Thermodynamics Ch 18 – The Laws of Thermodynamics 18.1 Temperature and the Zeroth Law of Thermodynamics The Zeroth Law of Thermodynamics If two objects are separately in thermal equilibrium with a 3rd object, then the first two objects are in thermal equilibrium with each other. Thermal equilibrium: If two objects are in thermal equilibrium then neither object will exchange energy by heat or electromagnetic radiation if they are placed in thermal contact. Temperature is a property that determines whether an object is in thermal equilibrium. Thermal contact: If in thermal contact two objects will exchange energy between them if a temperature difference. 18.2 The 1st Law of Thermodynamics The 1st law of thermodynamics (an energy conservation equation specifying that) the only type of energy that changes in the system are the internal energy, Eint or U. ΔU = Q - W Internal Energy is a state variable just like P, V, and T (State variable do not depend upon path, just state) thus Q - W is INDEPENDENT of path An isolated system is a system that no Non-isolated, but is cyclic (starts and ends in the same state) energy is transferred by heat and the work done on ΔU = 0 Joules the system is zero. (Doesn’t interact with Thus Q (energy added to system) is equal to the Work done environment) by the system. Q = Work Q = 0 Joules ΔUi = ΔUf Example Fill in the missing entries for an ideal gas that is taken through the three processes. Q W U AB -53 J (a) (b) BC -280 J -130 J (c) CA (e) 150 J (d) (a) WAB = PΔV WAB = 0 (b) (d) ΔUCA ΔUCA ΔUCA ΔUAB = QAB – WAB ΔUAB = -53 – 0 ΔUAB = -53 J (c) ΔUBC = QBC – WBC ΔUBC = -280 – (-130) ΔUBC = -150 J ΔU = 0 = -ΔUAB - ΔUBC = -(-53) – (-150) = 203 J (e) ΔUCA = QCA – WCA 203 = QCA – 150 QCA = 353 J Fire Syringe: TH-B-FS 18.3 Thermal Processes ΔEint (or U) = Q – W An adiabatic process is one that no energy enters or leaves from the system by heat. ΔEint = -Work As gas expands adiabatically the temperature reduces accordingly For a cloud in deep space that is spurting out material very fast, at that point the temperature can go below the ambient background radiation temperature of 3 Kelvin Q = 0 Joules Isobaric (Constant Pressure) W = P ΔV P is a constant A plot of P vs V for an ideal gas yields a hyperbolic curve (an isotherm) Isothermic (constant Temp) ΔEint = 0 Joules Q=W W = -∫ P dV W = -∫ (nRT/V) dV Work = -nRT ln(Vf/Vi) Work = nRT ln(Vi/Vf) Work = 0 ΔU = Q Isovolumetric If energy is added by heat to a system, all of the transferred energy remains in the system as increased internal energy Work and Heat in Thermodynamics Using a macroscopic approach, the state of the system is described using P, V, T, and internal energy, so these are called “state variables.” Work = force applied through a displacement Work = F ◦ Δr Work = -F Δy Work = -PA Δy Work = - P ΔV “Transfer variables” only involve transfer of energy. So no “change” or transfer of energy…no transfer variables. The work done on a gas as it is taken from an initial state to a final state depends on the path between these states Diffusion in Air: TH-D-DA 18.4 Specific Heats for an Ideal Gas: Constant Pressure, Constant Volume Q = n CVΔT The energy added to the gas by heat at a constant volume only the internal energy, U, of the gas increases. (No work is done; Area under curve is zero since a vertical line.) ΔU = Q +W ΔU = n CVΔT + W (but W = 0) ΔU = n CVΔT Constant Volume U = n CVT Etrans = n CVT 3/2 nRT = n CVT CV = 3/2 R From the previous chapter the theorem of equipartition of energy gives us three degrees of freedom This result is if the only internal energy is from translation motion …thus monatomic atoms. Thus we predict CV = 3/2 R for all monatomic atoms, CV = 3/2 (8.314 J/ K*mole) CV = 12.5 J/ K*mole We find that this is true experimentally Example: Calculate the change in internal energy of 3.00 mol of helium gas when its temperature is increased by 2.00 K. n = N / NA and kB = R / NA Etranslational = 3/2 nRT Eint = 3/2 n R ΔT Eint = 3/2 (3)(8.314)(2K) Eint = 74.8 Joules Q = n CPΔT The energy added to the gas by heat for constant pressure not only increases the internal energy, U, but also must account for the energy transferred out of the system by the increased volume, Work (area under the curve.) Etranslational = N (½mvave2) Etranslational = 3N(½kBT) Etranslational = 3/2 NkBT We see that T+ΔT is the same for both processes (constant pressure and constant volume), but the constant pressure path has a change of volume which represents the work that is also done on the system ΔU ΔU n CVT CP – CV CP – 3R/2 CP = Q = nCPΔT = nCPΔT =R =R = 5R/2 - W - P ΔV - nRΔT We know ΔU for both constant pressure and constant volume is the same, n CVΔT, due to both go to the same isotherm. A ratio of these two specific heats is useful in solving problems, thus γ = CP/CV = 5R/2 / 3R/2 γ = 1.67 18 Adiabatic Processes for an Ideal Gas Adiabatic Process is a process where no energy is transferred to surrounding environment. These processes are either quick processes or insulated processes and is represented by PVγ = constant Example Air in a thundercloud expands as it rises. If its initial temp is 300 K, and no energy is lost by thermal conduction on expansion, what is its temperature when the initial volume has doubled? PVγ PVγ T Vγ-1 300 Vγ-1 (V/2V)1.40-1 = constant = PfVfγ = Tf Vfγ-1 = Tf (2V)γ-1 = Tf /300 γ γ P V = Pf Vf γ γ (nRT/V)V = (nRTf/Vf)Vf γ γ (T/V) V = (Tf/Vf) Vf γ γT V -1 = T f Vf 1 γ for diatomic molecules, 1.40 Tf = 227 K The Equipartition of Energy As we’ve seen the model for molar specific heat agrees only with monatomic gases as expected. We need to include (a) translational KE AND (b) rotational As we can see the distance the diatomic atom is from the y-axis so the Inertial, KR = ½Iyω2 = 0 Joules, but Inertia is far from zero for rotation about the x & z-axes Also our value of AND CP – CV = R does prove (c) vibrational (see below) to be accurate for all gases. Thus the total inertia for any diatomic molecule will just be two of the three axes. (We can rotate the axis so that Inertia will always be zero about one of the axes.) To write Eint with both (a) translational and (b) rotational energy yields U = ETrans + ERot U = 3N(½kbT) + 2N(½kbT) U = 5N(½kbT) U = 5/2 nRT ΔEint = n CV ΔT (solve for CV) CV = ( ΔEint / ΔT) / n CV = ( 5/2 nRT / ΔT) / n CV = 5/2 R CP – CV = R CP – 5/2 R = R CP = 7/2 R U = QV + PΔV But with QV, PΔV = 0 J. So QV = U ΔEint = n CV ΔT (each degree of freedom contributes on average ½k bT per molecule, for an additional two degrees of freedom for rotation) We know from the previous section monatomic atoms γmono = 1.67 And for diatomic atoms γdi = 1.40 The results agree well with experimental data. CV = 1/n (ΔEint/ΔT) γ = CP / CV γ = 7R/2 / 5R/2 γ = 1.40 To write U with both (a) translational and (b) rotational energy (c) and vibrational yields U U U U = ETrans + ERot + EVib = 3N(½kBT) + 2N(½kBT) + 2N(½kBT) = 7/2 nRT = 7N(½kBT) (2 more degrees of freedom for vibration; each atom is vibrating) CV = 1/n (dEint/dT) CV = 7/2 R monatomic atoms, γmono = 1.67 CP – CV = R CP – 7/2 R = R CP = 9/2 R diatomic atoms, γdi = 1.40 γ = CP / CV γ = 9R/2 / 7R/2 γ = 1.29 And for polyatomic atoms, γpoly = 1.29 To explain molar specific heat of a solid at high temps, we use small displacements of an atom from its equilibrium position which is approximated by simple harmonic motion. Ex = ½mvx2 + ½kx2 (review from Ch 7 & 8) Similarly along the y & z-axes, thus for a total of 6 degrees of freedom. Eint = Ex + Ey + Ez (Remember…energy isn’t a vector) Eint = 2N(½kBT) + 2N(½kBT) + 2N(½kBT) Eint = 3NkBT = 3nRT CV = 1/n (dEint/dT) CV = 3 R (at lower temperatures classical physics just isn’t a good enough approximation; this is only good at high temps) Example A certain molecule has f degrees of freedom. Show that an ideal gas consisting of such molecules has the following properties: (1) total internal energy is fnRT/2; Eint = N(½kBT) for each degree of freedom theorem of equipartition energy So if, f, degrees of freedom…then Eint = fN(½kBT); where n = N/kB From previous chapter: kB = R / NA ; n = N / NA; N = nR / kB Eint = fn(½RT) (2) molar specific heat at constant vol. is fR/2; CV = 1/n ( dEint / dT) CV = 1/n (d [fn(½RT)] / dT) CV = ½fR (3) molar specific heat at constant pressure; is (f + 2)R/2; CP – CV = R CP = ½fR + R CP = fR/2 + 2R/2 CP = ½(f + 2)R (4) specific heat ratio is = CP/CV = (f + 2)/f γ= CP / CV γ = ½(f + 2)R / ½fR γ = (fR + 2R) / fR γ = (f + 2) / f 18.5 The 2nd Law of Thermodynamics When objects of different temperatures are brought into thermal contact, the spontaneous flow of heat that results is always from the high temperature object to the low temperature object. Spontaneous heat flow never proceeds in the reverse direction. A heat engine is a device A heat engine carries some working substance through a cyclic process that takes an energy input through heat an does a fraction of the input energy as work as a cyclic process. A sterling engine A steam locomotive Automotive engine Example Suppose a heat engine is connected to two energy reservoirs, one a pool of molten aluminum (660°C) and the other a block of solid mercury (–38.9°C). The engine runs by freezing 1.00 g of aluminum and melting 15.0 g of mercury during each cycle. The Lf of Al is during the working substance absorbs energy by HEAT from a high temp energy reservoir work is done by the engine energy is expelled by heat to a lower-temp reservoir Heat required to melt 15.0 g of Hg Energy absorbed by 1.00 g of aluminum the work output Q= m Lf Q = 0.015 (1.18x104) Qc = 177 Joules Q= m Lf Q = 0.001(3.97x105) Qh = 397 J Wengine = Qh – Qc Wengine = 397-177 Wengine = 220 J eff = Wengine / Qh eff = 220 / 397 eff = 55.4% The theoretical (Carnot) efficiency is 3.97 x 105 J/kg; Lf of Hg is What is the efficiency of this engine? 1.18 x 104 J/kg. 18.6 Heat Engines and the Carnot Cycle effmax = 1 – TC/TH effmax = 1 – (273.15-38.9) / (273.15+660) effmax = 74.9% Example Carnot’s theorem – No real heat engine operating between two energy reservoirs can be more efficient than a Carnot engine operating between the same two reservoirs. What is the coefficient of performance of a refrigerator that operates with Carnot efficiency between temperatures –3.00°C and +27.0°C? COPrefrig = TC / ∆T COPrefrig = (273.15+27) / 30 COPrefrig = 9 This figure is explained below in Gasoline engine section Example A heat engine operating between 200°C and 80.0°C achieves 20.0% of the maximum possible efficiency. What energy input will enable the engine to perform 10.0 kJ of work? Intake stroke O A The Carnot efficiency of the engine is effc = ∆T / Th effc = (200-80) / (273.15+200) effc = 25.3% Chemical PE In Positive Work on gas Compression stroke A PE to Qh B Gas expands adiabatically If 20% efficient we only get 25.3% * 20% = 5.06% eff 5.06% Qh = Wengine/ Qh = 10 KJ / Qh = 197 KJ Combustion B C P drops suddenly V drops V1 to V2 Power stroke C D Exhaust opens D A Exhaust stoke A O If we assume an ideal gas, then the efficiency of the Otto cycle is eff = 1 – (V1/V2)1-γ γ = CP/CV; where V1/V2 is the compression ratio Stirling Engine: TH-F-SC Example A gasoline engine has a compression ratio of 6.00 and uses a gas for which γ = 1.40. (a) What is the efficiency of the engine if it operates in an idealized Otto cycle? (b) What If? If the actual efficiency is 15.0%, what fraction of the fuel is wasted as a result of friction and energy losses by heat that could by avoided in a reversible engine? effotto = 1 – (V2 / V1)γ-1 effotto = 1 – (1 / 6)1.4 - 1 effotto = 51.2% losses = effotto - effactual losses = 51.2% - 15% losses = 36.2% 18.7 Refrigerators, Air Conditioners, and Heat Pumps A heat pump transfers energy from a cold to a hot reservoir. We must add energy to accomplish this process. Other common names, air conditioner, refrigerator, etc. For heating mode COP(heater) = Qh / Work For cooling mode COP(refrig) = Qc / Work Good refrigerators have a coefficient of performance, COP, of about 6 Clausius statement Energy does NOT transfer spontaneously by heat from a cold object to a hot object! Example a. COP(refrig) = Qc / Work A refrigerator has a coefficient of 5.00 = 120 J / Work performance equal to 5.00. The Work = 24.0 Joules refrigerator takes in 120 J of energy from a cold reservoir in each b. Heat expelled = Heat removed + Work done cycle. Find (a) the work required in each cycle and (b) the energy expelled to the hot reservoir. Qh Qh Qh = Qc = 120 = 144 Joules + Work + 24 18.8 Entropy Entropy is a measure of disorder in isolated systems. Entropy is another state variable of 2nd law of thermodynamics For a Carnot engine operating in a cycle |Qh|/Th = |Qc|/Tc Thus ∆S = 0 Example An ice tray contains 500 g of liquid water at 0°C. Calculate the change in entropy of the water as it freezes slowly and completely at 0°C. For a freezing process, change of entropy, ∆S = ∆Q / T Quasi-Static, Reversible Process for an Ideal Gas ∆S = nCv ln(Tf/Ti) + nR ln(Vf/Vi) ∆S = -mLf / T ∆S = -.5(3.33x105)/273.15 ∆S = -610 J/K The total entropy of an isolated system that undergoes a change CANNOT decrease In irreversible processes Entropy always increases In reversible processes (non-real processes) ∆S is constant Entropy in free expansion (no pressure increase) Entropy Change in Calorimetric Processes Tf = (m1c1Tc + m2c2Th) / (m1c1 + m2c2) ∆S = ∆Qr /T ∆S = (nRT/V) ∆V / T (utilize calculus to solve) ∆S = nRln(Vf/Vi) Example The temperature at the surface of the Sun is approximately 5700 K, and the temp at the surface of the Earth is approximately 290 K. What entropy change occurs when 1000 J of energy is transferred by radiation from the Sun to the Earth? ∆S = ∆Qr /T ∆S = m1c1 ln(Tf/Tc) + m2c2 ln(Tf/Th) ∆Ssystem = ∆(Q / T) ∆Ssystem = ∆(1000/290 – 1000/5700) ∆Ssystem = 3.27 J/K 18.9 Order, Disorder, and Entropy Entropy can be thought of as the increase in disorder in the universe. If we look at the ultimate fate of the universe in light of the continual increase in entropy, we might envision a future in which the entire universe would have come to the same temperature. At this point, it would no longer be possible to do any work, nor would any type of life be possible. This is referred to as the “heat death” of the universe. So if entropy is continually increasing, how is life possible? How is it that species can evolve into ever more complex forms? Doesn’t this violate the second law of thermodynamics? No – life and increasing complexity can exist because they use energy to drive their functioning. The overall entropy of the universe is still increasing. When a living entity stops using energy, it dies, and its entropy can increase rather quickly. Bromine Diffusion: TH-D-BD 18.10 The Third Law of Thermodynamics Absolute zero is a temperature that an object can get arbitrarily close to, but never attain. Temperatures as low as 2.0 x 10-8 K have been achieved in the laboratory, but absolute zero will remain ever elusive – there is simply nowhere to “put” that last little bit of energy. This is the third law of thermodynamics: It is impossible to lower the temperature of an object to absolute zero in a finite number of steps.