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Entropy

Physics 202 Professor Lee Carkner Lecture 17. Entropy. PAL #16 Internal Energy. 3 moles of gas, temperature raised from 300 to 400 K He gas, isochorically Q = nC V D T, C V = (f/2)R = (3/2) R Q = (3)(3/2)R(100) = 3740 J # 4 for heat, all in translational motion He gas, isobarically

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Entropy

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  1. Physics 202 Professor Lee Carkner Lecture 17 Entropy

  2. PAL #16 Internal Energy • 3 moles of gas, temperature raised from 300 to 400 K • He gas, isochorically • Q = nCVDT, CV = (f/2)R = (3/2) R • Q = (3)(3/2)R(100) = 3740 J • # 4 for heat, all in translational motion • He gas, isobarically • Q = nCPDT, CP = CV + R = (5/2) R • Q = (3)(5/2)R(100) = 6333 J • # 2 for heat, energy in translational and work • H2 gas, isochorically • Q = nCVDT, CV = (5/2) R, f = 5 for diatomic • Q = (3)(5/2)R(100) = 6333 J • # 2 for heat, energy into translational and rotational motion • H2 gas, isobarically • Q = nCPDT, CP = CV + R = (7/2) R • Q = (3)(7/2)R(100) = 8725 J • # 1 for heat, energy, into translation, rotation and work

  3. Randomness • Classical thermodynamics is deterministic • Every time! • But the real world is probabilistic • It is possible that you could add heat to a system and the temperature could go down • The universe only seems deterministic because the number of molecules is so large that the chance of an improbable event happening is absurdly low

  4. Reversible • Why? • The smashing plate is an example of an irreversible process, one that only happens in one direction • Examples: • Heat transfer

  5. Entropy • What do irreversible processes have in common? • The degree of randomness of system is called entropy • In any thermodynamic process that proceeds from an initial to a final point, the change in entropy depends on the heat and temperature, specifically: DS = Sf –Si = ∫ (dQ/T)

  6. Isothermal Entropy • In practice, the integral may be hard to compute • Let us consider the simplest case where the process is isothermal (T is constant): DS = (1/T) ∫ dQ DS = Q/T • Like heating something up by 1 degree

  7. Entropy Change • Imagine now a simple idealized system consisting of a box of gas in contact with a heat reservoir • If the system loses heat –Q to the reservoir and the reservoir gains heat +Q from the system isothermally: DSbox = (-Q/Tbox) DSres = (+Q/Tres)

  8. Second Law of Thermodynamics (Entropy) DS>0 • This is also the second law of thermodynamics • Entropy always increases • Why? • The 2nd law is based on statistics

  9. State Function • Entropy is a property of system • Can relate S to Q and W and thus P, T and V DS = nRln(Vf/Vi) + nCVln(Tf/Ti) • Not how the system changes • ln 1 = 0, so if V or T do not change, its term drops out

  10. Statistical Mechanics • We will use statistical mechanics to explore the reason why gas diffuses throughout a container • The box contains 4 indistinguishable molecules

  11. Molecules in a Box • There are 16 ways that the molecules can be distributed in the box • Since the molecules are indistinguishable there are only 5 configurations • If all microstates are equally probable than the configuration with equal distribution is the most probable

  12. Configurations and Microstates Configuration I 1 microstate Probability = (1/16) Configuration II 4 microstates Probability = (4/16)

  13. Probability • There are more microstates for the configurations with roughly equal distributions • Gas diffuses throughout a room because the probability of a configuration where all of the molecules bunch up is low

  14. Multiplicity • The multiplicity of a configuration is the number of microstates it has and is represented by: W = N! /(nL! nR!) n! = n(n-1)(n-2)(n-3) … (1) • For large N (N>100) the probability of the equal distribution configurations is enormous

  15. Microstate Probabilities

  16. Entropy and Multiplicity • The more random configurations are most probable • We can express the entropy with Boltzmann’s entropy equation as: S = k ln W • Sometimes it helps to use the Stirling approximation: ln N! = N (ln N) - N

  17. Irreversibility • Irreversible processes move from a low probability state to a high probability one • All real processes are irreversible, so entropy will always increases • The universe is stochastic

  18. Arrows of Time • Three arrows of time: • Thermodynamic • Psychological • Cosmological • Direction of increasing expansion of the universe

  19. Entropy and Memory • Memory requires energy dissipation as heat • Psychological arrow of time is related to the thermodynamic

  20. Synchronized Arrows • Why do all the arrows go in the same direction? • Can life exist with a backwards arrow of time? • Does life only exist because we have a universe with a forward thermodynamic arrow? (anthropic principle)

  21. Fate of the Universe • If the universe has enough mass, its expansion will reverse • Cosmological arrow will go backwards • Universe seems to be open

  22. Heat Death • Entropy keeps increasing • Stars burn out • Can live off of compact objects, but eventually will convert them all to heat

  23. Next Time • Read: 20.5-20.7 • Homework: Ch 20, P: 6, 7, 21, 22

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