Entropy: Ideal Gas Processes

Total Page:16

File Type:pdf, Size:1020Kb

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. Boltzmann Constant gas constant -23 R = 8.315 J/(mol⋅K) pV = nRT kB = 1.38×10 J/K = 0.0821 (L⋅atm)/(mol⋅K) pV = Nk T = 1.99 calories/(mol⋅K) B R = kBNA Work Done by Isothermal (ΔT = 0) Expansion/Compression of Ideal Gas On p-V graph, the green lines are isotherms… … each green line corresponds to a system at a constant temperature. From ideal gas law, this means that for a given isotherm: 1 pV = constant ⇒ p = (nRT) Relates p and V V Vf The work done by the gas€ is then: ⇒ Wby,isothermal = nRT ln T =0 Δ Vi V f V f V f nRT dV Wby = ∫ pdV = ∫ dV = nRT ∫ pi Vi Vi V Vi V = nRT ln p f For expansion, we have: Vf > Vi Wby > 0 € For compression, we have: V < V W < 0 f i € by Checkpoint 1: An ideal gas has an initial pressure of 3 pressure units and an initial volume of 4 volume units. The table gives the final pressure and volume of the gas in five processes. Which processes start and end on the same isotherm? – a b c d e • p 12 6 5 4 1 • V 1 2 7 3 12 pV=nRT in this case T is a constant so pV=C=12 Sample problem #19-2 One mole of oxygen expands at a constant temperature T of 310 K from an initial volume Vi of 12 L to a final volume Vf of 19 L. How much work is done by the gas during the expansion. We calculated W for isothermal W=nRT ln (Vf /VI) W= (1 mole)(8.31J/mole K)(310K) ln(19/12) W=1180 J Work Done by Isobaric (Δp = 0) Expansion of an Ideal Gas V f Wby = ∫ pdV Vi ⇒ Wby,isobaric = pΔV ΔP=0 € = nRΔT € Adiabac Expansion of an ideal gas (Q = 0) Because a gas is thermally insulated, or expansion/compression happens suddenly ⇒ adiabatic st Remember “Adiabatic means Q = 0” or, by 1 Law of Thermo ⇒ ΔEint = -Wby γ In this case pV = constant where γ = cp/cV = (R+ cV )/cV example: monatomic gas γ = 5/3 γ γ p1V1 = p2V2 γ −1 γ −1 T1V1 = T2V2 Compare with Isothermal Expansion (ΔT = 0) € T1 = T2 ⇔ [p1V1 = p2V2 ]isothermal € Pressure, Temperature, & RMS speed Assume the collision of the gas molecule with the wall is elastic then the : - Δpx = (−mvx ) − (mvx ) = 2mvx The molecule travels to the back wall, collides and comes back. The time it takes is 2L/vx. Δp 2mv mv2 = x = x The is F/A Δt 2l / vx L If we calculated the average velocity F 1 n mv2 m n p = x = xi = v2 and use the fact that the number in the sum 2 ∑ 3 ∑ xi is nN then: n A L i=1 L L i=1 A 2 2 vx = vxi nNA 2 ( )avg ∑ nmN A 2 nM (vx )avg i=1 p = 3 (vx )avg = L V 2 2 2 2 2 2 v = vx + vy + vz 2 nM (v )avg nMv € rms 2 (v )avg = vrms = = v 3V 3V v2 = x 3 RMS = Root-Mean-Square RMS Speeds We have nMv 2 pressure p = rms 3V For ideal gas pV = nRT € 1/2 1/2 3pV 3nRT v = = rms nM nM 3RT v = rms M The RMS velocity depends on: Molar mass & Temperature Problem #19-3: Here are five numbers: 5, 11, 32, 67, and 89. (a) What is the average value navg? (b) What is the rms value nrms of the numbers? (a) 5 + 11+ 32 + 67 + 89 n = = 40.8 avg 5 (b) n 2 2 2 2 2 2 1 2 5 + 11 + 32 + 67 + 89 (n )avg = ∑ni = = 2714.41 n i=1 5 2 (n )avg = 52.1 2 navg ≠ n = nrms ( )avg € Problem #19-21: (a) Compute the rms speed of a nitrogen molecule at 20.0 0C (each N atom has 7 protons and 7 neutrons). At what temperatures will the rms speed be (b) half that value and (c) twice that value? 3RT v = rms M Remember to use: T = 20 °C + 273 = 293 K € If we know the “average” speed of parcles, we then know the kinec energy, 1 2 1 3RT KE = m(vrms ) = m 2 2 M What is the relaonship between translaonal € kinec energy & internal energy? Translaonal Kinec Energy & Internal energy 1 2 1 3RT M = mN A KE = m(vrms ) = m 2 2 M kB= R N A 3 The KE of all ideal gas molecules KE = k T € 2 B depends only on the temperature € € (not mass!) € Monoatomic ideal gas : He, Ar, Ne, Kr… (no potential energies) 3 3 The internal energy Eint,monotonic = NA kBT = nRT ( 2 ) 2 of an ideal gas depends only on the temperature 3 ΔE int,monotonic = 2 nR(ΔT) € € Problem #19-26: What is the average translational kinetic energy of 1 mole nitrogen molecules at 1600 K? Molar Specific Heat at Constant Volume: Monatomic Ideal Gas Molar Specific Heat at Constant Volume (Wby=0) Q = ncV ΔT & Wby = 0 ΔEint = Q = ncV ΔT € 3 ΔE int = n( 2 R)ΔT = n(CV )ΔT = Q € 3 cV ,monatomic = R =12.5 ⋅ J/mol⋅ K € 2 € Molar Specific Heat: Monatomic ideal gas Molar Specific Heat at Constant Volume (Wby=0) ΔEint = Q = ncV ΔT 3 cV ,monatomic = R =12.5 ⋅ J/mol⋅ K € 2 Molar Specific Heat at Constant Pressure (W =pΔV) € by ΔEint = Q − Wby = nc p ΔT − pΔV ncV ΔT = nc p ΔT − nRΔT c = c − R or c = c + R € V p p V 5 € c = R = 20.8 ⋅ J/mol⋅ K p,monatomic 2 € € Remember special cases… Adiabatic expansion/contraction - NO TRANSFER OF ENERGY AS HEAT Q = 0 [ΔE int = −W]adiabatic Constant-volume processes (isochoric)- Wby = ∫ pdV V f =Vi NO WORK IS DONE = area under p −V graph W = 0 Wby = ∫ pdV = 0 ΔE = Q Vi € int QΔV = 0 = nCV ΔT € Constant-pressure processes V f =Vi € Wby = pdV = pΔV ΔE int = Q − pΔV ∫ € Vi CV = CP − R QΔP= 0 = nCP ΔT 3)Cyclical process (closed cycle) ΔEint,closed cycle =0 ΔE = 0 ⇒ Q = W €net area in p-V curve is Q int by € € Chapter 20: Entropy and the Second law of thermodynamics 0th law Thermal Equilibrium: A = B & B = C then A = C Q = ncΔT Q → 0 as ΔT → 0 st 1 law Conservation of energy: ΔEint = Q - Wby= Q + Won Change in Internal energy = heat added minus work done by Today: 2nd law HEAT FLOWS NATURALLY FROM HOT OBJECT TO A COLD OBJECT Heat will NOT flow spontaneously from cold to hot 0 ≤ ΔStotal € Hall of fame Ludwig Boltzmann (1844-1906) -23 Boltzmann constant kB =1.38×10 J/K W = number of states Irreversible Processes How to understand this: Entropy How to describe a system: Entropy, S, like T,V, P, Eint, and n is P, T, V, Eint, and n state variable How to define entropy? Easier to define Change of entropy during a process. f dQ ΔS = S − S = Temp in Kelvin part f i ∫ Units: [J/K] i T where Q is energy transferred to or from a system during a process [ Note: since T > 0, if Q is positive (negative) the ΔS is positive (negative) ] What€ is a process? expansion, compression, temperature rise, add mass Reversible process {processes can be done infinitely slowly to ensure thermal equilibrium} The Second Law of Thermodynamics The entropy of a closed system (no energy and no mass comes in and out) never decreases. It either stays constant (reversible process) or increases (irreversible process). 0 ≤ ΔStotal € Entropy: Ideal Gas Processes 1) For reversible process: dQ ΔScycle,rev = 0 = ∫ T 2) For isothermal process: € ΔE = 0 ⇒ Q = W Q int S V Δ isothermal = Vf f T W = nRT ln ⇒ ΔSisothermal = nR ln V Vi i 3) In general for gas, using 1st law: dE int = dQ − dW nC €dT dQ pdV nRT V € dQ nRT dV nCV dT = − & p€= ⇒ ∫ = ∫ + ∫ T T T V T V T T Now integrate: V f T f S S S nR ln nC ln pV nRT € Δ general,gas = f − i = + V ⇐ [ = ] € Vi Ti 4) For adiabatic (reversible) adiabatic compression/expansion (Q=0): Entropy is a State Function ΔSrev,adiabatic = 0 € € Checkpoint: An ideal gas has a temperature T1 at the inial state i shown in the p‐V diagram.
Recommended publications
  • On Entropy, Information, and Conservation of Information
    entropy Article On Entropy, Information, and Conservation of Information Yunus A. Çengel Department of Mechanical Engineering, University of Nevada, Reno, NV 89557, USA; [email protected] Abstract: The term entropy is used in different meanings in different contexts, sometimes in contradic- tory ways, resulting in misunderstandings and confusion. The root cause of the problem is the close resemblance of the defining mathematical expressions of entropy in statistical thermodynamics and information in the communications field, also called entropy, differing only by a constant factor with the unit ‘J/K’ in thermodynamics and ‘bits’ in the information theory. The thermodynamic property entropy is closely associated with the physical quantities of thermal energy and temperature, while the entropy used in the communications field is a mathematical abstraction based on probabilities of messages. The terms information and entropy are often used interchangeably in several branches of sciences. This practice gives rise to the phrase conservation of entropy in the sense of conservation of information, which is in contradiction to the fundamental increase of entropy principle in thermody- namics as an expression of the second law. The aim of this paper is to clarify matters and eliminate confusion by putting things into their rightful places within their domains. The notion of conservation of information is also put into a proper perspective. Keywords: entropy; information; conservation of information; creation of information; destruction of information; Boltzmann relation Citation: Çengel, Y.A. On Entropy, 1. Introduction Information, and Conservation of One needs to be cautious when dealing with information since it is defined differently Information. Entropy 2021, 23, 779.
    [Show full text]
  • Practice Problems from Chapter 1-3 Problem 1 One Mole of a Monatomic Ideal Gas Goes Through a Quasistatic Three-Stage Cycle (1-2, 2-3, 3-1) Shown in V 3 the Figure
    Practice Problems from Chapter 1-3 Problem 1 One mole of a monatomic ideal gas goes through a quasistatic three-stage cycle (1-2, 2-3, 3-1) shown in V 3 the Figure. T1 and T2 are given. V 2 2 (a) (10) Calculate the work done by the gas. Is it positive or negative? V 1 1 (b) (20) Using two methods (Sackur-Tetrode eq. and dQ/T), calculate the entropy change for each stage and ∆ for the whole cycle, Stotal. Did you get the expected ∆ result for Stotal? Explain. T1 T2 T (c) (5) What is the heat capacity (in units R) for each stage? Problem 1 (cont.) ∝ → (a) 1 – 2 V T P = const (isobaric process) δW 12=P ( V 2−V 1 )=R (T 2−T 1)>0 V = const (isochoric process) 2 – 3 δW 23 =0 V 1 V 1 dV V 1 T1 3 – 1 T = const (isothermal process) δW 31=∫ PdV =R T1 ∫ =R T 1 ln =R T1 ln ¿ 0 V V V 2 T 2 V 2 2 T1 T 2 T 2 δW total=δW 12+δW 31=R (T 2−T 1)+R T 1 ln =R T 1 −1−ln >0 T 2 [ T 1 T 1 ] Problem 1 (cont.) Sackur-Tetrode equation: V (b) 3 V 3 U S ( U ,V ,N )=R ln + R ln +kB ln f ( N ,m ) V2 2 N 2 N V f 3 T f V f 3 T f ΔS =R ln + R ln =R ln + ln V V 2 T V 2 T 1 1 i i ( i i ) 1 – 2 V ∝ T → P = const (isobaric process) T1 T2 T 5 T 2 ΔS12 = R ln 2 T 1 T T V = const (isochoric process) 3 1 3 2 2 – 3 ΔS 23 = R ln =− R ln 2 T 2 2 T 1 V 1 T 2 3 – 1 T = const (isothermal process) ΔS 31 =R ln =−R ln V 2 T 1 5 T 2 T 2 3 T 2 as it should be for a quasistatic cyclic process ΔS = R ln −R ln − R ln =0 cycle 2 T T 2 T (quasistatic – reversible), 1 1 1 because S is a state function.
    [Show full text]
  • Lecture 4: 09.16.05 Temperature, Heat, and Entropy
    3.012 Fundamentals of Materials Science Fall 2005 Lecture 4: 09.16.05 Temperature, heat, and entropy Today: LAST TIME .........................................................................................................................................................................................2� State functions ..............................................................................................................................................................................2� Path dependent variables: heat and work..................................................................................................................................2� DEFINING TEMPERATURE ...................................................................................................................................................................4� The zeroth law of thermodynamics .............................................................................................................................................4� The absolute temperature scale ..................................................................................................................................................5� CONSEQUENCES OF THE RELATION BETWEEN TEMPERATURE, HEAT, AND ENTROPY: HEAT CAPACITY .......................................6� The difference between heat and temperature ...........................................................................................................................6� Defining heat capacity.................................................................................................................................................................6�
    [Show full text]
  • 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).
    [Show full text]
  • IB Questionbank
    Topic 3 Past Paper [94 marks] This question is about thermal energy transfer. A hot piece of iron is placed into a container of cold water. After a time the iron and water reach thermal equilibrium. The heat capacity of the container is negligible. specific heat capacity. [2 marks] 1a. Define Markscheme the energy required to change the temperature (of a substance) by 1K/°C/unit degree; of mass 1 kg / per unit mass; [5 marks] 1b. The following data are available. Mass of water = 0.35 kg Mass of iron = 0.58 kg Specific heat capacity of water = 4200 J kg–1K–1 Initial temperature of water = 20°C Final temperature of water = 44°C Initial temperature of iron = 180°C (i) Determine the specific heat capacity of iron. (ii) Explain why the value calculated in (b)(i) is likely to be different from the accepted value. Markscheme (i) use of mcΔT; 0.58×c×[180-44]=0.35×4200×[44-20]; c=447Jkg-1K-1≈450Jkg-1K-1; (ii) energy would be given off to surroundings/environment / energy would be absorbed by container / energy would be given off through vaporization of water; hence final temperature would be less; hence measured value of (specific) heat capacity (of iron) would be higher; This question is in two parts. Part 1 is about ideal gases and specific heat capacity. Part 2 is about simple harmonic motion and waves. Part 1 Ideal gases and specific heat capacity State assumptions of the kinetic model of an ideal gas. [2 marks] 2a. two Markscheme point molecules / negligible volume; no forces between molecules except during contact; motion/distribution is random; elastic collisions / no energy lost; obey Newton’s laws of motion; collision in zero time; gravity is ignored; [4 marks] 2b.
    [Show full text]
  • Thermodynamics of Ideal Gases
    D Thermodynamics of ideal gases An ideal gas is a nice “laboratory” for understanding the thermodynamics of a fluid with a non-trivial equation of state. In this section we shall recapitulate the conventional thermodynamics of an ideal gas with constant heat capacity. For more extensive treatments, see for example [67, 66]. D.1 Internal energy In section 4.1 we analyzed Bernoulli’s model of a gas consisting of essentially 1 2 non-interacting point-like molecules, and found the pressure p = 3 ½ v where v is the root-mean-square average molecular speed. Using the ideal gas law (4-26) the total molecular kinetic energy contained in an amount M = ½V of the gas becomes, 1 3 3 Mv2 = pV = nRT ; (D-1) 2 2 2 where n = M=Mmol is the number of moles in the gas. The derivation in section 4.1 shows that the factor 3 stems from the three independent translational degrees of freedom available to point-like molecules. The above formula thus expresses 1 that in a mole of a gas there is an internal kinetic energy 2 RT associated with each translational degree of freedom of the point-like molecules. Whereas monatomic gases like argon have spherical molecules and thus only the three translational degrees of freedom, diatomic gases like nitrogen and oxy- Copyright °c 1998{2004, Benny Lautrup Revision 7.7, January 22, 2004 662 D. THERMODYNAMICS OF IDEAL GASES gen have stick-like molecules with two extra rotational degrees of freedom or- thogonally to the bridge connecting the atoms, and multiatomic gases like carbon dioxide and methane have the three extra rotational degrees of freedom.
    [Show full text]
  • 5.5 ENTROPY CHANGES of an IDEAL GAS for One Mole Or a Unit Mass of Fluid Undergoing a Mechanically Reversible Process in a Closed System, the First Law, Eq
    Thermodynamic Third class Dr. Arkan J. Hadi 5.5 ENTROPY CHANGES OF AN IDEAL GAS For one mole or a unit mass of fluid undergoing a mechanically reversible process in a closed system, the first law, Eq. (2.8), becomes: Differentiation of the defining equation for enthalpy, H = U + PV, yields: Eliminating dU gives: For an ideal gas, dH = and V = RT/ P. With these substitutions and then division by T, As a result of Eq. (5.11), this becomes: where S is the molar entropy of an ideal gas. Integration from an initial state at conditions To and Po to a final state at conditions T and P gives: Although derived for a mechanically reversible process, this equation relates properties only, and is independent of the process causing the change of state. It is therefore a general equation for the calculation of entropy changes of an ideal gas. 1 Thermodynamic Third class Dr. Arkan J. Hadi 5.6 MATHEMATICAL STATEMENT OF THE SECOND LAW Consider two heat reservoirs, one at temperature TH and a second at the lower temperature Tc. Let a quantity of heat | | be transferred from the hotter to the cooler reservoir. The entropy changes of the reservoirs at TH and at Tc are: These two entropy changes are added to give: Since TH > Tc, the total entropy change as a result of this irreversible process is positive. Also, ΔStotal becomes smaller as the difference TH - TC gets smaller. When TH is only infinitesimally higher than Tc, the heat transfer is reversible, and ΔStotal approaches zero. Thus for the process of irreversible heat transfer, ΔStotal is always positive, approaching zero as the process becomes reversible.
    [Show full text]
  • Chapter 3 3.4-2 the Compressibility Factor Equation of State
    Chapter 3 3.4-2 The Compressibility Factor Equation of State The dimensionless compressibility factor, Z, for a gaseous species is defined as the ratio pv Z = (3.4-1) RT If the gas behaves ideally Z = 1. The extent to which Z differs from 1 is a measure of the extent to which the gas is behaving nonideally. The compressibility can be determined from experimental data where Z is plotted versus a dimensionless reduced pressure pR and reduced temperature TR, defined as pR = p/pc and TR = T/Tc In these expressions, pc and Tc denote the critical pressure and temperature, respectively. A generalized compressibility chart of the form Z = f(pR, TR) is shown in Figure 3.4-1 for 10 different gases. The solid lines represent the best curves fitted to the data. Figure 3.4-1 Generalized compressibility chart for various gases10. It can be seen from Figure 3.4-1 that the value of Z tends to unity for all temperatures as pressure approach zero and Z also approaches unity for all pressure at very high temperature. If the p, v, and T data are available in table format or computer software then you should not use the generalized compressibility chart to evaluate p, v, and T since using Z is just another approximation to the real data. 10 Moran, M. J. and Shapiro H. N., Fundamentals of Engineering Thermodynamics, Wiley, 2008, pg. 112 3-19 Example 3.4-2 ---------------------------------------------------------------------------------- A closed, rigid tank filled with water vapor, initially at 20 MPa, 520oC, is cooled until its temperature reaches 400oC.
    [Show full text]
  • Ideal Gasses Is Known As the Ideal Gas Law
    ESCI 341 – Atmospheric Thermodynamics Lesson 4 –Ideal Gases References: An Introduction to Atmospheric Thermodynamics, Tsonis Introduction to Theoretical Meteorology, Hess Physical Chemistry (4th edition), Levine Thermodynamics and an Introduction to Thermostatistics, Callen IDEAL GASES An ideal gas is a gas with the following properties: There are no intermolecular forces, except during collisions. All collisions are elastic. The individual gas molecules have no volume (they behave like point masses). The equation of state for ideal gasses is known as the ideal gas law. The ideal gas law was discovered empirically, but can also be derived theoretically. The form we are most familiar with, pV nRT . Ideal Gas Law (1) R has a value of 8.3145 J-mol1-K1, and n is the number of moles (not molecules). A true ideal gas would be monatomic, meaning each molecule is comprised of a single atom. Real gasses in the atmosphere, such as O2 and N2, are diatomic, and some gasses such as CO2 and O3 are triatomic. Real atmospheric gasses have rotational and vibrational kinetic energy, in addition to translational kinetic energy. Even though the gasses that make up the atmosphere aren’t monatomic, they still closely obey the ideal gas law at the pressures and temperatures encountered in the atmosphere, so we can still use the ideal gas law. FORM OF IDEAL GAS LAW MOST USED BY METEOROLOGISTS In meteorology we use a modified form of the ideal gas law. We first divide (1) by volume to get n p RT . V we then multiply the RHS top and bottom by the molecular weight of the gas, M, to get Mn R p T .
    [Show full text]
  • Thermodynamics Molecular Model of a Gas Molar Heat Capacities
    Thermodynamics Molecular Model of a Gas Molar Heat Capacities Lana Sheridan De Anza College May 7, 2020 Last time • heat capacities for monatomic ideal gases Overview • heat capacities for diatomic ideal gases • adiabatic processes Quick Recap For all ideal gases: 3 3 K = NK¯ = Nk T = nRT tot,trans trans 2 B 2 and ∆Eint = nCV ∆T For monatomic gases: 3 E = K = nRT int tot,trans 2 and so, 3 C = R V 2 and 5 C = R P 2 Reminder: Kinetic Energy and Internal Energy In a monatomic gas the three translational motions are the only degrees of freedom. We can choose 3 3 E = K = N k T = nRT int tot,trans 2 B 2 (This is the thermal energy, so the bond energy is zero { if we liquify the gas the bond energy becomes negative.) Equipartition Consequences in Diatomic Gases Reminder: Equipartition of energy theorem Each degree of freedom for each molecule contributes an and 1 additional 2 kB T of energy to the system. A monatomic gas has 3 degrees of freedom: it can have translational KE due to motion in 3 independent directions. A diatomic gas has more ways to move and store energy. It can: • translate • rotate • vibrate 21.3 The Equipartition of Energy 635 Equipartition21.3 The Equipartition Consequences of Energy in Diatomic Gases Predictions based on our model for molar specific heat agree quite well with the Contribution to internal energy: Translational motion of behavior of monatomic gases, but not with the behavior of complex gases (see Table the center of mass 21.2).
    [Show full text]
  • Lecture 6: Entropy
    Matthew Schwartz Statistical Mechanics, Spring 2019 Lecture 6: Entropy 1 Introduction In this lecture, we discuss many ways to think about entropy. The most important and most famous property of entropy is that it never decreases Stot > 0 (1) Here, Stot means the change in entropy of a system plus the change in entropy of the surroundings. This is the second law of thermodynamics that we met in the previous lecture. There's a great quote from Sir Arthur Eddington from 1927 summarizing the importance of the second law: If someone points out to you that your pet theory of the universe is in disagreement with Maxwell's equationsthen so much the worse for Maxwell's equations. If it is found to be contradicted by observationwell these experimentalists do bungle things sometimes. But if your theory is found to be against the second law of ther- modynamics I can give you no hope; there is nothing for it but to collapse in deepest humiliation. Another possibly relevant quote, from the introduction to the statistical mechanics book by David Goodstein: Ludwig Boltzmann who spent much of his life studying statistical mechanics, died in 1906, by his own hand. Paul Ehrenfest, carrying on the work, died similarly in 1933. Now it is our turn to study statistical mechanics. There are many ways to dene entropy. All of them are equivalent, although it can be hard to see. In this lecture we will compare and contrast dierent denitions, building up intuition for how to think about entropy in dierent contexts. The original denition of entropy, due to Clausius, was thermodynamic.
    [Show full text]
  • The Discovery of Thermodynamics
    Philosophical Magazine ISSN: 1478-6435 (Print) 1478-6443 (Online) Journal homepage: https://www.tandfonline.com/loi/tphm20 The discovery of thermodynamics Peter Weinberger To cite this article: Peter Weinberger (2013) The discovery of thermodynamics, Philosophical Magazine, 93:20, 2576-2612, DOI: 10.1080/14786435.2013.784402 To link to this article: https://doi.org/10.1080/14786435.2013.784402 Published online: 09 Apr 2013. Submit your article to this journal Article views: 658 Citing articles: 2 View citing articles Full Terms & Conditions of access and use can be found at https://www.tandfonline.com/action/journalInformation?journalCode=tphm20 Philosophical Magazine, 2013 Vol. 93, No. 20, 2576–2612, http://dx.doi.org/10.1080/14786435.2013.784402 COMMENTARY The discovery of thermodynamics Peter Weinberger∗ Center for Computational Nanoscience, Seilerstätte 10/21, A1010 Vienna, Austria (Received 21 December 2012; final version received 6 March 2013) Based on the idea that a scientific journal is also an “agora” (Greek: market place) for the exchange of ideas and scientific concepts, the history of thermodynamics between 1800 and 1910 as documented in the Philosophical Magazine Archives is uncovered. Famous scientists such as Joule, Thomson (Lord Kelvin), Clau- sius, Maxwell or Boltzmann shared this forum. Not always in the most friendly manner. It is interesting to find out, how difficult it was to describe in a scientific (mathematical) language a phenomenon like “heat”, to see, how long it took to arrive at one of the fundamental principles in physics: entropy. Scientific progress started from the simple rule of Boyle and Mariotte dating from the late eighteenth century and arrived in the twentieth century with the concept of probabilities.
    [Show full text]