See also: Dimensional analysis and Nondimensionalization
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.
Fundamental units [ ]
A set of fundamental dimensions is a minimal set of units such that every physical quantity can be expressed in terms of this set and where no quantity in the set can be expressed in terms of the others.[1]
Fundamental units:
Some physicists have not recognized temperature as a fundamental dimension of physical quantity since it simply expresses the energy per particle per degree of freedom which can be expressed in terms of energy.
CGS system of units [ ]
From Wikipedia:Centimetre–gram–second system of units :
Quantity
Quantity symbol
CGS unit name
Unit symbol
Unit definition
Equivalent in SI units
length, position
L , x
centimetre
cm
1/100 of metre
= 10−2 m
mass
m
gram
g
1/1000 of kilogram
= 10−3 kg
time
t
second
s
1 second
= 1 s
velocity
v
centimetre per second
cm/s
cm/s
= 10−2 m/s
acceleration
a
gal
Gal
cm/s2
= 10−2 m/s2
force
F
dyne
dyn
g⋅cm/s2
= 10−5 N
energy
E
erg
erg
g⋅cm2 /s2
= 10−7 J
power
P
erg per second
erg/s
g⋅cm2 /s3
= 10−7 W
pressure
p
barye
Ba
g/(cm⋅s2 )
= 10−1 Pa
dynamic viscosity
μ
poise
P
g/(cm⋅s)
= 10−1 Pa⋅s
kinematic viscosity
ν
stokes
St
cm2 /s
= 10−4 m2 /s
wavenumber
k
kayser
cm−1
cm−1
= 100 m−1
charge
q
Statcoulomb
statC
cm3/2 g1/2 s−1
=
Natural units [ ]
From Wikipedia:natural units :
The surface area of a sphere
4
π
r
2
{\displaystyle 4\pi r^2}
In Lorentz–Heaviside units (rationalized units), Coulomb's law is:
F
=
q
1
q
2
r
2
1
4
π
{\displaystyle F=\frac{q_1 q_2}{r^2} \frac{1}{4 \pi}}
In Gaussian units (non-rationalized units), Coulomb's law is:
F
=
q
1
q
2
r
2
{\displaystyle F = \frac{q_1 q_2}{r^2} }
Planck units are defined by
c = ħ = G = k e = k B = 1 ,
Stoney units are defined by:
c = G = k e = e = k B = 1 ,
Hartree atomic units are defined by:
e = m e = ħ = k e = k B = 1
c = 1 α
Rydberg atomic units are defined by:
e √2 = 2m e = ħ = k e = k B = 1
c = 2 α
Quantum chromodynamics (QCD) units are defined by:
c = m p = ħ = k B = 1
Natural units generally means:
ħ = c = k B = 1 .
where:
c is the speed of light ,
ħ is the reduced Planck constant ,
G is the gravitational constant ,
k e is the Coulomb constant ,
k B is the Boltzmann constant
e is the elementary charge ,
Base units [ ]
Base units
Dimension
Planck (L-H)
Planck (Gauss)
Stoney
Hartree
Rydberg
Natural (L-H)
Natural (Gauss)
QCD (Original)
QCD (L-H)
QCD (Gauss)
Length (L)
4
π
ℏ
G
c
3
{\displaystyle \sqrt{4 \pi \hbar G \over c^3}}
ℏ
G
c
3
{\displaystyle \sqrt{\frac{\hbar G}{c^3}}}
G
k
e
e
2
c
4
{\displaystyle \sqrt{\frac{G k_\text{e} e^2}{c^4}}}
ℏ
2
(
4
π
ϵ
0
)
m
e
e
2
{\displaystyle \frac{\hbar^2 (4 \pi \epsilon_0)}{m_\text{e} e^2}}
ℏ
2
(
4
π
ϵ
0
)
m
e
e
2
{\displaystyle \frac{\hbar^2 (4 \pi \epsilon_0)}{m_\text{e} e^2}}
ℏ
c
1
eV
{\displaystyle \frac{\hbar c}{1\,\text{eV}} }
ℏ
c
1
eV
{\displaystyle \frac{\hbar c}{1\,\text{eV}} }
ℏ
m
p
c
{\displaystyle \frac{\hbar}{m_\text{p} c}}
ℏ
m
p
c
{\displaystyle \frac{\hbar}{m_\text{p} c}}
ℏ
m
p
c
{\displaystyle \frac{\hbar}{m_\text{p} c}}
Time (T)
4
π
ℏ
G
c
5
{\displaystyle \sqrt{4 \pi \hbar G \over c^5} }
ℏ
m
P
c
2
=
ℏ
G
c
5
{\displaystyle \frac{\hbar}{m_\text{P}c^2} = \sqrt{\frac{\hbar G}{c^5}} }
G
k
e
e
2
c
6
{\displaystyle \sqrt{\frac{G k_\text{e} e^2}{c^6}} }
ℏ
3
(
4
π
ϵ
0
)
2
m
e
e
4
{\displaystyle \frac{\hbar^3 (4 \pi \epsilon_0)^2}{m_\text{e} e^4} }
2
ℏ
3
(
4
π
ϵ
0
)
2
m
e
e
4
{\displaystyle \frac{2 \hbar^3 (4 \pi \epsilon_0)^2}{m_\text{e} e^4} }
ℏ
1
eV
{\displaystyle \frac{\hbar}{1\,\text{eV}} }
ℏ
1
eV
{\displaystyle \frac{\hbar}{1\,\text{eV}} }
ℏ
m
p
c
2
{\displaystyle \frac{\hbar}{m_\text{p} c^2}}
ℏ
m
p
c
2
{\displaystyle \frac{\hbar}{m_\text{p} c^2}}
ℏ
m
p
c
2
{\displaystyle \frac{\hbar}{m_\text{p} c^2}}
Mass (M)
ℏ
c
4
π
G
{\displaystyle \sqrt{\hbar c \over 4 \pi G}}
ℏ
c
G
{\displaystyle \sqrt{\frac{\hbar c}{G}}}
k
e
e
2
G
{\displaystyle \sqrt{\frac{k_\text{e} e^2}{G}}}
m
e
{\displaystyle m_\text{e} \ }
2
m
e
{\displaystyle 2 m_\text{e} \ }
1
eV
c
2
{\displaystyle \frac{1\,\text{eV}}{c^2}}
1
eV
c
2
{\displaystyle \frac{1\,\text{eV}}{c^2}}
m
p
{\displaystyle m_\text{p} \ }
m
p
{\displaystyle m_\text{p} \ }
m
p
{\displaystyle m_\text{p} \ }
Electric charge (Q)
ℏ
c
ϵ
0
{\displaystyle \sqrt{\hbar c \epsilon_0}}
e
α
{\displaystyle \frac{e}{\sqrt{\alpha}}}
e
{\displaystyle e \ }
e
{\displaystyle e \ }
e
2
{\displaystyle \frac{e}{\sqrt{2}} \ }
e
4
π
α
{\displaystyle \frac{e}{\sqrt{4\pi\alpha}}}
e
α
{\displaystyle \frac{e}{\sqrt{\alpha}}}
e
{\displaystyle e}
e
4
π
α
{\displaystyle \frac{e}{\sqrt{4\pi\alpha}}}
e
α
{\displaystyle \frac{e}{\sqrt{\alpha}}}
Temperature (Θ) with
f
=
2
{\displaystyle f=2}
ℏ
c
5
4
π
G
k
B
2
{\displaystyle \sqrt{\frac{\hbar c^5}{4 \pi G {k_\text{B}}^2}}}
m
P
c
2
k
B
=
ℏ
c
5
G
k
B
2
{\displaystyle \frac{m_\text{P} c^2}{k_\text{B}} = \sqrt{\frac{\hbar c^5}{G k_\text{B}^2}}}
c
4
k
e
e
2
G
k
B
2
{\displaystyle \sqrt{\frac{c^4 k_\text{e} e^2}{G {k_\text{B}}^2}}}
m
e
e
4
ℏ
2
(
4
π
ϵ
0
)
2
k
B
{\displaystyle \frac{m_\text{e} e^4}{\hbar^2 (4 \pi \epsilon_0)^2 k_\text{B}}}
m
e
e
4
2
ℏ
2
(
4
π
ϵ
0
)
2
k
B
{\displaystyle \frac{m_\text{e} e^4}{2 \hbar^2 (4 \pi \epsilon_0)^2 k_\text{B}}}
1
eV
k
B
⋅
2
f
{\displaystyle \frac{1\,\text{eV}}{k_\text{B}}\cdot\frac{2}{f}}
1
eV
k
B
⋅
2
f
{\displaystyle \frac{1\,\text{eV}}{k_\text{B}}\cdot\frac{2}{f}}
m
p
c
2
k
B
{\displaystyle \frac{m_\text{p} c^2}{k_\text{B}}}
m
p
c
2
k
B
{\displaystyle \frac{m_\text{p} c^2}{k_\text{B}}}
m
p
c
2
k
B
{\displaystyle \frac{m_\text{p} c^2}{k_\text{B}}}
Summary table [ ]
From Wikipedia:natural units :
Quantity / Symbol
Planck (L-H )
Planck (Gauss )
Stoney
Hartree
Rydberg
"Natural" (L-H )
"Natural" (Gauss )
QCD (original)
QCD (L-H )
QCD (Gauss )
Speed of light
c
{\displaystyle c \,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
α
{\displaystyle \frac{1}{\alpha} \ }
2
α
{\displaystyle \frac{2}{\alpha} \ }
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
Reduced Planck constant
ℏ
=
h
2
π
{\displaystyle \hbar = \frac{h}{2 \pi}}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
α
{\displaystyle \frac{1}{\alpha} \ }
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
Elementary charge
e
{\displaystyle e \,}
4
π
α
{\displaystyle \sqrt{4\pi\alpha} \,}
α
{\displaystyle \sqrt{\alpha} \,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
2
{\displaystyle \sqrt{2} \,}
4
π
α
{\displaystyle \sqrt{4\pi\alpha}}
α
{\displaystyle \sqrt{\alpha}}
1
{\displaystyle 1\,}
4
π
α
{\displaystyle \sqrt{4\pi\alpha} \,}
α
{\displaystyle \sqrt{\alpha} \,}
Vacuum permittivity
ε
0
{\displaystyle \varepsilon_0 \,}
1
{\displaystyle 1\,}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
{\displaystyle 1\,}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
4
π
α
{\displaystyle \frac{1}{4 \pi \alpha}}
1
{\displaystyle 1\,}
1
4
π
{\displaystyle \frac{1}{4\pi}}
Vacuum permeability
μ
0
=
1
ϵ
0
c
2
{\displaystyle \mu_0 = \frac{1}{\epsilon_0 c^2} \,}
1
{\displaystyle 1\,}
4
π
{\displaystyle 4\pi}
4
π
{\displaystyle 4\pi}
4
π
α
2
{\displaystyle 4 \pi \alpha^2}
π
α
2
{\displaystyle \pi \alpha^2}
1
{\displaystyle 1\,}
4
π
{\displaystyle 4\pi}
4
π
α
{\displaystyle 4 \pi \alpha}
1
{\displaystyle 1\,}
4
π
{\displaystyle 4\pi}
Impedance of free space
Z
0
=
1
ϵ
0
c
=
μ
0
c
{\displaystyle Z_0 = \frac{1}{\epsilon_0 c} = \mu_0 c \,}
1
{\displaystyle 1\,}
4
π
{\displaystyle 4\pi}
4
π
{\displaystyle 4\pi}
4
π
α
{\displaystyle 4 \pi \alpha}
2
π
α
{\displaystyle 2\pi\alpha}
1
{\displaystyle 1\,}
4
π
{\displaystyle 4\pi}
4
π
α
{\displaystyle 4 \pi \alpha}
1
{\displaystyle 1\,}
4
π
{\displaystyle 4\pi}
Josephson constant
K
J
=
e
π
ℏ
{\displaystyle K_\text{J} =\frac{e}{\pi \hbar} \,}
4
α
π
{\displaystyle \sqrt{\frac{4\alpha}{\pi}} \,}
α
π
{\displaystyle \frac{\sqrt{\alpha}}{\pi} \,}
α
π
{\displaystyle \frac{\alpha}{\pi} \,}
1
π
{\displaystyle \frac{1}{\pi} \,}
2
π
{\displaystyle \frac{\sqrt{2}}{\pi} \,}
4
α
π
{\displaystyle \sqrt{\frac{4\alpha}{\pi}} \,}
α
π
{\displaystyle \frac{\sqrt{\alpha}}{\pi} \,}
1
π
{\displaystyle \frac{1}{\pi} \,}
4
α
π
{\displaystyle \sqrt{\frac{4\alpha}{\pi}} \,}
α
π
{\displaystyle \frac{\sqrt{\alpha}}{\pi} \,}
von Klitzing constant
R
K
=
2
π
ℏ
e
2
{\displaystyle R_\text{K} =\frac{2 \pi \hbar}{e^2} \,}
1
2
α
{\displaystyle \frac{1}{2\alpha} }
2
π
α
{\displaystyle \frac{2\pi}{\alpha} \,}
2
π
α
{\displaystyle \frac{2\pi}{\alpha} \,}
2
π
{\displaystyle 2 \pi \, }
π
{\displaystyle \pi\,}
1
2
α
{\displaystyle \frac{1}{2\alpha} }
2
π
α
{\displaystyle \frac{2 \pi}{\alpha} }
2
π
{\displaystyle 2 \pi \, }
1
2
α
{\displaystyle \frac{1}{2\alpha} }
2
π
α
{\displaystyle \frac{2\pi}{\alpha} \,}
Coulomb constant
k
e
=
1
4
π
ϵ
0
{\displaystyle k_e=\frac{1}{4 \pi \epsilon_0}}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
{\displaystyle 1\,}
α
{\displaystyle \alpha}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
{\displaystyle 1\,}
Gravitational constant
G
{\displaystyle G \,}
1
4
π
{\displaystyle \frac{1}{4\pi}}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
α
G
α
{\displaystyle \frac{\alpha_\text{G}}{\alpha} \,}
8
α
G
α
{\displaystyle \frac{8 \alpha_\text{G}}{\alpha} \,}
α
G
m
e
2
{\displaystyle \frac{\alpha_\text{G}}{{m_\text{e}}^2} \,}
α
G
m
e
2
{\displaystyle \frac{\alpha_\text{G}}{{m_\text{e}}^2} \,}
μ
2
α
G
{\displaystyle \mu^2 \alpha_\text{G}}
μ
2
α
G
{\displaystyle \mu^2 \alpha_\text{G}}
μ
2
α
G
{\displaystyle \mu^2 \alpha_\text{G}}
Boltzmann constant
k
B
{\displaystyle k_\text{B} \,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
Proton rest mass
m
p
{\displaystyle m_\text{p} \,}
μ
4
π
α
G
{\displaystyle \mu \sqrt{4 \pi \alpha_\text{G}} \,}
μ
α
G
{\displaystyle \mu \sqrt{\alpha_\text{G}} \,}
μ
α
G
α
{\displaystyle \mu \sqrt{\frac{\alpha_\text{G}}{\alpha}} \,}
μ
{\displaystyle \mu \,}
μ
2
{\displaystyle \frac{\mu}{2} \,}
938
MeV
{\displaystyle 938 \text{ MeV}}
938
MeV
{\displaystyle 938 \text{ MeV}}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
1
{\displaystyle 1\,}
Electron rest mass
m
e
{\displaystyle m_\text{e} \,}
4
π
α
G
{\displaystyle \sqrt{4 \pi \alpha_\text{G}} \,}
α
G
{\displaystyle \sqrt{\alpha_\text{G}} \,}
α
G
α
{\displaystyle \sqrt{\frac{\alpha_\text{G}}{\alpha}} \,}
1
{\displaystyle 1\,}
1
2
{\displaystyle \frac{1}{2} \,}
511
keV
{\displaystyle 511 \text{ keV}}
511
keV
{\displaystyle 511 \text{ keV}}
1
μ
{\displaystyle \frac{1}{\mu}}
1
μ
{\displaystyle \frac{1}{\mu}}
1
μ
{\displaystyle \frac{1}{\mu}}
where:
α is the dimensionless fine-structure constant
α G is the dimensionless gravitational coupling constant
µ is dimensionless proton-to-electron mass ratio
Fine-structure constant [ ]
From Wikipedia:Fine-structure constant :
The Fine-structure constant , α , in terms of other fundamental physical constants :
α
=
1
4
π
ε
0
e
2
ℏ
c
=
μ
0
4
π
e
2
c
ℏ
=
k
e
e
2
ℏ
c
=
c
μ
0
2
R
K
=
e
2
4
π
Z
0
ℏ
{\displaystyle
\alpha = \frac{1}{4 \pi \varepsilon_0} \frac{e^2}{\hbar c} = \frac{\mu_0}{4 \pi} \frac{e^2 c}{\hbar} = \frac{k_\text{e} e^2}{\hbar c} = \frac{c \mu_0}{2 R_\text{K}} = \frac{e^2}{4 \pi}\frac{Z_0}{\hbar}
}
where:
e is the elementary charge
π is the mathematical constant pi
ħ is the reduced Planck constant
c is the speed of light in vacuum
ε 0 is the electric constant or permittivity of free space
µ 0 is the magnetic constant or permeability of free space
k e is the Coulomb constant
R K is the von Klitzing constant
Z 0 is the vacuum impedance or impedance of free space
Gravitational coupling constant [ ]
From Wikipedia:Gravitational coupling constant :
The Gravitational coupling constant , α G , is typically defined in terms of the gravitational attraction between two electrons. More precisely,
α
G
=
G
m
e
2
ℏ
c
=
(
m
e
m
P
)
2
≈
1.751751596
×
10
−
45
{\displaystyle \alpha_\mathrm{G} = \frac{G m_\mathrm{e}^2}{\hbar c} = \left( \frac{m_\mathrm{e}}{m_\mathrm{P}} \right)^2 \approx 1.751751596 \times 10^{-45} }
where:
G is the gravitational constant
m e is the electron rest mass
c is the speed of light in vacuum
ħ is the reduced Planck constant
m P is the Planck mass
Maxwell's equations [ ]
From Wikipedia:Lorentz–Heaviside units :
Name
SI units
Gaussian units
Lorentz–Heaviside units
Gauss's law
(macroscopic)
∇
⋅
D
=
ρ
f
{\displaystyle \nabla \cdot \mathbf{D} = \rho_\text{f}}
∇
⋅
D
=
4
π
ρ
f
{\displaystyle \nabla \cdot \mathbf{D} = 4\pi\rho_\text{f}}
∇
⋅
D
=
ρ
f
{\displaystyle \nabla \cdot \mathbf{D} = \rho_\text{f}}
Gauss's law
(microscopic)
∇
⋅
E
=
ρ
/
ϵ
0
{\displaystyle \nabla \cdot \mathbf{E} = \rho/\epsilon_0}
∇
⋅
E
=
4
π
ρ
{\displaystyle \nabla \cdot \mathbf{E} = 4 \pi \rho}
∇
⋅
E
=
ρ
{\displaystyle \nabla \cdot \mathbf{E} = \rho}
Gauss's law for magnetism :
∇
⋅
B
=
0
{\displaystyle \nabla \cdot \mathbf{B} = 0}
∇
⋅
B
=
0
{\displaystyle \nabla \cdot \mathbf{B} = 0}
∇
⋅
B
=
0
{\displaystyle \nabla \cdot \mathbf{B} = 0}
Maxwell–Faraday equation :
∇
×
E
=
−
∂
B
∂
t
{\displaystyle \nabla \times \mathbf{E} = -\frac {\partial \mathbf{B}}{\partial t}}
∇
×
E
=
−
1
c
∂
B
∂
t
{\displaystyle \nabla \times \mathbf{E} = -\frac{1}{c}\frac{\partial \mathbf{B}} {\partial t}}
∇
×
E
=
−
1
c
∂
B
∂
t
{\displaystyle \nabla \times \mathbf{E} = -\frac{1}{c}\frac{\partial \mathbf{B}} {\partial t}}
Ampère–Maxwell equation
(macroscopic):
∇
×
H
=
J
f
+
∂
D
∂
t
{\displaystyle \nabla \times \mathbf{H} = \mathbf{J}_{\text{f}} + \frac{\partial \mathbf{D}} {\partial t}}
∇
×
H
=
4
π
c
J
f
+
1
c
∂
D
∂
t
{\displaystyle \nabla \times \mathbf{H} = \frac{4\pi}{c}\mathbf{J}_{\text{f}} + \frac{1}{c}\frac{\partial \mathbf{D}} {\partial t}}
∇
×
H
=
1
c
J
f
+
1
c
∂
D
∂
t
{\displaystyle \nabla \times \mathbf{H} = \frac{1}{c}\mathbf{J}_{\text{f}} + \frac{1}{c}\frac{\partial \mathbf{D}} {\partial t}}
Ampère–Maxwell equation
(microscopic):
∇
×
B
=
μ
0
J
+
1
c
2
∂
E
∂
t
{\displaystyle \nabla \times \mathbf{B} = \mu_0\mathbf{J} + \frac{1}{c^2}\frac{\partial \mathbf{E}} {\partial t}}
∇
×
B
=
4
π
c
J
+
1
c
∂
E
∂
t
{\displaystyle \nabla \times \mathbf{B} = \frac{4\pi}{c}\mathbf{J} + \frac{1}{c}\frac{\partial \mathbf{E}} {\partial t}}
∇
×
B
=
1
c
J
+
1
c
∂
E
∂
t
{\displaystyle \nabla \times \mathbf{B} = \frac{1}{c}\mathbf{J} + \frac{1}{c}\frac{\partial \mathbf{E}} {\partial t}}
Gravitoelectromagnetism [ ]
See also: Einstein_field_equations
From Wikipedia:Gravitoelectromagnetism :
According to general relativity , the gravitational field produced by a rotating object (or any rotating mass–energy) can, in a particular limiting case, be described by equations that have the same form as in classical electromagnetism . Starting from the basic equation of general relativity, the Einstein field equation , and assuming a weak gravitational field or reasonably flat spacetime , the gravitational analogs to Maxwell's equations for electromagnetism , called the "GEM equations", can be derived. GEM equations compared to Maxwell's equations in SI units are:
GEM equations
Maxwell's equations
∇
⋅
E
g
=
−
4
π
G
ρ
g
{\displaystyle \nabla \cdot \mathbf{E}_\text{g} = -4 \pi G \rho_\text{g} \ }
∇
⋅
E
=
ρ
ϵ
0
{\displaystyle \nabla \cdot \mathbf{E} = \frac {\rho} {\epsilon_0}}
∇
⋅
B
g
=
0
{\displaystyle \nabla \cdot \mathbf{B}_\text{g} = 0 \ }
∇
⋅
B
=
0
{\displaystyle \nabla \cdot \mathbf{B} = 0 \ }
∇
×
E
g
=
−
∂
B
g
∂
t
{\displaystyle \nabla \times \mathbf{E}_\text{g} = -\frac{\partial \mathbf{B}_\text{g} } {\partial t} \ }
∇
×
E
=
−
∂
B
∂
t
{\displaystyle \nabla \times \mathbf{E} = -\frac{\partial \mathbf{B} } {\partial t} \ }
∇
×
B
g
=
−
4
π
G
c
2
J
g
+
1
c
2
∂
E
g
∂
t
{\displaystyle \nabla \times \mathbf{B}_\text{g} = -\frac{4 \pi G}{c^2} \mathbf{J}_\text{g} + \frac{1}{c^2} \frac{\partial \mathbf{E}_\text{g}} {\partial t} }
∇
×
B
=
1
ϵ
0
c
2
J
+
1
c
2
∂
E
∂
t
{\displaystyle \nabla \times \mathbf{B} = \frac{1}{\epsilon_0 c^2} \mathbf{J} + \frac{1}{c^2} \frac{\partial \mathbf{E}} {\partial t} }
where:
E g is the static gravitational field (conventional gravity , also called gravitoelectric in analogous usage) in m⋅s−2 ;
E is the electric field ;
B g is the gravitomagnetic field in s−1 ;
B is the magnetic field ;
ρ g is mass density in kg⋅m−3 ;
ρ is charge density :
J g is mass current density or mass flux (J g = ρ g v ρ , where v ρ is the velocity of the mass flow generating the gravitomagnetic field) in kg⋅m−2 ⋅s−1 ;
J is electric current density ;
G is the gravitational constant in m3 ⋅kg−1 ⋅s−2 ;
ε 0 is the vacuum permittivity ;
c is the speed of propagation of gravity (which is equal to the speed of light according to general relativity ) in m⋅s−1 .
Electromagnetism [ ]
The total energy in the electric field surrounding a hollow spherical shell of radius r and charge q is:
E
=
k
1
2
q
2
r
{\displaystyle E = k \frac{1}{2} \frac{q^2}{r}}
Therefore:
2
E
⋅
r
q
2
=
k
=
c
o
n
s
t
a
n
t
{\displaystyle {\color{red}2E \cdot \frac{r}{q^2} } = k =constant}
The constant k is a property of space. It is the "stiffness " of space. (If space were stiffer then c would be faster.)
Coulomb's law states that:
F
=
k
e
q
1
q
2
d
2
{\displaystyle F=k_e \frac{q_1 q_2}{d^2}}
The Coulomb constant has units of Energy * distance/charge2 which gives:
F
=
F
⋅
d
d
q
2
q
1
q
2
d
2
{\displaystyle F = {\color{red}F \cdot d \frac{d}{q^2}} \frac{q_1 q_2}{d^2}}
The factor of 1/2 in the first equation above comes from the fact that the field diminishes to zero as it penetrates the shell.
Gravity [ ]
Newton's law of universal gravitation states that:
F
=
G
m
1
m
2
d
2
{\displaystyle F = G \frac{m_1 m_2}{d^2} }
where:
F
=
F
⋅
d
d
m
2
m
1
m
2
d
2
{\displaystyle F = F \cdot d \frac{d}{m^2} \frac{m_1 m_2}{d^2}}
But its probably better to say that:
a
=
d
t
2
=
G
m
d
2
{\displaystyle a = \frac{d}{t^2} = G \frac{m}{d^2}\ }
The obvious unit of charge is one electron but there is no obvious unit of mass. We can, however, create one by setting the electric force between two electrons equal to the gravitational force between two equal masses:
G
m
1
m
2
d
2
=
k
e
q
1
q
2
d
2
{\displaystyle G \frac{m_1 m_2}{d^2} = k_e\frac{q_1 q_2}{d^2}}
Solving we get m = 1.859 × 10-6 g =
α
{\displaystyle \sqrt{\alpha}}
planck masses = 1 Stoney mass
The Schwarzschild radius of a Stoney mass is 2 Stoney lengths.
Boltzmann constant [ ]
Gas
Specific heat ratio
Degrees of freedom
Helium
1.667
3
Neon
1.667
3
Argon
1.667
3
Hydrogen
1.597[2]
3.35
Hydrogen
1.41
4.88
Nitrogen
1.4
5
Oxygen
1.395
5.06
Chlorine
1.34
5.88
Carbon dioxide
1.289
6.92
Methane
1.304
6.58
Ethane
1.187
10.7
Engineering ToolBox (2003) [3]
For monatomic gases:
P
V
5
3
=
C
o
n
s
t
a
n
t
{\displaystyle P V^{\frac{5}{3}} = Constant}
From Wikipedia:Boltzmann constant :
The Boltzmann constant , k , is a scaling factor between macroscopic (thermodynamic temperature ) and microscopic (thermal energy ) physics.
Macroscopically, the ideal gas law states:
k
B
T
=
P
V
n
{\displaystyle k_B T = P \frac{V}{n}}
where:
kB is the Boltzmann constant
T is the temperature
P is the pressure
V is the volume
n is the number of molecules of gas.
Single particle [ ]
The pressure exerted on one face of a cube of length d by a single particle bouncing back and forth perpendicular to the face with mass m and velocity
v
=
v
x
+
v
y
+
v
z
{\displaystyle v = \sqrt{v_x + v_y + v_z}}
is:
p
r
e
s
s
u
r
e
=
f
o
r
c
e
a
r
e
a
=
m
o
m
e
n
t
u
m
t
i
m
e
d
2
=
2
m
v
x
2
d
/
v
x
d
2
=
m
v
x
2
d
3
=
2
E
x
V
0
=
2
E
3
V
0
{\displaystyle pressure = \frac{force}{area} = \frac{\frac{momentum}{time}}{d^2} = \frac{\frac{2 m v_x}{2 d / v_x}}{d^2} = \frac{m v_x^2}{d^3} = \frac{2 E_x}{V_0} = \frac{2 \frac{E}{3}}{V_0}}
where:
V0 = d3 is the volume occupied by a single particle.
vx is the velocity perpendicular to the face
Twice the velocity means twice as much momentum transferred per collision and twice as many collisions per unit time.
Ex is the kinetic energy per particle
Therefore:
V
0
=
V
n
{\displaystyle V_0 = \frac{V}{n}}
Therefore:
T
=
p
V
n
=
p
V
0
=
m
v
2
=
2
E
{\displaystyle T = p \frac{V}{n} = p V_0 = m v^2 = 2 E}
Therefore temperature is twice the energy per degree of freedom per particle
T
=
2
E
{\displaystyle T = 2 E}
Blackbody radiation [ ]
From Wikipedia:Black-body radiation :
Planck's law states that
B
ν
(
ν
,
T
)
=
2
h
ν
3
c
2
1
e
h
ν
/
k
T
−
1
,
{\displaystyle B_\nu(\nu, T) = \frac{2h\nu^3}{c^2}\frac{1}{e^{h\nu/kT} - 1},}
where
Bν (T ) is the spectral radiance (the power per unit solid angle and per unit of area normal to the propagation) density of frequency ν radiation per unit frequency at thermal equilibrium at temperature T.
h is the Planck constant ;
c is the speed of light in a vacuum;
k is the Boltzmann constant ;
ν is the frequency of the electromagnetic radiation;
T is the absolute temperature of the body.
Most of the electromagnetic radiation is emitted (and absorbed) during the brief but intense acceleration's during the atomic collisions.
From Wikipedia:Larmor formula :
For velocities that are small relative to the speed of light , the total power radiated is given by the Larmor formula:
P
=
2
3
q
2
a
2
4
π
ε
0
c
3
=
q
2
a
2
6
π
ε
0
c
3
(SI units)
{\displaystyle P = {2 \over 3} \frac{q^2 a^2}{ 4 \pi \varepsilon_0 c^3}= \frac{q^2 a^2}{6 \pi \varepsilon_0 c^3} \mbox{ (SI units)} }
Uncertainty principle [ ]
References [ ]
External links [ ]