sqrt{\alpha}

Josephson constant
K_\text{J} =\frac{e}{\pi \hbar} \,

\frac{\sqrt{\alpha}}{\pi} \,

\frac{\alpha}{\pi} \,

\frac{1}{\pi} \,

\frac{\sqrt{2}}{\pi} \,

\sqrt{\frac{4\alpha}{\pi}} \,

\frac{\sqrt{\alpha}}{\pi} \,

von Klitzing constant
R_\text{K} =\frac{2 \pi \hbar}{e^2} \,

\frac{2\pi}{\alpha} \,

\frac{2\pi}{\alpha} \,

2\pi \,

\pi \,

\frac{1}{2\alpha}

\frac{2 \pi}{\alpha}

Gravitational constant
G \,

1 \,

1 \,

\frac{\alpha_\text{G}}{\alpha} \,

\frac{8 \alpha_\text{G}}{\alpha} \,

\frac{\alpha_\text{G}}^2} \,

\frac{\alpha_\text{G}}^2} \,

Boltzmann constant
k_\text{B} \,

1 \,

1 \,

1 \,

1 \,

1 \,

1 \,

Electron mass
m_\text{e} \,

\sqrt{\alpha_\text{G}} \,

\sqrt{\frac{\alpha_\text{G}}{\alpha}} \,

1 \,

\frac{1}{2} \,

511 \text{ keV}

511 \text{ keV}

where:
See also
Notes and references

^ Kowalski, Ludwik, 1986, "A Short History of the SI Units in Electricity," The Physics Teacher 24(2): 97–99. Alternate web link (subscription required)

^ Walter Greiner; Ludwig Neise; Horst Stöcker (1995). Thermodynamics and Statistical Mechanics. SpringerVerlag. p. 385.

^ See Gaussian units#General rules to translate a formula and references therein.

^ , by Guidry, Appendix AGauge field theories: an introduction with applications

^ ^{a} ^{b} , by DomínguezTenreiro and Quirós, p422An introduction to cosmology and particle physics

^ Ray, T.P. (1981). "Stoney's Fundamental Units". Irish Astronomical Journal 15: 152.

^ Turek, Ilja (1997). Electronic structure of disordered alloys, surfaces and interfaces (illustrated ed.). Springer. p. 3.

^ Relativistic Quantum Chemistry: The Fundamental Theory of Molecular Science, by Markus Reiher, Alexander Wolf, p7 [books.google.com/books?id=YwSpxCfsNsEC&pg=PA7 link]

^ lecture notesA note on units. See the atomic units article for further discussion.

^ Wilczek, Frank, 2007, "Fundamental Constants," Frank Wilczek web site.
External links

The NIST website (National Institute of Standards and Technology) is a convenient source of data on the commonly recognized constants.

NATURAL SYSTEMS OF UNITS; To the Centenary Anniversary of the Planck SystemK.A. Tomilin: A comparative overview/tutorial of various systems of natural units having historical use.

Pedagogic Aides to Quantum Field Theory Click on the link for Chap. 2 to find an extensive, simplified introduction to natural units.


Current



Background



Historic



Ancient



Other







Base Planck units



Derived Planck units



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