Название: Introduction to Mechanical Vibrations
Автор: Ronald J. Anderson
Издательство: John Wiley & Sons Limited
Жанр: Физика
isbn: 9781119053644
isbn:
(1.12)
To eliminate the constraining normal force from these two equations, we multiply Equation 1.12 by
(1.14)
where it is clear that both
which is the same nonlinear equation of motion (Equation 1.11) found in Subsection 1.1.1.
1.1.3 Lagrange's Equations of Motion
In this section, we consider the use of Lagrange's2 Equations of Motion.
Lagrange's Equations, since they are based on work/energy principles, give the analyst two distinct advantages when deriving the equations of motion. First, the vector kinematic analysis is shorter than it is with a direct application of Newton's Laws since acceleration vectors need not be found. This is because the kinetic and potential energy expressions can be derived from velocity vectors and position vectors respectively. Secondly, there is no need to draw free body diagrams for each of the rigid bodies in the system because the forces of constraint between the bodies do no work and are therefore not required for the analysis.
Of course, there are also disadvantages. The method requires a great deal of differentiation, sometimes of relatively complicated functions. Some analysts prefer the kinematics of Newton's method over the differentiation required when using Lagrange's Equations. Some point to a lack of physical feeling for problems without free body diagrams as being a disadvantage of the method. Finally, if the intent of analyzing the dynamics of a system is to predict loads, which could be carried forward into a structural analysis for instance, the forces of interaction between bodies are not available from a straightforward application of Lagrange's Equations.
1.1.3.1 The Bead on a Wire via Lagrange's Equations
We consider again the bead on the semicircular wire (Figure 1.1) and derive the equation of motion using Lagrange's Equations.
Lagrange's Equation is:
where:
= the total kinetic energy of the system
= the total potential energy of the system
= a generalized coordinate
= the time derivative of
= the generalized force corresponding to a variation of
We first determine the kinetic energy of the system. This requires that we have an expression for the absolute velocity of the mass. This was done previously and the result, from Equation 1.5, is
The kinetic energy of the system is then
(1.18)
which becomes, after substitution of Equation 1.17 and some simplification,
Alternatively, using the informal approach and referring to Figure 1.3, we can see that there will be a component of velocity equal to
(1.20)
After factoring
The potential energy of the system is due to gravity only. If the datum for potential energy is taken to be at point
(1.21)
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