Let us now go back to the particle densities (2.4). In general
these densities will not correspond to a conservation law, because
of chemical, nuclear or other reactions taking place in the
system. First we must ask ourselves which particle properties are
conserved, i.e. what charges are carried by the particles.
Assume, for instance, that the particles carry an electromagnetic
charge . The conserved charge density is then
and the corresponding current density
with the velocity derived from the kinetic energy
of the particles:
In general, particles will carry more than one conserved charge
, like atomic weight, lepton charge,
baryon charge, etc. Moreover, for non-relativistic systems, total
mass is strictly conserved which means that the mass number , with some convenient reference mass, is one of the
conserved quantum numbers. We take this into account by defining
For the sake of a compact notation, we combined charge and
current density into one four-vector . This allows us to write the continuity
equation
- Any conserved quantum number implies the existence of a
conserved macroscopic current density.
Exercise 2
- Consider a npe system. Electromagnetic charge, lepton
number and baryon number are conserved. Write down the
corresponding quantum numbers and conserved currents, and
tabulate the allowed two-particle reactions.
Momentum and energy are always conserved because of the
translational invariance of space-time. This means that we must
have
where is the total energy density and
the energy flow (density).
Similarly, the momentum conservation law reads
with the momentum density and the pressure tensor
Energy-momentum conservation may be combined into one single
conservation law
by defining the energy-momentum tensor as
In this expression one should read and
.
- Notice that in the non-relativistic case the energy-momentum
tensor is not symmetric: .