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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.

Short Answer

Expert verified

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

Step by step solution

01

Given Information

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

CV=-32NK

Where,

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

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

02

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 CVin the above equation, we get,

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

In this equation, fis the function of Nand 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:

03

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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Most popular questions from this chapter

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