The Perfect Gas
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Fundamentals of mechanical engineering [email protected] MOHAMMED ABASS ALI What is thermodynamics Thermodynamics is the branch of physics that studies the effects of temperature and heat on physical systems at the macroscopic scale. In addition, it also studies the relationship that exists between heat, work and energy. Thermal energy is found in many forms in today’s society including power generation of electricity using gas, coal or nuclear, heating water by gas or electric. THE BASICS OF THERMODYNAMICS Basic concepts Properties are Features of a system which include mass, volume, energy, pressure and temperature. Thermodynamics also considers other quantities that are not physical properties, such as mass flow rates and energy transfers by work and heat. Energy forms Fluids and solids can possess several forms of energy. All fluids possess energy due to their temperature and this is referred to as ‘internal energy’. They will also possess ‘ potential energy’ (PE) due to distance (z) above a datum level and if the fluid is moving at a velocity (v), it will also possess ‘kinetic energy’. If the fluid is pressurised, it will possess ‘flow energy’ (FE). Pressure and temperature are the two governing factors and internal energy can be added to FE to produce a single property called ‘enthalpy’. Internal energy The molecules of a fluid possess both kinetic energy (KE) and PE relative to an internal datum. Generally, this is regarded simply as the energy due to its temperature and the change in internal energy in a fluid that undergoes a temperature change is given by ΔU = mcΔT The total internal energy is denoted by the symbol ‘U’, which has values of J, kJ or MJ; also the specific internal energy ‘u’ has the values of kJ/kg. -
Fundamentals of Hypersonic Flow - Aerothermodynamics
FUNDAMENTALSOFHYPERSONICFLOW- AEROTHERMODYNAMICS D. G. Fletcher von Karman Institute, Belgium 1. Introduction To aid in understanding the different topics discussed in the current Lecture Series and to provide background material for interested participants who may not have specialized training in this field, a brief summary of the fundamental attributes of hypersonic flows is given. Many of the topics that are introduced in this section will be elaborated further in contributions related to specific subjects related to sustained hypersonic flight. The differencesbetweenthethermalandchemicalaspectsofhypersonicflowandsupersonic flow are therefore highlighted. The age of some of the figures used in the subsequent discussion reflect the fact that the problems of hypersonic flight are not newly discovered! Fig. 1.1 Flight trajectories for different hypersonic vehicles comparing sustained atmo- spheric flight with re-entry. The hypersonic flight regime includes atmospheric entry and re-entry, ground testing, and flight for both powered and unpowered vehicles. In the present Lecture Series, the main interest is on sustained and controlled hypersonic flight, whether for military or civil transport application. Even though it is not currently certified for flight, there is one operational hypersonic vehicle: the space shuttle of NASA. At least 20 years before the development of the shuttle a significant activity in hypersonic flight research was conducted by the US Air Force in their X-15 program. This vehicle has reached a flight Mach number of 6.7 on its final flight, which also used to test a hypersonic ramjet engine. Direct shock impingement on the pylon holding a dummy engine caused severe heating and structural damage, and this was one of many lessons learned from the program. -
4 Pressure and Viscosity
4 Pressure and Viscosity Reading: Ryden, chapter 2; Shu, chapter 4 4.1 Specific heats and the adiabatic index First law of thermodynamics (energy conservation): d = −P dV + dq =) dq = d + P dV; (28) − V ≡ ρ 1 = specific volume [ cm3 g−1] dq ≡ T ds = heat change per unit mass [ erg g−1] − s ≡ specific entropy [ erg g−1 K 1]: The specific heat at constant volume, @q −1 −1 cV ≡ [ erg g K ] (29) @T V is the amount of heat that must be added to raise temperature of 1 g of gas by 1 K. At constant volume, dq = d, and if depends only on temperature (not density), (V; T ) = (T ), then @q @ d cV ≡ = = : @T V @T V dT implying dq = cV dT + P dV: 1 If a gas has temperature T , then each degree of freedom that can be excited has energy 2 kT . (This is the equipartition theorem of classical statistical mechanics.) The pressure 1 ρ P = ρhjw~j2i = kT 3 m since 1 1 3kT h mw2i = kT =) hjw~j2i = : 2 i 2 m Therefore kT k P V = =) P dV = dT: m m Using dq = cV dT + P dV , the specific heat at constant pressure is @q dV k cP ≡ = cV + P = cV + : @T P dT m Changing the temperature at constant pressure requires more heat than at constant volume because some of the energy goes into P dV work. 19 For reasons that will soon become evident, the quantity γ ≡ cP =cV is called the adiabatic index. A monatomic gas has 3 degrees of freedom (translation), so 3 kT 3 k 5 k 5 = =) c = =) c = =) γ = : 2 m V 2 m P 2 m 3 A diatomic gas has 2 additional degrees of freedom (rotation), so cV = 5k=2m, γ = 7=5. -
AA210A Fundamentals of Compressible Flow
AA210A Fundamentals of Compressible Flow Chapter 2 -Thermodynamics of dilute gases 9/29/20 1 2.1 Introduction The power of thermodynamics comes from the fact that the change in the state of a fluid is independent of the actual physical process by which the change is achieved; thermodynamic theory is expressed in terms of perfect differentials. 2.2 Thermodynamics Piston-cylinder combination. First law of thermodynamics. 9/29/20 2 The work done by the system is the mechanical work by a force acting over a distance. When dealing with fluid flows it is convenient to work in terms of intensive (per unit mass) variables. If there is an equation of state for the substance inside the cylinder the first law is 9/29/20 3 According to Pfaff’s theorem there must exist an integrating factor such that the first law becomes a perfect differential. Once one accepts the first law and the existence of an equation of state then two new variables of state are implied; an integrating factor, the temperature, and an associated integral called entropy. The final result is the famous Gibbs equation which is the starting point for the field of thermodynamics The partial derivatives of the entropy are 9/29/20 4 2.3 The Carnot Cycle 9/29/20 5 Thermodynamic efficiency of the cycle First Law Over the cycle the change in internal energy is zero and the work done is So the efficiency is Since the temperature is constant during the heat interaction δq Q Q ds = = 1 + 2 = 0 Finally !∫ !∫ T T1 T2 9/29/20 6 2.3.1 The absolute scale of temperature For any Carnot cycle regardless of the working fluid This relation enables an absolute scale of temperature to be defined that is independent of the properties of any particular substance. -
On Classical Ideal Gases
Entropy 2013, 15, 960-971; doi:10.3390/e15030960 OPEN ACCESS entropy ISSN 1099-4300 www.mdpi.com/journal/entropy Article On Classical Ideal Gases Jacques Arnaud 1, Laurent Chusseau 2;* and Fabrice Philippe 3 1 Mas Liron, F30440 Saint Martial, France; E-Mail: [email protected] (J.A.) 2 IES, UMR n◦5214 au CNRS, Université Montpellier II, F34095 Montpellier, France 3 LIRMM, UMR n◦5506 au CNRS, 161 rue Ada, F34392 Montpellier, France; E-Mail: [email protected] (F.P.) * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +33-467414-975; Fax: +33-467547-134. Received: 12 December 2012; in revised form: 15 January 2013 / Accepted: 21 February 2013 / Published: 27 February 2013 Abstract: We show that the thermodynamics of ideal gases may be derived solely from the Democritean concept of corpuscles moving in vacuum plus a principle of simplicity, namely that these laws are independent of the laws of motion, aside from the law of energy conservation. Only a single corpuscle in contact with a heat bath submitted to a z and t-invariant force is considered. Most of the end results are known but the method appears to be novel. The mathematics being elementary, the present paper should facilitate the understanding of the ideal gas law and of classical thermodynamics even though not-usually-taught concepts are being introduced. Keywords: ideal gas law; relativistic gases submitted to gravity; corpuscular concepts; classical gas theory; Democritus physics; canonical single-corpuscle thermodynamics 1. Introduction This paper is devoted to an alternative derivation of the ideal gas law, which agrees with the accepted postulates of statistical mechanics, and may present pedagogical and scientific interest. -
Molecular Theory of Ideal Gases March 1, 2021
1 Statistical Thermodynamics Professor Dmitry Garanin Molecular theory of ideal gases March 1, 2021 I. PREFACE Molecular theory can be considered as a preliminary to statistical physics. While the latter employs a more sophisti- cated formalism encompassing quantum-mechanical systems, the former operates with a classical ideal gas. Molecular theory studies the relation between the temperature of the gas and the kinetic energy of the molecules, pressure on the walls due to the impact of the molecules, distribution of molecules over velocities etc. All these results can be obtained in a more formal way in statistical physics. However, it is convenient to first study molecular theory at a more elementary level. On the other hand, molecular theory includes kinetics of classical gases that studies nonequilibrium phenomena such as heat conduction and diffusion (not a part of this course) II. BASIC ASSUMPTIONS OF THE MOLECULAR THEORY 1. Motion of atoms and molecules is described by classical mechanics 2. The number of particles in a considered macroscopic volume is very large. As there are about 1019 molecules in 1 cm3 at normal conditions, this assumption holds down to high vacuums. Because of the large number of particles, the impacts of individual particles on the walls merge into time-independent pressure. 3. The characteristic distance between the molecules largely exceeds the molecular size and the typical radius of intermolecular forces. This assumption allows to consider the gas as ideal, with the internal energy dominated by the kinetic energy of the molecules. In describing equilibrium properties of the ideal gas collisions between the molecules can be neglected. -
Thermodynamics.Pdf
1 Statistical Thermodynamics Professor Dmitry Garanin Thermodynamics February 24, 2021 I. PREFACE The course of Statistical Thermodynamics consist of two parts: Thermodynamics and Statistical Physics. These both branches of physics deal with systems of a large number of particles (atoms, molecules, etc.) at equilibrium. 3 19 One cm of an ideal gas under normal conditions contains NL = 2:69×10 atoms, the so-called Loschmidt number. Although one may describe the motion of the atoms with the help of Newton's equations, direct solution of such a large number of differential equations is impossible. On the other hand, one does not need the too detailed information about the motion of the individual particles, the microscopic behavior of the system. One is rather interested in the macroscopic quantities, such as the pressure P . Pressure in gases is due to the bombardment of the walls of the container by the flying atoms of the contained gas. It does not exist if there are only a few gas molecules. Macroscopic quantities such as pressure arise only in systems of a large number of particles. Both thermodynamics and statistical physics study macroscopic quantities and relations between them. Some macroscopics quantities, such as temperature and entropy, are non-mechanical. Equilibruim, or thermodynamic equilibrium, is the state of the system that is achieved after some time after time-dependent forces acting on the system have been switched off. One can say that the system approaches the equilibrium, if undisturbed. Again, thermodynamic equilibrium arises solely in macroscopic systems. There is no thermodynamic equilibrium in a system of a few particles that are moving according to the Newton's law. -
Case File Cd
CASE FILE CD cY z 0 NATIONAL ADVISORY COMMITTEE FOR AERONAUTICS TECHNICAL NOTE 3226 SOME POSSIBILITIES OF USING GAS MIXTURES OTHER THAN AIR IN AERODYNAMIC RESEARCH By Dean R. Chapman Ames Aeronautical Laboratory Moffett Field, Calif. WASHINGTON bi August 1954 1 a i NATIONAL ADVISORY COMMITTEE FOR AERONAUTICS TECHNICAL NOTE 3226 .SOME POSSIBILITIES OF USING GAS MIXTURES OTHER THAN AIR IN AERODYNAMIC RESEARCH By Dean R. Chapman SUMMARY A study is made of the advantages that can be realized in compressible-flow research by employing a substitute heavy gas in place of air. Heavy gases considered in previous investigations are either toxic, chemically active, or (as in the case of the Freons) have a ratio of specific heats greatly different from air. The present report is based on the idea that by properly mixing a heavy monatomic gas with a suitable heavy polyatomic gas, it is possible to obtain a heavy gas mixture which has the correct ratio of specific heats and which is non- toxic, nonflammable, thermally stable, chemically inert, and comprised of commercially available components. Calculations were made of wind-tunnel characteristics for 63 gas pairs comprising 21 different polyatomic gases properly mixed with each of three monatomic gases (argon, krypton, and xenon). For a given Mach number, Reynolds number, and tunnel pressure, a gas-mixture wind tunnel having the same specific-heat ratio as air wou1d. be appreciably smaller and would require substantially less power than the corresponding air wind tunnel. Very roughly the results are as follows: Mixtures Argon Krypton Xenon Power required relative to air tunnel . -
High Accuracy Numerical Methods for Thermally Perfect Gas Flows with Chemistry
JOURNAL OF COMPUTATIONAL PHYSICS 132, 175±190 (1997) ARTICLE NO. CP965622 High Accuracy Numerical Methods for Thermally Perfect Gas Flows with Chemistry Ronald P. Fedkiw, Barry Merriman, and Stanley Osher1 Department of Mathematics, University of California, 405 Hilgard Avenue, Los Angeles, California 90095-1555 Received July 25, 1996 sider the total mixture as a single compressible ¯uid, with The compressible Navier Stokes equations can be extended to the species-averaged density, momentum, and energy model multi-species, chemically reacting gas ¯ows. The result is a evolving according to the corresponding conservation laws. large system of convection-diffusion equations with stiff source In addition, the mass fraction of each species evolves ac- terms. In this paper we develop the framework needed to apply cording to a separate continuity equation. These continuity modern high accuracy numerical methods from computational gas dynamics to this extended system. We also present representative equations are strongly coupled through the chemical reac- computational results using one such method. The framework de- tions, and they also couple strongly to the equations for veloped here is useful for many modern numerical schemes. We the mixture via the effect of reactions on temperature ®rst present an enthalpy based form of the equations that is well and pressure. suited both for physical modeling and for numerical implementa- Since chemical reactions can cause large localized tem- tion. We show how to treat the stiff reactions via time splitting, and in particular how to increase accuracy by avoidng the common perature variations during combustion, it is important to practice of approximating the temperature. -
A Perfect Gas James Joule, William Thomson and the Concept Of
Downloaded from rsnr.royalsocietypublishing.org on March 12, 2013 James Joule, William Thomson and the concept of a perfect gas J. S. Rowlinson Notes Rec. R. Soc. 2010 64, doi: 10.1098/rsnr.2009.0038 first published online October 14, 2009 Receive free email alerts when new articles cite this article - sign up Email alerting service in the box at the top right-hand corner of the article or click here To subscribe to Notes Rec. R. Soc. go to: http://rsnr.royalsocietypublishing.org/subscriptions Downloaded from rsnr.royalsocietypublishing.org on March 12, 2013 Notes Rec. R. Soc. (2010) 64, 43–57 doi:10.1098/rsnr.2009.0038 Published online 14 October 2009 JAMES JOULE, WILLIAM THOMSON AND THE CONCEPT OF A PERFECT GAS by J. S. ROWLINSON* Department of Chemistry, Physical and Theoretical Chemistry Laboratory, Oxford University, South Parks Road, Oxford OX1 3QZ, UK In the early 1850s Joule and Thomson measured the cooling experienced by a flowing gas on passing an obstacle that caused a decrease in pressure. The mythical ‘perfect gas’, which conforms exactly to Boyle’s and Charles’s laws, would show no such cooling. They used their results to put the new theory of thermodynamics on a more secure foundation and to establish a practical route for converting the measurement of temperature on a gas scale to an absolute temperature based on the second law of thermodynamics. Their experiments were sound but their calculations were in error. Later in the century William Hampson and Carl von Linde independently devised a simple method of liquefying air based on Joule–Thomson cooling, but whereas Linde understood the theory, Hampson, and many chemists, confused the process with the cooling of a gas doing external work, which is an effect that would occur also with a perfect gas. -
Problem Set #3 Assigned September 6, 2013 – Due Friday, September
Problem Set #3 Assigned September 6, 2013 – Due Friday, September 13, 2013 Please show all work for credit To “warm up” or practice try the Atkins Exercises, which are generally simple one step problems Partial Derivatives 1. Engle – P. 3.2 (First and second partial derivatives) f 2x2 5 x y Cos5x y Sin 5x 12 x e Cos y 2 x y lny . x y 2 2 f x x lny 2x 2 x Sin5x 3 e Siny y x y 2 y 2 f 2 2 10 y Cos 5x 25 x y Sin 5x 12 e2x Cos y 48 e2x x 2 Cos y 2 y lny 2 x y 2 2 f 2x 2 x lny 3 e Cosy - 3 2 2 y x 4y f f 2 x x lny 2 Sin5x 5 x Cos 5 x 12 e2x x Sin y x y x y y y 2 f f 2x 2 x x lny f f a) 5 x Cos5 x 12 e x Sin y Sin5x y x y y x y y x x y f f 2x 2 df dx dy 5 x y Cos5x y Sin 5x 12 x e Cos y 2 x y lny dx x y b) y x 2 2 x x lny 2 x Sin 5x 3 e 2x Sin y dy y 2 y 2. Atkins – P. 2.22 (Exact differentials) Show that the following functions have exact diffreentials: (a) x2y+3y2, (b) xcos(xy), (c) x3y2, (d) t(t+es)+s Real Gases 3. -
Digital Notes Thermodynamics
DIGITAL NOTES THERMODYNAMICS (R18A0303) B.Tech II Year I Semester DEPARTMENT OF MECHANICAL ENGINEERING MALLA REDDY COLLEGE OF ENGINEERING & TECHNOLOGY (An Autonomous Institution – UGC, Govt.of India) Recognizes under 2(f) and 12(B) of UGC ACT 1956 (Affiliated to JNTUH, Hyderabad, Approved by AICTE –Accredited by NBA & NAAC-“A” Grade-ISO 9001:2015 Certified) DEPATMENT OF MECHANICAL ENGINEERING,MRCET THERMODYNAMICS B.TECH II YEAR I SEM R18 MALLA REDDY COLLEGE OF ENGINEERING & TECHNOLOGY II Year B. Tech ME-I Sem L T/P/D C 4 1 4 (R17A0303) THERMODYNAMICS Objectives: To understand the concepts of energy transformation, conversion of heat into work. To understand the fundamentals of Differences between work producing and work consuming cycles. To apply the concepts of thermodynamics to basic energy systems. UNIT-I Basic Concepts : System - Types of Systems - Control Volume - Macroscopic and Microscopic viewpoints - Thermodynamic Equilibrium- State, Property, Process, Cycle – Reversibility – Quasi static Process, Irreversible Process, Causes of Irreversibility – Work and Heat, Point and Path functions. Zeroth Law of Thermodynamics – Principles of Thermometry –Constant Volume gas Thermometer – Scales of Temperature – PMM I - Joule’s Experiment – First law of Thermodynamics – Corollaries – First law applied to a Process – applied to a flow system – Steady Flow Energy Equation. UNIT-II Limitations of the First Law - Thermal Reservoir, Heat Engine, Heat pump, Parameters of performance, Second Law of Thermodynamics, Kelvin-Planck and Clausius Statements and their Equivalence / Corollaries, PMM of Second kind, Carnot’s principle, Carnot cycle and its specialties, Clausius Inequality, Entropy, Principle of Entropy Increase – Energy Equation, Availability and Irreversibility – Thermodynamic Potentials, Gibbs and Helmholtz Functions, Maxwell Relations – Elementary Treatment of the Third Law of Thermodynamics.