### 2.1 Thermodynamic processes

Thermodynamics, and in particular relativistic thermodynamics is a field theory with the primary
objective to determine the thermodynamic fields. These are typically the 14 fields of the number density of
particles, the particle flux vector and the fields of the stress-energy-momentum tensor. However, in extended
thermodynamics we have generally more fields and therefore it is better – at least for the initial arguments – to
leave the number of fields and their tensorial character unspecified. Therefore we consider n fields, combined
in the n-vector . denotes the space-time components of an event. We have and
.
For the determination of the n fields we need field equations – generally n of them – and these are
based on the equations of balance of mechanics and thermodynamics. The generic form of these balance
equations reads

The comma denotes partial differentiation with respect to , and is the n-vector of densities, while
is the n-vector of flux components. Thus represents n four-fluxes, and is the n-vector of
productions.
Obviously the balance equations (1) are not field equations for the fields , at least not in
this form. They must be supplemented by constitutive equations. These relate the four-fluxes
and the productions to the fields in a materially dependent manner. We write

and denote the constitutive functions. Note that the constitutive quantities and at one
event depend only on the values of at that same event. In particular there is no dependence on
gradients and time derivatives of .
If the constitutive functions and are explicitly known, we may eliminate and
between the balance equations (1) and the constitutive relations (2) and obtain a set of explicit field
equations for the fields . These are quasilinear partial differential equations of first order. Every solution
of the field equations is called a thermodynamic process.