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Change of entropy in the spontaneous thermalization of two distinct blocks

Variação da entropia na termalização espontânea de dois blocos distintos

Abstracts

When two blocks with distinct initial temperatures are placed in thermal contact, heat flows from the hotter block to the cooler until thermal equilibrium is reached. Given the initial temperatures, it is easy to predict the final temperature and, for identical blocks, to find a closed-form expression for the overall change of entropy, showing that it is a positive quantity. The change of entropy in the more general case of distinct blocks, however, is not mentioned in the introductory physics textbooks, which sounds as an indication of very complex mathematics underlying the problem. In this shortnote, I show that this is not the case by deriving a simple expression for the change of entropy and developing an elementary proof, at one-variable calculus level, that this change is a positive quantity.

heat transfer; thermal equilibrium; entropy change


Quando dois blocos com temperaturas iniciais distintas são postos em contato térmico, o calor passa do bloco mais quente para o mais frio até que o equilíbrio térmico seja atingido. Dadas as temperaturas iniciais, é fácil prever a temperatura final e, para blocos idênticos, encontrar uma fórmula simples para a variação da entropia do sistema, mostrando que ela é positiva. A variação de entropia no caso mais geral de blocos distintos, entretanto, não é mencionada nos livros-texto de física básica, o que soa como um indicativo de que há aspectos matemáticos muito complexos por trás do problema. Nesta nota, eu mostro que isto não ocorre e o faço determinando uma expressão simples para a variação da entropia e exibindo uma demonstração elementar, ao nível de cálculo diferencial de uma variável, de que tal variação é positiva.

transferência de calor; equilíbrio térmico; variação da entropia


When all parts of a material system are at the same temperature, the system is in thermal equilibrium. Otherwise, heat will flow from the hotter parts to the cooler via conduction, convection, and radiation. Although spontaneous thermalization is a common phenomenon in our everyday experience, as well as a topic covered in introductory physics courses, some questions are not addressed in textbooks. For instance, for distinct blocks, there would be a simple expression for the change of entropy? Could it be proved that it is a positive quantity? The absence of these discussions in introductory physics textbooks has bothered me since my own undergraduate times because heat exchange between two blocks is a central paradigm in thermodynamics, underlying the definition of temperature itself when we adopt the macroscopic point of view [1[1] M.W. Zemansky and R.H. Dittman, Heat and thermodynamics (McGraw-Hill, New York, 1997), 7th ed., p. 90–93.]. Fortunately, on teaching introductory physics for a class of devoted students, last year, I was asked just about those questions, which has motivated me to search for an elementary approach, presentable to first year undergraduates with knowledge of calculus of a single variable only, without mentioning partial derivatives.

Take into account two distinct blocks with initial (absolute) temperatures T1> T2 > 0, kept inside an insulated container, initially separated each other by a partition, as seen in Fig. 1(a). At time t = 0, the partition is removed and the blocks are put in thermal contact, see Fig. 1(b). Heat then will flow from the hotter block to the cooler until thermal equilibrium to be reached, at some final temperature Teq. Given the (in general, distinct) thermal capacities C1 and C2 of our blocks, the final temperature Teq is easily determined as follows. On neglecting any heat exchange other than that between the blocks, all heat that leaves block 1 is absorbed by block 2, i.e. Q1 + Q2 = 0. On assuming that both C1 and C2 are independent of temperature, one has C1 (TeqT1) + C2 (TeqT2) = 0,2 2 For a solid body, the thermal capacity is a positive quantity defined as C ≡ δQ/dT. For simplicity, we are neglecting changes of C with T, which is a good approximation for most pure solids beyond the low-temperature regime, according to the Dulong-Petit law (see Sec. 9.8 of Ref. [1]). so

(1)Teq=C1T1+C2T2C1+C2,
a well-known result (see, e.g., Sec. 18-8 of Ref. [2[2] D. Halliday, R. Resnick, and J. Walker, Fundamentals of Physics (Wiley, New York, 2011), 9th ed.]).3 3 Since Teq is a weighted mean of T1 and T2 (with statistical weights C1 and C2, respectively), then T2 < Teq < T1.

With the result for Teq in hands, let us determine the overall change of entropy in our system – i.e., its variation from the initial nonequilibrium state (at t = 0) to the final equilibrium state, in which the blocks attain the same temperature Teq.4 4 Note that at any time t < 0 the system is assumed to be composed by two insulated subsystems with distinct temperatures which are kept, each, in thermodynamic equilibrium. Of course, this demands the partition itself to be adiabatic. We begin with the simpler case of identical blocks, for which C1 = C2C. From Eq. (1), it promptly follows that Teq = (T1 + T2)/2. As this spontaneous heat transfer involves an internal thermal irreversibility, with an equilibrium state only in the final state, we cannot directly replace the actual irreversible process with a reversible one because the initial state itself is not an equilibrium state. For block 1, imagine that it is put in contact successively with a series of reservoirs ranging in temperature from T1 to Teq. We then have a very great number N of almost reversible processes and then the change of entropy can be determined by adding δQ/T for all these processes and taking the limits N and δQ → 0. The result is

(2)ΔS1=R1δQTT1TeqCdTT=Cln(TeqT1)=Cln(T1Teq),
where R1 is the sequence of reversible processes described above. Analogously, for block 2 one has
(3)ΔS2=R2δQTT2TeqCdTT=Cln(TeqT2).
From Eqs. (2) and (3), one has
(4)ΔSsystem=ΔS1+ΔS2=C[2lnTeqln(T1T2)]=2C(lnTeqlnT1T2).
For identical blocks, Teq = (T1 + T2)/2, which is the arithmetic mean of T1 and T2. It is easy to see that, for any positive numbers T1T2, the arithmetic mean is greater than the geometric mean T1T2 (by squaring both means), then ln Teq > ln T1T2, so ΔSsystem > 0. As our system is isolated from its neighborhood, the change of entropy of the universe ΔSuniv equals ΔSsystem and then ΔSuniv > 0, in agreement to the entropic version of the 2nd law of thermodynamics. This proof of increase of entropy can be found in some introductory physics textbooks (e.g., Sec. 20-3 of Ref. [2[2] D. Halliday, R. Resnick, and J. Walker, Fundamentals of Physics (Wiley, New York, 2011), 9th ed.]), though not in the general form given here, for their authors prefer to attribute numerical values for the initial temperatures and then compute ΔSsystem.

For distinct blocks, our rigorous analysis of the change of entropy demands the following result.

Theorem 1 (A positive function)Given a real constant α > 0, let

f(x)(1+α)ln(x+α1+α)lnx
be a real function defined for all x ≥ 1. Then f(x) > 0 for all x > 1.

Proof. The derivative of the given function f(x) is

f(x)=1+αx+α1x=α(x1)x(x+α),
so f(x) is a differentiable (hence continuous) function for all x ≥ 1. Being α > 0, then f′(x) = 0 for x = 1 only, and f′(x) > 0 for all x > 1. This implies that f(x) is an increasing function for all x ≥ 1, therefore f(x) ≥ f(1) = 0 for all x ≥ 1. Now, assume (towards a contradiction) that there is some x > 1 for which f(x) = 0. From Rolle’s theorem,5 5 This theorem establishes that, given a real function f(x) that is continuous on an interval [a, b] and differentiable on the open (a, b), if f(a) = f(b) then there is at least one number c in (a, b) such that f′(c) = 0. See, e.g., Sec. 3.2 of Ref. [3]. this would imply the existence of at least one point c, 1 < c < x, such that f′(c) = 0, which contradicts the fact that f′(x) > 0 for all x > 1. Then, f(x) > 0 for all x > 1.

By following the same strategy employed for identical blocks – i.e., to divide the actual irreversible thermalization process into an infinity of reversible stages –, one has

(5)ΔS1+ΔS2=T1TeqC1dTT+T2TeqC2dTT=C2ln(TeqT2)C1ln(T1Teq).
From the expression for Teq in Eq. (1), one finds
(6)ΔSsystem=C2(lnTeqlnT2)C1(lnT1lnTeq)=C2ln(C1x+C2C1+C2)+C1ln(C1+C2/xC1+C2)=C2ln(C1x+C2C1+C2)+C1ln(C1x+C2(C1+C2)x)=(C1+C2)ln(C1x+C2C1+C2)C1lnx,
where xT1/T2. On dividing both sides by C1, one has
(7)ΔSsystemC1=(1+C2C1)ln(x+C2/C11+C2/C1)lnx.
Finally, on putting α = C2/C1, which is of course a positive constant, Eq. (7) reduces to
(8)ΔSsystemC1=(1+α)ln(x+α1+α)lnx,
From Theorem 1, we know that the function at the right-hand side is positive for any x > 1, so ΔSsystem/C1 > 0 whenever T1 > T2, which implies that ΔSsystem > 0. I could not find a such proof in literature.

For those interested in approaching this topic in a deeper mathematical level, e.g. by analyzing other irreversible processes (or paths) with the same initial and final states, in a more advanced course (e.g., Classical Thermodynamics for physicists or Heat and Mass Transfer for engineers), a recent paper by Stilck and Brum (see Ref. [4[4] J.F. Stilck and R.M. Brum, Revista Brasileira de Ensino de Física 35, 4306 (2013).]) would be more appropriate.

  • 2
    For a solid body, the thermal capacity is a positive quantity defined as CδQ/dT. For simplicity, we are neglecting changes of C with T, which is a good approximation for most pure solids beyond the low-temperature regime, according to the Dulong-Petit law (see Sec. 9.8 of Ref. [1[1] M.W. Zemansky and R.H. Dittman, Heat and thermodynamics (McGraw-Hill, New York, 1997), 7th ed., p. 90–93.]).
  • 3
    Since Teq is a weighted mean of T1 and T2 (with statistical weights C1 and C2, respectively), then T2 < Teq < T1.
  • 4
    Note that at any time t < 0 the system is assumed to be composed by two insulated subsystems with distinct temperatures which are kept, each, in thermodynamic equilibrium. Of course, this demands the partition itself to be adiabatic.
  • 5
    This theorem establishes that, given a real function f(x) that is continuous on an interval [a, b] and differentiable on the open (a, b), if f(a) = f(b) then there is at least one number c in (a, b) such that f′(c) = 0. See, e.g., Sec. 3.2 of Ref. [3[3] R. Larson and B.H. Edwards, Calculus, 9th ed. (Brooks/Cole, Belmont, CA, 2010).].

References

  • [1]
    M.W. Zemansky and R.H. Dittman, Heat and thermodynamics (McGraw-Hill, New York, 1997), 7th ed., p. 90–93.
  • [2]
    D. Halliday, R. Resnick, and J. Walker, Fundamentals of Physics (Wiley, New York, 2011), 9th ed.
  • [3]
    R. Larson and B.H. Edwards, Calculus, 9th ed. (Brooks/Cole, Belmont, CA, 2010).
  • [4]
    J.F. Stilck and R.M. Brum, Revista Brasileira de Ensino de Física 35, 4306 (2013).

Figure

Figura 1
Our system is an insulated container within which there are two blocks with distinct initial temperatures T1 > T2. Panel (a): initially, the blocks are separated apart by an adiabatic partition. Panel (b): At t = 0 the partition is removed and the blocks are put in thermal contact. Heat will flow from block 1 to block 2, as indicated by the arrow, until thermal equilibrium to be reached, at a final temperature Teq.

Publication Dates

  • Publication in this collection
    30 Mar 2015
  • Date of issue
    Jan-Mar 2015

History

  • Received
    30 May 2014
  • Accepted
    01 Nov 2014
Sociedade Brasileira de Física Caixa Postal 66328, 05389-970 São Paulo SP - Brazil - São Paulo - SP - Brazil
E-mail: marcio@sbfisica.org.br