
January 12, 2011 9:34 World Scientific Book - 9in x 6in mathematics
Invariances, Symmetries, and Symmetry Breakings 153
consideration and to any systems displaying identical symmetries.
3
As a co nsequence, these mathematical invariants (these physica l laws
of conservation), by extricating the considered systems’ most structurally
stable quantities, constitute an ess e ntial part of their identity, that is, that
they determine them as mathematical structures associated with the sym-
metry groups (of invariance ) and as physical systems conserving certain
quantities during the changes, which affect them. We thus see that the
scope of the geodesic principle extends to specifying the essential aspects
of the physical system thus considered: what remains invariant during the
undergone changes, like a sort of s table base likely to then structure all
encountered varia bilities and modifications.
As for the role of symmetries, note that many empirical systems are
submitted to the s ame symmetry groups and that the geodesic principle
enables us to regroup them under the label of the realization of a same
general model. That is, in a way, to categorize them relative to their
fundamental invariants. One can even go further by showing how these
theoretico-conceptua l s chemes are applied to the theoretical framework of
contemporary physics, to relativistic theories (including cla ssical mechan-
ics), quantum theories, and critical theories.
In this perspective, that which fundamentally characterizes relativis-
tic theories, in the more general case of Riemannian metrics, is their in-
variance under the diffeomorphisms of external space-time. These are re-
ducible to the Lorentz-Po incaré invariance group
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and to spec ial relativity,
for Minkowskian metrics, and to the Galileo group for the Euclidean met-
3
Noether’s theorem is relative to the continuous transformation of symmetries which,
operating on the Lagrangians or the Lagrangian densities, preserve their equations of
movement such as derived from Hamilton’s principle (the Euler-Lagrange equations we
have just mentioned). To each of these transformations corresponds conserved physical
quantities. Thus, for instance, to the invariance of translation in space (impossibility
of physically defining an absolute origin) corresponds the conservation of the kinetic
moment; to the invariance of translation in time (impossibility of physically defining an
absolute origin for tim e) corresponds the conservation of energy. From a less classical
perspective, to the invariance in a change of the origin of the phases of a wave function
corresponds the conservation of the electric charge. These relationships between invari-
ances and conservations will prove to be at the origin of the gauge theories in quantum
physics. We will often go back to Noether’s theorem.
4
The Lorentz group corresponds to the rotations in the Minkow ski space (of which
a component is imaginary); the extension to translations in this space generates the
Poincaré group. The Maxwell equations of electromagnetism are invariant under the
Lorentz group, this being at the origin of special relativity and of its particular kinetics
(contraction of lengths, slowing of clocks, etc.).