Titlebook: Lecture Notes on Newtonian Mechanics; Lessons from Modern Ilya L. Shapiro,Guilherme de Berredo-Peixoto Textbook 2013 Springer Science+Busi

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Introduction,e same applies to space measures. We assume, in this book, that the spatial measures of a given object do not change when in motion. A more general approach, where these postulates of Classical Mechanics are violated, is called Theory of Relativity.

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,Newton’s Laws,rtial reference frames. Special attention will be paid to the Equivalence Principle (which is a key notion in General Relativity), turning out to be a useful tool in solving some problems of Classical Mechanics.

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Dynamics of Rotational Movements,e angular variable. This property means that after increasing the value of the variable for a certain period (equal to . in case of an angle), the body comes back to the same position. We will formulate the laws of rotational dynamics and find the corresponding conservation law.

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2192-4791 cipline between general courses of physics and analytical mechanics, using more sophisticated mathematical tools. .The aim of this book is to prepare a self-consistent and compact text that is very useful for teachers as well as for independent study.978-1-4614-7824-9978-1-4614-7825-6Series ISSN 2192-4791 Series E-ISSN 2192-4805

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Movement in a Potential Field: Oscillations,es include harmonic oscillations in the presence of damping force and external source. We shall present a few simple examples illustrating the treatment of multidimensional oscillators by means of normal modes.

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,Central Forces and Kepler’s Laws,rbit for a weakly non-Newtonian gravitational force. This problem has very special importance in General Relativity due to the Precession of Perihelion for the Mercury and some other relativistic tests.

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