Isaac Newton and the Revolution in Physics
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Classical Mechanics
Classical Mechanics Hyoungsoon Choi Spring, 2014 Contents 1 Introduction4 1.1 Kinematics and Kinetics . .5 1.2 Kinematics: Watching Wallace and Gromit ............6 1.3 Inertia and Inertial Frame . .8 2 Newton's Laws of Motion 10 2.1 The First Law: The Law of Inertia . 10 2.2 The Second Law: The Equation of Motion . 11 2.3 The Third Law: The Law of Action and Reaction . 12 3 Laws of Conservation 14 3.1 Conservation of Momentum . 14 3.2 Conservation of Angular Momentum . 15 3.3 Conservation of Energy . 17 3.3.1 Kinetic energy . 17 3.3.2 Potential energy . 18 3.3.3 Mechanical energy conservation . 19 4 Solving Equation of Motions 20 4.1 Force-Free Motion . 21 4.2 Constant Force Motion . 22 4.2.1 Constant force motion in one dimension . 22 4.2.2 Constant force motion in two dimensions . 23 4.3 Varying Force Motion . 25 4.3.1 Drag force . 25 4.3.2 Harmonic oscillator . 29 5 Lagrangian Mechanics 30 5.1 Configuration Space . 30 5.2 Lagrangian Equations of Motion . 32 5.3 Generalized Coordinates . 34 5.4 Lagrangian Mechanics . 36 5.5 D'Alembert's Principle . 37 5.6 Conjugate Variables . 39 1 CONTENTS 2 6 Hamiltonian Mechanics 40 6.1 Legendre Transformation: From Lagrangian to Hamiltonian . 40 6.2 Hamilton's Equations . 41 6.3 Configuration Space and Phase Space . 43 6.4 Hamiltonian and Energy . 45 7 Central Force Motion 47 7.1 Conservation Laws in Central Force Field . 47 7.2 The Path Equation . -
Trinity Physics – A.C.H. Cheung and G.L. Squires Isaac Newton
Trinity Physics – A.C.H. Cheung and G.L. Squires Isaac Newton Isaac Newton was born in Woolsthorpe Manor in the small village of Colsterworth, near Grantham, on Christmas day, 1642. His father, whose family had farmed a modest estate for several generations, died three months before Newton was born. At the age of twelve he was sent to the King’s School at Grantham, which still exists and where his signature can be seen, carved on the library wall. There, under the influence of the perceptive schoolmaster, Henry Stokes, his intellectual interests were gradually awakened. He was fascinated with the forces of moving air and water, and more abstractly with the concept of time. He built kites, a sundial, a water-clock, and a model windmill driven by a mouse urged on by corn placed in front of it. When he was seventeen his mother called him home, intending that he should manage the family farm. Fortunately, however, his uncle and the schoolmaster had recognised his talents, and persuaded her to allow him to go to university. In June 1661 he entered Trinity, his uncle’s alma mater, equipping himself with a lock for his desk, a quart bottle with ink to fill it, a notebook, a pound of candles, and a chamber-pot. He entered as a sub-sizar, a student who paid his way by waiting and performing menial duties for fellows and fellow commoners (wealthy students who dined on high table). He was awarded a scholarship in 1664, given a livery allowance of 13s 4d (67p) per annum, a stipend of the same amount, and commons, i.e. -
The Development of the Action Principle a Didactic History from Euler-Lagrange to Schwinger Series: Springerbriefs in Physics
springer.com Walter Dittrich The Development of the Action Principle A Didactic History from Euler-Lagrange to Schwinger Series: SpringerBriefs in Physics Provides a philosophical interpretation of the development of physics Contains many worked examples Shows the path of the action principle - from Euler's first contributions to present topics This book describes the historical development of the principle of stationary action from the 17th to the 20th centuries. Reference is made to the most important contributors to this topic, in particular Bernoullis, Leibniz, Euler, Lagrange and Laplace. The leading theme is how the action principle is applied to problems in classical physics such as hydrodynamics, electrodynamics and gravity, extending also to the modern formulation of quantum mechanics 1st ed. 2021, XV, 135 p. 23 illus., 1 illus. and quantum field theory, especially quantum electrodynamics. A critical analysis of operator in color. versus c-number field theory is given. The book contains many worked examples. In particular, the term "vacuum" is scrutinized. The book is aimed primarily at actively working researchers, Printed book graduate students and historians interested in the philosophical interpretation and evolution of Softcover physics; in particular, in understanding the action principle and its application to a wide range 54,99 € | £49.99 | $69.99 of natural phenomena. [1]58,84 € (D) | 60,49 € (A) | CHF 65,00 eBook 46,00 € | £39.99 | $54.99 [2]46,00 € (D) | 46,00 € (A) | CHF 52,00 Available from your library or springer.com/shop MyCopy [3] Printed eBook for just € | $ 24.99 springer.com/mycopy Order online at springer.com / or for the Americas call (toll free) 1-800-SPRINGER / or email us at: [email protected]. -
Faith-Based Unit on Isaac Newton
Marbles For Good Downloads are a work in progress. Please send your ideas and feedback to author Rich Maxwell. [email protected] Faith-based Unit on Isaac Newton Gravity explains the motions of the planets, but it cannot explain who set the planets in motion. God governs all things and knows all that is or can be done. – Isaac Newton It is widely held that Isaac Newton was one of the greatest scientists who ever lived. Unfortunately, less is written about his devotion to God. From a very early age, he learned to read from the Bible and in his lifetime, spent more time on theology than on science. Newton’s driving force; behind all of his discoveries and inventions, was to know God and God’s Creation. Sarah Dry in The Newton Papers writes, “Newton wrote roughly 10 million words. He in fact wrote over 10,000 letters. Only 3 million words are related to science and math. Over half of the writing, 5 million of the 10 million words, are about God.” Christianity Today add, “Newton wrote more than 1.3 million words on biblical subjects. Isaac Newton Pursued God “’You shall love the Lord your God with all your heart, with all your soul, and with all your mind.’ This is the first and great commandment. And the second is like it: ‘You shall love your neighbor as yourself.’ On these two commandments hang all the Law and the Prophets.” (Matthew 22:37-39) Introduction: More than 300 years ago, very early on a Christmas morning, a baby boy was born on a farm in England. -
Newton, Isaac, Sir (1642 – 1727), Natural Philosopher, Mathematician and Astronomer, Was Born at Woolsthorpe Manor, Near Colsterworth [Ketteringham, 1995]
Newton, Isaac, Sir (1642 – 1727), natural philosopher, mathematician and astronomer, was born at Woolsthorpe Manor, near Colsterworth [Ketteringham, 1995]. He attended School in Grantham and continued his studies at Cambridge University. Shortly after Newton graduated in 1665, Cambridge University was closed as a precaution against the Great Plague and Newton returned to Woolsthorpe, where during the next 18 months, he developed the method of “fluxions”, the basis of the calculus. He also continued his studies on light and optics, including the famous experiment in which he passed a beam of sunlight through a prism to split white light into its constituent colours. Perhaps most famous of all, he observed the apple fall, which led him to develop the concept of gravitation [English, 1977; See also Cambridge University Library; Fara; Maury; Newton Project; O’Connor and Robertson; Parsons; ODNB] Sites associated with Newton: There are several sites in Lincolnshire with connections with Newton, especially in the vicinity of Colsterworth and Grantham. Woolsthorpe Manor: In addition to the Manor House, there is also a Science Discovery Centre and exhibition [National Trust; Tanford and Reynolds]. Address: Woolsthorpe Manor, 23 Newton Way, Woolsthorpe-by-Colsterworth, nr Grantham, Lincs NG33 5NR Tel 01476 860338 E [email protected] Website: http://www.nationaltrust.org.uk/scripts/nthandbook.dll?ACTION=PROPERTY&PROPERTYID=82 Colsterworth Parish Church: Inside the church, mounted on the wall in a small gangway at the rear of the organ, is a sundial made by Isaac Newton as a boy. The sundial was formerly on the south front of Woolsthorpe Manor, but was moved to the church in 1877 [Antram]. -
Some Insights from Total Collapse
Some insights from total collapse S´ergio B. Volchan Abstract We discuss the Sundman-Weierstrass theorem of total collapse in its histor- ical context. This remarkable and relatively simple result, a type of stability criterion, is at the crossroads of some interesting developments in the gravi- tational Newtonian N-body problem. We use it as motivation to explore the connections to such important concepts as integrability, singularities and typ- icality in order to gain some insight on the transition from a predominantly quantitative to a novel qualitative approach to dynamical problems that took place at the end of the 19th century. Keywords: Celestial Mechanics; N-body problem; total collapse, singularities. I Introduction Celestial mechanics is one of the treasures of physics. With a rich and fascinating history, 1 it had a pivotal role in the very creation of modern science. After all, it was Hooke’s question on the two-body problem and Halley’s encouragement (and financial resources) that eventually led Newton to publish the Principia, a water- shed. 2 Conversely, celestial mechanics was the testing ground par excellence for the new mechanics, and its triumphs in explaining a wealth of phenomena were decisive in the acceptance of the Newtonian synthesis and the “clockwork universe”. arXiv:0803.2258v1 [physics.hist-ph] 14 Mar 2008 From the beginning, special attention was paid to the N-body problem, the study of the motion of N massive bodies under mutual gravitational forces, taken as a reliable model of the the solar system. The list of scientists that worked on it, starting with Newton himself, makes a veritable hall of fame of mathematics and physics; also, a host of concepts and methods were created which are now part of the vast heritage of modern mathematical-physics: the calculus, complex variables, the theory of errors and statistics, differential equations, perturbation theory, potential theory, numerical methods, analytical mechanics, just to cite a few. -
The Phase Space Elementary Cell in Classical and Generalized Statistics
Entropy 2013, 15, 4319-4333; doi:10.3390/e15104319 OPEN ACCESS entropy ISSN 1099-4300 www.mdpi.com/journal/entropy Article The Phase Space Elementary Cell in Classical and Generalized Statistics Piero Quarati 1;2;* and Marcello Lissia 2 1 DISAT, Politecnico di Torino, C.so Duca degli Abruzzi 24, Torino I-10129, Italy 2 Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari, Monserrato I-09042, Italy; E-Mail: [email protected] * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +39-0706754899; Fax: +39-070510212. Received: 05 September 2013; in revised form: 25 September 2013/ Accepted: 27 September 2013 / Published: 15 October 2013 Abstract: In the past, the phase-space elementary cell of a non-quantized system was set equal to the third power of the Planck constant; in fact, it is not a necessary assumption. We discuss how the phase space volume, the number of states and the elementary-cell volume of a system of non-interacting N particles, changes when an interaction is switched on and the system becomes or evolves to a system of correlated non-Boltzmann particles and derives the appropriate expressions. Even if we assume that nowadays the volume of the elementary cell is equal to the cube of the Planck constant, h3, at least for quantum systems, we show that there is a correspondence between different values of h in the past, with important and, in principle, measurable cosmological and astrophysical consequences, and systems with an effective smaller (or even larger) phase-space volume described by non-extensive generalized statistics. -
Isaac Newton
Isaac Newton Isaac Newton From Wikipedia, the free encyclopedia Sir Isaac Newton , PRS, (4 January 1643 - 31 March 1727) [OS: 25 December 1642 - 20 March 1727] was an English mathematician, physicist, astronomer, alchemist, chemist, inventor, and natural philosopher who is generally regarded as one of the most influential scientists and mathematicians in history.. Newton wrote the Philosophiae Naturalis Principia Mathematica in which he described universal gravitation and the three laws of motion, laying the groundwork for classical mechanics. By deriving Kepler's laws of planetary motion from this system, he was the first to show that the motion of objects on Earth and of celestial bodies are governed by the same set of natural laws. The unifying and deterministic power of his laws was integral to the scientific revolution and the advancement of heliocentrism. Among other scientific discoveries, Newton realized that the spectrum of colours observed when white light passes through a prism is inherent in the white light and not added by the prism (as Roger Bacon had claimed in the 13th century), and notably argued that light is composed of particles. He also developed a law of cooling, describing the rate of cooling of objects when exposed to air. He enunciated the principles of conservation of momentum and angular momentum. Finally, he studied the speed of sound in air, and voiced a theory of the origin of stars. Despite this renown in mainstream science, Newton spent more time working on either alchemy or chemistry, than physics. Newton played a major role in the history of calculus, sharing credit with Gottfried Leibniz. -
A Re-Interpretation of the Concept of Mass and of the Relativistic Mass-Energy Relation
A re-interpretation of the concept of mass and of the relativistic mass-energy relation 1 Stefano Re Fiorentin Summary . For over a century the definitions of mass and derivations of its relation with energy continue to be elaborated, demonstrating that the concept of mass is still not satisfactorily understood. The aim of this study is to show that, starting from the properties of Minkowski spacetime and from the principle of least action, energy expresses the property of inertia of a body. This implies that inertial mass can only be the object of a definition – the so called mass-energy relation - aimed at measuring energy in different units, more suitable to describe the huge amount of it enclosed in what we call the “rest-energy” of a body. Likewise, the concept of gravitational mass becomes unnecessary, being replaceable by energy, thus making the weak equivalence principle intrinsically verified. In dealing with mass, a new unit of measurement is foretold for it, which relies on the de Broglie frequency of atoms, the value of which can today be measured with an accuracy of a few parts in 10 9. Keywords Classical Force Fields; Special Relativity; Classical General Relativity; Units and Standards 1. Introduction Albert Einstein in the conclusions of his 1905 paper “Ist die Trägheit eines Körpers von seinem Energieinhalt abhängig?” (“Does the inertia of a body depend upon its energy content? ”) [1] says “The mass of a body is a measure of its energy-content ”. Despite of some claims that the reasoning that brought Einstein to the mass-energy relation was somehow approximated or even defective (starting from Max Planck in 1907 [2], to Herbert E. -
Sir Isaac Newton Did His Best Work While Working from Home During a Pandemic
Sir Isaac Newton did his best work while working from home during a pandemic. - The Washington Post 3/23/20, 10:32 AM Democracy Dies in Darkness During a pandemic, Isaac Newton had to work from home, too. He used the time wisely. By Gillian Brockell March 12, 2020 at 2:18 p.m. EDT Isaac Newton was in his early 20s when the Great Plague of London hit. He wasn’t a “Sir” yet, didn’t have that big formal wig. He was just another college student at Trinity College, Cambridge. It would be another 200 years before scientists discovered the bacteria that causes plague, but even without knowing exactly why, folks back then still practiced some of the same things we do to avoid illness. In 1665, it was a version of “social distancing” — a public health tool making a comeback this week as governments, schools and many businesses, including The Washington Post, send people home to try to slow the spread of the novel coronavirus. https://www.washingtonpost.com/history/2020/03/12/during-pandemic-isaac-newton-had-work-home-too-he-used-time-wisely/ Page 1 of 7 Sir Isaac Newton did his best work while working from home during a pandemic. - The Washington Post 3/23/20, 10:32 AM Cambridge sent students home to continue their studies. For Newton, that meant Woolsthorpe Manor, the family estate about 60 miles northwest of Cambridge. AD Without his professors to guide him, Newton apparently thrived. The year-plus he spent away was later referred to as his annus mirabilis, the “year of wonders.” First, he continued to work on mathematical problems he had begun at Cambridge; the papers he wrote on this became early calculus. -
NEWTON a Cura Di Roberto Maiocchi Grandangolo
GRANDANGOLO 27 NEWTON a cura di Roberto Maiocchi Grandangolo Vol. 27 – Newton © 2014 RCS MediaGroup S.p.A. Divisione Quotidiani, Milano È vietata la riproduzione dell’opera o di parte di essa, con qualsiasi mezzo, compresa stampa, copia fotostatica, microfilm e memorizzazione elettronica, se non espressamente autorizzata dall’editore. Tutti i diritti di copyright sono riservati. Ogni violazione sarà perseguita a termini di legge. Edizione speciale per Il Corriere della Sera pubblicata su licenza di Out of Nowhere S.r.l. ISBN: 9788861266117 Responsabile area collaterali Corriere della Sera: Luisa Sacchi Editor: Barbara Brambilla, Fabrizia Spina Focus e pagine scelte a cura di Roberto Maiocchi Concept e realizzazione: Out of Nowhere Progetto grafico e impaginazione: Marco Pennisi & C. Ideazione e coordinamento editoriale: Giorgio Rivieccio Redazione: Flavia Fiocchi NEWTON, LA LEGGE CHE UNIFICÒ TERRA E CIELO Di Armando Torno Matematico, fisico, astronomo ma anche filosofo (occorre aggiungere direttore della Zecca Reale, teologo e con interessi per l’alchimia), Sir Isaac Newton è ricordato persino dai bambini grazie all’aneddoto della mela che cadde dall’albero sulla sua testa, inducendolo a pensare alla gravitazione universale e ai motivi per i quali la Luna non precipitasse anch’essa come un frutto. Nato il 25 dicembre 1642 (morirà nel 1727), fu il primo a dimostrare che i movimenti della Terra e degli altri corpi celesti obbediscono alle medesime leggi di natura. Ebbe un ruolo fondamentale in fisica ma la sua opera contribuì a cambiare le prospettive della filosofia portando a compimento la rivoluzione scientifica cominciata con Copernico; anzi la pubblicazione del suo libro Principi matematici della filosofia naturale (1687) rappresenta il culmine di questo processo di idee, fondamentale per il mondo moderno e contemporaneo. -
Non-Equilibrium Continuum Physics
Non-Equilibrium Continuum Physics Lecture notes by Eran Bouchbinder (Dated: June 10, 2019) Abstract This course is intended to introduce graduate students to the essentials of modern continuum physics, with a focus on non-equilibrium solid mechanics and within a thermodynamic perspective. Emphasis will be given to general concepts and principles, such as conservation laws, symmetries, material frame-indifference, thermodynamics, dissipation inequalities and non-equilibrium behaviors, stability criteria and configurational forces. Examples will cover a wide range of physical phenomena and applications in diverse disciplines. The power of field theory as a mathematical structure that does not make direct reference to microscopic length scales well below those of the phenomenon of interest will be highlighted. Some basic mathematical tools and methods will be introduced. The course will be self-contained and will highlight essential ideas and basic physical intuition. Together with courses on fluid mechanics and soft condensed matter, a broad background and understanding of continuum physics will be established. The course will be given within a framework of 12-13 two-hour lectures and 12-13 two-hour tutorial sessions with a focus on problem-solving. No prior knowledge of the subject is assumed. Basic knowledge of statistical thermodynamics, vector calculus, differential equations and complex analysis is required. These extended lecture notes are self-contained and in principle no textbook will be followed. Some general references (mainly for the first half of the course), can be found below. 1 Contents I. Introduction: Background and motivation 4 II. Mathematical preliminaries: Tensor Analysis 7 III. Motion, deformation and stress 13 A.