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Q. 3.15

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An Introduction to Thermal Physics
Found in: Page 97
An Introduction to Thermal Physics

An Introduction to Thermal Physics

Book edition 1st
Author(s) Daniel V. Schroeder
Pages 356 pages
ISBN 9780201380279

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Short Answer

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.

The required expression for the entropy of a star is S=-32NKln2U3NK+f(N,V) and the graph can be sketched as below.

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Step by Step Solution

Step 1: Given Information

The heat capacity of a star that was estimated using the virial theorem is given as:

CV=-32NK

Where,

N is the number of particles (typically dissociated protons and electrons).

The negative sign symbolizes that it is a gravitational bound system.

Step 2: Calculation

The change in entropy is given as:

S=CV(T)TdT

Where,

CV = specific heat

T = Temperature in Kelvin

By substituting the value of CV in the above equation, we get,

S=-32NKTdTS=-32NK1TdTS=-32NKTln(T)+f(N,V) ..........(1)

In this equation, f is the function of N and volume V.

Total energy of gravitationally bound system is negative and from the virial theorem, it is found that:

U=-K=-32NKT

By rearranging the terms, we get,

T=-2U3NK

By substituting this value in equation (1), we get,

S=-32NKln2U3NK+f(N,V)

For plotting the graph, let us further simplify the above equation,

S=-32NKln(U)-32NKln3NK2+f(N,V)S=-32NKln(U)+g(N,V)

From the above equation, the graph can be plotted as below:

Step 3: Final answer

Hence, the required expression is: S=-32NKln2U3NK+f(N,V)

The graph of entropy as a function can be sketched as follow:

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