The Wave Theory of Heat: a Forgotten Stage in the Transition from the Caloric Theory to Thermodynamics
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
Physics H190 Spring 2005 Notes 1 Timeline for Nineteenth Century Physics
Physics H190 Spring 2005 Notes 1 Timeline for Nineteenth Century Physics In these notes we give a timeline of major events in 19th century physics, to orient ourselves to the way Planck and other physicists thought about physical problems in the late nineteenth century, and also to understand the open problems that existed at that time. We will start with thermal physics in the nineteenth century, which is most relevant to the story of black body radiation, although toward the end of the century thermal physics becomes mixed with electromagnetic theory. Indeed, the problem of black body radiation was fundamentally one of understanding the thermodynamics of the electromagnetic field. At the beginning of the nineteenth century, the prevailing theory of thermal physics was the caloric theory, in which heat was conceived of as a fluid, called caloric, which presumably permeated all bodies. A given body had more or less caloric, depending on its temperature. The theory gave a satisfactory accounting of a certain range of experimental data, including quantitative issues. For example, one could define a certain quantity of heat (the calorie) as the amount of heat (caloric) needed to heat one gram of water by one degree Centrigrade. If the water later cooled off by contact with colder bodies, one could say that the caloric had flowed out. It is remarkable that Carnot in 1824 gave a formulation of what is now considered the second law of thermodynamics, considering that it was based on the (defective) caloric the- ory. Of course, Carnot did not call it the second law, since the first law of thermodynamics was not known yet. -
Chapter IX Atoms, Caloric, and the Kinetic Theory of Heat
Chapter IX Atoms, Caloric, and the Kinetic Theory of Heat It troubled me as once I was, For I was once a child, Concluding how an Atom fell, And yet the Heavens held. The Heavens weighed the most by far, Yet Blue and solid stood, Without a bolt that I could prove. Would Giants understand? - Emily Dickinson The idea that there is an indivisible unit of matter, an atom, dates back to the Greeks. It was advocated by Leucippus and Democritus, and ridiculed by Aristotle. The modern theory got going around 1785-1803 with the experiments and interpretations of Lavoisier, Dalton, and Proust (Joseph the chemist, not Marcel the writer). The most important result was that chemical reactions always involved different substances in definite proportions – which Dalton interpreted as arising from the pairing of elements to form molecules, in definite proportions (1:1, 1:2, etc.) This didn't persuade many physicists, however; it was one fairly complex hypothesis to explain one type of experimental result. In addition, the postulated atoms had a size and mass smaller than anything that can be directly observed. Not observable... this sounded suspicious. Meanwhile, there was a fierce debate raging in physics about the nature of heat. Lying in a hot bath, or at the side of a hot fire, or under the hot Sun, one gets a strong impression that heat is a fluid. The fluid received an official name – caloric – and many books were written exploring the properties of caloric. For one thing, it's self-repellent – that's why heat always spreads to its - 2 - adjacent surroundings. -
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. -
Our World Is Burning
OUR WORLD IS BURNING John Scales Avery September 27, 2020 INTRODUCTION1 Two time scales The central problem which the world faces in its attempts to avoid catas- trophic climate change is a contrast of time scales. In order to save human civilization and the biosphere from the most catastrophic effects of climate change we need to act immediately, Fossil fuels must be left in the ground. Forests must be saved from destruction by beef or palm oil production. These vitally necessary actions are opposed by powerful economic inter- ests, by powerful fossil fuel corporations desperate to monetize their under- ground “assets”, and by corrupt politicians receiving money the beef or palm oil industries. However, although some disastrous effects climate change are already visible, the worst of these calamities lie in the distant future. Therefore it is difficult to mobilize the political will for quick action. We need to act immediately, because of the danger of passing tipping points beyond which climate change will become irreversible despite human efforts to control it. Tipping points are associated with feedback loops, such as the albedo effect and the methane hydrate feedback loop. The albedo effect is important in connection with whether the sunlight falling on polar seas is reflected or absorbed. While ice remains, most of the sunlight is reflected, but as areas of sea surface become ice-free, more sunlight is absorbed, leading to rising temperatures and further melting of sea ice, and so on, in a loop. The methane hydrate feedback loop involves vast quantities of the power- ful greenhouse gas methane, CH4, frozen in a crystalline form surrounded by water molecules. -
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. -
Physics, Chapter 15: Heat and Work
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Robert Katz Publications Research Papers in Physics and Astronomy 1-1958 Physics, Chapter 15: Heat and Work Henry Semat City College of New York Robert Katz University of Nebraska-Lincoln, [email protected] Follow this and additional works at: https://digitalcommons.unl.edu/physicskatz Part of the Physics Commons Semat, Henry and Katz, Robert, "Physics, Chapter 15: Heat and Work" (1958). Robert Katz Publications. 167. https://digitalcommons.unl.edu/physicskatz/167 This Article is brought to you for free and open access by the Research Papers in Physics and Astronomy at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Robert Katz Publications by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. 15 Heat and Work 15-1 The Nature of Heat Until about 1750 the concepts of heat and temperature were not clearly distinguished. The two concepts were thought to be equivalent in the sense that bodies at equal temperatures were thought to "contain" equal amounts of heat. Joseph Black (1728-1799) was the first to make a clear distinction between heat and temperature. Black believed that heat was a form of matter, which subsequently came to be called caloric, and that the change in temperature of a body when caloric was added to it was associated with a property of the body which he called the capacity. Later investigators endowed caloric with additional properties. The caloric fluid was thought to embody a kind of universal repulsive force. When added to a body, the repulsive force of the caloric fluid caused the body to expand. -
John James Waterston a Pioneer of the Kinetic Theory of Gases Jaime Wisniak*
PARA QUITARLE EL POLVO La química en la historia, para la enseñanza. John James Waterston A pioneer of the kinetic theory of gases Jaime Wisniak* Resumen mostly in straight lines, except when deflected with John James Waterston (1811-1883) puede ser consid- occasional collisions with the walls of the containing erado el último de los pioneros de la teoría cinética. vessel and with each other. The colliding particles El mejoró en forma notable la teoría desarrollada por are supposed to act upon each other only within very Herapath y demostró que la velocidad cuadrática small distances and for very short times before and media de las moléculas de un gas, puro o mezclado, after collision, their motion being free in the intervals está conectada directamente con su temperatura ab- between such distances and times (free path). The soluta. Fue el primero en publicar el teorema de duration of free paths are assumed to be indefinitely equipartición de la energía y demostró cómo su large as compared to the durations of the encounters teoría podía ser utilizada para calcular la velocidad and of the mutual actions. The motion as a whole is del sonido así como el diámetro de una molécula. conserved by reason of the absolute elasticity of the Lamentablemente su publicación fundamental su- moving particles, while the directions of the move- frió el mismo destino que la de Herapath: su rechazo ments of the individual particles are persistently por la Sociedad Real y, por tanto, desconocida por changed by their mutual collisions. Molecules of el mundo científico. Afortunadamente, Lord different gases differ in mass, but all molecules of the Rayleigh la encontró y publicó años después de la same gas have the same mass. -
MIJLPALEN in HET ONDERZOEK NAAR WARMTESTRALING De Bank Van Melloni En Infrarood Metingen Van Zwarte Stralerspectra
FACULTEIT WETENSCHAPPEN Fysica en Sterrenkunde 2010-2011 MIJLPALEN IN HET ONDERZOEK NAAR WARMTESTRALING De bank van Melloni en infrarood metingen van zwarte stralerspectra Thesis voorgelegd tot het behalen van de academische graad van Master in de Fysica en Sterrenkunde Door SIEN CROMPHOUT Promotor: Professor Dr. D. Segers Copromotor: Professor Dr. P. Smet Woord Vooraf In de eerste plaats wil ik mijn promotor Professor Dr. Danny Segers bedanken voor de kans die hij mij gegeven heeft om deze thesis in samenwerking met het Museum voor Geschiedenis van de Wetenschappen te maken. Dankzij zijn enthousiasme en feedback heb ik deze thesis tot een goed einde kunnen brengen. Ook de hulp van copromotor Professor Dr. Philippe Smet bij het uitvoeren en het interpreteren van de spectroscopie-, SEM- en XRD-metingen, het nalezen en verbeteren van de tekst en de feedback op het didactische gedeelte, was van onschatbare waarde. Daarnaast bedank ik ook graag alle medewerkers van het museum. In het bijzonder Roland voor de praktische hulp en de feedback tijdens en na de experimenten, en Alexander, zonder wie de video-opname onmogelijk zou geweest zijn. Bedankt ook aan alle mensen die het mogelijk gemaakt hebben om mijn studie met succes te voltooien: mijn ouders, familie, en vrienden die mij gesteund en/of geïnspireerd hebben in mijn keuze voor fysica. Tenslotte wil ik Ruben bedanken, niet enkel voor de onmisbare hulp bij het maken van de website en het nalezen van de tekst, maar meer nog voor de enorme steun die hij de voorbije vijf jaar voor mij betekende. Inhoud Lijst van figuren ...................................................................................................................................... 3 Lijst van tabellen ..................................................................................................................................... -
A Dynamical Systems Theory of Thermodynamics
© Copyright, Princeton University Press. No part of this book may be distributed, posted, or reproduced in any form by digital or mechanical means without prior written permission of the publisher. Chapter One Introduction 1.1 An Overview of Classical Thermodynamics Energy is a concept that underlies our understanding of all physical phenomena and is a measure of the ability of a dynamical system to produce changes (motion) in its own system state as well as changes in the system states of its surroundings. Thermodynamics is a physical branch of science that deals with laws governing energy flow from one body to another and energy transformations from one form to another. These energy flow laws are captured by the fundamental principles known as the first and second laws of thermodynamics. The first law of thermodynamics gives a precise formulation of the equivalence between heat (i.e., the transferring of energy via temperature gradients) and work (i.e., the transferring of energy into coherent motion) and states that, among all system transformations, the net system energy is conserved. Hence, energy cannot be created out of nothing and cannot be destroyed; it can merely be transferred from one form to another. The law of conservation of energy is not a mathematical truth, but rather the consequence of an immeasurable culmination of observations over the chronicle of our civilization and is a fundamental axiom of the science of heat. The first law does not tell us whether any particular process can actually occur, that is, it does not restrict the ability to convert work into heat or heat into work, except that energy must be conserved in the process. -
Thermodynamics Is the Branch of Physics Concerned with Heat and Its Relation to Energy and Work
General Concepts Thermodynamics is the branch of physics concerned with heat and its relation to energy and work. It defines macroscopic variables (such as temperature, internal energy, entropy, volume, and pressure) that characterize macroscopic substances (materials and radiation), and explains how they are related and by what laws they change with time. Thermodynamics describes the average behavior of very large numbers of microscopic constituents, and its laws can be derived from statistical mechanics. Specifically, thermodynamics focuses largely on how a heat transfer is related to various energy changes within a physical system undergoing a thermodynamic process. Such processes usually result in work being done by the system and are guided by the laws of thermodynamics. Lord Kelvin was the first to formulate a concise definition of thermodynamics in 1854: Thermo-dynamics is the subject of the relation of heat to forces acting between contiguous parts of bodies, and the relation of heat to electrical agency. Lord Kelvin is widely known for determining the correct value of absolute zero as approximately -273.15 Celsius. A lower limit to temperature was known prior to Lord Kelvin, as shown in "Reflections on the Motive Power of Heat", Sadi Carnot, ~1820, before Lord Kelvin's birth in 1824. "Reflections" used -267 as the absolute zero temperature. Absolute temperatures are stated in units of kelvin in his honor. William Thomson, 1st Baron Kelvin (1824 – 1907) Cannon boring experiment Rumford's most important scientific work took place in Munich, and centered on the nature of heat, which he contended in An Experimental Enquiry Concerning the Source of the Heat which is Excited by Friction (1798) was not the caloric of then-current scientific thinking but a form of motion.