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Can a "miserly" system, with a concave-up entropy-energy graph, ever be in stable thermal equilibrium with another system? Explain.

Short Answer

Expert verified

No, a "miserly" system, with a concave-up entropy-energy graph, cannot be in stable thermal equilibrium with another system.

Step by step solution

01

Given Introduction

If two objects are in thermal equilibrium, their temperatures are said to be the same. It can be expressed in terms of the system's entropy and energy, the measure of randomness being the entropy. It is determined by the amount of energy that is not available for work.

02

Explanation

Mathematically, temperature can be defined as:

1T=SU

Where,

Sis the change in entropy and Uis the change in the internal energy of the body.

Systems in thermal equilibrium have the same temperature because their entropy-versus-energy graphs have the same slopes. The systems are coupled by gravity in a concave-up graph between entropy-energy graphs, and the temperature lowers when energy is supplied because the energy is stored as potential energy and the average kinetic energy is reduced. To put it another way, the heat capacity is negative. The entropy energy plot will thus be concave up in that situation.

Assume that there are two miserly systems, A and B. The temperature for both systems is the same. When energy is transmitted from system B to system A, system B becomes hotter, and a runway effect is observed because more energy is transferred spontaneously from system B to system A. As a result, the temperature of system B rises significantly above the temperature of system A.

As a result, two miserly systems can exist in thermal equilibrium with one another. These systems, however, are not stable.

03

Final answer

Hence, a "miserly" system, with a concave-up entropy-energy graph, cannot be in stable thermal equilibrium with another system.

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Most popular questions from this chapter

Use the thermodynamic identity to derive the heat capacity formula

CV=TSTV

which is occasionally more convenient than the more familiar expression in terms of U. Then derive a similar formula for CP, by first writing dHin terms of dSand dP.

Use the result of Problem 2.42 to calculate the temperature of a black hole, in terms of its mass M. (The energy is Mc2. ) Evaluate the resulting expression for a one-solar-mass black hole. Also sketch the entropy as a function of energy, and discuss the implications of the shape of the graph.

In Problem 2.32you computed the entropy of an ideal monatomic gas that lives in a two-dimensional universe. Take partial derivatives with respect to U,A, and N to determine the temperature, pressure, and chemical potential of this gas. (In two dimensions, pressure is defined as force per unit length.) Simplify your results as much as possible, and explain whether they make sense.

Use a computer to study the entropy, temperature, and heat capacity of an Einstein solid, as follows. Let the solid contain 50 oscillators (initially), and from 0 to 100 units of energy. Make a table, analogous to Table 3.2, in which each row represents a different value for the energy. Use separate columns for the energy, multiplicity, entropy, temperature, and heat capacity. To calculate the temperature, evaluate ΔU/ΔSfor two nearby rows in the table. (Recall that U=qϵfor some constant ϵ.) The heat capacity (ΔU/ΔT)can be computed in a similar way. The first few rows of the table should look something like this:

(In this table I have computed derivatives using a "centered-difference" approximation. For example, the temperature .28is computed as 2/(7.15-0).) Make a graph of entropy vs. energy and a graph of heat capacity vs. temperature. Then change the number of oscillators to 5000 (to "dilute" the system and look at lower temperatures), and again make a graph of heat capacity vs. temperature. Discuss your prediction for the heat capacity, and compare it to the data for lead, aluminum, and diamond shown in Figure 1.14. Estimate the numerical value of εin electron-volts, for each of those real solids.

As shown in Figure 1.14, the heat capacity of diamond near room temperature is approximately linear in T. Extrapolate this function up to 500K, and estimate the change in entropy of a mole of diamond as its temperature is raised from298K to 500K. Add on the tabulated value at298K (from the back of this book) to obtain S(500K).

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