Mechanical Sytems, Classical Models
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Some applications connected to important phenomena of nature are presented, and this also gives one the possibility to solve problems of interest from the technical, engineering point of view. In this form, the book becomes - we dare say - a unique outline of the literature in the field; the author wishes to present the most important aspects connected with the study of mechanical systems, mechanics being regarded as a science of nature, as well as its links to other sciences of nature.
Implications in technical sciences are not neglected. This book examines the study of mechanical systems as well as its links to other sciences of nature. It presents the fundamentals behind how mechanical theories are constructed and details the solving methodology and mathematical tools used: vectors, tensors and notions of field theory. It also offers continuous and discontinuous phenomena as well as various mechanical magnitudes in a unitary form by means of the theory of distributions. Read more Read less.
Classical mechanics - Wikipedia
Product details Paperback: pages Publisher: Springer; Softcover reprint of hardcover 1st ed. Review From the reviews: "This book is the first volume of a treatise on the classical theory of mechanical systems. Audience: Librarians, and researchers interested in the fundamentals of mechanics See all Product description. No customer reviews. Share your thoughts with other customers. Write a customer review. Discover the best of shopping and entertainment with Amazon Prime. Prime members enjoy FREE Delivery on millions of eligible domestic and international items, in addition to exclusive access to movies, TV shows, and more.
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Get to Know Us. Classical mechanics provides extremely accurate results when studying large objects that are not extremely massive and speeds not approaching the speed of light. When the objects being examined have about the size of an atom diameter, it becomes necessary to introduce the other major sub-field of mechanics : quantum mechanics. To describe velocities that are not small compared to the speed of light, special relativity is needed. In case that objects become extremely massive, general relativity becomes applicable.
However, a number of modern sources do include relativistic mechanics into classical physics, which in their view represents classical mechanics in its most developed and accurate form. The following introduces the basic concepts of classical mechanics.
For simplicity, it often models real-world objects as point particles objects with negligible size. The motion of a point particle is characterized by a small number of parameters : its position, mass , and the forces applied to it. Each of these parameters is discussed in turn. In reality, the kind of objects that classical mechanics can describe always have a non-zero size.
The physics of very small particles, such as the electron , is more accurately described by quantum mechanics. Objects with non-zero size have more complicated behavior than hypothetical point particles, because of the additional degrees of freedom , e. However, the results for point particles can be used to study such objects by treating them as composite objects, made of a large number of collectively acting point particles.
The center of mass of a composite object behaves like a point particle. Classical mechanics uses common-sense notions of how matter and forces exist and interact.
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It assumes that matter and energy have definite, knowable attributes such as location in space and speed. Non-relativistic mechanics also assumes that forces act instantaneously see also Action at a distance. The position of a point particle is defined in relation to a coordinate system centered on an arbitrary fixed reference point in space called the origin O. A simple coordinate system might describe the position of a particle P with a vector notated by an arrow labeled r that points from the origin O to point P. In general, the point particle does not need to be stationary relative to O.
In cases where P is moving relative to O , r is defined as a function of t , time. In pre-Einstein relativity known as Galilean relativity , time is considered an absolute, i. The velocity , or the rate of change of position with time, is defined as the derivative of the position with respect to time:. In classical mechanics, velocities are directly additive and subtractive.
Velocities are directly additive as vector quantities ; they must be dealt with using vector analysis. The acceleration , or rate of change of velocity, is the derivative of the velocity with respect to time the second derivative of the position with respect to time :. Acceleration represents the velocity's change over time. Velocity can change in either magnitude or direction, or both. Occasionally, a decrease in the magnitude of velocity " v " is referred to as deceleration , but generally any change in the velocity over time, including deceleration, is simply referred to as acceleration.
While the position, velocity and acceleration of a particle can be described with respect to any observer in any state of motion, classical mechanics assumes the existence of a special family of reference frames in which the mechanical laws of nature take a comparatively simple form.
These special reference frames are called inertial frames. An inertial frame is an idealized frame of reference within which an object has no external force acting upon it. Because there is no external force acting upon it, the object has a constant velocity; that is, it is either at rest or moving uniformly in a straight line. A key concept of inertial frames is the method for identifying them. For practical purposes, reference frames that do not accelerate with respect to distant stars an extremely distant point are regarded as good approximations to inertial frames.
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Non-inertial reference frames accelerate in relation to an existing inertial frame. They form the basis for Einstein's relativity. Due to the relative motion, particles in the non-inertial frame appear to move in ways not explained by forces from existing fields in the reference frame. Hence, it appears that there are other forces that enter the equations of motion solely as a result of the relative acceleration. These forces are referred to as fictitious forces , inertia forces, or pseudo-forces. Consider two reference frames S and S'.
For observers in each of the reference frames an event has space-time coordinates of x , y , z , t in frame S and x' , y' , z' , t' in frame S'. This set of formulas defines a group transformation known as the Galilean transformation informally, the Galilean transform. The limiting case applies when the velocity u is very small compared to c , the speed of light.
For some problems, it is convenient to use rotating coordinates reference frames. Thereby one can either keep a mapping to a convenient inertial frame, or introduce additionally a fictitious centrifugal force and Coriolis force. A force in physics is any action which causes an object's velocity to change; that is, to accelerate.
A force originates from within a field , such as an electro-static field caused by static electrical charges , electro-magnetic field caused by moving charges , or gravitational field caused by mass , among others. Newton was the first to mathematically express the relationship between force and momentum. Some physicists interpret Newton's second law of motion as a definition of force and mass, while others consider it a fundamental postulate, a law of nature.
The quantity m v is called the canonical momentum. The net force on a particle is thus equal to the rate of change of the momentum of the particle with time. So long as the force acting on a particle is known, Newton's second law is sufficient to describe the motion of a particle. Once independent relations for each force acting on a particle are available, they can be substituted into Newton's second law to obtain an ordinary differential equation , which is called the equation of motion.
As an example, assume that friction is the only force acting on the particle, and that it may be modeled as a function of the velocity of the particle, for example:. Then the equation of motion is. This means that the velocity of this particle decays exponentially to zero as time progresses. In this case, an equivalent viewpoint is that the kinetic energy of the particle is absorbed by friction which converts it to heat energy in accordance with the conservation of energy , and the particle is slowing down. This expression can be further integrated to obtain the position r of the particle as a function of time.
Important forces include the gravitational force and the Lorentz force for electromagnetism. Illustrations of the weak form of Newton's third law are often found for magnetic forces. More generally, if the force varies as a function of position as the particle moves from r 1 to r 2 along a path C , the work done on the particle is given by the line integral. If the work done in moving the particle from r 1 to r 2 is the same no matter what path is taken, the force is said to be conservative. Gravity is a conservative force, as is the force due to an idealized spring , as given by Hooke's law.
The force due to friction is non-conservative. The kinetic energy E k of a particle of mass m travelling at speed v is given by. For extended objects composed of many particles, the kinetic energy of the composite body is the sum of the kinetic energies of the particles. The work—energy theorem states that for a particle of constant mass m , the total work W done on the particle as it moves from position r 1 to r 2 is equal to the change in kinetic energy E k of the particle:. Conservative forces can be expressed as the gradient of a scalar function, known as the potential energy and denoted E p :.follow
Mechanical Systems, Classical Models: Volume III: Analytical Mechanics
If all the forces acting on a particle are conservative, and E p is the total potential energy which is defined as a work of involved forces to rearrange mutual positions of bodies , obtained by summing the potential energies corresponding to each force. This result is known as conservation of energy and states that the total energy ,. It is often useful, because many commonly encountered forces are conservative.