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FrictionAh, friction. Friction is the universal scapegoat, the culprit any good physicist blames for all experimental error. Friction is the reason the world has engineers rather than just physicists. Friction can be a drag. And now that I’ve exhausted my repertoire of sardonic comments on the irksome menace that is friction, we should probably learn a thing or two about it. Friction is the force that opposes relative motion by converting kinetic energy into heat and sometimes sound and deformation. It is traditionally described by what is known as the Coulomb approximation, which states that , where is the frictional force, is the (dimensionless) coefficient of friction (most commonly , the coefficient of static friction, or , the coefficient of kinetic friction), and is the normal or support force provided by the surface an object is sliding on. The coefficient of static or kinetic friction is dependent on many factors including the two materials in question, the environmental temperature, relative speed, atmospheric conditions, and other things. Therefore it must be determined experimentally; when we work with it in labs we will either be determining it or looking it up in a reference source. Often we are concerned with the work done by friction. Since and , along the path traveled by the object in question. Since the work done by friction is path-dependent, we say that friction is a nonconservative force. If a force is identified as conservative, that means any of three equivalent things:
Conservative forces, then, are those that conserve mechanical energy, such as gravity, the electromagnetic force, and Hookian spring forces. As an example, take a mass sliding with initial velocity on a surface with . We consider the following questions:
To answer the first question, we note that , so the work done by friction is the energy dissipated. We consider that the mass has initial kinetic energy and must end with kinetic energy , so . To answer the second question, we notate as the distance the object slides as it comes to a stop. We first note that is constant and so we can pull it out of the integral leaving or . Then we calculate . We plug in the values to get . Solving for we have . To answer the final question, we consider that . We know that , so we plug in to get . Plugging in for the mass, we have for . Now and we know that , which gives . Then . |