Starting with the result of Problem 2.17, find a formula for the temperature of an Einstein solid in the limit qN. Solve for the energy as a function of temperature to obtain U=Nϵe-ϵ/kT (whereϵ is the size of an energy unit).

Short Answer

Expert verified

The required expression isU=Nεe-εkT.

Step by step solution

01

Given

Expression for the multiplicity of Einstein solid in low-temperature limit qNis given as:

role="math" localid="1646983518799" ΩNeqq..........(1)

Here, Nis number of oscillator in solid, qis number of energy unit.

02

Explanation

Mathematically, temperature can be defined as:

1T=SU..........(2)

Where,

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

Total energy of the system is given as:

U=qε

Where, qis number of energy unit.

Equation (1) can be written by substituting the values of qas:

ΩNeεUUε

Entropy is given as:

S=klnΩ

Here, kis Boltzmann constant and Ωis multiplicity.

By substituting the value of Ωin the above equation, we get,

S=klnNeεUUε

But lnab=bln(a), therefore, the above equation can be rewritten as:

S=kUεlnNeεU

Also, lnab=lna+lnband lnab=lna-lnbso, the above equation becomes:

S=UkεlnNε+lne-lnUS=UkεlnNε+1-lnU

By substituting this value of Sin equation (2), we get,

1T=SU=UUkεln(Nε)+1-ln(U)1T=kεln(Nε)+kε-UkUε-kεln(U)1T=kε[ln(Nε)-ln(U)]lnU=ln(Nε)-εkT

Take exponential for both the sides of the above equation,

U=elnNε-εkTU=eln(Nε)·e-εkTU=Nεe-εkT

This result is valid only for low temperature as U=qεN.

03

Final answer

Hence, the energy as a function of temperature can be solved to obtainU=Nϵe-ϵ/kT.

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Most popular questions from this chapter

Use the definition of temperature to prove the zeroth law of thermodynamics, which says that if system A is in thermal equilibrium with system B, and system B is in thermal equilibrium with system C, then system A is in thermal equilibrium with system C. (If this exercise seems totally pointless to you, you're in good company: Everyone considered this "law" to be completely obvious until 1931, when Ralph Fowler pointed out that it was an unstated assumption of classical thermodynamics.)

Sketch (or use a computer to plot) a graph of the entropy of a two-state paramagnet as a function of temperature. Describe how this graph would change if you varied the magnetic field strength.

In Problem 1.55 you used the virial theorem to estimate the heat capacity of a star. Starting with that result, calculate the entropy of a star, first in terms of its average temperature and then in terms of its total energy. Sketch the entropy as a function of energy, and comment on the shape of the graph.

What partial-derivative relation can you derive from the thermodynamic identity by considering a process that takes place at constant entropy? Does the resulting equation agree with what you already knew? Explain.

An ice cube (mass 30g)0°Cis left sitting on the kitchen table, where it gradually melts. The temperature in the kitchen is 25°C.

(a) Calculate the change in the entropy of the ice cube as it melts into water at 0°C. (Don't worry about the fact that the volume changes somewhat.)

(b) Calculate the change in the entropy of the water (from the melted ice) as its temperature rises from 0°Cto 25°C.

(c) Calculate the change in the entropy of the kitchen as it gives up heat to the melting ice/water.

(d) Calculate the net change in the entropy of the universe during this process. Is the net change positive, negative, or zero? Is this what you would expect?

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