Three Chances for Entropy [PDF]
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Network Map of Knowledge And
Humphry Davy George Grosz Patrick Galvin August Wilhelm von Hofmann Mervyn Gotsman Peter Blake Willa Cather Norman Vincent Peale Hans Holbein the Elder David Bomberg Hans Lewy Mark Ryden Juan Gris Ian Stevenson Charles Coleman (English painter) Mauritz de Haas David Drake Donald E. Westlake John Morton Blum Yehuda Amichai Stephen Smale Bernd and Hilla Becher Vitsentzos Kornaros Maxfield Parrish L. Sprague de Camp Derek Jarman Baron Carl von Rokitansky John LaFarge Richard Francis Burton Jamie Hewlett George Sterling Sergei Winogradsky Federico Halbherr Jean-Léon Gérôme William M. Bass Roy Lichtenstein Jacob Isaakszoon van Ruisdael Tony Cliff Julia Margaret Cameron Arnold Sommerfeld Adrian Willaert Olga Arsenievna Oleinik LeMoine Fitzgerald Christian Krohg Wilfred Thesiger Jean-Joseph Benjamin-Constant Eva Hesse `Abd Allah ibn `Abbas Him Mark Lai Clark Ashton Smith Clint Eastwood Therkel Mathiassen Bettie Page Frank DuMond Peter Whittle Salvador Espriu Gaetano Fichera William Cubley Jean Tinguely Amado Nervo Sarat Chandra Chattopadhyay Ferdinand Hodler Françoise Sagan Dave Meltzer Anton Julius Carlson Bela Cikoš Sesija John Cleese Kan Nyunt Charlotte Lamb Benjamin Silliman Howard Hendricks Jim Russell (cartoonist) Kate Chopin Gary Becker Harvey Kurtzman Michel Tapié John C. Maxwell Stan Pitt Henry Lawson Gustave Boulanger Wayne Shorter Irshad Kamil Joseph Greenberg Dungeons & Dragons Serbian epic poetry Adrian Ludwig Richter Eliseu Visconti Albert Maignan Syed Nazeer Husain Hakushu Kitahara Lim Cheng Hoe David Brin Bernard Ogilvie Dodge Star Wars Karel Capek Hudson River School Alfred Hitchcock Vladimir Colin Robert Kroetsch Shah Abdul Latif Bhittai Stephen Sondheim Robert Ludlum Frank Frazetta Walter Tevis Sax Rohmer Rafael Sabatini Ralph Nader Manon Gropius Aristide Maillol Ed Roth Jonathan Dordick Abdur Razzaq (Professor) John W. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. -
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. -
The Legacy of Henri Victor Regnault in the Arts and Sciences
International Journal of Arts & Sciences, CD-ROM. ISSN: 1944-6934 :: 4(13):377–400 (2011) Copyright c 2011 by InternationalJournal.org THE LEGACY OF HENRI VICTOR REGNAULT IN THE ARTS AND SCIENCES Sébastien Poncet Laboratoire M2P2, France Laurie Dahlberg Bard College Annandale, USA The 21 st of July 2010 marked the bicentennial of the birth of Henri Victor Regnault, a famous French chemist and physicist and a pioneer of paper photography. During his lifetime, he received many honours and distinctions for his invaluable scientific contributions, especially to experimental thermodynamics. Colleague of the celebrated chemist Louis-Joseph Gay- Lussac (1778-1850) at the École des Mines and mentor of William Thomson (1824-1907) at the École Polytechnique, he is nowadays conspicuously absent from all the textbooks and reviews (Hertz, 2004) dealing with thermodynamics. This paper is thus the opportunity to recall his major contributions to the field of experimental thermodynamics but also to the nascent field, in those days, of organic chemistry. Avid amateur of photography, he devoted more than twenty years of his life to his second passion. Having initially taken up photography in the 1840s as a potential tool for scientific research, he ultimately made many more photographs for artistic and self-expressive purposes than scientific ones. He was a founding member of the Société Héliographique in 1851 and of the Société Française de Photographie in 1854. Like his scientific work, his photography was quickly forgotten upon his death, but has begun to attract new respect and recognition. Keywords: Henri Victor Regnault, Organic chemistry, Thermodynamics, Paper photography. INTRODUCTION Henri Victor Regnault (1810–1878) (see Figures 1a & 1b) was undoubtedly one of the great figures of thermodynamics of all time. -
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. -
A Chronology of Significant Events in the History of Science and Technology
A Chronology of Significant Events in the History of Science and Technology c. 2725 B.C. - Imhotep in Egypt considered the first medical doctor c. 2540 B.C. - Pyramids of Egypt constructed c. 2000 B.C. - Chinese discovered magnetic attraction c. 700 B.C. - Greeks discovered electric attraction produced by rubbing amber c. 600 B.C. - Anaximander discovered the ecliptic (the angle between the plane of the earth's rotation and the plane of the solar system) c. 600 B.C. - Thales proposed that nature should be understood by replacing myth with logic; that all matter is made of water c. 585 B.C. - Thales correctly predicted solar eclipse c. 530 B.C. - Pythagoras developed mathematical theory c. 500 B.C. - Anaximenes introduced the ideas of condensation and rarefaction c. 450 B.C. - Anaxagoras proposed the first clearly materialist philosophy - the universe is made entirely of matter in motion c. 370 B.C. - Leucippus and Democritus proposed that matter is made of small, indestructible particles 335 B.C. - Aristotle established the Lyceum; studied philosophy, logic c. 300 B.C. - Euclid wrote "Elements", a treatise on geometry c. 300 B.C. - Aristarchus proposed that the earth revolves around the sun; calculated diameter of the earth c. 300 B.C. - The number of volumes in the Library of Alexandria reached 500,000 c. 220 B.C. - Archimedes made discoveries in mathematics and mechanics c. 150 A.D. - Ptolemy studied mathematics, science, geography; proposed that the earth is the center of the solar system 190 - Chinese mathematicians calculated pi -
Submission from Pat Naughtin
Inquiry into Australia's future oil supply and alternative transport fuels Submission from Pat Naughtin Dear Committee members, My submission will be short and simple, and it applies to all four terms of reference. Here is my submission: When you are writing your report on this inquiry, could you please confine yourself to using the International System Of Units (SI) especially when you are referring to amounts of energy. SI has only one unit for energy — joule — with these multiples to measure larger amounts of energy — kilojoules, megajoules, gigajoules, terajoules, petajoules, exajoules, zettajoules, and yottajoules. This is the end of my submission. Supporting material You probably need to know a few things about this submission. What is the legal situation? See 1 Legal issues. Why is this submission needed? See 2 Deliberate confusion. Is the joule the right unit to use? See 3 Chronology of the joule. Why am I making a submission to your inquiry? See: 4 Why do I care about energy issues and the joule? Who is Pat Naughtin and does he know what he's talking about? See below signature. Cheers and best wishes with your inquiry, Pat Naughtin ASM (NSAA), LCAMS (USMA)* PO Box 305, Belmont, Geelong, Australia Phone 61 3 5241 2008 Pat Naughtin is the editor of the 'Numbers and measurement' chapter of the Australian Government Publishing Service 'Style manual – for writers, editors and printers'; he is a Member of the National Speakers Association of Australia and the International Association of Professional Speakers. He is a Lifetime Certified Advanced Metrication Specialist (LCAMS) with the United States Metric Association. -
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. -
1. Lecture 1 Opening Remarks
1. LECTURE 1 OPENING REMARKS 1.1 Nature of Heat and Work Thermodynamics deals with heat and work - two processes by which a system transacts energy with its surroundings or with another system. Heat. By touching we can tell a hot body from a hotter body; we can tell a biting cold metal knob from the warm comfort of a wooden door1 on a winter morning. When a hot body comes into contact with a cold body, we often observe, it is the hot body which cools down and the cold body which warms up. Energy flows, naturally and spontaneously, from hot to cold and not and never the other way around2. Heat 3 is a process by which energy flows. Once the two bodies become equally warm, the flow stops. Thermal equilibrium obtains. Thus, an empirical notion of thermal equilibrium should have been known to man a long time ago. Work. Coming to the notion of work, we observe that when an object moves against an opposing force, work is done. • When you pull water up, from a well, against gravity, you do work. • If you want to push a car against the opposing friction, you must do work. • When you stretch a rubber band against the opposing entropic tension you do work. • When a fat man climbs up the stairs against gravity, he does work; • A fat man does more work when he climbs up the stairs than a not-so-fat man. Of course in a free fall, you do no work - you are not opposing gravity - though you will get hurt, for sure, when you hit the ground! 1 Incidentally, the door knob, the wooden door, and the cold surrounding atmosphere have been in contact with each other for so long they should have come into thermal equilibrium with each other. -
The Short History of Science
PHYSICS FOUNDATIONS SOCIETY THE FINNISH SOCIETY FOR NATURAL PHILOSOPHY PHYSICS FOUNDATIONS SOCIETY THE FINNISH SOCIETY FOR www.physicsfoundations.org NATURAL PHILOSOPHY www.lfs.fi Dr. Suntola’s “The Short History of Science” shows fascinating competence in its constructively critical in-depth exploration of the long path that the pioneers of metaphysics and empirical science have followed in building up our present understanding of physical reality. The book is made unique by the author’s perspective. He reflects the historical path to his Dynamic Universe theory that opens an unparalleled perspective to a deeper understanding of the harmony in nature – to click the pieces of the puzzle into their places. The book opens a unique possibility for the reader to make his own evaluation of the postulates behind our present understanding of reality. – Tarja Kallio-Tamminen, PhD, theoretical philosophy, MSc, high energy physics The book gives an exceptionally interesting perspective on the history of science and the development paths that have led to our scientific picture of physical reality. As a philosophical question, the reader may conclude how much the development has been directed by coincidences, and whether the picture of reality would have been different if another path had been chosen. – Heikki Sipilä, PhD, nuclear physics Would other routes have been chosen, if all modern experiments had been available to the early scientists? This is an excellent book for a guided scientific tour challenging the reader to an in-depth consideration of the choices made. – Ari Lehto, PhD, physics Tuomo Suntola, PhD in Electron Physics at Helsinki University of Technology (1971). -
Fysikaalisen Maailmankuvan Kehitys
Fysikaalisen maailmankuvan kehitys Reijo Rasinkangas 20. kesÄakuuta 2005 ii Kirjoittaja varaa tekijÄanoikeudet tekstiin ja kuviin itselleen; muuten tyÄo on kenen tahansa vapaasti kÄaytettÄavissÄa sekÄa opiskelussa ettÄa opetuksessa. Oulun yliopiston Fysikaalisten tieteiden laitoksen kÄayttÄoÄon teksti on tÄaysin vapaata. Esipuhe Fysikaalinen maailmankuva pitÄaÄa sisÄallÄaÄan kÄasityksemme ympÄarÄoivÄastÄa maa- ilmasta, maailmankaikkeuden olemuksesta aineen pienimpiin rakenneosiin ja niiden vuorovaikutuksiin. Kun vielÄa kurkotamme maailmankaikkeuden al- kuun, nÄaitÄa ÄaÄaripÄaitÄa, kosmologiaa ja kvanttimekaniikkaa, ei enÄaÄa voi erottaa toisistaan; tÄassÄa syy miksi fyysikot tavoittelevat | hieman mahtipontisesti mutta eivÄat aivan syyttÄa | 'kaiken teoriaa'. TÄamÄa johdanto fysikaaliseen maailmankuvaan etenee lÄahes kronologisessa jÄarjestyksessÄa. Aluksi tutustumme lyhyesti kehitykseen ennen antiikin aikaa. Sen jÄalkeen antiikille ja keskiajalle (johon renessanssikin kuuluu) on omat lu- kunsa. Uudelta ajalta alkaen materiaali on jaettu aikakausien pÄaÄatutkimusai- heiden mukaan lukuihin, jotka ovat osittain ajallisesti pÄaÄallekkÄaisiÄa. LiitteissÄa esitellÄaÄan mm. muutamia tieteen¯loso¯sia kÄasitteitÄa. Fysiikka tutkii luonnon perusvoimia eli -vuorovaikutuksia, niitÄa hallitse- via lakeja sekÄa niiden vÄalittÄomiÄa seurauksia. 'Puhtaan' fysiikan lisÄaksi tÄassÄa kÄasitellÄaÄan lyhyesti myÄos muita tieteenaloja. TÄahtitiede on melko hyvin edus- tettuna, koska sen kehitys on liittynyt lÄaheisesti fysiikan kehitykseen (toi- saalta jo -
Statistical Physics University of Cambridge Part II Mathematical Tripos
Preprint typeset in JHEP style - HYPER VERSION Statistical Physics University of Cambridge Part II Mathematical Tripos David Tong Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 OBA, UK http://www.damtp.cam.ac.uk/user/tong/statphys.html [email protected] { 1 { Recommended Books and Resources • Reif, Fundamentals of Statistical and Thermal Physics A comprehensive and detailed account of the subject. It's solid. It's good. It isn't quirky. • Kardar, Statistical Physics of Particles A modern view on the subject which offers many insights. It's superbly written, if a little brief in places. A companion volume, \The Statistical Physics of Fields" covers aspects of critical phenomena. Both are available to download as lecture notes. Links are given on the course webpage • Landau and Lifshitz, Statistical Physics Russian style: terse, encyclopedic, magnificent. Much of this book comes across as remarkably modern given that it was first published in 1958. • Mandl, Statistical Physics This is an easy going book with very clear explanations but doesn't go into as much detail as we will need for this course. If you're struggling to understand the basics, this is an excellent place to look. If you're after a detailed account of more advanced aspects, you should probably turn to one of the books above. • Pippard, The Elements of Classical Thermodynamics This beautiful little book walks you through the rather subtle logic of classical ther- modynamics. It's very well done. If Arnold Sommerfeld had read this book, he would have understood thermodynamics the first time round.