Conservation of Mechanical Energy
Conservation of mechanical energy is assumed if kinetic energy
(T) and potential energy (V) change back and forth in a conservative
system (the dissipation of energy is considered negligible). Equation
1.3.22 formalizes such a situation, where position 1 is the initial state
and position 2 is the ?nal state. The reference (datum) should be chosen to
reduce the number of terms in the equation.
T1 + V1 = T2 + V2
Linear and Angular Momentum Methods
The concept of linear momentum is useful in engineering when the
accelerations of particles are not known but the velocities are.
The linear momentum is derived from Newtons second law,
G = mv
The time rate of change of linear momentum is equal to force.
When mv is constant, the conservation of momentum equation results,

The method of angular momentum is based on the momentum of a
particle about a ?xed point, using the vector product in the general case
(Figure 1.3.8).
Ho = r x mv

FIGURE 1.3.8 De?nition of angular momentum for a particle.
The angular momentum equation can be solved using a scalar
method if the motion of the particle remains in a plane,

If the particle does not remain in a plane, then the general space motion
equations apply. They are derived from the cross-product r ? mv,

Time Rate of Change of Angular Momentum
In general, a force acting on a particle changes its angular momentum:
the time rate of change of angular momentum of a particle is equal to the
sum of the moments of the forces acting on the particle.

A special case is when the sum of the moments about point O is zero.
This is the conservation of angular momentum. In this case
(motion under a central force), if the distance r increases, the velocity
must decrease, and vice versa.
Impulse and Momentum
Impulse and momentum are important in considering the motion of
particles in impact. The linear impulse and momentum equation is

Conservation of Total Momentum of Particles
Conservation of total momentum occurs when the initial
momentum of n particles is equal to the ?nal momentum of those same
n particles,

When considering the response of two deformable bodies to direct
central impact, the coef?cient of restitution is used. This coef?cient e
relates the initial velocities of the particles to the ?nal velocities,

For real materials, 0 < e < 1. If both bodies are perfectly elastic, e = 1,
and if either body is perfectly plastic, e = 0.
Kinetics of Systems of Particles
There are three distinct types of systems of particles: discrete particles,
continuous particles in ?uids, and continuous particles in rigid or deformable
bodies. This section considers methods for discrete particles that have
relevance to the mechanics of solids. Methods involving particles in
rigid bodies will be discussed in later sections.
Newtons Second Law Applied to a System of Particles
Newtons second law can be extended to systems of particles,

Motion of the Center of Mass
The center of mass of a system of particles moves under the action of
internal and external forces as if the total mass of the system and all the
external forces were at the center of mass. Equation 1.3.32
de?nes the position, velocity, and acceleration of the center of mass of
a system of particles.

Work and Energy Methods for a System of Particles
Gravitational Potential Energy. The gravitational potential energy of
a system of particles is the sum of the potential energies of the individual
particles of the system.

where g = acceleration of gravity
yC = vertical position of center of mass with respect to a reference level
Kinetic Energy. The kinetic energy of a system of particles is the
sum of the kinetic energies of the individual particles of the system with
respect to a ?xed reference frame,

A translating reference frame located at the mass center C of a
system of particles can be used advantageously, with

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