equation

mass–energy equivalence

Mass-energy equivalence expresses that mass and energy are interchangeable, as described by E=mc².
14 related articles · 6 formulas · 3 who worked here

Description

The world's most famous formula — E=mc² — says that mass and energy can turn into each other. Even at rest, any object stores colossal energy: as if every pebble were a compressed spring ready to release. A little mass yields enormous energy because the speed of light (c) is very large, and its square is an astronomical number. This is how stars and nuclear reactors work.

History

Albert Einstein published the final formulation in 1905, though ideas about the connection between mass and electromagnetic energy were expressed earlier by Henri Poincaré in 1900. Experimental confirmations came with the discovery of nuclear reactions and mass defect in the 1930s. Today it has been verified with extremely high precision in accelerators.

How it works

Foundation of nuclear and particle physics: allows calculation of energy release in fusion and fission reactions, production of particle-antiparticle pairs. Limitations: applicable in inertial reference frames; in general relativity, energy becomes part of the energy-momentum tensor. The concept of mass becomes more complicated in curved spacetime.

Fun fact

The Sun converts about 4 million tons of its mass into light every second! We live thanks to that.

Concept graph →

Formulas

$$E = m c^2$$
Energy equals mass times the speed of light squared.
What is in the formula
EvariableEnergy — energy joule
mvariableMass — mass kilogram
cconstantUniversal constant representing the maximum speed at which information and energy can travel — speed of light = 299792458 metre per second
$e_γ\approxm_{dm}c^2$ · 2604.00579
e=mc^2 · 2607.21719v1
$$E_k = \frac{1}{2} m v^2$$
Kinetic energy equals one-half mass times velocity squared.
What is in the formula
E_kvariablekinetic energy — energy joule
mvariablemass — mass kilogram
vvariablevelocity — velocity metre per second
δ_{\max,a}=\frac{1}{2}μ_av_{\max}^2 · 2606.05299v1
e_{{specific}}=\frac{1}{2}v^2 · 2607.00202
$$c_{\rm app} = c_{\rm int} + E$$
Apparent color equals intrinsic color plus color excess.
What is in the formula
c_appvariableApparent color index of a celestial object — color index
c_intvariableIntrinsic color index of the object — color index
EvariableColor excess due to interstellar extinction — color excess
c_{\rmapp}=c_{\rmint}+e · 2606.06593v1
$$m_{\mathrm{eff}}^2 = \text{(expression depending on theory)}$$
Effective mass squared for tensor perturbations in a solid.
What is in the formula
m_effvariableeffective mass of tensor perturbation — effective mass kilogram
^2operatorsquare of the quantity — squaring
m_{{gw}}^2=\frac{64πg}{9}(k_{,y}+k_{,z}) · 2606.27290
$$E = \sqrt{(mc^2)^2 + (pc)^2}$$
Energy of a relativistic particle depends on mass and momentum.
What is in the formula
EvariableTotal energy of the particle — energy joule
mvariableRest mass of the particle — mass kilogram
pvariableMomentum of the particle — momentum kilogram metre per second
cconstantUniversal constant, speed of light in vacuum — speed of light = 299792458 metre per second
√operatorPrincipal square root — square root
e_μ(k)=\sqrt{m_μ^2+v_μ^2|k|^2} · 2606.28306
$$\sigma(E) \propto E^\alpha$$
Cross section scales as power of energy.
What is in the formula
σvariableCross section — cross section metre squared
EvariableEnergy of the incident particle — energy joule
αvariablePower-law exponent — dimensionless exponent
∝operatorProportional to, up to a constant factor — proportionality
σ_{νn}(e_ν)\approx10^{-34}{см}^2(\frac{e_ν}{1{тэв}})^{0.36} · 2607.02644v2

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