John James Waterston a Pioneer of the Kinetic Theory of Gases Jaime Wisniak*
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James Clerk Maxwell
James Clerk Maxwell JAMES CLERK MAXWELL Perspectives on his Life and Work Edited by raymond flood mark mccartney and andrew whitaker 3 3 Great Clarendon Street, Oxford, OX2 6DP, United Kingdom Oxford University Press is a department of the University of Oxford. It furthers the University’s objective of excellence in research, scholarship, and education by publishing worldwide. Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries c Oxford University Press 2014 The moral rights of the authors have been asserted First Edition published in 2014 Impression: 1 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, by licence or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this work in any other form and you must impose this same condition on any acquirer Published in the United States of America by Oxford University Press 198 Madison Avenue, New York, NY 10016, United States of America British Library Cataloguing in Publication Data Data available Library of Congress Control Number: 2013942195 ISBN 978–0–19–966437–5 Printed and bound by CPI Group (UK) Ltd, Croydon, CR0 4YY Links to third party websites are provided by Oxford in good faith and for information only. -
Acta Technica Jaurinensis
Acta Technica Jaurinensis Győr, Transactions on Engineering Vol. 3, No. 1 Acta Technica Jaurinensis Vol. 3. No. 1. 2010 The Historical Development of Thermodynamics D. Bozsaky “Széchenyi István” University Department of Architecture and Building Construction, H-9026 Győr, Egyetem tér 1. Phone: +36(96)-503-454, fax: +36(96)-613-595 e-mail: [email protected] Abstract: Thermodynamics as a wide branch of physics had a long historical development from the ancient times to the 20th century. The invention of the thermometer was the first important step that made possible to formulate the first precise speculations on heat. There were no exact theories about the nature of heat for a long time and even the majority of the scientific world in the 18th and the early 19th century viewed heat as a substance and the representatives of the Kinetic Theory were rejected and stayed in the background. The Caloric Theory successfully explained plenty of natural phenomena like gas laws and heat transfer and it was impossible to refute it until the 1850s when the Principle of Conservation of Energy was introduced (Mayer, Joule, Helmholtz). The Second Law of Thermodynamics was discovered soon after that explanation of the tendency of thermodynamic processes and the heat loss of useful heat. The Kinetic Theory of Gases motivated the scientists to introduce the concept of entropy that was a basis to formulate the laws of thermodynamics in a perfect mathematical form and founded a new branch of physics called statistical thermodynamics. The Third Law of Thermodynamics was discovered in the beginning of the 20th century after introducing the concept of thermodynamic potentials and the absolute temperature scale. -
Kinetyczno-Molekularnego Modelu Budowy Materii
Roskal Z. E.: Prekursorzy kinetycznej teorii gazów. Zenon E. Roskal Prekursorzy kinetycznej teorii gazów Twórcy kinetycznej teorii gazów są dobrze znani zarówno fizykom jak i filozo- fom przyrody1, ale wiedza na temat prekursorów tej teorii jest na ogół mniej dostępna i równie słabo rozpowszechniona. Według opinii S. Brusha2 kinetyczno-molekularny model budowy materii, a ściślej kinetyczną teorię gazów3, w istotny sposób inicjuje4 dopiero publikacja niemieckiego przyrodnika A. K. Kröniga z 1856. W tym roku mija zatem dokładnie 150 lat od tego wydarzenia5. Praca Kröniga nie pozostała niezauważona w XIX wieku. Powoływał się na nią – obok prac Joule’a i Clausiusa – J. C. Maxwell6. Twórcy kinetyczno-molekularnego mo- 1 W pierwszej kolejności zaliczamy w poczet twórców tej teorii R. Clausiusa (1822-1888) J. C. Maxwella (1831-1879), L. Boltzmanna (1844-1906) i J. W. Gibbsa (1839-1903). Popularne i skrótowe przedstawienie historii kinetycznej teorii gazów można znaleźć m.in. w E. Mendoza, A Sketch for a History of the Kinetic Theory of gases, ,,Physics Today’’ 14 nr 3 (1961): 36-39. 2 Por. S. G. Brush, The development of the kinetic theory of gases: III. Clausius, ,,Annals of Science’’, 14 (1958): 185-196. Na opinię tę powołuje się m.in. E. Daub, Waterston, Rankine, and Clausius on the Kinetic Theory of Gases, ,,Isis’’ 61 nr 1 (1970): 105, ale mylnie podaje, imię niemieckiego fizyka pisząc o Adolfie Krönigu. Tamże, s. 105. 3 W pierwotnym sformułowaniu tej teorii podanym przez J. C. Maxwella była ona nazywana dynamiczna teorią gazów. Taką nazwę zawierał np. tytuł wykładu Maxwella (Illustrations of the Dynamical Theory of Gases) przedstawionego w Aberdeen w 1859 r. -
TERMODYNAMIK En Kort Historik Christoffer Norberg
ISRN LUTMDN/TMHP-08/3032-SE ISSN 0282-1990 Institutionen f¨or Energivetenskaper TERMODYNAMIK en kort historik Christoffer Norberg Joules skovelanordning fr˚an 1845/7 f¨or att best¨amma den mekaniska v¨armeekvivalenten. Phil. Trans. Roy. Soc. 140 (1850). januari 2008 F¨orord Denna skrift g¨or inga anspr˚ak p˚aatt vara komplett eller utt¨ommande. D¨aremot har jag i m¨ojligaste m˚an f¨ors¨okt vara korrekt n¨ar det g¨aller ˚artal, biografiska data och prioritet av originalarbeten. F¨or en mer utt¨ommande beskrivning (fram till 1800-talets slut) re- kommenderas From Watt to Clausius av Donald Cardwell ([5]). Kommentarer och f¨orslag till korrigeringar emottages tacksamt. Portr¨att ¨ar huvudsakligen h¨amtade fr˚an Internet samt [2, 6, 25, 28, 20, 27], biografiska data v¨asentligen ur [1, 28, 7, 12, 21, 26, 30] och originalreferenser mestadels ur bibliotekss¨okningar, tillg¨angliga tidskrifter inom LU-n¨atet samt [23, 30]. 8 januari 20081 Christoffer Norberg Tel. 046-2228606 Christoff[email protected] Levnads˚ar f¨or 35 pionj¨arer inom termodynamikens historiska utveckling. Tjocka linjer motsvarar ˚aldern 20–65 ˚ar. “But although, as a matter of history, statistical mechanics owes its origin to investigations in thermodynamics, it seems eminently worthy of an independent development, both on account of the elegance and simplicity of its principles, and because it yields new results and places old truths in a new light in departments quite outside of thermodynamics.” Willard Gibbs 1Sedan tryckningen fr˚an januari 2008 har det gjorts ett par uppdateringar av biografiska data, liksom sm¨arre justeringar och till¨agg i texten samt i den bibliografiska delen; 15 december 2013. -
Nascimentos Da Fısica
56 Revista Brasileira de Ensino de F´ısica, vol. 20, no. 1, marc¸o, 1998 Nascimentos da F´ısica Jose´ Maria Filardo Bassalo Departamento de F´ısica da UFPA, 66075-900 - Belem,´ Para´ e-mail:[email protected] home-page: http://amazon.com.br/bassalo Trabalho recebido em 6 de junho de 1996 Com este trabalho, iniciamos uma nova saga. Desta vez, a exemplo do escritor uruguaio Eduardo Hughes Galeano (1940- ) em sua fantastica´ trilogia Memoria´ do Fogo (Nascimentos, 1986; As Caras e as Mascaras´ , 1985; OSeculo´ do Vento, 1988 - Editora Nova Fronteira), apresentaremos em forma de verbetes, e na ordem cronologica´ (seguindo a divisao˜ classica´ das idades historicas),´ os principais fatos (nascimentos) referentes aos conceitos f´ısicos, os quais serao˜ apresentados por temas separados. Para isso, basicamente, usaremos os dados que coletamos nos quatro tomos de nossas Cronicasˆ da F´ısica (EUFPA: 1987, 1990, 1992, 1994) e nas referenciasˆ a´ı indicadas. With this work, we begin a new saga. This time, as the Uruguayan writer Eduardo Hughes Galeano (1940- ) made in his fantastic trilogy Memoria´ do Fogo (Nascimentos, 1986; As Caras e as Mascaras´ , 1985; OSeculo´ do Vento, 1988 - Editora Nova Fronteira), we present in entries, and in chronological order (following the classical division of historical ages), the main events (births) concerned to the physical concepts, which will be presented in separated subjects. For that, basically, we use the data that we gather in our four books Cronicasˆ da F´ısica (EUFPA: 1987, 1990, 1992, 1994) and in the references therein. Idade Moderna: Calor Dalton demonstrou que se um gas´ e´ composto de uma mistura de gases, entao˜ a pressao˜ total e´ a soma das pressoes˜ Primeira Metade do Seculo´ 19 (1801-1850) parciais dos gases componentes. -
Principle of Equipartition of Energy -Dr S P Singh (Dept of Chemistry, a N College, Patna)
Principle of Equipartition of Energy -Dr S P Singh (Dept of Chemistry, A N College, Patna) Historical Background 1843: The equipartition of kinetic energy was proposed by John James Waterston. 1845: more correctly proposed by John James Waterston. 1859: James Clerk Maxwell argued that the kinetic heat energy of a gas is equally divided between linear and rotational energy. ∑ Experimental observations of the specific heat capacities of gases also raised concerns about the validity of the equipartition theorem. ∑ Several explanations of equipartition's failure to account for molar heat capacities were proposed. 1876: Ludwig Boltzmann expanded this principle by showing that the average energy was divided equally among all the independent components of motion in a system. ∑ Boltzmann applied the equipartition theorem to provide a theoretical explanation of the Dulong-Petit Law for the specific heat capacities of solids. 1900: Lord Rayleigh instead put forward a more radical view that the equipartition theorem and the experimental assumption of thermal equilibrium were both correct; to reconcile them, he noted the need for a new principle that would provide an "escape from the destructive simplicity" of the equipartition theorem. 1906: Albert Einstein provided that escape, by showing that these anomalies in the specific heat were due to quantum effects, specifically the quantization of energy in the elastic modes of the solid. 1910: W H Nernst’s measurements of specific heats at low temperatures supported Einstein's theory, and led to the widespread acceptance of quantum theory among physicists. Under the head we deal with the contributions of translational and vibrational motions to the energy and heat capacity of a molecule. -
1 the Course Is Taught on the Basis of Lecture Notes Which Can Be
1 I. SYLLABUS The course is taught on the basis of lecture notes which can be obtained from my web site ( http://www.niu.edu/ veenendaal/563.htm ). These notes contain the following topics: ∼ I. LITERATURE II. INTRODUCTION A. History up to Newton B. Daniel Bernoulli and the foundations of statistical mechanics C. History from Newton to Carnot D. Thermodynamics E. Atomism III. SYSTEMS OF NONINTERACTING ARTICLES OR SPINS A. Two-level spin system B. History of statistical mechanics: Clausius and Maxwell C. Thermal equilibrium and entropy D. History of statistical mechanics: Boltzmann E. Boltzmann factor G. Free energy H. Ideal gas I. Pressure J. The ideal gas law K. Gibbs' paradox L. History of statistical mechanics: Gibbs M. Link to classical partition function IV. Quantum mechanics A. Planck's quantum hypothesis B. Many-particle wavefunctions C. The chemical potential D. Quantum distribution functions V. Systems of interacting particles or spins A. Van der Waals gas B. Critical points C. The Ising model: mean field D. Relations between liquid-gases transition and magnetism E. Ising model: exact solution in one Dimension VI. Applications A. Superfluidity in Helium II 2 A. Literature Thermodynamics R. J. Baxter, Exactly Solved Models in Statistical Mechanics (Academic Press, London, 1982). A. H. Carter, Classical and Statistical Thermodynamics (Prentice Hall, Upper Saddle River, NJ, 2001). R. L. Pathria, Statistical Mechanics (Butterworth-Heinemann, Oxford, 1972). F. Reif, Statistical and Thermal Physics (McGraw-Hill, Boston, 1965). C. Kittel and H. Kroemer, Thermal Physics (W. H. Freeman and Company, New York, 1980) H. E. Stanley, Introduction to Phase Transitions and Critical Phenomena (Oxford University Press, Oxford, 1971). -
Ludwig Boltzmann, Transport Equation and the Second
Ludwig Boltzmann, Transport Equation and the Second law K. P. N. Murthy ∗ Theoretical Studies Section, Materials Science Division, Indira Gandhi Centre for Atomic Research, Kalpakkam 603 102, Tamilnadu, INDIA Abstract Ludwig Boltzmann had a hunch that irreversibility exhibited by a macroscopic system arises from the reversible dynamics of its microscopic constituents. He derived a nonlinear integro-differential equation - now called the Boltzmann equation - for the phase space density of the molecules of a dilute fluid. He showed that the Second law of thermodynamics emerges from Newton’s equations of motion. However Boltzmann realized that stosszahlansatz, em- ployed in the derivation, smuggles in an element of stochasticity into the transport equation. He then proposed a fully stochastic description of entropy which laid the foundation for statis- tical mechanics. Recent developments, embodied in different fluctuation theorems, have shown that Boltzmann’s hunch was, in essence, correct. Based on the invited talk given at the arXiv:cond-mat/0601566v3 [cond-mat.stat-mech] 6 Apr 2006 Sixteenth National Symposium on Radiation Physics, Meenakshi College for Women, Chennai, January 18-20, 2006. See A. K. Jena, R. Mathiyarasu and V. Gopalakrishnan (Eds.), Proc. Sixteenth National Symp. Rad. Phys., Indian Society for Radiation Physics (2006)p1. ∗[email protected] Everything existing in the Universe is the fruit of chance and necessity Diogenes Laertius IX 1 Prologue OLTZMANN transport equation has played an important role in basic and applied sciences. BIt is a nonlinear integro-differential equation for the phase space density of the molecules of a dilute gas. It remains today, an important theoretical technique for investigating non-equilibrium systems. -
Sadi Carnot's Réflexions and the Foundation of Thermodynamics
Firenze University Press www.fupress.com/substantia Historical Article Sadi Carnot’s Réflexionsand the foundation of thermodynamics Citation: P.R. Salvi, V. Schettino (2019) Sadi Carnot’s Réflexions and the foundation of thermodynamics. Substantia 3(2): 73-96. doi: 10.13128/ Pier Remigio Salvi, Vincenzo Schettino Substantia-638 Dipartimento di Chimica “Ugo Schiff”, Università di Firenze via della Lastruccia 3, Copyright: © 2019 P.R. Salvi, V. 50019 Sesto Fiorentino (FI), Italy Schettino. This is an open access, peer-reviewed article published by Firenze University Press (http://www. Abstract. The purpose of this article is to present a short review of Sadi Carnot work fupress.com/substantia) and distributed on heat engines and on the role his adherence to the caloric theory may have had. The under the terms of the Creative Com- essential points developed in the Réflexions are reviewed as forerunners of the science mons Attribution License, which per- of thermodynamics. The antecedents that may have inspired the brilliant scientific mits unrestricted use, distribution, and insights of Carnot are reviewed together with the reception of the Carnot principles in reproduction in any medium, provided the engineering and in the scientific community until the formulation of the two prin- the original author and source are credited. ciples of modern thermodynamics. Data Availability Statement: All rel- evant data are within the paper and its 1. INTRODUCTION Supporting Information files. Competing Interests: The Author(s) In several cases new important scientific theories have been outlined declare(s) no conflict of interest. starting from models or interpretative schemes that later developments have shown groundless or partially incorrect. -
Sketching the History of Statistical Mechanics and Thermodynamics
Sketching the History of Statistical Mechanics a... http://grdelin.phy.hr/~ivo/Nastava/StatistickaFiz... © 1996-2006 HyperJeff Network Sketching the History of History | Philo | Physics | Blog Statistical Mechanics [ Sources, Links, Notes ] and Thermodynamics (From about 1575 to 1980) Ideas of atomism, that heat is a mode Anti- of motion within bodies and that quity pressure is the result of such motion, are all floating around. Hero of Alexandria (see also here) writes Pneumatics, an investigation 1st on atmospheric air, summarizing a cent great deal of what was known at the AD time on syphons, pumps, the effects of heat on liquids, and engine designs. Al-Baqilani (d 1013) said to have 9th introduced atomism to the Muslim cent Kalam (perhaps influencing Leibniz). The loss of permanent magnetism 11th when materials are subjected to high The aeolipile of cent temperatures known in China. Hero F Commandine translates Hero of Alexandria's Pneumatics into Latin 1575 (translated earlier in 1547 into Italian by Aleotti). Santorre Santorio (see here also) (1561-1636) is known to have been using an early thermoscope and also writes Commentariar in artem medicinalem Galeni. Santorre writes 1612 to Galileo Galilei (1564-1642) including sketches of his device, to which Galileo replies that it was an invention of his. The priority remains unclear. 1 of 43 2018年03月27日 18:01 Sketching the History of Statistical Mechanics a... http://grdelin.phy.hr/~ivo/Nastava/StatistickaFiz... Thermoscopes of Santorio are 1615 sensitive enough to detect near-by body heat and candles. Johannes van Helmont defines "gas" 1620 (the Flemish word for chaos) for air-like substances. -
Kinetic Theory from Euler to Maxwell
Indian Journal of Chemical Technology Vol. 12, November 2005, pp. 730-742 Kinetic theory ⎯ From Euler to Maxwell Jaime Wisniak* Department of Chemical Engineering, Ben-Gurion University of the Negev, Beer-Sheva, Israel 84105 Acceptance of the kinetic theory of gases was the entrance to the development of the concepts that presently explain the structure of matter. The basic ideas of the Greek philosophers remained dormant for several centuries until Euler, Bernoulli, Herapath, Waterston, Clausius, and Maxwell, injected a sounder physical picture that led to our actual understanding of the structure of a gas. The demise of the phlogiston and caloric theories and assuming that the rebound by collision occurs without the acceptance of the kinetic theory of gases are three loss of kinetic energy or momentum. The kinetic of the main events that led to our present theory interprets the pressure, or elasticity of a gas, as understanding of the structure of matter. Here, we the aggregate of the pressures exerted by the various trace the development of the concepts of the kinetic molecules when they collide with the boundary; only theory of gases from the philosophical speculations of at relatively high pressures does the effect of the Greeks, the physical analysis of Leonhard Euler intermolecular forces become important. (1707-1783) and Daniel Bernoulli (1700-1782), to its The ideal gas laws are easily deduced from this shaping and decisive conception by James Clerk model by Newtonian mechanics, and the temperature Maxwell (1831-1879). is identified with the mean-square velocity1. All other The kinetic theory regards a mass of gas as a conclusions from the theory grow out of these collection of a great number of independently fundamental assumptions and are a direct moving minute solid particles, molecules, or atoms, consequence of them. -
James Clerk Maxwell - Wikipedia, the Free Encyclopedia Page 1 of 15
James Clerk Maxwell - Wikipedia, the free encyclopedia Page 1 of 15 James Clerk Maxwell From Wikipedia, the free encyclopedia James Clerk Maxwell of Glenlair [1] FRS FRSE (13 June James Clerk Maxwell 1831 – 5 November 1879) was a Scottish [2] physicist and mathematician. His most prominent achievement was formulating classical electromagnetic theory. This united all previously unrelated observations, experiments and equations of electricity, magnetism and even optics into a consistent theory. [3] Maxwell's equations demonstrated that electricity, magnetism and even light are all manifestations of the same phenomenon, namely the electromagnetic field. Subsequently, all other classic laws or equations of these disciplines became simplified cases of Maxwell's equations. Maxwell's achievements concerning electromagnetism have been called the "second great unification in physics", [4] after the first one realised by Isaac Newton. He was the first cousin of notable 19th century artist Jemima Blackburn. Maxwell demonstrated that electric and magnetic fields James Clerk Maxwell (1831–1879) travel through space in the form of waves, and at the Born 13 June 1831 constant speed of light. In 1865 Maxwell published A Edinburgh, Scotland Dynamical Theory of the Electromagnetic Field . It was with this that he first proposed that light was in fact Died 5 November 1879 undulations in the same medium that is the cause of electric (aged 48) and magnetic phenomena. [5] His work in producing a Cambridge, England unified model of electromagnetism is one of the greatest Citizenship British advances in physics. Nationality British Maxwell also helped develop the Maxwell –Boltzmann Fields Physics and mathematics distribution, which is a statistical means of describing Institutions Marischal College, aspects of the kinetic theory of gases.