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Chapter 4 Calculation of Standard Thermodynamic Properties of Aqueous Electrolytes and Non-Electrolytes
Chapter 4 Calculation of Standard Thermodynamic Properties of Aqueous Electrolytes and Non-Electrolytes Vladimir Majer Laboratoire de Thermodynamique des Solutions et des Polymères Université Blaise Pascal Clermont II / CNRS 63177 Aubière, France Josef Sedlbauer Department of Chemistry Technical University Liberec 46117 Liberec, Czech Republic Robert H. Wood Department of Chemistry and Biochemistry University of Delaware Newark, DE 19716, USA 4.1 Introduction Thermodynamic modeling is important for understanding and predicting phase and chemical equilibria in industrial and natural aqueous systems at elevated temperatures and pressures. Such systems contain a variety of organic and inorganic solutes ranging from apolar nonelectrolytes to strong electrolytes; temperature and pressure strongly affect speciation of solutes that are encountered in molecular or ionic forms, or as ion pairs or complexes. Properties related to the Gibbs energy, such as thermodynamic equilibrium constants of hydrothermal reactions and activity coefficients of aqueous species, are required for practical use by geologists, power-cycle chemists and process engineers. Derivative properties (enthalpy, heat capacity and volume), which can be obtained from calorimetric and volumetric experiments, are useful in extrapolations when calculating the Gibbs energy at conditions remote from ambient. They also sensitively indicate evolution in molecular interactions with changing temperature and pressure. In this context, models with a sound theoretical basis are indispensable, describing with a limited number of adjustable parameters all thermodynamic functions of an aqueous system over a wide range of temperature and pressure. In thermodynamics of hydrothermal solutions, the unsymmetric standard-state convention is generally used; in this case, the standard thermodynamic properties (STP) of a solute reflect its interaction with the solvent (water), and the excess properties, related to activity coefficients, correspond to solute-solute interactions. -
FUGACITY It Is Simply a Measure of Molar Gibbs Energy of a Real Gas
FUGACITY It is simply a measure of molar Gibbs energy of a real gas . Modifying the simple equation for the chemical potential of an ideal gas by introducing the concept of a fugacity (f). The fugacity is an “ effective pressure” which forces the equation below to be true for real gases: θθθ f µµµ ,p( T) === µµµ (T) +++ RT ln where pθ = 1 atm pθθθ A plot of the chemical potential for an ideal and real gas is shown as a function of the pressure at constant temperature. The fugacity has the units of pressure. As the pressure approaches zero, the real gas approach the ideal gas behavior and f approaches the pressure. 1 If fugacity is an “effective pressure” i.e, the pressure that gives the right value for the chemical potential of a real gas. So, the only way we can get a value for it and hence for µµµ is from the gas pressure. Thus we must find the relation between the effective pressure f and the measured pressure p. let f = φ p φ is defined as the fugacity coefficient. φφφ is the “fudge factor” that modifies the actual measured pressure to give the true chemical potential of the real gas. By introducing φ we have just put off finding f directly. Thus, now we have to find φ. Substituting for φφφ in the above equation gives: p µ=µ+(p,T)θ (T) RT ln + RT ln φ=µ (ideal gas) + RT ln φ pθ µµµ(p,T) −−− µµµ(ideal gas ) === RT ln φφφ This equation shows that the difference in chemical potential between the real and ideal gas lies in the term RT ln φφφ.φ This is the term due to molecular interaction effects. -
Chapter 8 Thermodynamic Properties of Mixtures
Chapter 8 Thermodynamic Properties of Mixtures 2012/3/29 1 Abstract The thermodynamic description of mixtures, extended from pure fluids. The equations of change, i.e., energy and entropy balance, for mixtures are developed. The criteria for phase and chemical equilibrium in mixtures 2012/3/29 2 8.1 THE THERMODYNAMIC DESCRIPTION OF MIXTURES Thermodynamic property for pure fluids, θθ=()TPN , , where N is the number of moles. θθ=()TP , where the number of mole equals to 1. Thermodynamic property for mixtures, θθ=()TPN , ,12 , N ,L , Nc where Ni is the number of moles of the ith component. θθ=()TPx , ,12 , x ,L , xci where x is the mole fraction of the ith component. For example UUTPNN=() , ,12 , ,LL , Ncc or UUTPxx=() , , 12 , , , x VVTPNN=() , ,12 , ,L , Nc or VVTPxx=() , ,12 , ,L , xc 2012/3/29 3 Summation of the properties of pure fluids (before mixing at TP and ) C UTPxx(), ,12 , ,L , xci− 1= ∑ xUTPi () , (8.1-1) i=1 where UU is the molar internal energy, i is the internal energy of the pure i-th component at TP and . C ˆˆ UTPww()(), ,12 , ,L , wcii− 1= ∑ wUTP , (8.1-2) i=1 where wi is the mass fraction of component i. 2012/3/29 4 At the same T and P 50 cc 25 cc + 25 cc H2O H2O or 52 cc 25 cc + 25 cc 48 cc + 2 cc A B -2 cc Attractive Repulsive 2012/3/29 5 Property change upon mixing (at constantTP and ) C Δ=mixθθ()TPx,,ii −∑ x θi () TP , i=1 Volume change upon mixing C Δ=mixVTP(),,,, VTPx()ii −∑ xVTPi () i=1 Enthalpy change upon mixing C Δ=mix HTP(),,,, HTPx()ii −∑ xHTPi () i=1 2012/3/29 6 Experimental data : properties changes upon mixing (H and V) Figure 8.1-1 Enthalpy-concentration diagram for aqueous sulfuric acid at 0.1 MPa. -
Selection of Thermodynamic Methods
P & I Design Ltd Process Instrumentation Consultancy & Design 2 Reed Street, Gladstone Industrial Estate, Thornaby, TS17 7AF, United Kingdom. Tel. +44 (0) 1642 617444 Fax. +44 (0) 1642 616447 Web Site: www.pidesign.co.uk PROCESS MODELLING SELECTION OF THERMODYNAMIC METHODS by John E. Edwards [email protected] MNL031B 10/08 PAGE 1 OF 38 Process Modelling Selection of Thermodynamic Methods Contents 1.0 Introduction 2.0 Thermodynamic Fundamentals 2.1 Thermodynamic Energies 2.2 Gibbs Phase Rule 2.3 Enthalpy 2.4 Thermodynamics of Real Processes 3.0 System Phases 3.1 Single Phase Gas 3.2 Liquid Phase 3.3 Vapour liquid equilibrium 4.0 Chemical Reactions 4.1 Reaction Chemistry 4.2 Reaction Chemistry Applied 5.0 Summary Appendices I Enthalpy Calculations in CHEMCAD II Thermodynamic Model Synopsis – Vapor Liquid Equilibrium III Thermodynamic Model Selection – Application Tables IV K Model – Henry’s Law Review V Inert Gases and Infinitely Dilute Solutions VI Post Combustion Carbon Capture Thermodynamics VII Thermodynamic Guidance Note VIII Prediction of Physical Properties Figures 1 Ideal Solution Txy Diagram 2 Enthalpy Isobar 3 Thermodynamic Phases 4 van der Waals Equation of State 5 Relative Volatility in VLE Diagram 6 Azeotrope γ Value in VLE Diagram 7 VLE Diagram and Convergence Effects 8 CHEMCAD K and H Values Wizard 9 Thermodynamic Model Decision Tree 10 K Value and Enthalpy Models Selection Basis PAGE 2 OF 38 MNL 031B Issued November 2008, Prepared by J.E.Edwards of P & I Design Ltd, Teesside, UK www.pidesign.co.uk Process Modelling Selection of Thermodynamic Methods References 1. -
Physical Chemistry
Subject Chemistry Paper No and Title 10, Physical Chemistry- III (Classical Thermodynamics, Non-Equilibrium Thermodynamics, Surface chemistry, Fast kinetics) Module No and Title 10, Free energy functions and Partial molar properties Module Tag CHE_P10_M10 CHEMISTRY Paper No. 10: Physical Chemistry- III (Classical Thermodynamics, Non-Equilibrium Thermodynamics, Surface chemistry, Fast kinetics) Module No. 10: Free energy functions and Partial molar properties TABLE OF CONTENTS 1. Learning outcomes 2. Introduction 3. Free energy functions 4. The effect of temperature and pressure on free energy 5. Maxwell’s Relations 6. Gibbs-Helmholtz equation 7. Partial molar properties 7.1 Partial molar volume 7.2 Partial molar Gibb’s free energy 8. Question 9. Summary CHEMISTRY Paper No. 10: Physical Chemistry- III (Classical Thermodynamics, Non-Equilibrium Thermodynamics, Surface chemistry, Fast kinetics) Module No. 10: Free energy functions and Partial molar properties 1. Learning outcomes After studying this module you shall be able to: Know about free energy functions i.e. Gibb’s free energy and work function Know the dependence of Gibbs free energy on temperature and pressure Learn about Gibb’s Helmholtz equation Learn different Maxwell relations Derive Gibb’s Duhem equation Determine partial molar volume through intercept method 2. Introduction Thermodynamics is used to determine the feasibility of the reaction, that is , whether the process is spontaneous or not. It is used to predict the direction in which the process will be spontaneous. Sign of internal energy alone cannot determine the spontaneity of a reaction. The concept of entropy was introduced in second law of thermodynamics. Whenever a process occurs spontaneously, then it is considered as an irreversible process. -
Lecture Outline
LECTURE OUTLINE 1. Equilibrium of heterogeneous system 2. Phase transformations R&Y, Chapter 2 Salby, Chapter 4 C&W, Chapter 4 A Short Course in Cloud Physics, R.R. Rogers and M.K. Yau; R&Y Thermodynamics of Atmospheres Fundamentals of Atmospheric Physics, and Oceanes, M.L. Salby; Salby J.A. Curry and P.J. Webster; C&W 2 /25 LECTURE OUTLINE 1. Equilibrium of heterogeneous system 2. Phase transformations Equilibrium conditions for a homogeneous system: • thermal equilibrium • mechanical equilibrium (at most an infinitesimal pressure difference exists between the system and its environment). A heterogeneous system must also be in: • chemical equilibrium. No conversion of mass occurs from one phase to the other. Chemical equilibrium requires a certain state variables to have no difference between the phases present. 4 /30 For a homogeneous system, two intensive properties describe the thermodynamic state. Only two state variables may be varied independently, so a homogeneous system has two thermodynamic degrees of freedom. For a heterogeneous system, each phase may be regarded as a homogeneous sub-system, one that is ‚open’ due to exchanges with the other phases present. The number of intensive properties that describes the thermodynamic state is proportional to the number of phases present. However, thermodynamic equilibrium between phases introduces additional constraints that actually reduce the degrees of freedom of a heterogeneous system below those of a homogeneous system. The system we consider is a two-component mixture of: • dry -
Molecular Thermodynamics
Chapter 1. The Phase-Equilibrium Problem Homogeneous phase: a region where the intensive properties are everywhere the same. Intensive property: a property that is independent of the size temperature, pressure, and composition, density(?) Gibbs phase rule ( no reaction) Number of independent intensive properties = Number of components – Number of phases + 2 e.g. for a two-component, two-phase system No. of intensive properties = 2 1.2 Application of Thermodynamics to Phase-Equilibrium Problem Chemical potential : Gibbs (1875) At equilibrium the chemical potential of each component must be the same in every phase. i i ? Fugacity, Activity: more convenient auxiliary functions 0 i yi P i xi fi fugacity coefficient activity coefficient fugacity at the standard state For ideal gas mixture, i 1 0 For ideal liquid mixture at low pressures, i 1, fi Psat In the general case Chapter 2. Classical Thermodynamics of Phase Equilibria For simplicity, we exclude surface effect, acceleration, gravitational or electromagnetic field, and chemical and nuclear reactions. 2.1 Homogeneous Closed Systems A closed system is one that does not exchange matter, but it may exchange energy. A combined statement of the first and second laws of thermodynamics dU TBdS – PEdV (2-2) U, S, V are state functions (whose value is independent of the previous history of the system). TB temperature of thermal bath, PE external pressure Equality holds for reversible process with TB = T, PE =P dU = TdS –PdV (2-3) and TdS = Qrev, PdV = Wrev U(S,V) is state function. The group of U, S, V is a fundamental group. Integrating over a reversible path, U is independent of the path of integration, and also independent of whether the system is maintained in a state of internal equilibrium or not during the actual process. -
Equation of State. Fugacities of Gaseous Solutions
ON THE THERMODYNAMICS OF SOLUTIONS. V k~ EQUATIONOF STATE. FUGACITIESOF GASEOUSSOLUTIONS' OTTO REDLICH AND J. N. S. KWONG Shell Development Company, Emeryville, California Received October 15, 1948 The calculation of fugacities from P-V-T data necessarily involves a differentia- tion with respect to the mole fraction. The fugacity rule of Lewis, which in effect would eliminate this differentiation, does not furnish a sufficient approximation. Algebraic representation of P-V-T data is desirable in view of the difficulty of nu- merical or graphical differentiation. An equation of state containing two individ- ual coefficients is proposed which furnishes satisfactory results above the critical temperature for any pressure. The dependence of the coefficients on the composi- tion of the gas is discussed. Relations and methods for the calculation of fugacities are derived which make full use of whatever data may be available. Abbreviated methods for moderate pressure are discussed. The old problem of the equation of state has a practical aspect which has become increasingly important in recent times. The systematic description of gas reactions under high pressure requires information about the fugacities, derived sometimes from extensive data but frequently from nothing more than t,he critical pressure and temperature. For practical purposes a representation of the relation between pressure, vol- ume, and temperature based on two or three individual coefficients is desirable, although a representation of this type satisfies the theorem of corresponding states and therefore cannot be accurate. Since the calculation of fugacities involves a differentiation with respect to the mole fraction, an algebraic repre- sentation by means of an equation of state appears to be desirable. -
Fugacity of Condensed Media
Fugacity of condensed media Leonid Makarov and Peter Komarov St. Petersburg State University of Telecommunications, Bolshevikov 22, 193382, St. Petersburg, Russia ABSTRACT Appearance of physical properties of objects is a basis for their detection in a media. Fugacity is a physical property of objects. Definition of estimations fugacity for different objects can be executed on model which principle of construction is considered in this paper. The model developed by us well-formed with classical definition fugacity and open up possibilities for calculation of physical parameter «fugacity» for elementary and compound substances. Keywords: fugacity, phase changes, thermodynamic model, stability, entropy. 1. INTRODUCTION The reality of world around is constructed of a plenty of the objects possessing physical properties. Du- ration of objects existence – their life time, is defined by individual physical and chemical parameters, and also states of a medium. In the most general case any object, under certain states, can be in one of three ag- gregative states - solid, liquid or gaseous. Conversion of object substance from one state in another refers to as phase change. Evaporation and sublimation of substance are examples of phase changes. Studying of aggregative states of substance can be carried out from a position of physics or on the basis of mathematical models. The physics of the condensed mediums has many practical problems which deci- sion helps to study complex processes of formation and destruction of medium objects. Natural process of object destruction can be characterized in parameter volatility – fugacity. For the first time fugacity as the settlement size used for an estimation of real gas properties, by means of the thermodynamic parities de- duced for ideal gases, was offered by Lewis in 1901. -
Lecture 4. Thermodynamics [Ch. 2]
Lecture 4. Thermodynamics [Ch. 2] • Energy, Entropy, and Availability Balances • Phase Equilibria - Fugacities and activity coefficients -K-values • Nonideal Thermodynamic Property Models - P-v-T equation-of-state models - Activity coefficient models • Selecting an Appropriate Model Thermodynamic Properties • Importance of thermodyyppnamic properties and equations in separation operations – Energy requirements (heat and work) – Phase equilibria : Separation limit – Equipment sizing • Property estimation – Specific volume, enthalpy, entropy, availability, fugacity, activity, etc. – Used for design calculations . Separator size and layout . AiliAuxiliary components : PiPipi ing, pumps, va lves, etc. EnergyEnergy,, Entropy and Availability Balances Heat transfer in and out Q ,T Q ,T in s out s OfdOne or more feed streams flowing into the system are … … separated into two or more prodttduct streams thtflthat flow Streams in out of the system. n,zi ,T,P,h,s,b,v : Separation : : : process n Molar flow rate : (system) : z Mole fraction Sirr , LW Streams out T Temperature n,zi ,T,P,h,s,b,v P Pressure h Molar enthalpy … … (Surroundings) s Molar entropy T b Molar availability 0 (W ) (W ) s in s out v Specific volume Shaft work in and out Energy Balance • Continuous and steady-state flow system • Kinetic, potential, and surface energy changes are neglected • First law of thermodynamics (conservation of energy) (stream enthalpy flows + heat transfer + shaft work)leaving system - (t(stream en thlthalpy flows +h+ hea ttt trans fer + s hfthaft wor k)entering -
Thermodynamics, Experimental, and Modelling of Aqueous Electrolyte and Amino Acid Solutions
Downloaded from orbit.dtu.dk on: Sep 26, 2021 Thermodynamics, Experimental, and Modelling of Aqueous Electrolyte and Amino Acid Solutions Breil, Martin Peter Publication date: 2001 Document Version Publisher's PDF, also known as Version of record Link back to DTU Orbit Citation (APA): Breil, M. P. (2001). Thermodynamics, Experimental, and Modelling of Aqueous Electrolyte and Amino Acid Solutions. General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Users may download and print one copy of any publication from the public portal for the purpose of private study or research. You may not further distribute the material or use it for any profit-making activity or commercial gain You may freely distribute the URL identifying the publication in the public portal If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Thermodynamics, Experimental, and Modelling of Aqueous Electrolyte and Amino Acid Solutions Martin P. Breil 2001 IVC-SEP Department of Chemical Engineering Technical University of Denmark DK-2800 Kongens Lyngby, Denmark Preface iii Preface This thesis is submitted as a partial fulfilment of the Ph.D. degree at the Technical University of Denmark. The project, granted by the IVC-SEP, has been carried out from October 1998 to September 2001 at the Department of Chemical Engineering, Technical University of Denmark under the supervision of Jørgen Mollerup. -
Activity and Fugacity Ray Fu
Activity and Fugacity Ray Fu Notation symbol description m, M intensive (molar) and extensive property of pure species mi, Mi as above, but specifically for species i m◦, mig, mid reference state, ideal gas, and ideal solution conditions msat saturation (liquid-vapor equilibrium) conditions mα, mβ, ml, mv α, β arbitrary and l, v liquid and vapor phases ^ f, ', fi,' ^i fugacity (coeffcient) of pure species and of species i in mixture xi, yi liquid and gas phase mole fraction of species i PT total pressure of mixture * a harder exercise Fugacity in the gas phase For an ideal gas, and assuming constant T and N, we have P dµ = dg = v dP () µ − µ◦ = g − g◦ = RT ln : (1) P ◦ Exercise 1 Prove the above identity. For non-ideal gases and fluids, we can extend this identity by defining an effective pressure f such that f f µ − µig =: RT ln = RT ln : (2) P ig f ig We call f the fugacity; it is the pressure that an ideal gas with the same chemical potential would have. By construction, f ig = P ig, and the second equality follows. The pressure P ig is the pressure of the (real) gas; the superscript ig reminds us that we are considering an ideal gas reference state. It is also convenient to define the fugacity coefficient ', satisfying 'P ig f =: 'P ig () µ − µig = RT ln = RT ln ': (3) P ig The fugacity coefficient ' contains no new thermodynamics. It simply hides all the complicated intermolec- ular interactions that real gases possess, and we can interpret it as a measure of a gas's deviation from ideality: the further the fugacity coefficient of a gas diverges from one, the less ideal is the gas.