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Energy–momentum relation

Relativistic equation relating total energy to mass and momentum

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Through Physics, Equation and Energy

It can be formulated as

This equation holds for a body or system, such as one or more particles, with total energy E, mass m, and momentum of magnitude p; the constant c is the speed of light. It assumes the special relativity case of flat spacetime and that the particles are free. Total energy is the sum of rest energy E0 = mc2 and relativistic kinetic energy: EK=E−E0=(pc)2+(mc2)2−mc2.

The Dirac sea model, which was used to predict the existence of antimatter, is closely related to the energy–momentum relation.

Origins and derivation of the equation

The energy–momentum relation goes back to Max Planck's article published in 1906. It was used by Walter Gordon in 1926 and then by Paul Dirac in 1928 under the form E=c2p2+(mc2)2+V, where V is the potential energy.

The equation can be derived in a number of ways. The simplest include the following:

  1. Considering the relativistic dynamics of a massive particle, or
  2. Evaluating the norm of the four-momentum of the particle. This method applies to both massive and massless particles, and can be extended to multi-particle systems with relatively little effort: see § Many-particle systems.

Heuristic approach for massive particles

For a massive object moving at speed v in the lab frame, the total energy E of the object is given in the lab frame as E=γmc2. The three dimensional relativistic momentum p of the object in the lab frame has the following magnitude p: p=γmv. These quantities include the Lorentz factor γ: γ=11−(vc)2. Squaring the magnitude of the three-momentum gives p2=m2v21−(vc)2. Solving for v2 and substituting into the Lorentz factor, one obtains its alternative form in terms of 3-momentum and mass, rather than 3-velocity: γ=1+(pmc)2. Inserting this form of the Lorentz factor into the energy equation gives E=mc21+(pmc)2. Squaring both sides and rearranging yields the standard form (1).

This approach is not applicable to massless particles due to issues detailed in § Massless particles.

Norm of the four-momentum

Special relativity

In Minkowski space, energy (divided by c) and momentum are two components of a Minkowski four-vector, namely the four-momentum: P=(Ec,p) (these are the contravariant components).

The Minkowski inner product ⟨⋅, ⋅⟩ of this vector with itself gives the square of the norm of this vector, which is proportional to the square of the mass m of the body: ⟨P,P⟩=|P|2=(mc)2. This is a Lorentz invariant quantity, and therefore independent of the frame of reference. Using the Minkowski metric η with metric signature (+ − − −), the inner product is ⟨P,P⟩=PαηαβPβ=(Ecpxpypz)(10000−10000−10000−1)(Ecpxpypz)=(Ec)2−p2, so (mc)2=(Ec)2−p2.

General relativity

In general relativity, the four-momentum is a four-vector defined in a local coordinate frame, although by definition the inner product is similar to that of special relativity, ⟨P,P⟩=|P|2=(mc)2, in which the Minkowski metric η is replaced by the metric tensor field g: ⟨P,P⟩=|P|2=PαgαβPβ, solved from the Einstein field equations. Then PαgαβPβ=(mc)2.

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