MECHANICAL SYSTEMS, CLASSICAL MODELS
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moments
m
M and
r
M , respectively). There exist, in general, two tendencies of
displacement, corresponding to the increasing or the decreasing of the parameter which
is fixing the position of the mechanical system. We call direct motion that one which
corresponds to the direction of displacement due to the motive force and inverse motion
that one which corresponds to the direction of displacement of the resistent force. One
determines the magnitudes of the motive force corresponding to the two tendencies of
displacement from the position of equilibrium; these two limit magnitudes depend on
the resistent force
r
F (or on the couple
r
M ), on the geometry of the static position of
equilibrium of the mechanism (distances or angles), on the fixed geometric elements
(independent of the configuration of the mechanism) and on the coefficients of friction.
The two limit magnitudes coincide if we do not take into account the phenomenon of
friction.
We say that a system of rigid solids is subjected to a phenomenon of self-fixing (or
self-braking), the position of equilibrium being maintained if the motive mechanical
element is no more acting (
m
F or
m
M ), but the resistent mechanical element (
r
F or
r
M ) still acts. We can say that the system is in equilibrium under the limit (or at the
limit) of sliding, rolling or pivoting, in the opposite tendency of a direct motion; to have
a motion in this case,
m
F (or
m
M ) must change of direction. Analogously, a system of
rigid solids is subjected to a phenomenon of self-locking if, to obtain a tendency of
direct motion, in a certain configuration of the system, the motive mechanical element
(
m
F or
m
M ) must tend to infinity. The first of these phenomena may be useful in
practice, but the second one must be avoid; thus, the study of those phenomena has a
particular importance.
Using the above exposure, we may emphasize three important methods of
computation. Thus, in the method of isolating the solids, each rigid solid of the system
is isolated by introducing the corresponding constraint forces and the conditions of
equilibrium (the torsor of the system of given and constraint forces with respect to an
arbitrary pole vanishes); there are obtained
6n
equations of equilibrium for the
6n
unknowns of the problem (corresponding to the position of equilibrium and to the
constraint forces). In the plane case, there remain only
3n
equations of equilibrium.
Taking into account the principle of action and reaction, some of the unknowns may
affect two solids in linkage. The solving of the system of
6n
equations may –
sometimes – require a very arduous computation.
In the method of equilibrium of parts, subsystems of the considered system are
isolated, introducing the corresponding external and internal given and constraint
forces, and necessary conditions of global equilibrium (the torsor of the external given
and constraint forces with respect to an arbitrary pole vanishes) are written for each
subsystem. Choosing conveniently the subsystems, one can obtain thus some constraint
forces (selecting the forces which we wish to determine) from a system of equations
with a smaller number of unknowns. In the method of rigidity (which is, in fact, a
particular case of the previous method, corresponding to the case in which the part is
the whole system), only six equations of equilibrium are written, which may be
sufficient to obtain the external constraint forces of the given mechanical system; the
application of this method as a first attempt to compute is thus justified. We notice that
the equations which are obtained by the method of equilibrium of parts or, in particular,