History and Evolution of Concepts in Physics by Harry Varvoglis

By Harry Varvoglis

» in accordance with a winning direction held via the author
» excellent for giving first 12 months scholars a "flavor" of the elemental concepts
» Unifies the advance of varied very important fields inside a typical old framework
» a different technique that may additionally entice the professional and the layperson
» "Witty, fascinating and useful!" [referee remark]

Our knowing of nature, and specifically of physics and the legislation governing it, has replaced substantially because the days of the traditional Greek typical philosophers. This publication explains how and why those alterations happened, via landmark experiments in addition to theories that - for his or her time - have been innovative. The presentation covers Mechanics, Optics, Electromagnetism, Thermodynamics, Relativity concept, Atomic Physics and Quantum Physics. The booklet locations emphasis on rules and on a qualitative presentation, instead of on arithmetic and equations. hence, even though basically addressed to people who are learning or have studied technological know-how, it may even be learn via non-specialists. the writer concludes with a dialogue of the evolution and association of universities, from precedent days until eventually this present day, and of the association and dissemination of information via clinical guides and conferences.

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L = T - W. 7 The resulting differential equations are of second order and, in the general case, they are equal in number to the degrees of freedom of the system. Therefore, for a free point mass we obtain three equations, while for a point mass forced to move on a surface we obtain two. , its total mechanical energy); so, it is represented symbolically by the relation: H ¼T þW The axiom (principle) giving the equations of motion is the same as that of Lagrangian mechanics; however, the resulting equations are first order differential equations equal in number to twice that of the degrees of freedom of the system.

5 Title page of the first edition of Philosiphiae Naturalis Principia Mathematica by I. Newton various forms of force, he found that the solutions of the equation for planetary motion were ellipses with the Sun at one focus, just as predicted by Kepler’s laws, when the force is proportional to the inverse square of the distance between the two bodies (the Sun and one planet at a time), F ¼ GMSun Á mplanet =r 2 ; where G is the gravitational constant (Fig. 6). In this way, he took two major steps towards the completion of mechanics: • using his laws of dynamics, he interpreted Kepler’s laws, which until then were of purely kinematic-geometric nature, and • he eliminated the distinction between terrestrial and celestial bodies—which was introduced by Aristotle—by showing that the very same laws of physics apply to both.

Of course nothing happens abruptly in nature and, thus, the spirit of late Antiquity persisted for some time during the Middle Ages. Good examples of this are two Greek natural philosophers, Philoponus and Simplicius, and their debate, which will be presented later in this paragraph. However, science, in general, as well as arts and letters, came into a standstill, and the reason was that during the first period of Middle Ages (from the 6th to the 13th century AD), dominated a culture which was completely different from that of the Greek spirit.

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