History of the Kinetic Theory of Gases* by Stephen G. Brush
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Biochemical Thermodynamics
Biochemical Thermodynamics Biochemical Thermodynamics By Juan S. Jiménez Biochemical Thermodynamics By Juan S. Jiménez This book first published 2020 Cambridge Scholars Publishing Lady Stephenson Library, Newcastle upon Tyne, NE6 2PA, UK British Library Cataloguing in Publication Data A catalogue record for this book is available from the British Library Copyright © 2020 by Juan S. Jiménez All rights for this book reserved. No part of this book may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the copyright owner. ISBN (10): 1-5275-5359-0 ISBN (13): 978-1-5275-5359-0 To the memory of Brígida and Francisco Jiménez CONTENTS PREFACE ..................................................................................................... x CHAPTER 1 .................................................................................................. 1 INTRODUCTION 1.1 The Atomic Theory of John Dalton and the Hypothesis of Amedeo Avogadro 1.2 The Mole and Avogadro’s Number 1.3 The ideal gas model 1.4 The Periodic Table and Initial Atomic Theories 1.5 The Hydrogen Atom and the Schrödinger Equation 1.6 Atomic Structure 1.7 Molecules CHAPTER 2 ................................................................................................ 35 ENTROPY 2.1 Systems, Properties and States 2.2 The First Law of Thermodynamics 2.3 Enthalpy 2.4 Reversible changes 2.5 The Second Law of Thermodynamics 2.6 A Particle in a One-dimensional Box 2.7 Quantum States 2.8 The Boltzmann Equation CHAPTER 3 ................................................................................................ 63 THE CHEMICAL EQUILIBRIUM 3.1 The Gibbs Function 3.2 The Chemical Potential 3.3 Chemical Equilibrium 3.4 Model Systems 3.5 The Equilibrium Constant for Chemical Reactions between Gases. -
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. -
Entropy: Ideal Gas Processes
Chapter 19: The Kinec Theory of Gases Thermodynamics = macroscopic picture Gases micro -> macro picture One mole is the number of atoms in 12 g sample Avogadro’s Number of carbon-12 23 -1 C(12)—6 protrons, 6 neutrons and 6 electrons NA=6.02 x 10 mol 12 atomic units of mass assuming mP=mn Another way to do this is to know the mass of one molecule: then So the number of moles n is given by M n=N/N sample A N = N A mmole−mass € Ideal Gas Law Ideal Gases, Ideal Gas Law It was found experimentally that if 1 mole of any gas is placed in containers that have the same volume V and are kept at the same temperature T, approximately all have the same pressure p. The small differences in pressure disappear if lower gas densities are used. Further experiments showed that all low-density gases obey the equation pV = nRT. Here R = 8.31 K/mol ⋅ K and is known as the "gas constant." The equation itself is known as the "ideal gas law." The constant R can be expressed -23 as R = kNA . Here k is called the Boltzmann constant and is equal to 1.38 × 10 J/K. N If we substitute R as well as n = in the ideal gas law we get the equivalent form: NA pV = NkT. Here N is the number of molecules in the gas. The behavior of all real gases approaches that of an ideal gas at low enough densities. Low densitiens m= enumberans tha oft t hemoles gas molecul es are fa Nr e=nough number apa ofr tparticles that the y do not interact with one another, but only with the walls of the gas container. -
Amedeo Avogadro
Amedeo Avogadro ALSO LISTED IN Physicists FAMOUS AS Chemist and Physicist NATIONALITY Italian Famous Italian Men RELIGION Roman Catholic BORN ON 09 August 1776 AD Famous 9th August Birthdays ZODIAC SIGN Leo Leo Men BORN IN Turin, Italy DIED ON 09 July 1856 AD PLACE OF DEATH Turin, Italy FATHER Filippo Avogadro MOTHER Anna Maria Vercellone SPOUSE: Felicita Mazzé Lorenzo Romano Amedeo Carlo Avogadro de Quaregna e di Cerreto, more popularly known as Amedeo Avogadro was born on August 9, 1776, in Turin, Italy. He was a gifted physicist and chemist who proposed the molecular theory, which is more popularly known as ‘Avogadro’s Law’. Although he earned a doctorate in ecclesiastical law, he developed a passion for studying mathematics and physics. He then gave up his career in law and pursued a career teaching natural physics at the Royal College of Vercelli. Years later, he was offered the chair of mathematical physics at the University of Turin. Avogadro conducted experiments in both physics and chemistry using mathematics as a basis for his findings. His hypothesis, known as the ‘Avogadro’s Law’ is recognized all over the world. He also published many works during his lifetime. The number 6.02214199 x 10^23 is named as Avogadro’s number to honor him for his contribution in molecular theory. Read on to know more about this great physicist and chemist. Read more at http://www.thefamouspeople.com/profiles/amadeo-avogadro- 532.php#09s5lE6QjEOdfSro.99 Career After studying philosophy in 1789, Amedeo Avogadro graduated in jurisprudence in 1792 and earned his doctorate in ecclesiastical law in 1796. -
Chemistry in Italy During Late 18Th and 19Th Centuries
CHEMISTRY IN ITALY DURING LATE 18TH AND 19TH CENTURIES Ignazio Renato Bellobono, CSci, CChem, FRSC LASA, Department of Physics, University of Milan. e-mail add ress : i.bell obon o@ti scali.it LASA, Dept.Dept. ofPhysics, Physics, University of Milan The birth of Electrochemistry Luigi Galvani, Alessandro Volta, and Luigi Valentino Brugnatelli From Chemistry to Radiochemistry The birth of Chemistry and Periodic Table Amedeo Avogadro and Stanislao Cannizzaro Contributions to Organic Chemistry LASA, Dept.Dept. ofPhysics, Physics, University of Milan 1737 At the Faculty of Medicine of the Bologna University, the first chair of Chemistry is establishedestablished,,andandassigned to Jacopo Bartolomeo BECCARI (1692-1766). He studied phosphorescence and the action of light on silver halides 1776 In some marshes of the Lago Maggiore, near AngeraAngera,, Alessandro VOLTA ((17451745--18271827),),hi gh school teacher of physics in Como, individuates a flammable gas, which he calls aria infiammabile. Methane is thus discovereddiscovered.. Two years laterlater,,heheis assignedassigned,,asas professor of experimental phihysicscs,,toto the UiUniversi ty of PiPavia LASA, DtDept. of PhPhys icscs,, University of Milan 1778 In aletter a letter to Horace Bénédict de Saussure, aaSwissSwiss naturalist, VOLTA introduces, beneath that of electrical capacitycapacity,, the fundamental concept of tensione elettrica (electrical tension), exactly the name that CITCE recommended for the difference of potential in an electrochemical cell. 17901790--17911791 VOLTA anticipatesanticipates,,bybyabout 10 yearsyears,,thethe GAYGAY--LUSSACLUSSAC linear de ppyendency of gas volume on tem pp,erature, at constant pressurepressure,,andandafew a fewyears later ((17951795)) anticipatesanticipates,,byby about 6years 6 years,,thethe soso--calledcalled John Dalton’s rules ((18011801))ononvapour pressure LASA, Dept.Dept. -
On the Equation of State of an Ideal Monatomic Gas According to the Quantum-Theory, In: KNAW, Proceedings, 16 I, 1913, Amsterdam, 1913, Pp
Huygens Institute - Royal Netherlands Academy of Arts and Sciences (KNAW) Citation: W.H. Keesom, On the equation of state of an ideal monatomic gas according to the quantum-theory, in: KNAW, Proceedings, 16 I, 1913, Amsterdam, 1913, pp. 227-236 This PDF was made on 24 September 2010, from the 'Digital Library' of the Dutch History of Science Web Center (www.dwc.knaw.nl) > 'Digital Library > Proceedings of the Royal Netherlands Academy of Arts and Sciences (KNAW), http://www.digitallibrary.nl' - 1 - 227 high. We are uncertain as to the cause of this differencc: most probably it is due to an nncertainty in the temperature with the absolute manometer. It is of special interest to compare these observations with NERNST'S formula. Tbe fourth column of Table II contains the pressUl'es aceord ing to this formula, calc111ated witb the eonstants whieb FALCK 1) ha~ determined with the data at bis disposal. FALOK found the following expression 6000 1 0,009983 log P • - --. - + 1. 7 5 log T - T + 3,1700 4,571 T . 4,571 where p is the pressure in atmospheres. The correspondence will be se en to be satisfactory considering the degree of accuracy of the observations. 1t does riot look as if the constants could be materially improved. Physics. - "On the equation of state oj an ideal monatomic gflS accoJ'ding to tlw quantum-the01'Y." By Dr. W. H. KEEsmr. Supple ment N°. 30a to the Oommunications ft'om the PhysicaL Labora tory at Leiden. Oommunicated by Prof. H. KAl\IERLINGH ONNES. (Communicated in the meeting of May' 31, 1913). -
Chapter 6 - Engineering Equations of State II
Introductory Chemical Engineering Thermodynamics By J.R. Elliott and C.T. Lira Chapter 6 - Engineering Equations of State II. Generalized Fluid Properties The principle of two-parameter corresponding states 50 50 40 40 30 30 T=705K 20 20 ρ T=286K L 10 10 T=470 T=191K T=329K 0 0 0 0.1 0.2 0.3 0.4 0 0.1 0.2 0.3 0.4 0.5 -10 T=133K -10 ρV Density (g/cc) Density (g/cc) VdW Pressure (bars) in Methane VdW Pressure (bars) in Pentane Critical Definitions: Tc - critical temperature - the temperature above which no liquid can exist. Pc - critical pressure - the pressure above which no vapor can exist. ω - acentric factor - a third parameter which helps to specify the vapor pressure curve which, in turn, affects the rest of the thermodynamic variables. ∂ ∂ 2 P = P = 0 and 0 at Tc and Pc Note: at the critical point, ∂ρ ∂ρ 2 T T Chapter 6 - Engineering Equations of State Slide 1 II. Generalized Fluid Properties The van der Waals (1873) Equation Of State (vdW-EOS) Based on some semi-empirical reasoning about the ways that temperature and density affect the pressure, van der Waals (1873) developed the equation below, which he considered to be fairly crude. We will discuss the reasoning at the end of the chapter, but it is useful to see what the equations are and how we use them before deriving the details. The vdW-EOS is: bρ aρ 1 aρ Z =+1 −= − ()1− bρ RT()1− bρ RT van der Waals’ trick for characterizing the difference between subcritical and supercritical fluids was to recognize that, at the critical point, ∂P ∂ 2 P = 0 and = 0 at T , P ∂ρ ∂ρ 2 c c T T Since there are only two “undetermined parameters” in his EOS (a and b), he has reduced the problem to one of two equations and two unknowns. -
On the Van Der Waals Gas, Contact Geometry and the Toda Chain
entropy Article On the van der Waals Gas, Contact Geometry and the Toda Chain Diego Alarcón, P. Fernández de Córdoba ID , J. M. Isidro * ID and Carlos Orea Instituto Universitario de Matemática Pura y Aplicada, Universidad Politécnica de Valencia, 46022 Valencia, Spain; [email protected] (D.A.); [email protected] (P.F.d.C.); [email protected] (C.O.) * Correspondence: [email protected] Received: 7 June 2018; Accepted: 16 July 2018; Published: 26 July 2018 Abstract: A Toda–chain symmetry is shown to underlie the van der Waals gas and its close cousin, the ideal gas. Links to contact geometry are explored. Keywords: van der Waals gas; contact geometry; Toda chain 1. Introduction The contact geometry of the classical van der Waals gas [1] is described geometrically using a five-dimensional contact manifold M [2] that can be endowed with the local coordinates U (internal energy), S (entropy), V (volume), T (temperature) and p (pressure). This description corresponds to a choice of the fundamental equation, in the energy representation, in which U depends on the two extensive variables S and V. One defines the corresponding momenta T = ¶U/¶S and −p = ¶U/¶V. Then, the standard contact form on M reads [3,4] a = dU + TdS − pdV. (1) One can introduce Poisson brackets on the four-dimensional Poisson manifold P (a submanifold of M) spanned by the coordinates S, V and their conjugate variables T, −p, the nonvanishing brackets being fS, Tg = 1, fV, −pg = 1. (2) Given now an equation of state f (p, T,...) = 0, (3) one can make the replacements T = ¶U/¶S, −p = ¶U/¶V in order to obtain ¶U ¶U f − , ,.. -
Physics/9803005
UWThPh-1997-52 27. Oktober 1997 History and outlook of statistical physics 1 Dieter Flamm Institut f¨ur Theoretische Physik der Universit¨at Wien, Boltzmanngasse 5, 1090 Vienna, Austria Email: [email protected] Abstract This paper gives a short review of the history of statistical physics starting from D. Bernoulli’s kinetic theory of gases in the 18th century until the recent new developments in nonequilibrium kinetic theory in the last decades of this century. The most important contributions of the great physicists Clausius, Maxwell and Boltzmann are sketched. It is shown how the reversibility and the recurrence paradox are resolved within Boltzmann’s statistical interpretation of the second law of thermodynamics. An approach to classical and quantum statistical mechanics is outlined. Finally the progress in nonequilibrium kinetic theory in the second half of this century is sketched starting from the work of N.N. Bogolyubov in 1946 up to the progress made recently in understanding the diffusion processes in dense fluids using computer simulations and analytical methods. arXiv:physics/9803005v1 [physics.hist-ph] 4 Mar 1998 1Paper presented at the Conference on Creativity in Physics Education, on August 23, 1997, in Sopron, Hungary. 1 In the 17th century the physical nature of the air surrounding the earth was es- tablished. This was a necessary prerequisite for the formulation of the gas laws. The invention of the mercuri barometer by Evangelista Torricelli (1608–47) and the fact that Robert Boyle (1627–91) introduced the pressure P as a new physical variable where im- portant steps. Then Boyle–Mariotte’s law PV = const. -
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. -
Transitions Still to Be Made Philip Ball
impacts Transitions still to be made Philip Ball A collection of many particles all interacting according to simple, local rules can show behaviour that is anything but simple or predictable. Yet such systems constitute most of the tangible Universe, and the theories that describe them continue to represent one of the most useful contributions of physics. hysics in the twentieth century will That such a versatile discipline as statisti- probably be remembered for quantum cal physics should have remained so well hid- Pmechanics, relativity and the Standard den that only aficionados recognize its Model of particle physics. Yet the conceptual importance is a puzzle for science historians framework within which most physicists to ponder. (The topic has, for example, in operate is not necessarily defined by the first one way or another furnished 16 Nobel of these and makes reference only rarely to the prizes in physics and chemistry.) Perhaps it second two. The advances that have taken says something about the discipline’s place in cosmology, high-energy physics and humble beginnings, stemming from the quantum theory are distinguished in being work of Rudolf Clausius, James Clerk important not only scientifically but also Maxwell and Ludwig Boltzmann on the philosophically, and surely that is why they kinetic theory of gases. In attempting to have impinged so forcefully on the derive the gas laws of Robert Boyle and consciousness of our culture. Joseph Louis Gay-Lussac from an analysis of But the central scaffold of modern the energy and motion of individual physics is a less familiar construction — one particles, Clausius was putting thermody- that does not bear directly on the grand ques- namics on a microscopic basis. -
Kinetic Theory of Gases and Thermodynamics
Kinetic Theory of Gases Thermodynamics State Variables Kinetic Theory of Gases and Thermodynamics Zeroth law of thermodynamics Reversible and Irreversible processes Bedanga Mohanty First law of Thermodynamics Second law of Thermodynamics School of Physical Sciences Entropy NISER, Jatni, Orissa Thermodynamic Potential Course on Kinetic Theory of Gasses and Thermodynamics - P101 Third Law of Thermodynamics Phase diagram 1/112 Principles of thermodynamics, thermodynamic state, extensive/intensive variables. internal energy, Heat, work First law of thermodynamics, heat engines Second law of thermodynamics, entropy Thermodynamic potentials References: Thermodynamics, kinetic theory and statistical thermodynamics by Francis W. Sears, Gerhard L. Salinger Thermodynamics and introduction to thermostatistics, Herbert B. Callen Heat and Thermodynamics: an intermediate textbook by Mark W. Zemansky and Richard H. Dittman About 5-7 Tutorials One Quiz (10 Marks) and 2 Assignments (5 Marks) End Semester Exam (40 Marks) Course Content Suppose to be 12 lectures. Kinetic Theory of Gases Kinetic Theory of Gases Thermodynamics State Variables Zeroth law of thermodynamics Reversible and Irreversible processes First law of Thermodynamics Second law of Thermodynamics Entropy Thermodynamic Potential Third Law of Thermodynamics Phase diagram 2/112 internal energy, Heat, work First law of thermodynamics, heat engines Second law of thermodynamics, entropy Thermodynamic potentials References: Thermodynamics, kinetic theory and statistical thermodynamics by Francis W. Sears, Gerhard L. Salinger Thermodynamics and introduction to thermostatistics, Herbert B. Callen Heat and Thermodynamics: an intermediate textbook by Mark W. Zemansky and Richard H. Dittman About 5-7 Tutorials One Quiz (10 Marks) and 2 Assignments (5 Marks) End Semester Exam (40 Marks) Course Content Suppose to be 12 lectures.